An Observational Determination of the Bolometric Quasar Luminosity Function

Abstract

We combine a large set of quasar luminosity function (QLF) measurements from the rest-frame optical, soft and hard X-ray, and near- and mid-infrared bands to determine the bolometric QLF in the redshift interval z=0-6. Accounting for the observed distributions of quasar column densities and variation of spectral energy distribution (SED) shapes, and their dependence on luminosity, makes it possible to integrate the observations in a reliable manner and provides a baseline in redshift and luminosity larger than that of any individual survey. We infer the QLF break luminosity and faint-end slope out to z~4.5 and confirm at high significance (>10sigma) previous claims of a flattening in both the faint- and bright-end slopes with redshift. With the best-fit estimates of the column density distribution and quasar SED, which both depend on luminosity, a single bolometric QLF self-consistently reproduces the observed QLFs in all bands and at all redshifts for which we compile measurements. Ignoring this luminosity dependence does not yield a self-consistent bolometric QLF and there is no evidence for any additional dependence on redshift. We calculate the expected relic black hole mass function and mass density, cosmic X-ray background, and ionization rate as a function of redshift and find they are consistent with existing measurements. The peak in the total quasar luminosity density is well-constrained at z=2.15+/-0.05. We provide a number of fitting functions to the bolometric QLF and its manifestations in various bands, and a script to return the QLF at arbitrary frequency and redshift from these fits, as the most simple inferences from the QLF measured in a single band can be misleading.

24 pages, 11 figures. Submitted to ApJ. A routine to return the QLF from the fits herein is available at http://www.cfa.harvard.edu/~phopkins/Site/qlf.html

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• Clustering of obscured and unobscured quasars in the Bootes field: Placing rapidly growing black holes in the cosmic web
• Quasar Proximity Zones and Patchy Reionization
• The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift
• The Origins of AGN Obscuration: The 'Torus' as a Dynamical, Unstable Driver of Accretion
• Detailed Shape and Evolutionary Behavior of the X-ray Luminosity Function of Active Galactic Nuclei
• Revisiting the relationship between 6 μm and 2-10 keV continuum luminosities of AGN
• The ultra-dense, interacting environment of a dual AGN at z $\sim$ 3.3 revealed by JWST/NIRSpec IFS
• An uncontaminated measurement of the escaping Lyman continuum at $z\sim 3$
• The cosmic growth of the active black hole population at 1<z<2 in zCOSMOS, VVDS and SDSS
• The Demography of Super-Massive Black Holes: Growing Monsters at the Heart of Galaxies
• The Extended Baryon Oscillation Spectroscopic Survey: Variability Selection and Quasar Luminosity Function
• Black Hole and Galaxy Coevolution from Continuity Equation and Abundance Matching
• Recovering Stellar Population Properties and Redshifts from Broad-Band Photometry of Simulated Galaxies: Lessons for SED Modeling
• The Subaru high-z quasar survey: discovery of faint z~6 quasars
• Linking black-hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution
• The impact of local stellar radiation on the HI column density distribution
• On the radiative efficiencies, Eddington ratios, and duty cycles of luminous high-redshift quasars
• The Co-Formation of Spheroids and Quasars Traced in their Clustering
• Large scale opacity fluctuations in the Lyman alpha forest: evidence for QSOs dominating the ionising UV background at z ~ 5.5-6 ?
• VLT/ISAAC Spectra of the Hbeta Region in Intermediate-Redshift Quasars III. Hbeta Broad Line Profile Analysis and Inferences about BLR Structure
• A Kiloparsec-Scale Binary Active Galactic Nucleus Confirmed by the Expanded Very Large Array
• The Photon Underproduction Crisis
• New Insights on the QSO Radio-Loud/Radio-Quiet Dichotomy: SDSS Spectra in the Context of the 4D Eigenvector1 Parameter Space
• The Complete Infrared View of Active Galactic Nuclei from the 70-month Swift/BAT Catalog
• The cosmological properties of AGN in the XMM-Newton Hard Bright Survey
• Luminosity Function from dedicated SDSS-III and MMT data of quasars in 0.7<z<4.0 selected with a new approach
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: II. The clustering of quasars and their dark environment
• An unbiased measurement of the UV background and its evolution via the proximity effect in quasar spectra
• The Chandra COSMOS legacy survey: Energy Spectrum of the Cosmic X-ray Background and constraints on undetected populations
• The XMM-Newton Serendipitous Survey. VI. The X-ray Luminosity Function
• Galaxy Evolution in the Radio Band: The Role of Starforming Galaxies and Active Galactic Nuclei
• The Prospects of Observing Tidal Disruption Events with the LSST
• A survey of dual active galactic nuclei in simulations of galaxy mergers: frequency and properties
• The low-end of the black hole mass function at cosmic dawn
• Supermassive Black Hole Growth in Starburst Galaxies over Cosmic Time: Constraints from the Deepest Chandra Fields
• Hot dust in Panchromatic SED Fitting: Identification of AGN and improved galaxy properties
• Observational Constraints on the Dependence of Radio-Quiet Quasar X-ray Emission on Black Hole Mass and Accretion Rate
• Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 III: Far-IR to Radio Properties and Optical Spectral Diagnostics
• Extreme-Velocity Quasar Outflows and the Role of X-ray Shielding
• A High-Resolution Hubble Space Telescope Study of Apparent Lyman Continuum Leakers at $z\sim 3$
• The X-ray luminosity function of Active Galactic Nuclei in the redshift interval z=3-5
• A backward evolution model for infrared surveys: the role of AGN- and Color-L_TIR distributions
• Models of the Thermal Evolution of the Intergalactic Medium After Reionization
• Radio galaxies of the local universe: all-sky catalog, luminosity functions, and clustering
• A New Constraint on the Escape Fraction in Distant Galaxies Using Gamma-ray Burst Afterglow Spectroscopy
• The MOSDEF survey: AGN multi-wavelength identification, selection biases and host galaxy properties
• The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
• The Role of Galactic Winds on Molecular Gas Emission from Galaxy Mergers
• Supermassive Black Holes in the Hierarchical Universe: A General Framework and Observational Tests
• The Star-Forming Molecular Gas in High Redshift Submillimeter Galaxies
• Determining the fraction of cosmic-ray protons at ultra-high energies with cosmogenic neutrinos
• Cosmic reionization after Planck II: contribution from quasars
• High-resolution VLA Imaging of SDSS Stripe 82 at 1.4 GHz
• Variability selected high-redshift quasars on SDSS Stripe 82
• The History and Morphology of Helium Reionization
• A direct measurement of the linear bias of mid-infrared-selected quasars at z~1 using cosmic microwave background lensing
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from the Third Data Release Quasar Lens Catalog
• The X-ray Energy Dependence of the Relation between Optical and X-ray Emission in Quasars
• PRIMUS: Infrared and X-ray AGN Selection Techniques at 0.2<z<1.2
• Relative Role of Stars and Quasars in Cosmic Reionization
• The Sloan Digital Sky Survey Quasar Lens Search. VI. Constraints on Dark Energy and the Evolution of Massive Galaxies
• Compton Thick AGN in the XMM-COSMOS survey
• Gravitational waves and stalled satellites from massive galaxy mergers at z <= 1
• The XMM-Newton Serendipitous Survey V. Optical identification of the XMM-Newton Medium sensitivity Survey (XMS)
• Black-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation Rate
• Black Hole -- Galaxy Correlations in Simba
• A Flat Photoionization Rate at 2<z<4.2: Evidence for a Stellar-Dominated UV Background and Against a Decline of Cosmic Star Formation Beyond z~3
• High-Energy Neutrino and Gamma-Ray Emission from Tidal Disruption Events
• The Evolution of the M_BH-sigma relation Inferred from the Age Distribution of Local Early-Type Galaxies and AGN Evolution
• Testing the binary hypothesis: pulsar timing constraints on supermassive black hole binary candidates
• Is there an upper limit to black hole masses?
