Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe

Abstract

Scaling relations between central black hole (BH) mass and host galaxy properties are of fundamental importance to studies of BH and galaxy evolution throughout cosmic time. Here we investigate the relationship between BH mass and host galaxy total stellar mass using a sample of 262 broad-line active galactic nuclei (AGN) in the nearby Universe (z < 0.055), as well as 79 galaxies with dynamical BH masses. The vast majority of our AGN sample is constructed using Sloan Digital Sky Survey spectroscopy and searching for Seyfert-like narrow-line ratios and broad H-alpha emission. BH masses are estimated using standard virial techniques. We also include a small number of dwarf galaxies with total stellar masses M_stellar < 10^9.5 Msun and a sub-sample of the reverberation-mapped AGNs. Total stellar masses of all 341 galaxies are calculated in the most consistent manner feasible using color-dependent mass-to-light ratios. We find a clear correlation between BH mass and total stellar mass for the AGN host galaxies, with M_BH proportional to M_stellar, similar to that of early-type galaxies with dynamically-detected BHs. However, the relation defined by the AGNs has a normalization that is lower by more than an order of magnitude, with a BH-to-total stellar mass fraction of M_BH/M_stellar ~ 0.025% across the stellar mass range 10^8 < M_stellar/Msun < 10^12. This result has significant implications for studies at high redshift and cosmological simulations in which stellar bulges cannot be resolved.

Accepted for publication in the Astrophysical Journal. 15 pages, 12 figures

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• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• How AGN feedback drives the size growth of the first quasars
• Differences in Halo-Scale Environments between Type 1 and Type 2 AGNs at Low Redshift
• An Unusual Mid-Infrared Flare in a Type 2 AGN: An Obscured Turning-on AGN or Tidal Disruption Event?
• Hubble Space Telescope Imaging of the Active Dwarf Galaxy RGG 118
• The connection between star formation and supermassive Black Hole activity in the local Universe
• The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function
• The population of tidal disruption events discovered with eROSITA
• Measuring black hole masses from tidal disruption events and testing the $M_{\mathrm{BH}}-{\sigma }_{\ast }$ relation
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass 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
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• On the AGN Nature of Broad Balmer Emission in Four Low-Redshift Metal-Poor Galaxies
• Prior-Informed AGN-Host Spectral Decomposition Using PyQSOFit
• Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies at z ~ 0.7
• Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?
• The environment of AGN dwarf galaxies at z$\sim$0.7 from the VIPERS survey
• No evidence for a significant evolution of $M_{\bullet }$-$M_{\ast }$ relation in massive galaxies up to z$\sim$4
• The MBHBM${}^{\star }$ Project -- II. Molecular Gas Kinematics in the Lenticular Galaxy NGC 3593 Reveal a Supermassive Black Hole
• Outflows, Shocks and Coronal Line Emission in a Radio-Selected AGN in a Dwarf Galaxy
• Placing High-Redshift Quasars in Perspective: a Catalog of Spectroscopic Properties from the Gemini Near Infrared Spectrograph -- Distant Quasar Survey
• Statistical study of a large and cleaned sample of ultraluminous and hyperluminous X-ray sources
• The CGM${}^2$ Survey: Quenching and the Transformation of the Circumgalactic Medium
• Mixing between Seyfert and HII-region excitation in local active galaxies
• A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
• A hidden population of massive black holes in simulated dwarf galaxies
• PSFGAN: a generative adversarial network system for separating quasar point sources and host galaxy light
• Black holes as the source of dark energy: a stringent test with high-redshift JWST AGNs
• The dawn of disks: unveiling the turbulent ionised gas kinematics of the galaxy population at $z\sim 4-6$ with JWST/NIRCam grism spectroscopy
