Revisiting the Scaling Relations of Black Hole Masses and Host Galaxy Properties

Abstract

New kinematic data and modeling efforts in the past few years have substantially expanded and revised dynamical measurements of black hole masses (Mbh) at the centers of nearby galaxies. Here we compile an updated sample of 72 black holes and their host galaxies, and present revised scaling relations between Mbh and stellar velocity dispersion (sigma), V-band luminosity (L), and bulge stellar mass (Mbulge), for different galaxy subsamples. Our best-fitting power law relations for the full galaxy sample are log(Mbh) = 8.32 + 5.64*log(sigma/200 kms), log(Mbh) = 9.23 + 1.11*log(L/10^{11} Lsun), and log(Mbh) = 8.46 + 1.05*log(Mbulge/10^{11} Msun). A log-quadratic fit to the Mbh-sigma relation with an additional term of beta_2*[log(sigma/200 kms)]^2 gives beta_2 = 1.68 +/- 1.82 and does not decrease the intrinsic scatter in Mbh. When the early- and late-type galaxies are fit separately, we obtain similar slopes of 5.20 and 5.06 for the Mbh-sigma relation but significantly different intercepts -- Mbh in early-type galaxies are about 2 times higher than in late types at a given sigma. Within early-type galaxies, our fits to Mbh(sigma) give Mbh that is about 2 times higher in galaxies with central core profiles than those with central power-law profiles. Our Mbh-L and Mbh-Mbulge relations for early-type galaxies are similar to those from earlier compilations. When the conventional quadrature method is used to determine the intrinsic scatter in Mbh, our dataset shows weak evidence for increased scatter at Mbulge < 10^{11} Msun or L_V < 10^{10.3} Lsun, while the scatter stays constant for 10^{11} < Mbulge < 10^{12.3} Msun and 10^{10.3} < L_V < 10^{11.5} Lsun. A Bayesian analysis indicates a larger sample of Mbh measurements would be needed to detect any statistically significant trend in the scatter with galaxy properties.

Final version accepted for publication in ApJ. 15 pages, 5 figures, 3 tables. Our list of black hole masses is available at http://blackhole.berkeley.edu

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• The UV/optical peak and X-ray brightening in TDE candidate AT2019azh: A case of stream-stream collision and delayed accretion
• Unravelling the complex structure of AGN-driven outflows III. The outflow size-luminosity relation
• The hidden heart of the luminous infrared galaxy IC 860 I. A molecular inflow feeding opaque, extreme nuclear activity
• Gravitational wave emission from binary supermassive black holes
• Black hole mass estimation for Active Galactic Nuclei from a new angle
• A Local Baseline of the Black Hole Mass Scaling Relations for Active Galaxies. III. The BH mass - $\sigma$ relation
• Dark matter contraction and stellar-mass-to-light ratio gradients in massive early-type galaxies
• The Black Hole in the Compact, High-dispersion Galaxy NGC 1271
• MRK 1216 & NGC 1277 - An orbit-based dynamical analysis of compact, high velocity dispersion galaxies
• Correlation Between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies
• The Chandra Deep Fields: Lifting the Veil on Distant Active Galactic Nuclei and X-Ray Emitting Galaxies
• The M_BH - sigma relation for intermediate-mass black holes in globular clusters
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST
• Radio observations of extreme ULXs: revealing the most powerful ULX radio nebula ever or the jet of an intermediate-mass black hole?
• ALMA Observations of a Candidate Molecular Outflow in an Obscured Quasar
• Kinetic or thermal AGN feedback in simulations of isolated and merging disk galaxies calibrated by the M-sigma relation
• Properties of simulated galaxies and supermassive black holes in cosmic voids
• Overmassive black holes in the $M_{\mathrm{BH}}-\sigma$ diagram do not belong to over (dry) merged galaxies
• The Hunt for Intermediate Mass Black Holes in the JWST Era
• The redshift evolution of major merger triggering of luminous AGN: a slight enhancement at z$\sim$2
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• Probing the Physics of Narrow Line Regions in Active Galaxies IV: Full data release of The Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)
• NuSTAR Resolves the First Dual AGN above 10 keV in SWIFT J2028.5+2543
• BASS XXVI: DR2 Host Galaxy Stellar Velocity Dispersions
• CIV Black Hole Mass Measurements with the Australian Dark Energy Survey (OzDES)
• Separating Line Emission from Star Formation, Shocks, and AGN Ionisation in NGC 1068
• Tidal Disruptions of White Dwarfs: Theoretical Models and Observational Prospects
• A sub-kpc-scale binary AGN with double narrow-line regions
• The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
• The Mass of the Central Black Hole in the Nearby Seyfert Galaxy NGC5273
• Evidence for radial variations in the stellar mass-to-light ratio of massive galaxies from weak and strong lensing
• A quartet of black holes and a missing duo: probing the low-end of the Mbh - sigma relation with the adaptive optics assisted integral-field spectroscopy
• The SLUGGS Survey: A comparison of total-mass profiles of early-type galaxies from observations and cosmological simulations, to $\sim$4 effective radii
• The SLUGGS Survey: New evidence for a tidal interaction between the early type galaxies NGC 4365 and NGC 4342
• Discovery of rare double-lobe radio galaxies hosted in spiral galaxies
• Intermediate-Mass Black Hole Growth and Feedback in Dwarf Galaxies at High Redshifts
• The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei II: Kinematic Classifications for the Population at z < 0.1
• A Reverberation-Based Black Hole Mass for MCG-06-30-15
• Six new supermassive black hole mass determinations from adaptive-optics assisted SINFONI observations
• FOREVER22: galaxy formation in protocluster regions
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Constraining the supermassive black holes evolution through the continuity equation
• Rapid "Turn-on" of type 1 AGN in a quiescent early type galaxy SDSS1115+0544
• Can winds driven by active galactic nuclei account for the extragalactic gamma-ray and neutrino backgrounds?
• WISDOM project -- V. Resolving molecular gas in Keplerian rotation around the supermassive black hole in NGC 0383
• An elliptical accretion disk following the tidal disruption event AT 2020zso
• Calcium-Rich Gap Transients: Tidal Detonations of White Dwarfs?