• X-ray bubbles in the circumgalactic medium of TNG50 Milky Way- and M31-like galaxies: signposts of supermassive black hole activity
• Sizes and Kinematics of Extended Narrow-Line Regions in Luminous Obscured AGN Selected by Broadband Images
• Statistics of gamma-ray point sources below the Fermi detection limit
• Narrowband Lyman-Continuum Imaging of Galaxies at z ~ 2.85
• Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
• The Mid-IR and X-ray Selected QSO Luminosity Function
• Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS
• Radiation pressure force and black hole mass determination in low redshift type-I and type-II active galactic nuclei
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• Ultra-High Energy Cosmic Rays and Neutrinos from Tidal Disruptions by Massive Black Holes
• Spectral Energy Distributions of Type 1 AGN in the COSMOS Survey I - The XMM-COSMOS Sample
• Massive BH Binaries as Periodically-Variable AGN
• Evolution in the Black Hole - Galaxy Scaling Relations and the Duty Cycle of Nuclear Activity in Star-Forming Galaxies
• The Impact of the Uncertainty in Single-Epoch Virial Black Hole Mass Estimates on the Observed Evolution of the Black Hole - Bulge Scaling Relations
• Constraining the contribution of active galactic nuclei to reionisation
• Constraining the Solution to the Last Parsec Problem with Pulsar Timing
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• Electromagnetic counterparts of supermassive black hole binaries resolved by pulsar timing arrays
• Origins and Demographics of Wandering Black Holes
• The Interaction of the Fermi Bubbles with the Milky Way's Hot Gas Halo
• Understanding black hole mass assembly via accretion and mergers at late times in cosmological simulations
• Temperature and abundance profiles of hot gas in galaxy groups - II. Implications for feedback and ICM enrichment
• Measuring the accretion rate and kinetic luminosity functions of supermassive black holes
• 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
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• The deepest X-ray view of high-redshift galaxies: constraints on low-rate black-hole accretion
• Black hole growth in the early Universe is self-regulated and largely hidden from view
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• Long-Term X-ray Variability of Typical Active Galactic Nuclei in the Distant Universe
• Constraining the UV emissivity of AGN throughout cosmic time via X-ray surveys
• $\text{Herschel}$-ATLAS:The connection between star formation and AGN activity in radio-loud and radio-quiet active galaxies
• The Spitzer mid-infrared AGN survey. II-the demographics and cosmic evolution of the AGN population
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• An enhanced rate of tidal disruptions in the centrally overdense E+A galaxy NGC 3156
• Polar Dust, Nuclear Obscuration and IR SED Diversity in Type-1 AGNs
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• AGN-driven outflows and the AGN feedback efficiency in young radio galaxies
• Obscuring Fraction of Active Galactic Nuclei: Implications from Radiation-driven Fountain Models
• Evidence for Merger-Driven Growth in Luminous, High-z, Obscured AGN in the CANDELS/COSMOS Field
• The Lyman-alpha forest in a blazar-heated Universe
• Eight-Dimensional Mid-Infrared/Optical Bayesian Quasar Selection
• Dark-ages Reionization and Galaxy Formation Simulation - X. The small contribution of quasars to reionization
• Assessing the redshift evolution of massive black holes and their hosts
• Towards a Complete Census of AGNs in Nearby Galaxies: The Incidence of Growing Black Holes
• Scale-dependent bias in the BAO-scale intergalactic neutral hydrogen
• A probable Milli-Parsec Supermassive Binary Black Hole in the Nearest Quasar Mrk 231
• Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions
• The Angular Clustering of Infrared-Selected Obscured and Unobscured Quasars
• First CO(17-16) emission line detected in a z > 6 quasar
• Evident black hole-bulge coevolution in the distant universe
• Modeling the Dust Properties of z ~ 6 Quasars with ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• Do We Expect Most AGN to Live in Disks?
• Low accretion rates at the AGN cosmic downsizing epoch
• On the X-ray properties of submm-selected galaxies
• The Millennium Galaxy Catalogue: The $M_{bh}$--$L_{spheroid}$ derived supermassive black hole mass function
• Mass Functions of Supermassive Black Holes Across Cosmic Time
• Multi-wavelength properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• Revealing the Accretion Physics of Supermassive Black Holes at Redshift z~7 with Chandra and Infrared Observations
• Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-z Universe
• On the Radio and Optical Luminosity Evolution of Quasars
• Are Most Low-Luminosity AGN Really Obscured?