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Evolution Of Massive Black Hole Binaries In Rotating Stellar Nuclei: Implications For Gravitational Wave Detection
• Detection of faint broad emission lines in type 2 AGN: III. On the $M_{BH}-{\sigma }_{\star }$ relation of type 2 AGN
• X-ray properties of dust-obscured galaxies with broad optical/UV emission lines
• Subaru Hyper Suprime-Cam View of Quasar Host Galaxies at z < 1
• Nature of Compton-thick Active Galactic Nuclei in "Non-merging'' Luminous Infrared Galaxies UGC 2608 and NGC 5135 Revealed with Broadband X-ray Spectroscopy
• A Low Incidence of Mid-Infrared Variability in Dwarf Galaxies
• Dark-ages Reionization and Galaxy Formation Simulation -- XVII. Sizes, angular momenta and morphologies of high redshift galaxies
• Discovery of a Luminous Radio Transient 460 pc from the Central Supermassive Black Hole in Cygnus A
• Optical and JWST Mid-IR Emission Line Diagnostics for Simultaneous IMBH and Stellar Excitation in z~0 Dwarf Galaxies
• The host galaxy properties of variability selected AGN in the Pan-STARRS1 Medium-Deep Survey
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• Two Candidates for Dual AGN in Dwarf-Dwarf Galaxy Mergers
• The BAT AGN Spectroscopic Survey -- XVIII. Searching for Supermassive Black Hole Binaries in the X-rays
• Active Galactic Nuclei outflows in galaxy discs
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• Evolution of galaxy habitability
• GA-NIFS and EIGER: A merging quasar host at z=7 with an overmassive black hole
• Observational Evidence for Enhanced Black Hole Accretion in Giant Elliptical Galaxies
• The rapid transition from star-formation to AGN dominated rest-frame UV light at z ~ 4
• Tidal disruption events can power the observed AGN in dwarf galaxies
• The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources
• Study of gravitational fields and globular cluster systems of early-type galaxies
• Rejuvenation triggers nuclear activity in nearby galaxies
• A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR
• On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences
• Revisiting the Rates and Demographics of Tidal Disruption Events: Effects of the Disk Formation Efficiency
• SRG/eROSITA No. 5: Discovery of quasi-periodic eruptions every ~3.7 days from a galaxy at z>0.1
• An X-ray + Radio Search for Massive Black Holes in Blue Compact Dwarf Galaxies
• Active Galactic Nuclei with a Low-Metallicity Narrow-Line Region
• Difficulties in Mid-Infrared selection of AGN in dwarf galaxies
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• HYPERION. Coevolution of supermassive black holes and galaxies at $z>6$ and the build-up of massive galaxies
• Multiwavelength observations of the extraordinary accretion event AT2021lwx
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Identification and Characterization of a Large Sample of Distant Active Dwarf Galaxies in XMM-SERVS
• SDSS1335+0728: The awakening of a $\sim 10^6{M}_{\odot }$ black hole
• AGN accretion and black hole growth across compact and extended galaxy evolution phases
• Inception of a first quasar at cosmic dawn
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Non-isotropic feedback from accreting spinning black holes
• Testing the evolutionary pathways of galaxies and their supermassive black holes and the impact of feedback from Active Galactic Nuclei via large multiwavelength datasets
• Growth of Massive Black-Holes in FFB Galaxies at Cosmic Dawn
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• Black Hole Growth in Disk Galaxies Mediated by the Secular Evolution of Short Bars
• JWST ERS Program Q3D: The pitfalls of virial BH mass constraints shown in a z = 3 quasar with an ultramassive host
• A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization
• A systematic search for hidden type 1 AGNs: gas kinematics and scaling relations
• 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
• The Black Hole Mass Function Across Cosmic Times II. Heavy Seeds and (Super)Massive Black Holes
• Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-Triggered AGN-Galaxy Coevolution Models?