• The NANOGrav 11-Year Data Set: Limits on Gravitational Wave Memory
• Accretion disc cooling and narrow absorption lines in the tidal disruption event AT 2019dsg
• The Diagnostic Potential of JWST in Characterizing Elusive AGNs
• The fraction of AGN in major merger galaxies and its luminosity dependence
• Constraints on Black Hole/Host Galaxy Co-evolution and Binary Stalling Using Pulsar Timing Arrays
• Resolving flows around black holes: numerical technique and applications
• Searching for Dual AGN in Galaxies with Double-Peaked Emission Line Spectra using Radio Observations
• Prospects for measuring supermassive black hole masses with future extremely large telescopes
• Ionized gas outflows in infrared-bright dust-obscured galaxies selected with WISE and SDSS
• Detection of a $\sim$100,000 M${}_{\odot }$ black hole in M31's most massive globular cluster: A tidally stripped nucleus
• The most massive black holes on the Fundamental Plane of Black Hole Accretion
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
• Gravitational torques imply molecular gas inflow towards the nucleus of M51
• A Precision Measurement of the Mass of the Black Hole in NGC 3258 from High-Resolution ALMA Observations of its Circumnuclear Disk
• WISDOM project - IV. A molecular gas dynamical measurement of the supermassive black hole mass in NGC 524
• Extended Structure and Fate of the Nucleus in Henize 2-10
• Black Hole Demography: From scaling relations to models
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• A remarkably large depleted core in the Abell 2029 BCG IC 1101
• The Combined Effects of Two-Body Relaxation Processes and the Eccentric Kozai-Lidov Mechanism on the EMRI Rate
• Investigation on Young radio AGNs based on SDSS spectroscopy
• Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature
• A concordance scenario for the observed neutrino from a Tidal Disruption Event
• A figure of merit for black hole mass measurements with molecular gas
• Sifting for Sapphires: Systematic Selection of Tidal Disruption Events in iPTF
• Black Hole Starvation and Bulge Evolution in a Milky Way-like Galaxy
• J1649+2635: A Grand-Design Spiral with a Large Double-Lobed Radio Source
• Binary Active Galactic Nuclei in Stripe 82: Constraints on Synchronized Black Hole Accretion in Major Mergers
• Glimmering in the dark: modeling the low-mass end of the $M_{\bullet }-\sigma$ relation and of the quasar luminosity function
• Long-Term Decline of the Mid-Infrared Emission of Normal Galaxies: Dust Echo of Tidal Disruption Flare?
• [OIII] Emission Line Properties in a New Sample of Heavily Reddened Quasars at $z>2$
• Sensitivity of gravitational wave searches to the full signal of intermediate mass black hole binaries during the LIGO O1 Science Run
• Nature and statistical properties of quasar associated absorption systems in the XQ-100 Legacy Survey
• The AGN fuelling/feedback cycle in nearby radio galaxies II. Kinematics of the molecular gas
• Revealing the relation between black-hole growth and host-galaxy compactness among star-forming galaxies
• A deep X-ray view of the bare AGN Ark120. V. Spin determination from disc-Comptonisation efficiency method
• The origin of the red sequence galaxy population in the EAGLE simulation
• Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters
• ALMA Observations of Nearby Luminous Infrared Galaxies with Various AGN Energetic Contributions Using Dense Gas Tracers
• Eddington ratio Distribution of X-ray selected broad-line AGNs at 1.0<z<2.2
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• Delayed Appearance and Evolution of Coronal Lines in the TDE AT2019qiz
• A quasar-based supermassive black hole binary population model: implications for the gravitational-wave background
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• How the central black hole may shape its host galaxy through AGN feedback
• A glance at the host galaxy of high-redshift quasars using strong damped Lyman-alpha systems as coronagraphs
• Dynamical Evolution and Merger Time-scales of LISA Massive Black Hole Binaries in Disk Galaxy Mergers
• Effect of Black Holes in Local Dwarf Spheroidal Galaxies on Gamma-Ray Constraints on Dark Matter Annihilation
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• The origin of compact galaxies with anomalously high black hole masses
• Dwarf AGNs from Optical Variability for the Origins of Seeds (DAVOS): Insights from the Dark Energy Survey Deep Fields
• Supermassive black holes in disk-dominated galaxies outgrow their bulges and co-evolve with their host galaxies
• A normal supermassive black hole in NGC 1277
• Stars and Black Holes from the very Early Universe
• Galaxy-scale Bars in Late-type Sloan Digital Sky Survey Galaxies Do Not Influence the Average Accretion Rates of Supermassive Black Holes
• The NANOGrav Program for Gravitational Waves and Fundamental Physics
• Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations
• Type 2 AGN host galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching
• A Population of Relic Intermediate-Mass Black Holes in the Halo of the Milky Way
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Black hole growth and AGN feedback under clumpy accretion
• Do model emission line galaxies live in filaments at z~1?
• A Candidate Dual AGN in a Double-peaked Emission-line Galaxy with Precessing Radio Jets
• Reverberation mapping of narrow-line Seyfert 1 galaxy I Zwicky 1: black hole mass
• The weak neutral Fe fluorescence line and long-term X-ray evolution of the Compton-thick AGN in NGC 7674
• The mass of the black hole in RE J1034+396
• Infrared signature of active massive black holes in nearby dwarf galaxies
• A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
• X-ray bolometric corrections for Compton-thick active galactic nuclei
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster
• Green Valley galaxies as a transition population in different environments
• Massive black holes in central cluster galaxies
• Two channels of supermassive black hole growth as seen on the galaxies mass-size plane
• Do Some AGN Lack X-ray Emission?