• The radio afterglow of Swift J1644+57 reveals a powerful jet with fast core and slow sheath
• Sources of the Radio Background Considered
• Toward precise constraints on growth of massive black holes
• A Comparison of X-ray and Mid-Infrared Selection of Obscured AGN
• The Spectral Slope and Escape Fraction of Bright Quasars at $z\sim 3.8$: the Contribution to the Cosmic UV Background
• QSO obscuration at high redshift ($z\gtrsim 7$): Predictions from the BlueTides simulation
• The Cosmological Impact of Luminous TeV Blazars III: Implications for Galaxy Clusters and the Formation of Dwarf Galaxies
• AGN proximity zone fossils and the delayed recombination of metal lines
• Observational constraints on the spin of the most massive black holes from radio observations
• Spectroscopic Identification of Type 2 Quasars at Z < 1 in SDSS-III/BOSS
• The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
• Episodic Random Accretion and the Cosmological Evolution of Supermassive Black Hole Spins
• X-ray emission from high-redshift miniquasars: self-regulating the population of massive black holes through global warming
• [On the jet contribution to the AGN cosmic energy budget
• Outflow Bubbles from Compact Binary Mergers Embedded in Active Galactic Nuclei: Cavity Formation and the Impact on Electromagnetic Counterparts
• Modeling the Nuclear Infrared Spectral Energy Distribution of Type II Active Galactic Nuclei
• The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy
• Identifying Decaying Supermassive Black Hole Binaries from their Variable Electromagnetic Emission
• Efficient computation of the gravitational wave spectrum emitted by eccentric massive black hole binaries in stellar environments
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• Mass without radiation: heavily obscured AGN, the X-ray Background and the Black Hole Mass Density
• The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey
• Characterising and Identifying Galaxy Protoclusters
• The Habitable Exoplanet Observatory (HabEx) Mission Concept Study Interim Report
• Blazar candidates beyond redshift 4 observed by Swift
• The role of relativistic jets in the heaviest and most active supermassive black holes at high redshift
• Clustering properties of moderate luminosity X-ray selected Type 1 and Type 2 AGN at z~3
• Photo-heating and the fate of hard photons during the reionisation of HeII by quasars
• The Quasar Feedback Survey: Discovering hidden Radio-AGN and their connection to the host galaxy ionised gas
• Discovery of a close-separation binary quasar at the heart of a z~0.2 merging galaxy and its implications for low-frequency gravitational waves
• The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
• Quasar Probabilities and Redshifts from WISE mid-IR through GALEX UV Photometry
• Binary Quasars at High Redshift II: Sub-Mpc Clustering at z ~ 3-4
• Seeding Black Holes in Cosmological Simulations
• AGN evolution from a galaxy evolution viewpoint
• Intergalactic Lyman continuum photon budget in the past 5 billion years
• New observational Constraints on the Growth of the First Supermassive Black Holes
• On the Lack of Correlation Between [OIII]/[OII] and Lyman-Continuum Escape Fraction
• On the Evolution of the Cosmic Ionizing Background
• BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes
• Star formation history, dust attenuation and extragalactic background light
• Hydrogen Reionization in the Illustris universe
• AGN contamination of galaxy-cluster thermal X-ray emission: predictions for eRosita from cosmological simulations
• The X-ray and Mid-Infrared luminosities in Luminous Type 1 Quasars
• Reionization constraints using Principal Component Analysis
• The Rise of Active Galactic Nuclei in the GAlaxy Evolution and Assembly semi-analytic model
• The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback
• The evolution of SMBH spin and AGN luminosities for $z<6$ within a semi-analytic model of galaxy formation
• Accurate Identification of Galaxy Mergers with Imaging
• X-ray selected AGN Hosts are Similar to Inactive Galaxies out to z=3: Results from CANDELS/CDF-S
• Sub-parsec supermassive Binary Quasars: expectations at z<1
• Heating the IGM by X-rays from Population III Binaries in High Redshift Galaxies
• A Simple Likelihood Method for Quasar Target Selection
• Exploring SMBH Assembly with Semi-analytic Modelling
• PRIMUS: An observationally motivated model to connect the evolution of the AGN and galaxy populations out to z~1
• Constraints on the Lyman continuum escape fraction for faint star forming galaxies
• Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations
• Studying the relationship between X-ray emission and accretion in AGNs using the XMM-Newton Bright Serendipitous Survey
• Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z=3.35: A Detailed Look at an Early Progenitor of Local Most Massive Ellipticals
• High-redshift galaxies and black holes in the eyes of JWST: a population synthesis model from infrared to X-rays
• Lyman continuum galaxies and the escape fraction of Lyman break galaxies
• Identifying Reionization Sources from 21cm Maps using Convolutional Neural Networks
• A Flexible Method of Estimating Luminosity Functions
• The merger-driven evolution of warm infrared luminous galaxies
• Properties of simulated galaxies and supermassive black holes in cosmic voids
• On the Radio and Optical Luminosity Evolution of Quasars II - The SDSS Sample
• Updating quasar bolometric luminosity corrections. II. Infrared bolometric corrections
• AMUSE-Field I: Nuclear X-ray Properties of Local Field and Group Spheroids across the Stellar Mass Scale
• Quasar UV luminosity function evolution up to z=8
• The Signatures of Large-scale Temperature and Intensity Fluctuations in the Lyman-alpha Forest
• Exploring AGN and Star Formation Activity of Massive Galaxies at Cosmic Noon
• The Carbon Content of Intergalactic Gas at z=4.25 and its Evolution Toward z=2.4
• AGN-driven outflows and the formation of Ly$\alpha$ nebulae around high-z quasars
• Finding high-redshift dark stars with the James Webb Space Telescope
• Survival of the obscuring torus in the most powerful active galactic nuclei
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• SpIES: The Spitzer IRAC Equatorial Survey
• Ultra-Short-Period Massive Black Hole Binary Candidates in LSST as LISA "Verification Binaries"
• The contribution of spin to jet-disk coupling in black holes
• No redshift evolution of non-repeating fast radio-burst rates
• The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
• Supersonic Relative Velocity between Dark Matter and Baryons: A Review
• Properties of QSO Metal Line Absorption Systems at High Redshifts: Nature and Evolution of the Absorbers and New Evidence on Escape of Ionizing Radiation from Galaxies
• Nature and evolution of powerful radio galaxies and their link with the quasar luminosity function
• Separating Accretion and Mergers in the Cosmic Growth of Black Holes with X-ray and Gravitational Wave Observations
• Cosmological Evolution of Supermassive Black Holes. II. Evidence for Downsizing of Spin Evolution
• AGN host galaxies at redshift z~0.7: peculiar or not?
• Constraining the supermassive black holes evolution through the continuity equation
• The kinetic luminosity function and the jet production efficiency of growing black holes
• The hidden quasar nucleus of a WISE-selected, hyperluminous, dust-obscured galaxy at z ~ 2.3
• Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
• Tracing the evolution of Active Galactic Nuclei host galaxies over the last 9 Gyrs of Cosmic time
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Can winds driven by active galactic nuclei account for the extragalactic gamma-ray and neutrino backgrounds?