• TXS 2116$-$077: A Gamma-ray Emitting Relativistic Jet Hosted in a Galaxy Merger
• A New Channel of Bulge Formation via The Destruction of Short Bars
• 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 Diverse Morphologies and Structures of Dwarf Galaxies Hosting Optically-Selected Active Massive Black Holes
• The fast transient AT 2023clx in the nearby LINER galaxy NGC 3799 as a tidal disruption of a very low-mass star
• Evidence for non-merger co-evolution of galaxies and their supermassive black holes
• Consistency of JWST Black Hole Observations with NANOGrav Gravitational Wave Measurements
• Formation of the Little Red Dots from the Core-collapse of Self-interacting Dark Matter Halos
• AT 2023clx: the Faintest and Closest Optical Tidal Disruption Event Discovered in Nearby Star-forming Galaxy NGC 3799
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• BAT AGN Spectroscopic Survey -- XIII. The nature of the most luminous obscured AGN in the low-redshift universe
• Jellyfish: Resolving the kinematics of extreme ram-pressure stripping at $z\sim 0.3$
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• An Accreting, Anomalously Low Mass Black Hole at the Center of Low Mass Galaxy IC 750
• The galaxy's gas content regulated by the dark matter halo mass results in a super-linear M${}_{\mathrm{BH}}$-M${}_{\star }$ relation
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• An X-ray Census of Fast Radio Burst Host Galaxies: Constraints on AGN and X-ray Counterparts
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• Light-Curve Structure and Halpha Line Formation in the Tidal Disruption Event AT 2019azh
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• X-Ray Bright Active Galactic Nuclei in Local Dwarf Galaxies: Insights from eROSITA
• The role of gravitational recoil in the assembly of massive black hole seeds
• Impact of Resonance, Raman, and Thomson Scattering on Hydrogen Line Formation in Little Red Dots
• The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
• Dark-ages reionization and galaxy formation simulation -- XVIII. The high-redshift evolution of black holes and their host galaxies
• SDSS-IV MaNGA: The Incidence of Major Mergers in type I and II AGN Host Galaxies in the DR15 sample
• The X-ray Properties of Million Solar Mass Black Holes
• A catalogue sample of low mass galaxies observed in X-rays with central candidate black holes
• Discovery and Follow-up of ASASSN-23bd (AT 2023clx): The Lowest Redshift and Least Luminous Tidal Disruption Event To Date
• Merger Histories and Environments of Dwarf AGN in IllustrisTNG
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• The LOFAR Two Metre Sky Survey Data Release 2: Probabilistic Spectral Source Classifications and Faint Radio Source Demographics
• The impact of magnetic fields on cosmological galaxy mergers -- II. Modified angular momentum transport and feedback
• Discovery of a strong ionized-gas outflow in an AKARI-selected Ultra-luminous Infrared Galaxy at z = 0.5
• Weighing the IMBH candidate CO-0.40-0.22* in the Galactic Centre
• Testing the fidelity of simulations of black hole - galaxy co-evolution at z ~ 1.5 with observations
• Demographics of Tidal Disruption Events with L-Galaxies: I. Volumetric TDE rates and the abundance of Nuclear Star Clusters
• A Flat-Spectrum Radio Transient at 122 Mpc consistent with an Emerging Pulsar Wind Nebula
• Ultramassive black holes formed by triple quasar mergers at $z\sim 2$
• Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• The Discovery of a Hidden Broad Line AGN in a Bulgeless Galaxy: Keck NIR Spectroscopic Observations of SDSS J085153.64+392611.76
• Multiwavelength Scrutiny of X-ray Sources in Dwarf Galaxies: ULXs versus AGN
• Evidence for an accreting massive black hole in He 2-10 from adaptive optics integral field spectroscopy
• Probing supermassive black hole seed scenarios with gravitational wave measurements
• Probing supermassive black hole growth and its dependence on stellar mass and star-formation rate in low-redshift galaxies
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• Predicting the black hole mass and correlations in X-ray reverberating AGN using neural networks
• An Effective Selection Method for Low-Mass Active Black Holes and First Spectroscopic Identification
• Galaxy Core Formation by Supermassive Black Hole Binaries: the Importance of Realistic Initial Conditions and Galaxy Morphology
• Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• JADES reveals a large population of low mass black holes at high redshift
