The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies

Abstract

We simulate the growth of galaxies and their central supermassive black holes by implementing a suite of semi-analytic models on the output of the Millennium Run, a very large simulation of the concordance LCDM cosmogony. Our procedures follow the detailed assembly history of each object and are able to track the evolution of all galaxies more massive than the Small Magellanic Cloud throughout a volume comparable to that of large modern redshift surveys. In this first paper we supplement previous treatments of the growth and activity of central black holes with a new model for `radio' feedback from those AGN that lie at the centre of a quasistatic X-ray emitting atmosphere in a galaxy group or cluster. We show that for energetically and observationally plausible parameters such a model can simultaneously explain: (i) the low observed mass drop-out rate in cooling flows; (ii) the exponential cut-off at the bright end of the galaxy luminosity function; and (iii) the fact that the most massive galaxies tend to be bulge-dominated systems in clusters and to contain systematically older stars than lower mass galaxies. This success occurs because static hot atmospheres form only in the most massive structures, and radio feedback (in contrast, for example, to supernova or starburst feedback) can suppress further cooling and star formation without itself requiring star formation. We discuss possible physical models which might explain the accretion rate scalings required for our phenomenological `radio mode' model to be successful.

21 pages, 12 figures, accepted MNRAS, Millennium Run semi-analytic galaxy catalogues are available for download at http://www.mpa-garching.mpg.de/galform/agnpaper (~9 million galaxies brighter than -17.4 in r), mini Millennium Run catalogues also available for testing purposes

References in corpus (82)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Stellar population synthesis at the resolution of 2003
• The Global Schmidt Law in Star Forming Galaxies
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• The Demography of Massive Dark Objects in Galaxy Centres
• Cosmological parameters from SDSS and WMAP
• The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
• Energy input from quasars regulates the growth and activity of black holes and their host galaxies
• Populating a cluster of galaxies - I. Results at z=0
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• How Do Galaxies Get Their Gas?
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Modeling feedback from stars and black holes in galaxy mergers
• The Formation of Galactic Disks
• The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
• High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• Hierarchical Galaxy Formation
• The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
• Gasdynamics and Starbursts in Major Mergers
• GADGET: A code for collisionless and gasdynamical cosmological simulations
• On the Black Hole Mass - Bulge Mass Relation
• New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
• Quantifying the bimodal color-magnitude distribution of galaxies
• A Unified Model for the Evolution of Galaxies and Quasars
• Virial shocks in galactic haloes?
• Semi-Analytic Modelling of Galaxy Formation: The Local Universe
• Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
• Clustering of Galaxies in a Hierarchical Universe: I. Methods and Results at z=0
• The 2dF Galaxy Redshift Survey: Near Infrared Galaxy Luminosity Functions
• A Survey of z>5.8 Quasars in the Sloan Digital Sky Survey I: Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z~6
• Observational constraints on growth of massive black holes
• A universal angular momentum profile for galactic halos
• What Shapes the Luminosity Function of Galaxies?
• A Recipe for Galaxy Formation Shaun Cole
• The Baryonic Tully-Fisher Relation
• Effect of Reionization on the Structure Formation in the Universe
• A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
• The Nature of High-Redshift Galaxies
• Chandra X-ray Observations of the Hydra A Cluster: An Interaction Between the Radio Source and the X-Ray-Emitting Gas
• A deep Chandra observation of the Perseus cluster: shocks and ripples
• The tumultuous lives of galactic dwarfs and the missing satellites problem
• The history of star formation in a LCDM universe
• X-ray Imaging Spectroscopy of Abell 1835
• Dark Matter Halos within Clusters
• Primordial Nucleosynthesis: Theory and Observations
• The 2dF Galaxy Redshift Survey: The b_J-band galaxy luminosity function and survey selection function
• Properties of Galactic Outflows: Measurements of the Feedback from Star Formation
• The Effects of Photoionization on Galaxy Formation - II: Satellites in the Local Group
• Chemical enrichment of the intra-cluster and intergalactic medium in a hierarchical galaxy formation model
• X-ray Spectroscopy of the Cluster of Galaxies Abell 1795 with XMM-Newton
• A Review of Bondi--Hoyle--Lyttleton Accretion
• Cooling Flows as a Calorimeter of AGN Mechanical Power
• The Metallicity-Luminosity Relation, Effective Yields, and Metal Loss in Spiral and Irregular Galaxies
• Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra
• The 2dF Galaxy Redshift Survey: Galaxy luminosity functions per spectral type
• GALICS I: A hybrid N-body semi-analytic model of hierarchical galaxy formation
• A Massive X-Ray Outflow from the Quasar PDS 456
• Supermassive Black Holes in Elliptical Galaxies: Switching from Very Bright to Very Dim
• Hot Bubbles from Active Galactic Nuclei as a Heat Source in Cooling Flow Clusters
• Heating cooling flows with jets
• Disk galaxies at Z=0 and at High Redshift: an explanation of the observed evolution of damped Ly-alpha systems
• Heating, conduction and minimum temperatures in cooling flows
• The anti-hierarchical growth of supermassive black holes
• Squelched Galaxies and Dark Halos
• Likelihood Analysis of Cosmic Shear on Simulated and VIRMOS-DESCART Data
• Keck Hires Observations of the QSO First J104459.6+365605: Evidence for a Large Scale Outflow
• A New Parallel N-body Gravity Solver: TPM
• HST STIS Observations of PG 0946+301: the Highest Quality UV Spectrum of a BALQSO
• The K-band Hubble diagram for the brightest cluster galaxies: a test of hierarchical galaxy formation models
• Generating Hot Gas in Simulations of Disk-Galaxy Major Mergers
• Simple models of cooling flows
• The Hawaii-AAO K-band Galaxy Redshift Survey -- Paper I: The Local K-band Luminosity Function