• A Deep Narrowband Imaging Search for CIV and He II Emission from Ly$\alpha$ Blobs
• Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts
• Determining Quasar Black Hole Mass Functions from their Broad Emission Lines: Application to the Bright Quasar Survey
• Color Distributions, Number and Mass Densities of Massive Galaxies at 1.5 < z < 3: Comparing Observations with Merger Simulations
• The optical-UV spectral energy distribution of the unabsorbed AGN population in the XMM-Newton Bright Serendipitous Survey
• Missing Gamma-ray Halos and the Need for New Physics in the Gamma-ray Sky
• Constraining reionization using 21 cm observations in combination with CMB and Lyman-alpha forest data
• Decomposing Star Formation and Active Galactic Nucleus with Spitzer Mid-Infrared Spectra: Luminosity Functions and Co-Evolution
• Weighing obscured and unobscured quasar hosts with the CMB
• Observational constraints on the co-evolution of supermassive black holes and galaxies
• Inhomogeneous Helium Reionization and the Equation of State of the Intergalactic Medium
• Probing black hole accretion tracks, scaling relations and radiative efficiencies from stacked X-ray active galactic nuclei
• The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei. IV. Association with Galaxy Mergers
• Super Star Clusters in the Central Starburst of NGC 4945
• Dust Reverberation Mapping in Distant Quasars from Optical and Mid-Infrared Imaging Surveys
• The Chandra Multi-Wavelength Project: Optical Spectroscopy and the Broadband Spectral Energy Distributions of X-ray Selected AGN
• Black hole obscuration and duty cycles mediated by AGN feedback in high redshift galaxies
• ALMA Twenty-six arcmin${}^2$ Survey of GOODS-S at One-millimeter (ASAGAO): X-ray AGN Properties of Millimeter-Selected Galaxies
• An Evolutionary Model For Submillimeter Galaxies
• Impact of X-rays on CO emission from high-z galaxies
• Jet enhanced accretion growth of supermassive black holes
• VLT/X-Shooter Survey of BAL Quasars: Large Distance Scale and AGN Feedback
• The Halo Occupation Distribution of Active Galactic Nuclei
• SRG/eROSITA prospects for the detection of stellar tidal disruption flares
• The Nature of CO Emission From z~6 Quasars
• Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature
• The Formation of Galaxies Hosting z~6 Quasars
• A Candidate Dual AGN at z=1.175
• The AGN-Star Formation Connection: Future Prospects with JWST
• X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim 2$
• The Evolution of the HeII-Ionizing Background at Redshifts 2.3<z<3.8 Inferred from a Statistical Sample of 24 HST/COS HeII Ly$\alpha$ Absorption Spectra
• Does black-hole growth depend on the cosmic environment?
• Cosmological evolution of supermassive black holes. I. mass function at 0<z<2
• Cosmological evolution of massive black holes: effects of Eddington ratio distribution and quasar lifetime
• Multi-messenger tests of cosmic-ray acceleration in radiatively inefficient accretion flows
• The Line-of-Sight Proximity Effect and the Mass of Quasar Host Halos
• Seeking the growth of the first black hole seeds with JWST
• Glimmering in the dark: modeling the low-mass end of the $M_{\bullet }-\sigma$ relation and of the quasar luminosity function
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• Eddington ratio Distribution of X-ray selected broad-line AGNs at 1.0<z<2.2
• The Sloan Digital Sky Survey Reverberation Mapping Project: Post-Starburst Signatures in Quasar Host Galaxies at z < 1
• X-ray Constraints on the AGN Properties in Spitzer-IRS identified z~2 Ultraluminous Infrared Galaxies
• Faint-end Quasar Luminosity Functions from Cosmological Hydrodynamic Simulations
• Unveiling the Population of Wandering Black Holes via Electromagnetic Signatures
• The Chandra X-ray point source catalog in the DEEP2 Galaxy Redshift Survey fields
• Helium Reionization Simulations. II. Signatures of Quasar Activity on the IGM
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• The Ionized Absorber and Nuclear Environment of IRAS 13349+2438: Multi-wavelength insights from coordinated Chandra HETGS, HST STIS, HET, and Spitzer IRS
• Revealing the relation between black-hole growth and host-galaxy compactness among star-forming galaxies
• Are There Enough Ionizing Photons to Reionize the Universe by z=6?
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• The first Super Massive Black Holes: indications from models for future observations
• A quasar-based supermassive black hole binary population model: implications for the gravitational-wave background
• Low density, radiatively inefficient rotating-accretion flow onto a black hole
• Updated measurements of the dark matter halo masses of obscured quasars with improved WISE and Planck data
• An enhanced fraction of starbursting galaxies among high Eddington ratio AGNs
• The physical scale of the far-infrared emission in the most luminous submillimetre galaxies II: evidence for merger-driven star formation
• Type 2 AGN host galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching
• The space density of z>4 blazars
• Black hole growth and AGN feedback under clumpy accretion
• Panchromatic SED modelling of spatially-resolved galaxies
• Constraints on light bending and reflection from the hard X-ray background
• Soft gamma rays from low accreting supermassive black holes and connection to energetic neutrinos
• The evolution of the helium-ionizing background at z ~ 2-3
• X-ray bolometric corrections for Compton-thick active galactic nuclei
• The Contribution of z<6 Sources to the Spatial Coherence in the Unresolved Cosmic near-Infrared and X-ray Backgrounds
• On the co-evolution of supermassive black holes and their host galaxies since z = 3
• Modelling Galaxy and AGN Evolution in the IR: Black Hole Accretion versus Star-Formation Activity
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• Spectral Energy Distributions of Type 1 AGN in XMM-COSMOS Survey II - Shape Evolution
• Constraints on the faint end of the quasar luminosity function at z~5 in the COSMOS field
• Spiral-Induced Star Formation in the Outer Disks of Galaxies
• A growth-rate indicator for Compton-thick active galactic nuclei
• Stellar Populations of UV-Selected Active Galactic Nuclei Host Galaxies at z ~ 2 - 3
• Large 21 cm signals from AGN-dominated reionization
• Obscured GOODS AGN and Their Host Galaxies at z < 1.25: The Slow Black Hole Growth Phase
• Fluctuations in the Ionizing Background During and After Helium Reionization
• Probing the assembly history and dynamical evolution of massive black hole binaries with pulsar timing arrays
• Testing the disk-corona interplay in radiatively-efficient broad-line AGN
• Low-luminosity AGN and X-ray binary populations in COSMOS star-forming galaxies