• How to constrain mass and spin of supermassive black holes through their disk emission
• Classification of Tidal Disruption Events Based on Stellar Orbital Properties
• Ionized Gas Outflows from the MAGNUM Survey: NGC 1365 and NGC 4945
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• The Largest X-ray Selected Sample of z>3 AGNs: C-COSMOS & ChaMP
• Stability of the Broad Line Region Geometry and Dynamics in Arp 151 Over Seven Years
• Radiation hydrodynamics models of Active Galactic Nuclei: Beyond the central parsec
• The nuclear transient AT 2017gge: a tidal disruption event in a dusty and gas-rich environment and the awakening of a dormant SMBH
• An evolving and mass dependent ${\sigma }_{\text{sSFR}}$-${\mathrm{M}}_{\star }$ relation for galaxies
• Abell 1201: Detection of an Ultramassive Black Hole in a Strong Gravitational Lens
• Constraints on Individual Supermassive Black Hole Binaries from Pulsar Timing Array Limits on Continuous Gravitational Waves
• ALMA Investigation of Vibrationally Excited HCN/HCO+/HNC Emission Lines in the AGN-Hosting Ultraluminous Infrared Galaxy IRAS 20551-4250
• On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• Population Estimates for Electromagnetically-Distinguishable Supermassive Binary Black Holes
• Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA
• Low-luminosity AGN and X-ray binary populations in COSMOS star-forming galaxies
• BASS XXIX: The near-infrared view of the BLR: the effects of obscuration in BLR characterisation
• Milliarcsec-scale radio emission of ultraluminous X-ray sources: steady jet emission from an intermediate-mass black hole?
• Tidal Disruption Events by a Massive Black Hole Binary
• Galaxy wide radio induced feedback in a radio quiet quasar
• The NANOGrav 11yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500Mpc
• The Sloan Digital Sky Survey Reverberation Mapping Project: An Investigation of Biases in CIV Emission-Line Properties
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• A significant excess in major merger rate for AGNs with the highest Eddington ratios at z<0.2
• A Black Hole Mass Determination for the Compact Galaxy Mrk 1216
• What triggers black-hole growth? Insights from star formation rates
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• A Global Inventory of Feedback
• Not So Heavy Metals: Black Hole Feedback Enriches The Circumgalactic Medium
• Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
• Anti-hierarchical evolution of the Active Galactic Nucleus space density in a hierarchical universe
• Towards Precision Supermassive Black Hole Masses using Megamaser Disks
• Novel calibrations of virial black hole mass estimators in active galaxies based on X-ray luminosity and optical/NIR emission lines
• How Ram Pressure Drives Radial Gas Motions in the Surviving Disk
• From X-rays to physical parameters: a comprehensive analysis of thermal tidal disruption event X-ray spectra
• Effects of Inclination on Measuring Velocity Dispersion and Implications for Black Holes
• The effect of bars on the M-sigma relation: offset, scatter and residuals correlations
• Selection bias in dynamically-measured supermassive black hole samples: Scaling relations and correlations between residuals in semi-analytic galaxy formation models
• Quenching Timescales in the IllustrisTNG Simulation
• A Low-Mass Black Hole in the Nearby Seyfert Galaxy UGC 06728
• The Nanohertz Gravitational Wave Astronomer
• Semi-Analytic Galaxies - II. Revealing the role of environmental and mass quenching in galaxy formation
• On the Offset of Barred Galaxies From the Black Hole $M_{BH}$-$\sigma$ Relationship
• Investigating AGN Black Hole Masses and the M-${\sigma }_e$ relation for Low Surface Brightness Galaxies
• The mass fraction of AGN and the Fundamental Plane of black hole activity from a large X-ray selected sample of LINERs
• Lense-Thirring Precession after a Supermassive Black Hole Disrupts a Star
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• The local black hole mass function derived from the M_{BH}-P and the M_{BH}-n relations
• Imaging Extended Emission-Line Regions of Obscured AGN with the Subaru Hyper Suprime-Cam Survey
• The dual role of starburst and active galactic nuclei in driving extreme molecular outflows
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• A population of galaxy-scale jets discovered using LOFAR
• Cosmic CARNage I: on the calibration of galaxy formation models
• The secular tidal disruption of stars by low-mass Super Massive Black Holes secondaries in galactic nuclei
• Star formation quenching stages of active and non-active galaxies
• Evaporation of planetary atmospheres due to XUV illumination by quasars
• The MASSIVE Survey -- XV. A Stellar Dynamical Mass Measurement of the Supermassive Black Hole in Massive Elliptical Galaxy NGC 1453
• Circumnuclear star-formation and AGN activity: Clues from surface brightness radial profile of PAHs and [SIV]
• No tension between assembly models of supermassive black hole binaries and pulsar observations
• 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
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Refining the M_BH-V_c scaling relation with HI rotation curves of water megamaser galaxies
• Bounds on Ultralight Dark Matter from NANOGrav
• Black hole clustering and duty cycles in the Illustris simulation
• The Illustris Simulation: Supermassive Black Hole - Galaxy Connection Beyond the Bulge
• Ionised gas outflows over the radio AGN life cycle
• Central Engine and Host Galaxy of RXJ 1301.9+2747: A Multiwavelength View of a Low-mass Black Hole Active Galactic Nuclei with Ultra-soft X-ray Emission
• The Sloan Digital Sky Survey Reverberation Mapping Project: The M_BH-Host Relations at 0.2<z<0.6 from Reverberation Mapping and Hubble Space Telescope Imaging
• The Active Fraction of Massive Black Holes in Dwarf Galaxies
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• Tidal disruption by extreme mass ratio binaries and application to ASASSN-15lh
• Photometric decomposition of mergers in disk galaxies
• Triaxial Orbit-based Dynamical Modeling of Galaxies with Supermassive Black Holes and an Application to Massive Elliptical Galaxy NGC 1453
• The Origin of Double-Peaked Narrow Lines in Active Galactic Nuclei III: Feedback from Biconical AGN Outflows
• Following Black Hole Scaling Relations Through Gas-Rich Mergers
• Calibrating stellar velocity dispersions based on spatially-resolved h-band spectra for improving the m-sigma relation
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• How AGN feedback drives the size growth of the first quasars
• The minimum and maximum gravitational-wave background from supermassive binary black holes
• VLBI Imaging of the Double Peaked Emission Line Seyfert KISSR1494
• Did massive black holes in globular clusters initially satisfy galactic scaling relations?
• The bulge masses of TDE host galaxies and their scaling with black hole mass
• A low upper mass limit for the central black hole in the late-type galaxy NGC 4414
• Subaru Adaptive-optics High-spatial-resolution Infrared K- and L'-band Imaging Search for Deeply Buried Dual AGNs in Merging Galaxies
• Active Galactic Nuclei: Boon or Bane for Biota?