• Gas cooling in simulations of the formation of the galaxy population
• The Tully-Fisher Relation and H_not
• Fuelling quasars with hot gas
• Hydrodynamic Simulations of Galaxy Formation. I. Dissipation and the Maximum Mass of Galaxies
• The Tree-Particle-Mesh N-body Gravity Solver
• A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
• Precision Cosmology from the Lyman-alpha Forest: Power Spectrum and Bispectrum

Cited by in corpus (2875)

• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Observational Evidence of AGN Feedback
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
• Simulating Galaxy Formation with the IllustrisTNG Model
• The Aquarius Project: the subhalos of galactic halos
• A Unified, Merger-Driven Model for the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes and Galaxy Spheroids
• UV Star Formation Rates in the Local Universe
• The hierarchical formation of the brightest cluster galaxies
• The reversal of the star formation-density relation in the distant universe
• Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
• First results from the IllustrisTNG simulations: the galaxy color bimodality
• Hot Accretion Flows Around Black Holes
• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• Galactic star formation and accretion histories from matching galaxies to dark matter haloes
• Physical Models of Galaxy Formation in a Cosmological Framework
• Heating Hot Atmospheres with Active Galactic Nuclei
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
• UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
• From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
• Constraints on the relationship between stellar mass and halo mass at low and high redshift
• Cosmological Parameters from Observations of Galaxy Clusters
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation
• The Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria
• Simba: Cosmological Simulations with Black Hole Growth and Feedback
• An Observational Determination of the Bolometric Quasar Luminosity Function
• Cool Gas in High Redshift Galaxies
• Galaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
• The formation history of elliptical galaxies
• First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
• Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
• A model for cosmological simulations of galaxy formation physics
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• Massive Molecular Outflows and Evidence for AGN Feedback from CO Observations
• Resolving Cosmic Structure Formation with the Millennium-II Simulation
• Galaxy bimodality versus stellar mass and environment
• A unified model for AGN feedback in cosmological simulations of structure formation
• Dancing in the dark: galactic properties trace spin swings along the cosmic web
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
• The physics driving the cosmic star formation history
• The Growth of Massive Galaxies Since z=2
• The Two Phases of Galaxy Formation
• The Connection between Galaxies and their Dark Matter Halos
• Dusty Star-Forming Galaxies at High Redshift
• Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity
• Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• The large-scale structure of the Universe
• Observational evidence for AGN feedback in early-type galaxies
• Galaxies in a simulated $\Lambda$CDM Universe I: cold mode and hot cores
• Different star formation laws for disks versus starbursts at low and high redshifts
• How do galaxies populate Dark Matter halos?
• Theoretical Challenges in Galaxy Formation
• The Atlas3D project - XX. Mass-size and mass-sigma distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function
• 3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope
• Galaxy Stellar Mass Assembly between 0.2<z<2 from the S-COSMOS survey
• De Re Metallica: The cosmic chemical evolution of galaxies
• On the fundamental dichotomy in the local radio-AGN population: accretion, evolution, and host galaxy properties
• Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
• The RAVE Survey: Constraining the Local Galactic Escape Speed
• The Mass Assembly History of Field Galaxies: Detection of an Evolving Mass Limit for Star Forming Galaxies
• The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• Galaxy Zoo: the dependence of morphology and colour on environment
• Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
• The Sydney-AAO Multi-object Integral field spectrograph (SAMI)
• What Drives the Growth of Black Holes?
• Dwarf Galaxies with Optical Signatures of Active Massive Black Holes
• Galactic stellar haloes in the CDM model
• A Steep Faint-End Slope of the UV Luminosity Function at z~2-3: Implications for the Global Stellar Mass Density and Star Formation in Low Mass Halos
• Direct cosmological simulations of the growth of black holes and galaxies
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Quasar Feedback: More Bang for Your Buck
• How Do Disks Survive Mergers?
• UV Luminosity Functions from 132 z~7 and z~8 Lyman-Break Galaxies in the ultra-deep HUDF09 and wide-area ERS WFC3/IR Observations
• A primer on hierarchical galaxy formation: the semi-analytical approach
• New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy-galaxy lensing, clustering, and stellar mass functions from z=0.2 to z=1
• Self-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency
• The relation between accretion rate and jet power in X-ray luminous elliptical galaxies
• Physical properties and environments of nearby galaxies
• An Analytic Model for the Evolution of the Stellar, Gas, and Metal Content of Galaxies
• Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs
• Connecting Galaxies, Halos, and Star Formation Rates Across Cosmic Time
• Structure and Kinematics of Early-Type Galaxies from Integral-Field Spectroscopy
• The Horizon-AGN simulation: morphological diversity of galaxies promoted by AGN feedback
• Feedback and Recycled Wind Accretion: Assembling the z=0 Galaxy Mass Function
• The Evolution of Galaxy Structure over Cosmic Time
• A relationship between AGN jet power and radio power
• Supermassive black holes and their feedback effects in the IllustrisTNG simulation
• Structure and star formation in galaxies out to z=3: evidence for surface density dependent evolution and upsizing
• The Evolution of the Star-forming Interstellar Medium across Cosmic Time
• Advection-Dominated Accretion and the Black Hole Event Horizon
• Mergers and Bulge Formation in Lambda-CDM: Which Mergers Matter?