• Radio-AGN Feedback: When the Little Ones were Monsters
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• The effect of baryonic streaming motions on the formation of the first supermassive black holes
• A new z=0 metagalactic UV background limit
• Short time-scale optical variability properties of the largest AGN sample observed with Kepler/K2
• Determining the core radio luminosity function of radio AGNs via copula
• Merger Signatures in the Dynamics of Star-forming Gas
• Wide-field LOFAR imaging of the field around the double-double radio galaxy B1834+620: A fresh view on a restarted AGN and doubeltjes
• Variability and Multiwavelength Detected AGN in the GOODS Fields
• HST/COS Observations of Thirteen New He II Quasars
• Cosmic downsizing of powerful radio galaxies to low radio luminosities
• A comparative analysis of virial black-hole mass estimates of moderate-luminosity active galactic nuclei using Subaru/FMOS
• Eddington ratios of faint AGN at intermediate redshift: Evidence for a population of half-starved black holes
• Linking the fate of massive black hole binaries to the active galactic nuclei luminosity function
• A Global Inventory of Feedback
• A significant excess in major merger rate for AGNs with the highest Eddington ratios at z<0.2
• Radiative Efficiency of Disk Accretion in Individual SDSS QSOs
• Dark Matter Accretion into Supermassive Black Holes
• Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions
• High redshift AGNs and HI reionisation: limits from the unresolved X-ray background
• The Ultraviolet-X-ray connection in AGN outflows
• Selection bias in dynamically-measured supermassive black hole samples: Scaling relations and correlations between residuals in semi-analytic galaxy formation models
• A Spectroscopic Survey of WISE-selected Obscured Quasars with the Southern African Large Telescope
• Dust-Enshrouded AGN can Dominate Host-Galaxy-Scale Cold-Dust Emission
• He II absorption and the sawtooth spectrum of the cosmic far-UV background
• Tidal Disruption Flares of Stars From Moderately Recoiled Black Holes
• The local supermassive black hole mass density: corrections for dependencies on the Hubble constant
• Large-Scale Fluctuations in the HeII Lyman-alpha Forest and HeII Reionization
• AGN evolution from galaxy evolution viewpoint - II
• Panchromatic Spectral Energy Distributions of Dusty Galaxies with RADISHE. I. Predictions for Herschel: Correlating Colors with Galactic Energy Sources
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• Population statistics of intermediate mass black holes in dwarf galaxies using the NewHorizon simulation
• A Catalog of Host Galaxies for WISE-Selected AGN: Connecting Host Properties with Nuclear Activity and Identifying Contaminants
• Bridging Star-Forming Galaxy and AGN Ultraviolet Luminosity Functions at $z=4$ with the SHELA Wide-Field Survey
• Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3
• The HELLAS2XMM survey. XIII. Multi-component analysis of the spectral energy distribution of obscured AGN
• Measuring large-scale structure with quasars in narrow-band filter surveys
• The cosmic evolution of massive black holes and galaxy spheroids: global constraints at redshift z<~1.2
• Physical conditions of the interstellar medium in star-forming galaxies at z~1.5
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Black hole clustering and duty cycles in the Illustris simulation
• Anisotropic AGN Outflows and Enrichment of the Intergalactic Medium
• Exploring the effects of pressure on the radial accretion of dark matter by a Schwarzschild supermassive black hole
• Extragalactic gamma-ray background from AGN winds and star-forming galaxies in cosmological galaxy formation models
• Evolution of active galactic nuclei
• The cosmological consequence of an obscured AGN population on the radiation efficiency
• Observing Supermassive Black Holes across cosmic time: from phenomenology to physics
• The LSST era of supermassive black holes accretion-disk reverberation mapping
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• A Quasar-Galaxy Mixing Diagram: Quasar Spectral Energy Distribution Shapes in the Optical to Near-Infrared
• Witnessing the Birth of a Quasar
• A self-consistent 3D model of fluctuations in the helium-ionizing background
• Probing high-redshift galaxies with Ly$\alpha$ intensity mapping
• Tidal disruption events in the first billion years of a galaxy
• Implications of Plasma Beam Instabilities for the Statistics of the Fermi Hard Gamma-ray Blazars and the Origin of the Extragalactic Gamma-Ray Background
• The Past and Future of Mid-Infrared Studies of AGN
• First study of reionization in the Planck 2015 normalized closed $\Lambda$CDM inflation model
• Does black-hole growth depend fundamentally on host-galaxy compactness?
• Ultraviolet Emission-Line Correlations in Hubble/COS Spectra of Active Galactic Nuclei: Single-Epoch Black Hole Masses
• The Effect of Fluctuations on the Helium-Ionizing Background
• Modeling the HeII Transverse Proximity Effect: Constraints on Quasar Lifetime and Obscuration
• The hyperluminous Compton-thick $z\sim 2$ quasar nucleus of the hot DOG W1835+4355 observed by NuSTAR
• MaNGIA: 10,000 mock galaxies for stellar population analysis
• XXL-HSC: The link between AGN activity and star formation in the Early Universe ($z⩾3.5$)
• Constraining the quasar population with the broad-line width distribution
• The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function
• First HETDEX Spectroscopic Determinations of Ly$\alpha$ and UV Luminosity Functions at $z=2-3$: Bridging a Gap Between Faint AGN and Bright Galaxies
• The evolution of the Lyman-alpha forest effective optical depth following HeII reionisation
• Optical colours of AGN in the Extended Chandra Deep Field South: Obscured black holes in early type galaxies
• The case against large intensity fluctuations in the z ~ 2.5 HeII Lyman-alpha forest
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• Cosmic evolution of radio-AGN feedback: confronting models with data
• The Escape Fraction of Ionizing Radiation from Galaxies
• The Variable Sky of Deep Synoptic Surveys
• Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function
• The relative growth of Optical and Radio Quasars in SDSS
• Hard X-ray selected giant radio galaxies - I. The X-ray properties and radio connection
• The Luminosity Function of bright QSOs at z~4 and implications for the cosmic ionizing background
• X-ray spectroscopy of the z=6.4 quasar J1148+5251
• Quasar-driven outflows account for the missing extragalactic gamma-ray background
• The evolution of the heaviest super-massive black-holes in jetted AGNs
• Baryons: What, When and Where?