• Investigating the Nature of the Luminous Ambiguous Nuclear Transient ASASSN-17jz
• A Curved 150 Parsec Long Jet in the Double-Peaked Emission-Line AGN KISSR 434
• Interpreting the possible break in the Black Hole - Bulge mass relation
• Hubble Space Telescope Imaging of the Active Dwarf Galaxy RGG 118
• The Effect of Spatial Gradients in Stellar Mass-to-Light Ratio on Black Hole Mass Measurements
• The connection between star formation and supermassive Black Hole activity in the local Universe
• Implications of the pulsar timing array detections for massive black hole mergers in the LISA band
• The overmassive black hole in NGC 1277: new constraints from molecular gas kinematics
• Stronger Constraints on the Evolution of the $M_{\mathrm{BH}}-{\sigma }_{\ast }$ Relation up to $z\sim 0.6$
• Direct collapse of exceptionally heavy black holes in the merger-driven scenario
• WISDOM project -- XIV. SMBH mass in the early-type galaxies NGC0612, NGC1574, and NGC4261 from CO dynamical modelling
• Gravitational Wave Driven Mergers and Coalescence Time of Supermassive Black Holes
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas
• Measuring black hole masses from tidal disruption events and testing the $M_{\mathrm{BH}}-{\sigma }_{\ast }$ relation
• AMUSE-Field II. Nucleation of early-type galaxies in the field vs. cluster environment
• Light Curves of Partial Tidal Disruption Events
• Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• The Blackhole-Dark Matter Halo Connection
• Does the intermediate mass black hole in LEDA 87300 (RGG 118) follow the near-quadratic (M_bh)-(M_spheroid) relation?
• Growth of Supermassive Black Hole Seeds in ETG Star-Forming Progenitors: Multiple Merging of Stellar Compact Remnants via Gaseous Dynamical Friction and Gravitational Wave Emission
• The Complete Local Volume Groups Sample -- III. Characteristics of group central radio galaxies in the Local Universe
• Starburst-AGN mixing: TYPHOON observations of NGC 1365, NGC 1068, and the effect of spatial resolution on the AGN fraction
• Stellar Velocity Dispersion in Dissipative Galaxy Mergers with Star Formation
• Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
• Detection of Enhanced Central Mass-to-Light Ratios in Low-Mass Early-Type Galaxies: Evidence for Black Holes?
• The Correlation between Black Hole Mass and Stellar Mass for Classical Bulges and the Cores of Ellipticals
• Systematic Redshift of the Fe III UV Lines in Quasars. Measuring Supermassive Black Hole Masses under the Gravitational Redshift Hypothesis
• Implications of Symmetry and Pressure in Friedmann Cosmology. II. Stellar Remnant Black Hole Mass Function
• Dust evolution with MUPPI in cosmological volumes
• Robotic Reverberation Mapping of the Southern Seyfert NGC 3783
• Placing High-Redshift Quasars in Perspective: a Catalog of Spectroscopic Properties from the Gemini Near Infrared Spectrograph -- Distant Quasar Survey
• Searching for Ultra-light Bosons and Constraining Black Hole Spin Distributions with Stellar Tidal Disruption Events
• Deep Chandra Observations of ESO 428-G014: IV. The Morphology of the Nuclear Region in the Hard Continuum and Fe Kα Line
• Reaching the Peak of the quasar spectral energy distribution - II. Exploring the accretion disc, dusty torus and host galaxy
• Bright vigorous winds as signposts of supermassive black hole birth
• Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies
• The SLUGGS survey: Probing the supermassive black hole connection with bulges and haloes using red and blue globular cluster systems
• The gravitational wave background signal from tidal disruption events
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Cosmic variance in the nanohertz gravitational wave background
• A universal minimal mass scale for present-day central black holes
• Searching for Intermediate Mass Black Holes in galaxies with Low Luminosity AGN: A multiple-method approach
• Evolution Of Massive Black Hole Binaries In Rotating Stellar Nuclei: Implications For Gravitational Wave Detection
• On the Possibility that Ultra-Light Boson halos host and form Super-massive Black Holes
• Radio-mode feedback in local AGNs: dependence on the central black hole parameters
• The Black Hole Mass of NGC 4151 from Stellar Dynamical Modeling
• Chemical abundances in the nuclear region of nearby galaxies from the Palomar Survey
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• The (black hole mass)-(color) relations for early- and late-type galaxies: red and blue sequences
• Suzaku observations of the type 2 QSO in the central galaxy of the Phoenix cluster
• The host galaxy properties of variability selected AGN in the Pan-STARRS1 Medium-Deep Survey
• Ultramassive black holes in the most massive galaxies: $M_{\mathrm{BH}}-\sigma$ versus $M_{\mathrm{BH}}-R_{\mathrm{b}}$
• Detection of faint broad emission lines in type 2 AGN: III. On the $M_{BH}-{\sigma }_{\star }$ relation of type 2 AGN
• ALMA Multiple-Transition Molecular Line Observations of the Ultraluminous Infrared Galaxy IRAS 20551-4250: Different HCN, HCO+, HNC Excitation and Implications for Infrared Radiative Pumping
• A Uniform History for Galaxy Evolution
• Orientation and quasar black hole mass estimation
• Comparing Simple Quasar Demographics Models
• A deep Chandra observation of the hot gaseous halo around a rare, extremely massive and relativistic jet launching spiral galaxy
• The MASSIVE Survey -- XVII. A Triaxial Orbit-based Determination of the Black Hole Mass and Intrinsic Shape of Elliptical Galaxy NGC 2693
• Resolving the Interstellar Medium in Ultraluminous Infrared QSO Hosts with ALMA
• Considerations for the Observability of Kinematically Offset Binary AGN
• The Relativistic Jet Orientation and Host Galaxy of the Peculiar Blazar PKS 1413+135
• Active Galactic Nuclei outflows in galaxy discs
• SDSS J0159 as an outlier in the Mbh-sigma space: further clues to support a central tidal disruption event?
• Dust formation in AGN winds
• The black hole mass of the $z=2.805$ multiply imaged quasar SDSS J2222+2745 from velocity-resolved time lags of the CIV emission line
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Observational Evidence for Enhanced Black Hole Accretion in Giant Elliptical Galaxies
• Elliptical accretion disk as a model for tidal disruption events
• An ALMA Gas-dynamical Mass Measurement of the Supermassive Black Hole in the Local Compact Galaxy UGC 2698
• Pulsar timing arrays and the challenge of massive black hole binary astrophysics
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• Intermittent AGN episodes drive outflows with a large spread of observable loading factors
• Star formation in AGNs at the hundred parsec scale using MIR high resolution images
• Exploring Proxies for the Supermassive Black Hole Mass Function: Implications for Pulsar Timing Arrays
• 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
• Radio Morphology of Red Geysers
• WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
• The X-ray and radio activity of typical and luminous Lya emitters from z~2 to z~6: evidence for a diverse, evolving population
• Studying the [OIII]$\lambda$5007A emission-line width in a sample of $\sim$80 local active galaxies: A surrogate for ${\sigma }_{\star }$?