• Modelling the Galaxy Bimodality: Shutdown Above a Critical Halo Mass
• Evidence of strong quasar feedback in the early Universe
• The Origin and Evolution of the Galaxy Mass-Metallicity Relation
• The Major and Minor Galaxy Merger Rates at z < 1.5
• The UV-optical Galaxy Color-Magnitude Diagram I: Basic Properties
• A Stellar Mass Threshold for Quenching of Field Galaxies
• Chaotic cold accretion onto black holes
• EMU: Evolutionary Map of the Universe
• Galaxy Evolution in Cosmological Simulations with Outflows II: Metallicities and Gas Fractions
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• A unified multi-wavelength model of galaxy formation
• Mid-Infrared Selection of Active Galactic Nuclei with the Wide-Field Infrared Survey Explorer. II. Properties of WISE-Selected Active Galactic Nuclei in the NDWFS Boötes Field
• Dynamical Friction and Galaxy Merging Timescales
• New Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency
• Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4
• Distant Radio Galaxies and their Environments
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
• Science with ASKAP - the Australian Square Kilometre Array Pathfinder
• Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies
• The role of black holes in galaxy formation and evolution
• Hot and cold gas accretion and feedback in radio-loud active galaxies
• Dark matter and cosmic structure
• The distribution of stellar mass in the low-redshift Universe
• Radiative Efficiency and Content of Extragalactic Radio Sources: Toward a Universal Scaling Relation Between Jet Power and Radio Power
• Ages and metallicities of early-type galaxies in the SDSS: new insight into the physical origin of the colour-magnitude and the Mg2-sigmaV relations
• A White Paper on keV Sterile Neutrino Dark Matter
• The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release
• The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background
• The Many Manifestations of Downsizing: Hierarchical Galaxy Formation Models confront Observations
• Radiative feedback from massive black holes in elliptical galaxies. AGN flaring and central starburst fueled by recycled gas
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function at z < 0.06
• The Confinement of Star-Forming Galaxies into a Main Sequence through Episodes of Gas Compaction, Depletion, and Replenishment
• ZOBOV: a parameter-free void-finding algorithm
• On the cosmic evolution of the scaling relations between black holes and their host galaxies: Broad Line AGN in the zCOSMOS survey
• Galacticus: A Semi-Analytic Model of Galaxy Formation
• Self-regulated growth of supermassive black holes by a dual jet/heating AGN feedback mechanism: methods, tests and implications for cosmological simulations
• Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters
• The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
• The ACS Virgo Cluster Survey XV. The Formation Efficiencies of Globular Clusters in Early-Type Galaxies: The Effects of Mass and Environment
• Thermal Instability & the Feedback Regulation of Hot Halos in Clusters, Groups, and Galaxies
• Observations of Feedback from Radio-Quiet Quasars - II. Kinematics of Ionized Gas Nebulae
• The Role of Cold Flows in the Assembly of Galaxy Disks
• Eddington-limited accretion and the black hole mass function at redshift 6
• Galaxies at z~6: The UV Luminosity Function and Luminosity Density from 506 UDF, UDF-Ps, and GOODS i-dropouts
• Galaxy Formation Theory
• Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges
• The ATLAS${}^{3D}$ project - XXV: Two-dimensional kinematic analysis of simulated galaxies and the cosmological origin of fast and slow rotators
• Galaxy Evolution in Cosmological Simulations With Outflows I: Stellar Masses and Star Formation Rates
• Ray-tracing through the Millennium Simulation: Born corrections and lens-lens coupling in cosmic shear and galaxy-galaxy lensing
• Halo assembly bias and its effects on galaxy clustering
• Three years Swift-BAT Survey of AGN: reconciling theory and observations?
• MUFASA: Galaxy Formation Simulations With Meshless Hydrodynamics
• Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
• The Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs
• Galaxy Groups in the SDSS DR4: II. halo occupation statistics
• The Bolometric Quasar Luminosity Function at z = 0-7
• A physical model for cosmological simulations of galaxy formation: multi-epoch validation
• The accretion of galaxies into groups and clusters
• The Evolving Luminosity Function of Red Galaxies
• On the prevalence of radio-loud AGN in brightest cluster galaxies: implications for AGN heating of cooling flows
• Evidence for powerful AGN winds at high redshift: Dynamics of galactic outflows in radio galaxies during the "Quasar Era"
• Galaxy formation in WMAP1 and WMAP7 cosmologies
• Environment and self-regulation in galaxy formation
• Quantifying the effect of baryon physics on weak lensing tomography
• Inclination- and dust-corrected galaxy parameters: Bulge-to-disc ratios and size-luminosity relations
• The non-causal origin of the black hole-galaxy scaling relations
• Discovery of an AGN-Driven Molecular Outflow in the Local Early-Type Galaxy NGC 1266
• Cold dark matter heats up
• Evidence for Mature Bulges and an Inside-out Quenching Phase 3 Billion Years After the Big Bang
• A synthesis model for AGN evolution: supermassive black holes growth and feedback modes
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• The Colours of Satellite Galaxies in Groups and Clusters
• The star formation histories of galaxies in the Sloan Digital Sky Survey
• Feast and Famine: Regulation of Black Hole Growth in Low Redshift Galaxies
• A Link Between Star Formation Quenching and Inner Stellar Mass Density in SDSS Central Galaxies
• PRIMUS: The dependence of AGN accretion on host stellar mass and color
• Forming Compact Massive Galaxies
• The evolution of the star formation activity in galaxies and its dependence on environment
• The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyears. Evidence for a major build up of the red sequence between z=2 and z=1
• SDSS IV MaNGA - Metallicity and nitrogen abundance gradients in local galaxies
• What turns galaxies off? The different morphologies of star-forming and quiescent galaxies since z~2 from CANDELS
• The massive end of the luminosity and stellar mass functions: Dependence on the fit to the light profile
• A simplified view of blazars: clearing the fog around long-standing selection effects
• Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
• AGN-controlled cooling in elliptical galaxies
• Driving Outflows with Relativistic Jets and the Dependence of AGN Feedback Efficiency on ISM Inhomogeneity
• Satellite Kinematics III: Halo Masses of Central Galaxies in SDSS
• The mass evolution of the first galaxies: stellar mass functions and star formation rates at $4<z<7$ in the CANDELS GOODS-South field
• Evolution of Density Profiles in High-z Galaxies: Compaction and Quenching Inside-Out
• The Baryonic Assembly of Dark Matter Halos
• The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end
• Radio and Millimeter Continuum Surveys and their Astrophysical Implications
• Extreme gas kinematics in the z=2.2 powerful radio galaxy MRC1138-262: Evidence for efficient AGN feedback in the early Universe?