• Testing Models of Radio Galaxy Evolution and the Cosmological Impact of FR II Radio Galaxies
• Spectral Energy Distribution of Hyper-Luminous Infrared Galaxies
• On Constraining the Growth History of Massive Black Holes via Their Distribution on the Spin-Mass Plane
• Mapping quasar light echoes in 3D with Lyα forest tomography
• The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution Functions
• The Role of Star-Formation and AGN in Dust Heating of z=0.3-2.8 Galaxies - II. Informing IR AGN fraction estimates through simulations
• Constraints on Quasar Lifetimes and Beaming from the HeII Lyman-alpha Forest
• The Type II AGN-host galaxy connection: insights from the VVDS and VIPERS surveys
• Imprints of quasar duty cycle on the 21cm signal from the Epoch of Reionization
• Electromagnetic signatures of supermassive black hole binaries resolved by PTAs
• Angular size test on the expansion of the Universe
• High-density disc reflection spectroscopy of low-mass active galactic nuclei
• IGM Transmission Bias for $z$ $\ge$ 2.9 Lyman Continuum Detected Galaxies
• The impact of spatial fluctuations in the ultra-violet background on intergalactic carbon and silicon
• Is IRAS 01072+4954 a True-Seyfert 2? Hints from Near Infrared Integral Field Spectroscopy
• A mixture evolution scenario of the AGN radio luminosity function. II. Do low- and high-power radio-loud AGNs evolve differently?
• Bright vigorous winds as signposts of supermassive black hole birth
• Recurring tidal disruption events a decade apart in IRAS F01004-2237
• Do the spectral energy distributions of type 1 AGN show diversity?
• Constraints on the Local Sources of Ultra High-Energy Cosmic Rays
• Relation Between Globular Clusters and Supermassive Black Holes in Ellipticals as a Manifestation of the Black Hole Fundamental Plane
• Empirical Constraints on the Evolution of the Relationship between Black Hole and Galaxy Mass: Scatter Matters
• A Multiwavelength Study of Binary Quasars and Their Environments
• X-ray properties of dust-obscured galaxies with broad optical/UV emission lines
• Origin and evolution of dust-obscured galaxies in galaxy mergers
• A Southern Photometric Quasar Catalog from the Dark Energy Survey Data Release 2
• Can the 21 cm signal probe Population III and II star formation?
• The AGN Luminosity Fraction in Merging Galaxies
• Cumulative neutrino background from quasar-driven outflows
• He II optical depth and UV escape fraction of galaxies
• AGN Feedback in Groups and Clusters of Galaxies
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$): Detection of a dusty star-forming galaxy within the enormous Lyman $\alpha$ nebula at $z=2.3$ sheds light on its origin
• Helium Reionization Simulations. I. Modeling Quasars as Radiation Sources
• AGN X-ray luminosity function and absorption function in the Early Universe ($3\le z\le 6$)
• Analysis of Spitzer-IRS spectra of hyperluminous infrared galaxies
• Observational Evidence for Enhanced Black Hole Accretion in Giant Elliptical Galaxies
• Quasar Host Environments: The view from Planck
• Growth of Early Supermassive Black Holes and the High-Redshift Eddington Ratio Distribution
• Optical and infrared properties of active galactic nuclei in the Lockman Hole
• Lyman Continuum Galaxy Candidates in COSMOS
• The cosmic web in Lyman-alpha emission
• The Gaseous Environments of Quasars: Associate Absorption Lines with Density and Distance Constraints
• Anisotropic AGN Outflows and Enrichment of the Intergalactic Medium. II. Metallicity
• A Joint Model of the X-ray And Infrared Extragalactic Backgrounds: I. Model Construction And First Results
• Fossil Ionized Bubbles Around Dead Quasars During Reionization
• Evidence that Emission and Absorption Outflows in Quasars Are Related
• The influence of metagalactic ultra-violet background fluctuations on the high-redshift Ly$\alpha$ forest
• X-ray observations of sub-mm LABOCA galaxies in the eCDFS
• Patchy blazar heating: diversifying the thermal history of the intergalactic medium
• Gravitational waves from supermassive black hole binaries in ultra-luminous infrared galaxies
• The imprint of the cosmic supermassive black hole growth history on the 21 cm background radiation
• A possible sub-kiloparsec dual AGN buried behind the galaxy curtain
• The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
• The Accretion History of AGN: A Newly Defined Population of Cold Quasars
• Constraining Star Formation and AGN in z~2 Massive Galaxies using High Resolution MERLIN Radio Observations
• Time-dependent fluctuations in the metagalactic photoionization background
• A Cigale module tailored (not only) for Low-Luminosity AGN
• Accretion History of AGN III: Radiative Efficiency and AGN Contribution to Reionization
• Magnetohydrodynamic stability of broad line region clouds
• Simulations Find Our Accounting of Dust-Obscured Star Formation May Be Incomplete
• Stellar and gas dynamical model for tidal disruption events in a quiescent galaxy
• Photometric Properties of the Most Massive High-Redshift Galaxies
• Distinctive 21 cm structures of the first stars, galaxies, and quasars
• On the Search for Quasar Light Echoes
• The spatial distribution of X-ray selected AGN in the Chandra deep fields: a theoretical perspective
• First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
• Feedback and feeding in the context of galaxy evolution with SPICA: direct characterization of molecular outflows and inflows
• The Black Hole Mass Function Across Cosmic Times II. Heavy Seeds and (Super)Massive Black Holes
• The XXL Survey XIX. A realistic population of simulated X-ray AGN: Comparison of models with observations
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
• Tracing the evolution of dust obscured star-formation and accretion back to the reionisation epoch with SPICA
• The Mass Function of Supermassive Black Holes in the Direct-collapse Scenario
• Rapid formation of black holes in galaxies: a self-limiting growth mechanism
• The Origin and Evolution of Lyman-alpha Blobs in Cosmological Galaxy Formation Simulations
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Big and young supermassive black holes in the early Universe
• Reliable Identification of Binary Supermassive Black Holes from Rubin Observatory Time-Domain Monitoring
• Pure Density Evolution of the Ultraviolet Quasar Luminosity Function at $2\lesssim z\lesssim 6$
• The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function
• Characterization of Optical Light Curves of Extreme Variability Quasars Over a ~16-yr Baseline
• Using Real and Simulated Measurements of the Thermal Sunyaev-Zel'dovich Effect to Constrain Models of AGN Feedback
• The Flatness and Sudden Evolution of the Intergalactic Ionizing Background
• On possible proxies of AGN light curves cadence selection in future time domain surveys
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8
• Ultra high energy cosmic rays from non-relativistic quasar outflows
• Cosmological growth and feedback from supermassive black holes
• A multi-wavelength approach to the properties of Extremely Red Galaxy populations: I - Contribution to the Star Formation Rate density and AGN content
• The Properties of Radio and Mid-infrared Detected Galaxies and the Effect of Environment on the Co-evolution of AGN and Star Formation at $z\sim 1$
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
• Dark-ages reionization and galaxy formation simulation -- XVIII. The high-redshift evolution of black holes and their host galaxies