• Astrometric microlensing
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Tracing the co-evolution path of super massive black holes and spheroids with AKARI-selected ultra-luminous IR galaxies at intermediate redshifts
• Constraining the Low-Mass End of the Black Hole Mass Function and the Active Fraction of the Intermediate-mass Black Holes
• Supermassive Black Hole Demographics: Evading $M-\sigma$
• HSC-XD 52: An X-ray detected AGN in a low-mass galaxy at $z\sim 0.56$
• An Ultraluminous Supersoft Source in a Dwarf Galaxy of Abell 85: An Intermediate-Mass Black Hole Candidate
• The ALPINE-CRISTAL-JWST Survey: Revealing Less Massive Black Holes in High-Redshift Galaxies
• Active galactic nuclei-heated dust revealed in "little red dots"
• The properties of primordially-seeded black holes and their hosts in the first billion years: implications for JWST
• A big red dot at cosmic noon
• COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16
• X-ray AGN in Boötes: The lack of growth of the most massive black holes since z=4
• The rate of extreme coronal line emitting galaxies in the Sloan Digital Sky Survey and their relation to tidal disruption events
• The relation between globular cluster systems and supermassive black holes in spiral galaxies III. The link to the $M_{\bullet }-M_{\ast }$ correlation
• Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies
• Probing the Delay Time of Supermassive Black Hole Binary Mergers With Gravitational Waves
• SCAT Uncovers ATLAS's First Tidal Disruption Event ATLAS18mlw: A Faint and Fast TDE in a Quiescent Balmer Strong Galaxy
• Dark Energy Survey Identification of A Low-Mass Active Galactic Nucleus at Redshift 0.823 from Optical Variability
• Infrared fine-structure lines at high redshift
• Intermediate-Mass Black Holes in Green Pea Galaxies (IMBH-GP) I: a Candidate Sample from LAMOST and SDSS
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• Flaires: A Comprehensive Catalog of Dust-Echo-like Infrared Flares
• The VMC Survey -- XLIX. Discovery of a population of quasars dominated by nuclear dust emission behind the Magellanic Clouds
• Do gas clouds in narrow-line regions of Seyfert galaxies come from their nuclei?
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Not all peaks are created equal: the early growth of Supermassive Black Holes
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• Dwarf AGNs from Variability for the Origins of Seeds (DAVOS): Optical Variability of Broad-line Dwarf AGNs from the Zwicky Transient Facility
• An Eddington ratio-driven origin for the ${\mathrm{L}}_{\mathrm{X}}-{\mathrm{M}}_{\ast }$ relation in quiescent and star forming active galaxies
• Multiple giant eruptions and X-ray emission in the recoiling AGN/LBV candidate SDSS1133
• Extreme Tidal Stripping May Explain the Overmassive Black Hole in Leo I: a Proof of Concept
• Is GN-z11 powered by a super-Eddington massive black hole?
• COSMOS2020: Investigating the AGN-obscured accretion phase at $z\sim 1$ via [NeV] selection
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Ultraviolet Spectral Evidence for Ansky as a Slowly Evolving Featureless Tidal Disruption Event with Quasiperiodic Eruptions
• The Average Soft X-ray Spectra of eROSITA Active Galactic Nuclei
• On the detectability of massive black hole merger eventsby LISA
• Wandering and escaping: recoiling massive black holes in cosmological simulations
• Gravitational Waves from Massive Black Hole Mergers in ASTRID: Predictions for LISA
• Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies
• Evidence for a steeper SMBH-Bulge mass relationship extended to low masses using TDE host galaxies
• Relativistic scattering of a fast spinning neutron star by a massive black hole
• Probing gaseous halos of galaxies with radio jets
• The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• The Success of Optical Variability in Uncovering AGNs in Low-stellar Mass Galaxies
• Evolution of black hole and galaxy growth in a semi-numerical galaxy formation model
• Correlations of the feedback energy and BCG radio luminosity in galaxy clusters
• Astrophysics with the Laser Interferometer Space Antenna
• The Evolution of Brightest Cluster Galaxies in the Nearby Universe II: The star-formation activity and the Stellar Mass from Spectral Energy Distribution
• Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model
• The X-shaped radio galaxy J0725+5835 is associated with an AGN pair
• On the Structure of the AGN Torus through the Fraction of Optically-Selected Type 1 AGNs
• What is the origin of the JWST SMBHs?