• GA-NIFS: A massive black hole in a low-metallicity AGN at $z\sim 5.55$ revealed by JWST/NIRSpec IFS
• The case for AGN feedback in galaxy groups
• z~7-10 Galaxies in the HUDF and GOODS fields, and their UV Luminosity Functions
• The Origin of Disks and Spheroids in Simulated Galaxies
• The impact of angular momentum on black hole accretion rates in simulations of galaxy formation
• Radio galaxies and feedback from AGN jets
• Dark matter and the early Universe: a review
• The Hubble Space Telescope Wide Field Camera 3 Early Release Science data: Panchromatic Faint Object Counts for 0.2-2 microns wavelength
• How Mergers May Affect The Mass Scaling Relations Between Black Holes, Galaxies, and Other Gravitationally Bound Systems
• AGN-driven quenching of star formation: morphological and dynamical implications for early-type galaxies
• A Revised Model for the Formation of Disk Galaxies: Low Spin and Dark-Halo Expansion
• The Current Status of Galaxy Formation
• Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8
• Physical properties of galactic winds using background quasars
• The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations
• The cosmic evolution of massive black holes in the Horizon-AGN simulation
• Angular momentum and galaxy formation revisited
• The Frequency of Tidal Features Associated with Nearby Luminous Elliptical Galaxies from a Statistically Complete Sample
• Towards a more realistic population of bright spiral galaxies in cosmological simulations
• The high redshift galaxy population in hierarchical galaxy formation models
• The Relation Between Quasar and Merging Galaxy Luminosity Functions and the Merger-Induced Star Formation Rate of the Universe
• Grand unification of AGN activity in the LambdaCDM cosmology
• The Greater Impact of Mergers on the Growth of Massive Galaxies: Implications for Mass Assembly and Evolution Since z~1
• The evolution of massive black holes and their spins in their galactic hosts
• The effect of radiation pressure on virial black hole mass estimates and the case of Narrow Line Seyfert 1 galaxies
• The (black hole mass)-(host spheroid luminosity) relation at high and low masses, the quadratic growth of black holes, and intermediate-mass black hole candidates
• Feedback from Central Black Holes in Elliptical Galaxies: Two-dimensional Models Compared to One-dimensional Models
• A universal structural and star-forming relation since $z\sim 3$: connecting compact star-forming and quiescent galaxies
• The Megamaser Cosmology Project. III. Accurate Masses of Seven Supermassive Black Holes in Active Galaxies with Circumnuclear Megamaser Disks
• Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results
• The Milky Way: An Exceptionally Quiet Galaxy; Implications for the formation of spiral galaxies
• Natural Downsizing in Hierarchical Galaxy Formation
• Selection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation
• AEGIS: The color-magnitude relation for X-ray selected AGN
• Bulge mass is king: The dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey
• The Representative XMM-Newton Cluster Structure Survey (REXCESS) of an X-ray Luminosity Selected Galaxy Cluster Sample
• The DEEP2 Galaxy Redshift Survey: The Relationship Between Galaxy Properties and Environment at z ~ 1
• Relativistic jet feedback III: feedback on gas disks
• Dissipation and Extra Light in Galactic Nuclei: IV. Evolution in the Scaling Relations of Spheroids
• The Regulation of Cooling and Star Formation in Luminous Galaxies by AGN Feedback and the Cooling-Time/Entropy Threshold for the Onset of Star Formation
• A High Stellar Velocity Dispersion and ~100 Globular Clusters for the Ultra Diffuse Galaxy Dragonfly 44
• Galaxy Zoo: Passive Red Spirals
• Accreting SMBHs in the COSMOS field and the connection to their host galaxies
• Deep Spitzer 24mic COSMOS imaging -- I. The evolution of luminous dusty galaxies - Confronting the models
• Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1
• Galaxies-Intergalactic Medium Interaction Calculation --I. Galaxy formation as a function of large-scale environment
• Precise Black Hole Masses From Megamaser Disks: Black Hole-Bulge Relations at Low Mass
• UV/Optical Detections of Candidate Tidal Disruption Events by GALEX and CFHTLS
• The Effect of Mass Ratio on the Morphology and Time-scales of Disc Galaxy Mergers
• Shark: introducing an open source, free and flexible semi-analytic model of galaxy formation
• Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations
• An Entropy Threshold for Strong H-alpha and Radio Emission in the Cores of Galaxy Clusters
• Cosmic evolution of the atomic and molecular gas content of galaxies
• The COSMOS-WIRCam near-infrared imaging survey: I: BzK selected passive and star forming galaxy candidates at z>1.4
• Gemini Near-infrared Spectroscopy of Luminous z~6 Quasars: Chemical Abundances, Black Hole Masses, and MgII Absorption
• Jet-induced star formation in gas-rich galaxies
• The Luminosity Function of Fermi-detected Flat-Spectrum Radio Quasars
• Fast outflows in compact radio sources: evidence for AGN-induced feedback in the early stages of radio source evolution
• Equal- and unequal-mass mergers of disk and elliptical galaxies with black holes
• Ubiquitous seeding of supermassive black holes by direct collapse
• The Galaxy-Halo Connection Over The Last 13.3 Gyrs
• The MORGANA model for the rise of galaxies and active nuclei
• The Galaxy Content of SDSS Clusters and Groups
• Masses for the Local Group and the Milky Way
• The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
• Quasar Clustering from SDSS DR5: Dependences on Physical Properties
• MaxBCG: A Red Sequence Galaxy Cluster Finder
• The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey
• The dramatic size evolution of elliptical galaxies and the quasar feedback
• Galaxy Properties from the Ultra-violet to the Far-Infrared: Lambda-CDM models confront observations
• Compact steep-spectrum and peaked-spectrum radio sources
• The relation between metallicity, stellar mass and star formation in galaxies: an analysis of observational and model data
• Feedback and metal enrichment in cosmological SPH simulations - II. A multiphase model with supernova energy feedback
• Near infrared spectroscopy and star-formation histories of 3<z<4 quiescent galaxies
• Ongoing and co-evolving star formation in zCOSMOS galaxies hosting Active Galactic Nuclei
• Mergers in Lambda-CDM: Uncertainties in Theoretical Predictions and Interpretations of the Merger Rate
• The DEEP2 Galaxy Redshift Survey: Color and Luminosity Dependence of Galaxy Clustering at z~1
• Galaxy-Induced Transformation of Dark Matter Halos
• Galaxy growth in the concordance $\Lambda$CDM cosmology