• A Triple AGN in the NGC 7733-7734 Merging Group
• Likelihood for Detection of Sub-parsec Supermassive Black Hole Binaries in Spectroscopic Surveys
• Jet-accretion system in the nearby mJy Radio Galaxies
• Galaxies with monstrous black holes in galaxy cluster environments
• Expanding the Sample: The Relationship Between the Black Hole Mass of BCGs and the Total Mass of Galaxy Clusters
• Black Hole Mass Estimation: How good is the virial estimate?
• Double-Peaked Emission Lines due to A Radio Outflow in KISSR1219
• No sign of strong molecular gas outflow in an infrared-bright dust-obscured galaxy with strong ionized-gas outflow
• Unbeamed tidal disruption events at hard X-rays
• Ultramassive Black Hole Coalescence
• Black Hole Mass Measurements of Early-Type Galaxies NGC 1380 and NGC 6861 Through ALMA and HST Observations and Gas-Dynamical Modeling
• AGN Jet Power, Formation of X-ray Cavities, and FR I/II Dichotomy in Galaxy Clusters
• Low-Mass Active Galactic Nuclei with Rapid X-Ray Variability
• An Upper Limit on the Mass of a Central Black Hole in the Large Magellanic Cloud from the Stellar Rotation Field
• The massive dark halo of the compact, early-type galaxy NGC 1281
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• The X-ray coronae of the two brightest galaxies in the Coma cluster
• SDSS1335+0728: The awakening of a $\sim 10^6{M}_{\odot }$ black hole
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• Identifying Host Galaxies of Supermassive Black Hole Binaries Found by PTAs
• Circumnuclear Media of Quiescent Supermassive Black Holes
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Theoretical reevaluations of the black hole mass - bulge mass relation - I. Effect of the seed black hole mass
• The MASSIVE Survey XIII -- Spatially Resolved Stellar Kinematics in the Central 1 kpc of 20 Massive Elliptical Galaxies with the GMOS-North Integral-Field Spectrograph
• The Effect of Environment on Galaxy Spiral Arms, Bars, Concentration, and Quenching
• J1216+0709 : A radio galaxy with three episodes of AGN jet activity
• SMM J04135+10277: A distant QSO-starburst system caught by ALMA
• LLAMA: Stellar populations in the nuclei of ultra hard X-ray selected AGN and matched inactive galaxies
• An evolutionary missing link? A modest-mass early-type galaxy hosting an over-sized nuclear black hole
• A complete catalogue of broad-line AGNs and double-peaked emission lines from MaNGA integral-field spectroscopy of 10K galaxies: stellar population of AGNs, supermassive black holes, and dual AGNs
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Non-isotropic feedback from accreting spinning black holes
• The $z\lesssim 1$ drop of cosmic dust abundance in a semi-analytic framework
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• 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 Black Hole Mass Function Across Cosmic Times II. Heavy Seeds and (Super)Massive Black Holes
• Powerful Radio-Loud Quasars are Triggered by Galaxy Mergers in the Cosmic Bright Ages
• eRASSt J074426.3+291606: prompt accretion disc formation in a 'faint and slow' tidal disruption event
• Diffuse Gamma Ray Background from Annihilating Dark Matter in Density Spikes around Supermassive Black Holes
• The Role of AGN in Luminous Infrared Galaxies from the Multiwavelength Perspective
• Long-term X-ray stability and UV variability of the ionized absorption in NGC 3783
• Investigating the Covering Fraction Distribution of Swift/BAT AGN with X-ray and IR Observations
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Activity in Galactic Nuclei of Compact Group Galaxies in the Local Universe
• Effects of environment on sSFR profiles of late-type galaxies in the CALIFA survey
• Quasar clustering in a galaxy and quasar formation model based on ultra high-resolution N-body simulations
• Rates of Stellar Tidal Disruption Events around Intermediate-Mass Black Holes
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Low-frequency radio observations of Seyfert galaxies: A test to the unification scheme
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Hunting for Metals Using XQ-100 Legacy Survey Composite Spectra
• From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments
• Scary Barbie: An Extremely Energetic, Long-Duration Tidal Disruption Event Candidate Without a Detected Host Galaxy at z = 0.995
• Late-time X-ray Observations of the Jetted Tidal Disruption Event AT2022cmc: The Relativistic Jet Shuts Off
• The (Black Hole Mass)-(Spheroid Stellar Density) Relations: $M_{\mathrm{BH}}$--$\mu$ (and $M_{\mathrm{BH}}$--$\Sigma$) and $M_{\mathrm{BH}}$--$\rho$
• Application of The Wind-Driven Model to A Sample of Tidal Disruption Events
• Constraints from dwarf galaxies on black hole seeding and growth models with current and future surveys
• Evidence for non-merger co-evolution of galaxies and their supermassive black holes
• Effect of richness on AGN and star formation activities in SDSS galaxy groups
• The Relative Growth of Black Holes and of the Stellar Components of Galaxies
• SDSS J163459.82+204936.0: A Ringed Infrared-Luminous Quasar with Outflows in both Absorption and Emission Lines
• An Accreting, Anomalously Low Mass Black Hole at the Center of Low Mass Galaxy IC 750
• Supermassive Binary Black Hole Evolution can be traced by a small SKA Pulsar Timing Array
• Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
• Hidden Cooling Flows in Clusters of Galaxies III: Accretion onto the Central Black Hole
• The role of environment in the observed Fundamental Plane of radio Active Galactic Nuclei
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• The Most Massive Active Galactic Nuclei at $1\lesssim z\lesssim 2$
• A Multi-wavelength Study of the Dual Nuclei in Mrk 212
• An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation
• The Influence of Uniform Magnetic Fields on Strong Field Gravitational Lensing by Kerr Black Holes
• BAT AGN Spectroscopic Survey -- XIII. The nature of the most luminous obscured AGN in the low-redshift universe
• Misclassified type 1 AGNs in the local universe
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• A maximum X-ray luminosity scale of disc-dominated tidal disruption events
• Black hole wind speeds and the M-sigma relation
• The Quasar-LBG Two-point Angular Cross-correlation Function at z ~ 4 in the COSMOS Field
• A Nearly Naked Supermassive Black Hole
• The nuclear dust lane of Circinus: collimation without a torus
• Discovering new forces with gravitational waves from supermassive black holes
• The Properties of Massive Star-forming galaxies with Outside-in Assembly Mode
• An upper observable black hole mass scale for tidal disruption events with thermal X-ray spectra
• Probing the gaseous halo of galaxies through non-thermal emission from AGN-driven outflows
• The role of gravitational recoil in the assembly of massive black hole seeds
• Globular Cluster Systems of Relic Galaxies
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• Powerful ionized gas outflows in the interacting radio galaxy 4C +29.30
• Providing stringent star formation rate limits of z$\sim$2 QSO host galaxies at high angular resolution
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• The Complex Gaseous and Stellar environments of the nearby dual AGN Mrk 739
• Hidden AGNs in Early-Type Galaxies
• Quasars at intermediate redshift are not special; but they are often satellites
• Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes
• Black hole and nuclear cluster scaling relations: M_bh ~ M_nc^{2.7+/-0.7}
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• The Black Hole Mass and the Stellar Ring in NGC 3706
• NGC 5195 in M51: Feedback `Burps' after a Massive Meal?