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass
• Black Hole Scaling Relations in the Dwarf-galaxy Regime with $Gaia$-Sausage/Enceladus and $\omega$Centauri
• Multiple AGN activity during the BCG assembly of XDCPJ0044.0-2033 at z~1.6
• Central accumulation of magnetic flux in massive Seyfert galaxies as a possible engine to trigger ultrahigh energy cosmic rays
• The Properties of Nuclear Star Clusters and their Host Galaxies
• The relationship of SMBHs and host galaxies at $z<4$ in the deep optical variability-selected AGN sample in the COSMOS field
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• The miniJPAS & J-NEP surveys: Identification and characterization of the Ly$\alpha$ Emitter population and the Ly$\alpha$ Luminosity Function
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Very Large Array Multi-band Radio Imaging of the Triple AGN Candidate SDSS J0849+1114
• Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with [CII]
• Velocity offset between emission and absorption lines might be an effective indicator of dual core system
• SDSS-IV MaNGA: Identification and Multiwavelength Properties of Type-1 AGN in the DR15 sample
• The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
• A LOFAR sample of luminous compact sources coincident with nearby dwarf galaxies
• X-ray Properties of Optically Variable Low-mass AGN Candidates
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• 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
• A comprehensive radio study of narrow-line Seyfert 1 galaxies
• The Host Galaxy of a Dormant, Overmassive Black Hole at $z=6.7$ May Be Restarting Star Formation
• 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
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• Gas excitation in galaxies and active galactic nuclei with He IIλ4686 and X-ray emission
• Probing the rapid formation of black holes and their galaxy hosts in QSOs
• Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• the impact of the AGN and the torus properties on the evolution of spiral galaxies
• No Significant Redshift Evolution in the Intrinsic Scatter of the $M_{\bullet }$-$M_{\star }$ Relation for Overmassive Black Holes
• Insights from the "Red devil" AT 2022fpx: A Dust-reddened Family of Tidal Disruption Events Excluded by Their Apparent Red Color?
• X-ray Unveiling Events in a z~1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South
• Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation
• Constraints on dynamically-formed massive black holes in Little Red Dots from X-ray non-detections
• Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar
• NICER observations reveal doubled timescales in Ansky's quasi-periodic eruptions (QPEs)
• A Flaring AGN In a ULIRG candidate in Stripe 82
• The impact of cosmic ray feedback during the epoch of reionisation
• The Morphology of Dwarf Galaxies Hosting Variable Active Galactic Nuclei
• Method for Determining AGN Accretion Phase in Field Galaxies
• A Recent Supermassive Black Hole Binary in the Galactic Center Unveiled by the Hypervelocity Stars
• Photometric variability in star-forming galaxies as evidence for low-mass AGN and a precursor to quenching
• In Search of the Biggest Bangs since the Big Bang
• Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
• Gravitational Wave Memory Imprints on the CMB from Populations of Massive Black Hole Mergers
• The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z=3.55$
• Robust AGN and host-galaxy decomposition in optical spectral fitting
• Toward measuring the spin of obscured supermassive black holes: a critical assessment with disk megamasers
• Identifying Long Radio Transients with Accompanying X-Ray Emission as Disk-Jet Precessing Black Holes: The Case of ASKAP J1832-0911
• Revisiting the unification of tidal disruption events with polarimetry
• A Spatially Resolved Evolutionary Sequence of Multi-wavelength AGN Host Galaxies
• The early Universe with JWST and ALMA
• Variability as a new discovery channel for Intermediate-Mass Black Holes in the Time Domain Era
• Formation of A Nuclear Star Cluster Through A Merger Event In The Low Surface Brightness Galaxy AGC 223218
• On the signature of black holes on the quenched stellar mass function
• AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• AT 2021hdr: A candidate tidal disruption of a gas cloud by a binary super massive black hole system
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
• It is Feasible to Directly Measure Black Hole Masses in the First Galaxies
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• X-ray properties of massive compact relic galaxies
• Revised event rates for extreme and extremely large mass-ratio inspirals
• A population of luminous globular clusters and stripped nuclei with elevated mass to light ratios around NGC 5128
• Discovery of low-redshift analogues to "Little Red Dots" in DESI: A later evolutionary stage of compact LRDs?