• How stellar feedback simultaneously regulates star formation and drives outflows
• Simulations of the galaxy population constrained by observations from z=3 to the present day: implications for galactic winds and the fate of their ejecta
• Black hole evolution: I. Supernova-regulated black hole growth
• Spatially-Resolved Spectroscopic Properties of Low-Redshift Star-Forming Galaxies
• Blossoms from black hole seeds: properties and early growth regulated by supernova feedback
• Feedback in Luminous Obscured Quasars
• On the Correlations between Galaxy Properties and Supermassive Black Hole Mass
• Measuring the kinetic power of AGN in the radio mode
• The Hierarchical Build-Up of Massive Galaxies and the Intracluster Light since z=1
• Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
• Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters
• Discovery of extreme [OIII]5007A outflows in high-redshift red quasars
• A New Diagnostic of Active Galactic Nuclei: Revealing Highly-Absorbed Systems at Redshift>0.3
• A Large Population of Massive Compact Post-Starburst Galaxies at z>1: Implications for the Size Evolution and Quenching Mechanism of Quiescent Galaxies
• The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history
• Dependence of Galaxy Quenching on Halo Mass and Distance from its Centre
• Stellar masses of SDSS-III BOSS galaxies at z~0.5 and constraints to galaxy formation models
• An Over-Massive Black Hole in the Compact Lenticular Galaxy NGC1277
• Relativistic jet feedback in high-redshift galaxies I: Dynamics
• The clustering of intermediate redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey
• MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II - Star Formation Histories and Galaxy Quenching
• Energy Feedback from X-ray Binaries in the Early Universe
• Galaxies in a Simulated $\Lambda$CDM Universe II: Observable Properties and Constraints on Feedback
• Evidence for Wide-Spread AGN Driven Outflows in the Most Massive z~1-2 Star Forming Galaxies
• Feedback from Active Galactic Nuclei: Energy- versus momentum-driving
• On the galaxy stellar mass function, the mass-metallicity relation, and the implied baryonic mass function
• The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
• Energetic galaxy-wide outflows in high-redshift ultra-luminous infrared galaxies hosting AGN activity
• The Galaxy and its stellar halo: insights on their formation from a hybrid cosmological approach
• Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects: A Millimetre/Submillimetre Probe of the Warm and Hot Universe
• The Effects of Gas on Morphological Transformation in Mergers: Implications for Bulge and Disk Demographics
• Using the Fundamental Plane of Black Hole Activity to Distinguish X-ray Processes from Weakly Accreting Black Holes
• The STAGES view of red spirals and dusty red galaxies: Mass-dependent quenching of star-formation in cluster infall
• The Era of Star Formation in Galaxy Clusters
• COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation Since z~3 from new Wide Field WFC3 Imaging Combined with CANDELS/3DHST
• The LoTSS view of radio AGN in the local Universe. The most massive galaxies are always switched on
• The DEEP2 Galaxy Redshift Survey: Evolution of the Color-Density Relation at 0.4 < z < 1.35
• The KMOS^3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6 - 2.7
• Do Hot Haloes Around Galaxies Contain the Missing Baryons?
• Spectroscopic Identification of Massive Galaxies at z~2.3 with Strongly Suppressed Star Formation
• Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z\sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg${}^2$ Sky
• The Aspen--Amsterdam Void Finder Comparison Project
• Star Formation in Semi-Analytic Galaxy Formation Models with Multiphase Gas
• A calibration of the relation between the abundance of close galaxy pairs and the rate of galaxy mergers
• Bursting and Quenching in Massive Galaxies without Major Mergers or AGNs
• The suppression of star formation by powerful active galactic nuclei
• Stellar and Quasar Feedback in Concert: Effects on AGN Accretion, Obscuration, and Outflows
• Simulations of Cosmic Chemical Enrichment
• Tracking the impact of environment on the Galaxy Stellar Mass Function up to z~1 in the 10k zCOSMOS sample
• The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3
• Galactic accretion and the outer structure of galaxies in the CDM model
• Inspiralling Supermassive Black Holes: A New Signpost for Galaxy Mergers
• Galaxy Morphology and Star Formation in the Illustris Simulation at z=0
• The SDSS-III Baryon Oscillation Spectroscopic Survey: The Quasar Luminosity Function from Data Release Nine
• Mass Distribution in Galaxy Clusters: the Role of AGN Feedback
• Are Brightest Halo Galaxies Central Galaxies?
• Gravitational Quenching in Massive Galaxies and Clusters by Clumpy Accretion
• Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source population
• The Rise and Fall of Passive Disk Galaxies: Morphological Evolution Along the Red Sequence Revealed by COSMOS
• Cosmic ray feedback in hydrodynamical simulations of galaxy formation
• Suppressing star formation in quiescent galaxies with supermassive black hole winds
• Hydrodynamical simulations of cluster formation with central AGN heating
• The Blast Wave Model for AGN Feedback: Effects on AGN Obscuration
• Evolution of the atomic and molecular gas content of galaxies
• Moving mesh cosmology: numerical techniques and global statistics
• The VLT LEGA-C Spectroscopic Survey: The Physics of Galaxies at a Lookback Time of 7 Gyr
• What are Protoclusters? -- Defining High Redshift Galaxy Clusters and Protoclusters
• Energy, momentum and mass outflows and feedback from thick accretion discs around rotating black holes
• Observations of Feedback from Radio-Quiet Quasars: I. Extents and Morphologies of Ionized Gas Nebulae
• The faint radio sky: radio astronomy becomes mainstream
• The Prevalence of Gas Outflows in Type 2 AGNs
• The Evolution of Swift/BAT blazars and the origin of the MeV background
• The LABOCA Survey of the Extended Chandra Deep Field South: Clustering of submillimetre galaxies
• The SINS/zC-SINF survey of z~2 galaxy kinematics: Evidence for powerful AGN-driven nuclear outflows in massive star-forming galaxies
• Color-Magnitude Relations of Active and Non-Active Galaxies in the Chandra Deep Fields: High-Redshift Constraints and Stellar-Mass Selection Effects
• Half of the Most Luminous Quasars May Be Obscured: Investigating the Nature of WISE-Selected Hot, Dust-Obscured Galaxies
• Tracing the cosmic growth of super massive black holes to z ~ 3 with Herschel
• Evolution of Galaxies and their Environments at z = 0.1 to 3 in COSMOS
• The evolution of AGN across cosmic time: what is downsizing?