• FIRST J153350.8+272729: the radio afterglow of a decades-old tidal disruption event
• Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries
• What has quenched the massive spiral galaxies?
• Orbital orientation evolution of massive binary black holes at the centres of non-spherical galaxies
• Black hole fueling in galaxy mergers: A high-resolution analysis
• The Velocity Dispersion Function for Massive Quiescent and Star-Forming Galaxies at 0.6 $<$ z $\le$ 1.0
• Surprisingly Strong K-band Emission Found in Low Luminosity Active Galactic Nuclei
• Hard X-ray emission from a Compton scattering corona in large black hole mass tidal disruption events
• Black hole mass measurement using molecular gas kinematics: what ALMA can do
• On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
• Gravitational waves from merging intermediate-mass black holes : II Event rates at ground-based detectors
• The Opaque Heart of the Galaxy IC 860: Analogous Protostellar, Kinematics, Morphology, and Chemistry
• The Impact of Black Hole Scaling Relation Assumptions on the Mass Density of Black Holes
• The incidence of AGN in galaxies with different stellar population ages
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• The Discovery of a Hidden Broad Line AGN in a Bulgeless Galaxy: Keck NIR Spectroscopic Observations of SDSS J085153.64+392611.76
• Robotic reverberation mapping of the broad-line radio galaxy 3C 120
• Triaxial Schwarzschild Models of NGC 708: a 10-billion solar mass black hole in a low dispersion galaxy with a Kroupa IMF
• The Pairing Probability of Massive Black Holes in Merger Galaxies in the Presence of Radiative Feedback
• Optical/UV Emission in the Tidal Disruption Event ASASSN-14li: Implications of Disc Modeling
• SDSS J1058+5443: A blue quasar does not have optical/NUV broad emission lines
• Probing supermassive black hole growth and its dependence on stellar mass and star-formation rate in low-redshift galaxies
• The MASSIVE survey -- XIX. Molecular gas measurements of the supermassive black hole masses in the elliptical galaxies NGC 1684 and NGC 0997
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• A geometric approach to non-linear correlations with intrinsic scatter
• Resolving the nano-Hz gravitational wave sky: the detectability of eccentric binaries with PTA experiments
• X-ray Emission of the $\gamma$-ray Loud Young Radio Galaxy NGC 3894
• The Host Galaxies of Radio AGN: New Views from Combining LoTSS and MaNGA Observations
• Jetted Tidal Disruptions of Stars as a Flag of Intermediate Mass Black Holes at High Redshifts
• The $M-\sigma$ relation between supermassive black holes and their host galaxies
• Galaxy Core Formation by Supermassive Black Hole Binaries: the Importance of Realistic Initial Conditions and Galaxy Morphology
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• Coevolution of broad emission lines and X-ray spectrum in changing-look AGNs
• Hydrodynamic simulations of the Disk of Gas Around Supermassive black holes (HDGAS) -I; Molecular Gas Dynamics
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: II. Photoionization and Kinematics of the ISM
• Resolving the Vicinity of Supermassive Black Holes with Gravitational Microlensing
• ULISSE: A Tool for One-shot Sky Exploration and its Application to Active Galactic Nuclei Detection
• SCAT Uncovers ATLAS's First Tidal Disruption Event ATLAS18mlw: A Faint and Fast TDE in a Quiescent Balmer Strong Galaxy
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• An XMM-Newton study of active-inactive galaxy pairs
• The XXL Survey: XXXIV. Double irony in XXL-North. A tale of two radio galaxies in a supercluster at z = 0.14
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Radial Gas Inflow and Shock Excitation in NGC 1042
• Dark Energy Survey Identification of A Low-Mass Active Galactic Nucleus at Redshift 0.823 from Optical Variability
• Jets from SANE Super-Eddington Accretion Disks: Morphology, Spectra, and Their Potential as Targets for ngEHT
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• AT2018fyk: Candidate Tidal Disruption Event by a (Super)massive Black Hole Binary
• Near-Infrared Spectroscopy of Quasars at z~3 and Estimates of Their Supermassive Black Hole Masses
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• AGN Triality of Triple Mergers: Multi-wavelength Classifications
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Dark matter halos and the M-σrelation for supermassive black holes
• Accretion onto supermassive and intermediate mass black holes in cosmological simulations
• On the Mean Radiative Efficiency of Accreting Massive Black Holes in AGNs And QSOs
• Do gas clouds in narrow-line regions of Seyfert galaxies come from their nuclei?