• How Black Holes Stop Their Host Galaxy from Growing Without AGN Feedback
• A search for H${}_2$O masers in 100 active dwarf galaxies
• Updated predictions for gravitational wave emission from TDEs for next generation observatories
• A Search for Wandering Black Holes in the Milky Way with Gaia and DECaLS
• Early emission characterization of TDE 2025aarm
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Insights for Early Massive Black Hole Growth from JWST Detection of the [Ne v] λ3427 Emission Line
• When Stars Mimic Monsters: Spectral Evidence for an $\eta$ Carinae-like Giant Eruption in SBS 0335$-$052 E
• Off-center black hole seed formation? Implications for high and low redshift massive black holes
• Black Hole merger rates in the first billion years in light of JWST data
• A Comprehensive JWST/NIRSpec Census of Broad-line Active Galactic Nuclei: Faint, Low-mass Accretors and a Population of Little Red Dots
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Early results in the search for extreme coronal line emitters with the Dark Energy Spectroscopic Instrument
• The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\sim 4$
• Gravitational Wave Measurement of the $M_{\mathrm{BH}}$-$M_{\mathrm{bulge}}$ Intrinsic Scatter at High Redshift
• AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release
• Enhanced activity in close dual-AGN systems in the local Universe
• Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
• Nuclear Activity and Host Galaxy Properties of Low-Luminosity AGN Identified from VLA Observations
• AT2019ijn: a fast-rising, slow-decaying blue optical transient with exceptionally bright radio emission
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• Massive black holes and their galaxies
• The Drivers of the Decline in Supermassive Black Hole Growth at $z<2$
• Fueling, Evolution, and Diversity of AGN in Dwarf Galaxies: Insights from Star Formation and Black Hole Scaling Relations
• Hyperluminous Supersoft X-Ray Sources in the Chandra Catalog
• Detection of Anisotropies in the Circumgalactic Medium of Disk Galaxies: Supermassive Black Hole Activity or Star Formation-driven Outflows?
• The nature of the X-ray sources in dwarf galaxies in nearby clusters from the KIWICS
• HOLESOM: Constraining the Properties of Slowly-Accreting Massive Black Holes with Self-Organizing Maps
• Implication of a galaxy-scale negative feedback by one of the most powerful multi-phase outflows in a hyper-luminous infrared galaxy at the intermediate redshift
• High-$z$ Universe probed via Lensing by QSOs (HULQ) II. Deep GMOS spectroscopy of a QSO lens candidate
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Massive black holes in the first billion years with JWST
• A Near-Infrared look at AGN Feedback in Bulgeless Galaxies
• Capturing dual AGN activity and kiloparsec-scale outflows in IRAS 20210+1121
• BASS XXX: Distribution Functions of DR2 Eddington-ratios, Black Hole Masses, and X-ray Luminosities
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• The role of AGN activity in the building up of the BCG at z~1.6
• Tips learned from panchromatic modeling of AGNs