• Structure Finding in Cosmological Simulations: The State of Affairs
• ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433
• Properties of Galaxy Groups in the SDSS: II.- AGN Feedback and Star Formation Truncation
• Satellite Kinematics II: The Halo Mass-Luminosity Relation of Central Galaxies in SDSS
• Cosmic Evolution of Black Holes and Spheroids. I: The M_BH-sigma Relation at z=0.36
• A chronicle of galaxy mass assembly in the EAGLE simulation
• Evolution of the Color-Magnitude Relation in Galaxy Clusters at z ~1 from the ACS Intermediate Redshift Cluster Survey
• Quasar Luminosity Functions from Joint Evolution of Black Holes and Host Galaxies
• Linking the spin evolution of massive black holes to galaxy kinematics
• Red Galaxy Growth and the Halo Occupation Distribution
• A new model of galaxy formation: How sensitive are predicted galaxy luminosities to the choice of SPS model?
• Herschel-ATLAS Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies
• The Missing Massive Satellites of the Milky Way
• The WIRCam Deep Survey I: Counts, colours and mass-functions derived from near-infrared imaging in the CFHTLS deep fields
• Simulation of the Cosmic Evolution of Atomic and Molecular Hydrogen in Galaxies
• FIRST-2MASS Red Quasars: Transitional Objects Emerging from the Dust
• CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies
• Radiative efficiency, variability and Bondi accretion onto massive black holes: from mechanical to quasar feedback in brightest cluster galaxies
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z$\lesssim$6
• The Correlation of Star Formation Quenching with Internal Galaxy Properties and Environment
• The evolution of star formation histories of quiescent galaxies
• The Demographics of Broad Line Quasars in the Mass-Luminosity Plane II. Black Hole Mass and Eddington Ratio Functions
• Global simulations of galactic winds including cosmic ray streaming
• Constraints on Black Hole Growth, Quasar Lifetimes, and Eddington Ratio Distributions from the SDSS Broad Line Quasar Black Hole Mass Function
• The Evolution of AGN Host Galaxies: From Blue to Red and the Influence of Large-Scale Structures
• The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations
• The Unorthodox Orbits of Substructure Halos
• Shaping the galaxy stellar mass function with supernova- and AGN-driven winds
• The dependence of Star Formation on Galaxy Stellar Mass
• A census of metals and baryons in stars in the local Universe
• The ACS Fornax Cluster Survey. I. Introduction to the Survey and Data Reduction Procedures
• Large Structures and Galaxy Evolution in COSMOS at z < 1.1
• Galaxy clustering in the CFHTLS-Wide: the changing relationship between galaxies and haloes since z ~ 1.2
• Comparing and calibrating black hole mass estimators for distant active galactic nuclei
• Dependence of Interstellar Turbulent Pressure on Supernova Rate
• The dark matter halos of massive, relaxed galaxy clusters observed with Chandra
• An Explanation for the Observed Weak Size Evolution of Disk Galaxies
• AGN heating and ICM cooling in the HIFLUGCS sample of galaxy clusters
• Gravitational-wave Limits from Pulsar Timing Constrain Supermassive Black Hole Evolution
• The physics and the structure of the quasar-driven outflow in Mrk 231
• An algorithm to build mock galaxy catalogues using MICE simulations
• Morphologies of z~0.7 AGN Host Galaxies in CANDELS: No trend of merger incidence with AGN luminosity
• The JWST Extragalactic Mock Catalog: Modeling galaxy populations from the UV through the near-IR over thirteen billion years of cosmic history
• Numerical modelling of the lobes of radio galaxies in cluster environments
• Mechanical AGN Feedback: Controlling the Thermodynamical Evolution of Elliptical Galaxies
• On Halo Formation Times and Assembly Bias
• Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
• Cosmic Evolution of Black Holes and Spheroids. II: Scaling Relations at z=0.36
• The HI content of star-forming galaxies at z = 0.24
• Jet-Powered Molecular Hydrogen Emission from Radio Galaxies
• The Morphologies of Massive Galaxies at 1<z<3 in the CANDELS-UDS Field: Compact Bulges, and the Rise and Fall of Massive Disks
• Radio-loud AGN in the first LoTSS data release: The lifetimes and environmental impact of jet-driven sources
• The SDSS DR6 Luminosity Functions of Galaxies
• Diagnostics of AGN-driven Molecular Outflows in ULIRGs from Herschel-PACS Observations of OH at 119um
• A direct measurement of the baryonic mass function of galaxies & implications for the galactic baryon fraction
• Do Moderate-Luminosity Active Galactic Nuclei Suppress Star Formation?
• Black hole evolution: III. Statistical properties of mass growth and spin evolution using large-scale hydrodynamical cosmological simulations
• A Mechanism for Stimulating AGN Feedback by Lifting Gas in Massive Galaxies
• Forming Early-Type Galaxies in LambdaCDM Simulations -I. Assembly histories
• Galaxy And Mass Assembly (GAMA): Galaxy close-pairs, mergers, and the future fate of stellar mass
• Modelling galaxy clustering in a high resolution simulation of structure formation
• Clustering of intermediate redshift quasars using the final SDSS III-BOSS sample
• A Re-examination of Galactic Conformity and a Comparison with Semi-analytic Models of Galaxy Formation
• The abundance of (not just) dark matter haloes
• The Rising Star-Formation Histories of Distant Galaxies and Implications for Gas Accretion with Time
• Every BCG with a strong radio AGN has an X-ray cool core: is the cool core - noncool core dichotomy too simple?