• A Joint Model Of X-ray And Infrared Backgrounds. II. Compton-Thick AGN Abundance
• The impact of temperature fluctuations on the large-scale clustering of the Ly$\alpha$ forest
• The link between star-formation and supermassive black hole properties
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Bow Ties in the Sky II: Searching for Gamma-ray Halos in the Fermi Sky Using Anisotropy
• SDSS-IV MaNGA: The Incidence of Major Mergers in type I and II AGN Host Galaxies in the DR15 sample
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• Searching for gravitational waves via Doppler tracking by future missions to Uranus and Neptune
• Lyman-alpha emitters as tracers of the transitioning Universe
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• Evolution of Supermassive Black Holes from Cosmological Simulations
• A low-luminosity type-1 QSO sample: II. Tracing circumnuclear star formation in HE 1029-1831 with SINFONI
• The mid-IR Luminosity Function at z<0.3 from 5MUSES: Understanding the Star-formation/AGN Balance from a Spectroscopic View
• Infrared Imaging of SDSS Quasars: Implications for the Quasar K correction
• The Clustering of Undetected High-redshift Black Holes and Their Signatures in Cosmic Backgrounds
• AGNs at the cosmic dawn: predictions for future surveys from a $\Lambda$CDM cosmological model
• The infrared-luminous progenitors of high-z quasars
• Mapping the low surface brightness Universe in the UV band with Lya emission from IGM filaments
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Active Galactic Nuclei Selected from GALEX Spectroscopy: The Ionizing Source Spectrum at z~1
• Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys
• Unveiling the inner morphology and gas kinematics of NGC 5135 with ALMA
• The role of AGN jets in the reionization epoch
• A low-luminosity type-1 QSO sample. V. Overluminous host spheroids and their excitation mechanisms
• Proof of CMB-driven X-ray brightening of high-z radio galaxies
• Do current X-ray observations capture most of the black-hole accretion at high redshifts?
• Semi-numeric simulations of helium reionization and the fluctuating radiation background
• The incidence of AGN in galaxies with different stellar population ages
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• Quasar UV Luminosity Function at $3.5<z<5.0$ from SDSS Deep Imaging Data
• Determination of supermassive black hole spins in local active galactic nuclei
• The growth of supermassive black holes fed by accretion disks
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• Episodic activities of supermassive black holes at redshift $z\le 2$: driven by mergers?
• The Star Formation and Nuclear Accretion Histories of Normal Galaxies in the AGES Survey
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• A Mid-infrared Flare in the Active Galaxy MCG-02-04-026: Dust Echo of a Nuclear Transient Event
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Resolving the nano-Hz gravitational wave sky: the detectability of eccentric binaries with PTA experiments
• The Impact of the CMB on the Evolution of high-z Blazars
• No black holes from light
• Detecting the Orbital Motion of Nearby Supermassive Black Hole Binaries with Gaia
• Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared
• Optically faint X-ray sources in the CDFN: Spitzer constraints
• Constraints on the X-ray Luminosity Function of AGN at z=5.7-6.4 with the Extragalactic Serendipitous Swift Survey
• Jets, black holes and disks in blazars
• The Highest-Energy Cosmic Rays Cannot be Dominantly Protons from Steady Sources
• The Mid-Infrared Luminosity Evolution and Luminosity Function of Quasars with SDSS and WISE
• CDFS-6664: A candidate of Lyman-continuum Emission at z~3.8 detected by HDUV
• Non-parametric Reconstruction of Photon Escape Fraction from Reionization
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Constraining the contribution of Seyfert galaxies to the diffuse neutrino flux in light of point source observations
• The Evolution of the Low-Frequency Radio AGN Population to $z\simeq 1.5$ in the ELAIS N1 Field
• AGN jets versus accretion as reionization sources
• On the Evolution of High-Redshift Active Galactic Nuclei
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• Optical Selection of Faint AGN in the COSMOS Field
• Combined constraints on intergalactic dust from quasar colours and the soft X-ray background
• Finding of a population of active galactic nuclei showing a significant luminosity decline in the past $\sim 10^{3-4}$ yrs
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• Spatial Correlations in the Helium-Ionizing Background
• The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena
• Dark matter halos and the M-σrelation for supermassive black holes
• Upper Limit on Dimming of Cosmological Sources by Intergalactic Grey Dust from the Soft X-ray Background
• Carbon ionization states and the cosmic far-UV background with HeII absorption
• Sub-Eddington super-massive black hole activity in Fornax early type galaxies
• On the Mean Radiative Efficiency of Accreting Massive Black Holes in AGNs And QSOs
• Unveiling the 100 pc scale nuclear radio structure of NGC 6217 with e-MERLIN and the VLA
• The Circumgalactic Medium of Submillimeter Galaxies. II. Unobscured QSOs within Dusty Starbursts and QSO Sightlines with Impact Parameters below 100 Kiloparsec
• On merger bias and the clustering of quasars
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• Probing the roles of orientation and multi-scale gas distributions in shaping the obscuration of Active Galactic Nuclei through cosmic time
• The WiggleZ Dark Energy Survey: Star-formation in UV-luminous galaxies from their luminosity functions
• Growth and anisotropy of ionization fronts near high redshift quasars in the MassiveBlack simulation
• Supermassive Black Holes: Connecting the Growth to the Cosmic Star Formation Rate
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Accretion History of AGN: Estimating the Host Galaxy Properties in X-ray Luminous AGN from z=0-3
• Evidence for cosmic evolution in the spin of the most massive black holes
• Fundamental Physics and Cosmology with TianQin
• COSMOS2020: Investigating the AGN-obscured accretion phase at $z\sim 1$ via [NeV] selection
• Fundamental properties of Fanaroff-Riley II radio galaxies investigated via Monte Carlo simulations
• Evidence of a fraction of LIGO/Virgo/KAGRA events coming from active galactic nuclei
• Geometric Distances of Quasars Measured by Spectroastrometry and Reverberation Mapping:Monte Carlo Simulations
• Growth of massive black holes at their late stage
• Structure of the super-Eddington outflow and itsimpact on the cosmological scale
• The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX) II. Luminosity Function
• Rapidly spinning massive black holes in active galactic nuclei: evidence from the black hole mass function
• Evolution of black hole and galaxy growth in a semi-numerical galaxy formation model
• A Sample Bias in Quasar Variability Studies
• Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
• Contribution of Flares from Tidal Disruption of Stars to high-redshift AGN
• Unresolved z~8 point sources and their impact on the bright end of the galaxy luminosity function
• Unveiling the solution to the final-parsec problem by combining milli-Hertz gravitational-wave observation and AGN survey
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• Molecular Gas Heating and Modified Dust Properties in Active Galaxies: Growing Black Holes or Tidal Shocks?