• The Impact of Dust in Host Galaxies on Quasar Luminosity Functions
• Using angular momentum maps to detect kinematically distinct galactic components
• Black hole virial masses from single-epoch photometry: the miniJPAS test case
• Assessing indirect methods to determine black hole masses using NGC 4151
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Unveiling Gargantua: A new search strategy for the most massive central cluster black holes
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• Off-centre supermassive black holes in bright central galaxies
• Gas inflows in the polar ring of NGC 4111: the birth of an AGN
• Ultraviolet Spectral Evidence for Ansky as a Slowly Evolving Featureless Tidal Disruption Event with Quasiperiodic Eruptions
• Limits on the growth rate of supermassive black holes at early cosmic epochs
• The Intriguing Parsec-Scale Radio Structure in the "Offset AGN" KISSR 102
• SMBH Seeds: Model Discrimination with High Energy Emission Based on Scaling Relation Evolution
• `Zwicky's Nonet': a compact merging ensemble of nine galaxies and 4C 35.06, a peculiar radio galaxy with dancing radio jets
• Early Type Galaxy Core Phase Densities
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• eROSITA Detection Rates for Tidal Disruptions of White Dwarfs by Intermediate Mass Black Holes
• Properties of radio-loud quasars in Sloan Digital Sky Survey
• Prospects for Observing High-redshift Radio-loud Quasars in the SKA Era: Paving the Way for 21-cm Forest Observations
• On the detectability of massive black hole merger eventsby LISA
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Critical Stellar Central Densities Drive Galaxy Quenching in the Nearby Universe
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• ALMA resolves the stellar birth explosion in distant quasar 3C298
• Evidence for a steeper SMBH-Bulge mass relationship extended to low masses using TDE host galaxies
• Circumgalactic Environments around Distant Quasars 3C 9 and 4C 05.84
• Long-term variability of the composite galaxy SDSS J103911-000057: A candidate of true Type-2 AGN
• A SysTematic seaRch fOr Dual Agns in meRgINg Galaxies (ASTRO-DARING) II: first results from long-slit spectroscopic observations
• The InfraRed Imaging Spectrograph (IRIS) for TMT: Overview of innovative science programs
• Gravitational Waves from Massive Black Hole Mergers in ASTRID: Predictions for LISA
• Galaxy populations of ProtoClusters in cosmological hydrodynamical simulations
• The optically elusive, changing-look active nucleus in NGC 4156
• Intermediate-mass ratio inspirals in merging elliptical galaxies
• Detection of disk-jet co-precession in a tidal disruption event
• M31 circum-nuclear region: a molecular survey with the IRAM-interferometer
• On the Structure of the AGN Torus through the Fraction of Optically-Selected Type 1 AGNs
• Astrophysics with the Laser Interferometer Space Antenna
• Effective power-law dependence of Lyapunov exponents on the central mass in galaxies
• QSO2 outflow characterization using data obtained with OSIRIS at the Gran Telescopio Canarias
• Exploring Gravitationally-Lensed $z\gtrsim 6$ X-ray AGN Behind the RELICS clusters
• Spectropolarimetric measurements of hidden broad lines in nearby megamaser galaxies: a lack of clear evidence for a correlation between black hole masses and virial products
• X-ray monitoring of gravitationally lensed radio-loud quasars with Chandra
• The influence of mergers and ram-pressure stripping on black hole-bulge correlations
• Reading signatures of supermassive binary black holes in pulsar timing array observations
• Warping and tearing of misaligned circumbinary disks around eccentric SMBH binaries
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• Prospects for probing small-scale dark matter models with pulsars around Sagittarius A*
• The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT $610\mathrm{MHz}$ continuum observations
• Lensing of gravitational waves from tidal disruption events
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• VLA detects CO(1-0) emission in the z=3.65 quasar SDSS J160705+533558
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• Stringent limits on the masses of the supermassive black holes in seven nearby galaxies
• Black hole-galaxy co-evolution and the role of feedback
• 3D spectroscopy with GTC-MEGARA of the triple AGN candidate in SDSS J102700.40+174900.8
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• Eccentricity Boost of Stars Around Shrinking Massive Black Hole Binaries
• WISDOM Project -- XXII. A 5% precision CO-dynamical supermassive black hole mass measurement in the galaxy NGC 383
• AGN Reverberation Mapping
• Spherical accretion in giant elliptical galaxies: multi-transonicity, shocks, and implications on AGN feedback
• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
• Measuring the Virial Factor in SDSS DR7 AGNs with Redshifted H$\beta$ and H$\alpha$ Broad Emission Lines
• Powerful Radio Emission From Low-mass Supermassive Black Holes Favors Disk-like Bulges
• Central accumulation of magnetic flux in massive Seyfert galaxies as a possible engine to trigger ultrahigh energy cosmic rays
• Low-redshift quasars in the SDSS Stripe 82 II: associated companion galaxies and signature of star formation
• The relationship of SMBHs and host galaxies at $z<4$ in the deep optical variability-selected AGN sample in the COSMOS field
• Exploring Dark Forces with Multimessenger Studies of Extreme Mass Ratio Inspirals
• Measuring the Spin of the Galactic Center Supermassive Black Hole with Two Pulsars
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Dynamical Measurement of Supermassive Black Hole Masses: QPE Timing Method
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Unravelling the nature of the dual AGN in the galaxy pair system IRAS 05589+2828 and 2MASX J06021107+2828382
• LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
• Cosmic distributions of stellar tidal disruptions by massive black holes at galactic centers
• Quasar Host Galaxies and the $M_{SMBH}$ - ${\sigma }_{\ast }$ Relation
• Deep Hubble Space Telescope Imaging on the Extended Ly$\alpha$ Emission of a QSO at $z=2.19$ with Damped Lyman Alpha System as a Natural Coronagraph
• Supernova remnant mass cumulated along the star formation history of the z=3.8 radiogalaxies 4C41.17 and TN J2007-1316
• Sommerfeld enhancement of invisible dark matter annihilation in galaxies and galaxy clusters
• Massive Black Hole Mergers
• UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Early Growing Supermassive Black Holes Strengthen Bars and Boxy/Peanut Bulges
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Inferring Mbh-Mbulge Evolution from the Gravitational Wave Background
• The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
• The correlations of stellar tidal disruption rates with properties of massive black holes and their host galaxies
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• A possible binary AGN in Mrk\,622?