• Extreme AGN feedback in the Massive Cluster Survey (MACS): a detailed study of X-ray cavities at z > 0.3
• The 2dF-SDSS LRG and QSO survey: Evolution of the Luminosity Function of Luminous Red Galaxies to z=0.6
• What Shapes the Galaxy Mass Function? Exploring the Roles of Supernova-Driven Winds and AGN
• X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: Tracing the evolution of AGN feedback in clusters of galaxies out to z=1.2
• Essential physics of early galaxy formation
• The impact of feedback on cosmological gas accretion
• Effects of AGN feedback on LCDM galaxies
• The Kinematic Connection Between Galaxies and Dark Matter Haloes
• Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
• LOFAR/H-ATLAS: A deep low-frequency survey of the Herschel-ATLAS North Galactic Pole field
• Effect of local environment and stellar mass on galaxy quenching and morphology at $0.5<z<2.0$
• Angular Momentum Acquisition in Galaxy Halos
• Growing the first bright quasars in cosmological simulations of structure formation
• Evidence for AGN Feedback in Galaxy Clusters and Groups
• X-ray coronae in simulations of disc galaxy formation
• The impact of mechanical AGN feedback on the formation of massive early-type galaxies
• The origin of cold gas in giant elliptical galaxies and its role in fueling radio-mode AGN feedback
• Size Evolution of Spheroids in a Hierarchical Universe
• Predictions for ASKAP Neutral Hydrogen Surveys
• Building galaxies by accretion and in-situ star formation
• The Dawn of the Red: Star formation histories of group galaxies over the past 5 billion years
• Energetics of the molecular gas in the H_2 luminous radio galaxy 3C 326: Evidence for negative AGN feedback
• ALMA reveals the feeding of the Seyfert 1 nucleus in NGC 1566
• The Atomic to Molecular Transition and its Relation to the Scaling Properties of Galaxy Disks in the Local Universe
• The evolution of post-starburst galaxies from z=2 to z= 0.5
• The Properties and Prevalence of Galactic Outflows at z = 1 in the Extended Groth Strip
• The Spiderweb galaxy: a forming massive cluster galaxy at z~2
• On the Dearth of Compact, Massive, Red Sequence Galaxies in the Local Universe
• A fundamental problem in our understanding of low mass galaxy evolution
• Cosmic evolution of radio selected active galactic nuclei in the COSMOS field
• The evolution of active galactic nuclei and their spins
• Strong lensing optical depths in a \LambdaCDM universe
• Understanding the shape of the halo-mass and galaxy-mass cross-correlation functions
• The Impact of Feedback on Disk Galaxy Scaling Relations
• AEGIS: The Clustering of X-ray AGN Relative to Galaxies at z~1
• The baryon fraction of LambdaCDM haloes
• The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model
• Black Hole Growth in Hierarchical Galaxy Formation
• The Biases of Optical Line-Ratio Selection for Active Galactic Nuclei, and the Intrinsic Relationship between Black Hole Accretion and Galaxy Star Formation
• Disentangling satellite galaxy populations using orbit tracking in simulations
• A Stochastic Model for the Luminosity Fluctuations of Accreting Black Holes
• Feedback from central black holes in elliptical galaxies. I: models with either radiative or mechanical feedback but not both
• The Abundance of Distant and Extremely Red Galaxies: The Role of AGN Feedback in Hierarchical Models
• Cosmic evolution of stellar quenching by AGN feedback: clues from the Horizon-AGN simulation
• First Results from Z-FOURGE: Discovery of a Candidate Cluster at z = 2.2 in COSMOS
• The origin of fast molecular outflows in quasars: molecule formation in AGN-driven galactic winds
• AGN-driven outflows without immediate quenching in simulations of high-redshift disk galaxies
• Inside the Bondi radius of M87
• The DEEP2 galaxy redshift survey: the evolution of the blue fraction in groups and the field
• An XMM-Newton study of the environments, particle content and impact of low-power radio galaxies
• A Ten Billion Solar Mass Outflow of Molecular Gas Launched by Radio Bubbles in the Abell 1835 Brightest Cluster Galaxy
• Cosmic Evolution of Size and Velocity Dispersion for Early Type Galaxies
• How do central and satellite galaxies quench? -- Insights from spatially resolved spectroscopy in the MaNGA survey
• Classifying Radio Galaxies with Convolutional Neural Network
• The Different Physical Mechanisms that Drive the Star-Formation Histories of Giant and Dwarf Galaxies
• Early-type galaxies at large galactocentric radii - II. Metallicity gradients, and the [Z/H]--mass, [alpha/Fe]--mass relations
• The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space
• Suppression of star formation in early-type galaxies by feedback from supermassive black holes
• X-ray constraints on the local supermassive black hole occupation fraction
• Galaxy Merger Statistics and Inferred Bulge-to-Disk Ratios in Cosmological SPH Simulations
• The cold veil of the Milky Way stellar halo
• A new measurement of the evolving near-infrared galaxy luminosity function out to z~4: a continuing challenge to theoretical models of galaxy formation
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume
• Science with the TianQin observatory: Preliminary results on massive black hole binaries
• Low redshift AGN in the Hamburg/ESO Survey: II. The active black hole mass function and the distribution function of Eddington ratios
• The Luminosity Dependence of the Galaxy Merger Rate
• The population of Milky Way satellites in the LambdaCDM cosmology
• Science with a lunar low-frequency array: from the dark ages of the Universe to nearby exoplanets
• Evolution in the Halo Masses of Isolated Galaxies between z~1 and z~0: From DEEP2 to SDSS
• The Supermassive Black Hole Mass - Spheroid Stellar Mass Relation for Sérsic and Core-Sérsic Galaxies
• Recalibration of the virial factor and M-sigma relation for local active galaxies
• Galaxy And Mass Assembly: Deconstructing Bimodality - I. Red ones and blue ones
• From haloes to Galaxies - I. The dynamics of the gas regulator model and the implied cosmic sSFR history
• Satellite abundances around bright isolated galaxies
• SHARDS: an optical spectro-photometric survey of distant galaxies
• Ultra Fast Outflows: Galaxy-Scale Active Galactic Nucleus Feedback
• The VLA-COSMOS 3~GHz Large Project: Cosmic evolution of radio AGN and implications for radio-mode feedback since z~5
• The SAURON project - XV. Modes of star formation in early-type galaxies and the evolution of the red sequence
• The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
• Breaking the law: the M_{bh}-M_{spheroid} mass relations for core-Sersic and Sersic galaxies
• LoCuSS: The steady decline and slow quenching of star formation in cluster galaxies over the last four billion years
• Is AGN feedback necessary to form red elliptical galaxies?
• Evolution in the black hole mass-bulge mass relation: a theoretical perspective
• Star formation quenching in massive galaxies
• On the Origin of Stars in Bulges and Elliptical Galaxies
• Are galactic star formation and quenching governed by local, global or environmental phenomena?