• Astrophysics with the Laser Interferometer Space Antenna
• Observations of Ly$\alpha$ Emitters at High Redshift
• Realistic consecutive galaxy mergers form eccentric PTA sources
• Modelling radio luminosity functions of radio-loud AGN by the cosmological evolution of supermassive black holes
• Coalescence Rate of Supermassive Black Hole Binaries Derived from Cosmological Simulations: Detection Rates for LISA and ET
• The Complex X-ray Obscuration Environment in the Radio Loud Type 2 Quasar 3C 223
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES): II enhanced nuclear accretion rate in galaxy groups at z$\sim$0.2
• Prospects for detecting cosmic filaments in Lyman-alpha emission across redshifts $z=2-5$
• Accretion mediated spin-eccentricity correlations in LISA massive black hole binaries
• Reionization Models Classifier using 21cm Map Deep Learning
• HeII Ly$\alpha$ Transmission Spikes and Absorption Troughs in Eight High-resolution Spectra Probing the End of HeII Reionization
• Detecting quasars at very high redshift with next generation X-ray telescopes
• Estimating black hole masses in young radio sources using CFHT spectroscopy
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• Rest-Frame Ultraviolet to Near Infrared Observations of an Interacting Lyman Break Galaxy at z = 4.42
• Ultraviolet background fluctuations with clustered sources
• CGM cloud sizes from refractive FRB scattering
• Using Machine Learning to Determine Morphologies of $z<1$ AGN Host Galaxies in the Hyper Suprime-Cam Wide Survey
• The luminosity function of TDEs from fallback-powered emission: implications for the black hole mass function
• A Complete 16 micron-Selected Galaxy Sample at $z\sim 1$: Mid-infrared Spectral Energy Distributions
• X-ray absorption in Compton-thin AGN: the predictions of a model revisited
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Detection of eccentric close-binary supermassive black holes with incomplete interferometric data
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• The PAU Survey: The quasar UV and Ly$\alpha$ luminosity functions at $2.7<z<5.3$
• Early Growth of Massive Black Holes in Quasars
• Estimate of SMBH Spin for Narrow-Line Seyfert 1 Galaxies
• Learning Transient Universe in Near-Ultraviolet By Wide-angle Cameras
• Scattering of emission lines in galaxy cluster cores: measuring electron temperature
• Newly born extragalactic millisecond pulsars as efficient emitters of PeV neutrinos
• Seeking Neutrino Emission from AGN through Temporal and Spatial Cross Correlation
• Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency
• Constraining blazar heating with the 2<z<3 Lyman-$\alpha$ forest
• Measuring photo-ionization rate and mean free path of HeII ionizing photons at $2.5\le z\le 3.6$: Evidence for late and rapid HeII reionization Part-II
• Automatic Machine Learning Framework to Study Morphological Parameters of AGN Host Galaxies within $z<1.4$ in the Hyper Supreme-Cam Wide Survey
• The distant red galaxy neighbour population of 1 < z < 2 QSOs and optically obscured sources
• Probing AGN with spectropolarimetry: accretion disk and SMBH parameters
• Identifying massive black hole binaries via light curve variability in optical time-domain surveys
• Method for Determining AGN Accretion Phase in Field Galaxies
• Constraining $z\lesssim 2$ ultraviolet emission with the upcoming ULTRASAT satellite
• Determination of the Physical Parameters of AGNs in Seyfert 1 Galaxies LEDA 3095839 and VII Zw 244 Based on Spectropolarimetric Observations
• Spins of SMBHs in distant low luminosity AGNs
• Diffuse flux of PeV neutrinos from centrifugally accelerated protons in active galactic nuclei
• Helium reionization in the presence of self-annihilating clumpy dark matter
• Cosmological Evolution of Supermassive Black Holes: Mass Functions and Spins
• Disk evolution of the M87's nucleus observed in 2008
• Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation
• X-ray luminosity functions of different morphological and X-ray type AGN populations
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Tidal disruption event rates across cosmic time: forecasts for LSST, Roman, and JWST and their constraints on the supermassive black hole mass function
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• PHL 6625: A Minor Merger-Associated QSO Behind NGC 247
• AGN variability in the age of VRO
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• On the non-evolution of the dependence of black hole masses on bolometric luminosities for QSOs
• Identification of high-redshift X-ray active galactic nuclei in the 4XMM-DR11 serendipitous catalogue using DES data: Comparative analysis with optically-selected QSOs
• Estimating the spins of supermassive black holes in distant ultraluminous quasars
• BASS XXX: Distribution Functions of DR2 Eddington-ratios, Black Hole Masses, and X-ray Luminosities
• Fast and optimal nonparametric sequential design for astronomical observations
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• Revisiting Disk Winds in Active Galactic Nuclei as an Origin of Cosmic Gamma-ray and Neutrino Backgrounds
• Exploiting the IRT-THESEUS capability to observe lensed Quasars
• Detectability of a spatial correlation between stellar-mass black hole mergers and Active Galactic Nuclei in the Local Universe
• The clustering of simulated quasars
• Ultra-luminous high-redshift quasars from SkyMapper -- II. New quasars and the bright end of the luminosity function
• The Drivers of the Decline in Supermassive Black Hole Growth at $z<2$
• A multiwavelength study of near- and mid-infrared selected galaxies at high redshift: ERGs, AGN-identification and the contribution from dust
• Solving the multi-messenger puzzle of the AGN-starburst composite galaxy NGC 1068