• A LOFAR sample of luminous compact sources coincident with nearby dwarf galaxies
• Investigating orientation effects considering angular resolution for a sample of radio-loud quasars using VLA observations
• Quantum vorticity in nature
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• Environmental effects on associations of dwarf galaxies
• Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
• Chandra View of the LINER-type Nucleus in the Radio-Loud Galaxy CGCG 292-057: Ionized Iron Line and Jet-ISM Interactions
• Low-mass and High-mass Supermassive Blackholes In Radio-Loud AGNs Are Spun-up in Different Evolution Paths
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Warped Circumbinary Disks in Active Galactic Nuclei
• Probing the mass relation between supermassive black holes and dark matter halos at high redshifts by gravitational wave experiments
• IC 630: Piercing the Veil of the Nuclear Gas
• Cosmic spin and mass evolution of black holes and its impact
• The Host Galaxies of PTA Sources: Converting Supermassive BH Binary Parameters into EM Observables
• ALMA detects molecular gas in the halo of the powerful radio galaxy TXS 0828+193
• Stellar rotation as a new observable to test general relativity in the Galactic Center
• A Flaring AGN In a ULIRG candidate in Stripe 82
• Ionised AGN outflows in the Goldfish galaxy -- The illuminating and interacting red quasar eFEDSJ091157.4+014327 at z $\sim$ 0.6
• Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186
• Probing the Growth of Massive Black Holes with Black Hole-Host Galaxy Spin Correlations
• Supernovae at the cosmic dawn
• Learning Transient Universe in Near-Ultraviolet By Wide-angle Cameras
• An approach to robust Bayesian regression in astronomy
• Astrophysical black holes
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• NuSTAR Observes Two Bulgeless Galaxies: No Hard X-ray AGN Detected in NGC 4178 or J0851+3926
• Do Red Galaxies Form More Stars Than Blue Galaxies?
• Distribution of orbital inclinations for tidal disruption events by Kerr black holes
• Cosmic quenching and scaling laws for the evolution of supermassive black holes and host galaxies
• A Spatially Resolved Evolutionary Sequence of Multi-wavelength AGN Host Galaxies
• No dependence of radio properties of brightest group galaxies on the luminosity gap
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Multi-phase investigation of outflows in the circumgalactic and interstellar media of luminous quasars at z~5
• Study of Central Intensity Ratio of Seyfert Galaxies in nearby Universe
• Spatially Resolved [O III] Emission Line Kinematics of Reverberation-Mapped AGNs with the Keck Cosmic Web Imager
• Photometric variability in star-forming galaxies as evidence for low-mass AGN and a precursor to quenching
• Gamma-ray emission in radio galaxies under the VLBI scope -- II. The relationship between gamma-ray emission and parsec-scale jets in radio galaxies
• Study of central intensity ratio of early-type galaxies from low density environment
• Accretion Flares from Stellar Collisions in Galactic Nuclei
• Probabilistic eccentricity bifurcation for stars around shrinking massive black hole binaries
• Determination of the angular momentum of the Kerr black hole from equatorial geodesic motion
• The $M_{\bullet }-\sigma$ relation in spherical systems
• Feeding and feedback in nuclei of galaxies
• Deciphering galaxy images using machine vision -- Combining variational autoencoder and principal component analysis for feature extraction
• Extended Hernquist-Springel formalism for cosmic star formation
• A search for H${}_2$O masers in 100 active dwarf galaxies
• Recoiling supermassive black holes in analytical and numerical galaxy potential
• Feeding supermassive black holes by collisional cascades
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• High-Redshift Merger Model for Low-Frequency Gravitational Wave Background
• 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
• A stellar dynamical mass measurement of an inactive black hole at redshift 2
• Tracing black hole and galaxy growth across environments since cosmic noon
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Obscured and unobscured X-ray AGNs I: Host galaxy properties
• A Search for Wandering Black Holes in the Milky Way with Gaia and DECaLS
• Radio Variability in Recently-Quenched Galaxies: The Impact of TDE or AGN Driven Outflows
• The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies
• BASS XXX: Distribution Functions of DR2 Eddington-ratios, Black Hole Masses, and X-ray Luminosities
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• WISDOM Project -- XXVI. Cross-checking supermassive black hole mass estimates from ALMA CO gas kinematics and SINFONI stellar kinematics in the galaxy NGC 4751
• Growth of black holes at the centre of early-type galaxies in MOND
• Thermomagnetic Ettingshausen-Nernst effect in tachocline, magnetic reconnection phenomenon in lower layers, axion mechanism of solar luminosity variations, coronal heating problem solution and mechanism of ADM variations around BH
• A Near-Infrared look at AGN Feedback in Bulgeless Galaxies
• Probing the Jet Turnover Frequency Dependence on Black Hole Mass and Mass Accretion Rate
• A Comprehensive JWST/NIRSpec Census of Broad-line Active Galactic Nuclei: Faint, Low-mass Accretors and a Population of Little Red Dots
• Search of Intermediate Mass Black Holes at Low Redshift with Intra-night Variability
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Preliminary census of galaxies in the LISA localisation volume: I. Searching for LISA candidate massive black hole binary merger hosts using Sloan Digital Sky Survey photometry
• Gravitational Wave Measurement of the $M_{\mathrm{BH}}$-$M_{\mathrm{bulge}}$ Intrinsic Scatter at High Redshift
• The most massive galaxies with large depleted cores: structural parameter relations and black hole masses
• Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor
• Investigating the AGN activity and black hole masses in Low Surface brightness galaxies
• Enhanced activity in close dual-AGN systems in the local Universe
• Rate of Repeating Tidal Disruption Events with 5--19 years interval
• Circular Mystery: Exploring Diffuse Emission Surrounding a Radio Galaxy with uGMRT and VLA Multiwavelength Observations
• A new model of quasar mass evolution
• Constraining Nuclear Molecular Gas Content with High-resolution CO Imaging of GOALS Galaxies
• Investigating the Bulge Morphology of Dual AGN Host Galaxies from the GOTHIC survey
• Discriminating between different scenarios for the formation and evolution of massive black holes with LISA
• Are Active Galactic Nuclei in Post-Starburst Galaxies Driving the Change or Along for the Ride?
• Testing the Limits of AGN Feedback and the Onset of Thermal Instability in the Most Rapidly Star Forming Brightest Cluster Galaxies
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• The Nature of Jets in Double-Peaked Emission Line AGN in the KISSR Sample
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Tests for the existence of horizon through gravitational waves from a small binary in the vicinity of a massive object