• The VLA Survey of the Chandra Deep Field South. V. Evolution and Luminosity Functions of sub-mJy radio sources and the issue of radio emission in radio-quiet AGN
• The Star Formation Epoch of the Most Massive Early-Type Galaxies
• Impact of Cosmic Ray Transport on Galactic Winds
• Substructure of the galaxy clusters in the REXCESS sample: observed statistics and comparison to numerical simulations
• AGN Jet Kinetic Power and the Energy Budget of Radio Galaxy Lobes
• The role of mergers in driving morphological transformation over cosmic time
• Mapping stellar content to dark matter halos. II. Halo mass is the main driver of galaxy quenching
• Evolution of the Stellar-to-Dark Matter Relation: Separating Star-Forming and Passive Galaxies from z=1 to 0
• The formation and evolution of low-surface-brightness galaxies
• The clustering of narrow-line AGN in the local Universe
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function to $z=0.1$ from the r-band selected equatorial regions
• The virialized mass of dark matter haloes
• The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
• Key Science Goals for the Next-Generation Event Horizon Telescope
• The mass of the black hole in Centaurus A from SINFONI AO-assisted integral-field observations of stellar kinematics
• Surface density effects in quenching: cause or effect?
• Confronting theoretical models with the observed evolution of the galaxy population out to z=4
• Downsizing by Shutdown in Red Galaxies
• The Concentration Dependence of the Galaxy-Halo Connection: Modeling Assembly Bias with Abundance Matching
• Dark-ages reionization and galaxy formation simulation - III. Modelling galaxy formation and the epoch of reionization
• Virialization of the inner CGM in the FIRE simulations and implications for galaxy discs, star formation and feedback
• An X-ray survey of the 2Jy sample. I: is there an accretion mode dichotomy in radio-loud AGN?
• Feedback from Active Galactic Nuclei in Galaxy Groups
• Revealing velocity dispersion as the best indicator of a galaxy's color, compared to stellar mass, surface mass density or morphology
• Resolving the Discrepancy of Galaxy Merger Fraction Measurements at z ~ 0 - 3
• Chandra Survey of Nearby Highly-Inclined Disk Galaxies I: X-ray Measurements of Galactic Coronae
• Two Conditions for Galaxy Quenching: Compact Centres and Massive Haloes
• Are luminous radio-loud active galactic nuclei triggered by galaxy interactions?
• The XMM Cluster Survey: Active Galactic Nuclei and Starburst Galaxies in XMMXCS J2215.9-1738 at z=1.46
• AEGIS: New Evidence Linking Active Galactic Nuclei to the Quenching of Star Formation
• Color and stellar population gradients in galaxies. Correlation with mass
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• Chaotic cold accretion on to black holes in rotating atmospheres
• Modern yields per stellar generation: the effect of the IMF
• The density field of the 10k zCOSMOS galaxies
• Blowing cold flows away: the impact of early AGN activity on the formation of a brightest cluster galaxy progenitor
• Bulge-forming galaxies with an extended rotating disk at z~2
• AGN and Starburst Radio Emission from Optically Selected QSOs
• Mergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster Virial Radii
• The SL2S Galaxy-scale Lens Sample. II. Cosmic evolution of dark and luminous mass in early-type galaxies
• Smoothly-Rising Star Formation Histories During the Reionization Epoch
• Numerical Relativity and Astrophysics
• Cluster Galaxies Die Hard
• Cosmic rays can drive strong outflows from gas-rich high-redshift disk galaxies
• An optical group catalogue to z = 1 from the zCOSMOS 10k sample
• Are Radio AGN Powered by Accretion or Black Hole Spin?
• Stellar Ages and Metallicities of Central and Satellite Galaxies: Implications for Galaxy Formation and Evolution
• The duty cycle of local radio galaxies
• Radio Jets in Galaxies with Actively Accreting Black Holes: new insights from the SDSS
• The Argo Simulation: I. Quenching of Massive Galaxies at High Redshift as a Result of Cosmological Starvation
• The Properties of Galaxies in Voids
• Parametrizing the Stellar Haloes of Galaxies
• Suppression of Star Formation in NGC 1266
• Searching for Evidence of Energetic Feedback in Distant Galaxies: A Galaxy Wide Outflow in a z~2 Ultraluminous Infrared Galaxy
• The IMACS Cluster Building Survey: IV. The Log-normal Star Formation History of Galaxies
• The Chandra Deep Protocluster Survey: Ly-alpha Blobs are powered by heating, not cooling
• The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
• Supermassive black holes in the EAGLE Universe. Revealing the observables of their growth
• Quenching star formation with quasar outflows launched by trapped IR radiation
• The 2dF-SDSS LRG and QSO survey: evolution of the clustering of luminous red galaxies since z = 0.6
• The evolution of the brightest cluster galaxies since z~1 from the ESO Distant Cluster Survey (EDisCS)
• A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole
• The (black hole)-bulge mass scaling relation at low masses
• The main sequence of star forming galaxies I. The local relation and its bending
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: I. BH scaling relations and the AGN luminosity function
• The Growth of Massive Black Holes in Galaxy Merger Simulations with Feedback by Radiation Pressure
• How to quench a galaxy
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• Ages and Abundances of Red Sequence Galaxies as a Function of LINER Emission Line Strength
• Synthetic Spectra from PIC Simulations of Relativistic Collisionless Shocks
• Orbital structure of merger remnants: Trends with gas fraction in 1:1 mergers
• Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach
• Interactions, star formation and AGN activity
• The mass-metallicity gradient relation of early-type galaxies
• Galaxy-Scale Outflows Driven by Active Galactic Nuclei
• A massive, dead disk galaxy in the early Universe
• Adding Environmental Gas Physics to the Semi-Analytic Method for Galaxy Formation: Gravitational Heating
• On the origin of radio-loudness in AGNs and its relationship with the properties of the central supermassive black hole
• The Next Generation Fornax Survey (NGFS): II. The Central Dwarf Galaxy Population
• The Evolution of Central Group Galaxies in Hydrodynamical Simulations
• M87 at metre wavelengths: the LOFAR picture
• Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift
• Fast Hamiltonian sampling for large scale structure inference
• What Does Clustering Tell Us About the Buildup of the Red Sequence?
• A consistent measure of the merger histories of massive galaxies using close-pair statistics I: Major mergers at $z<3.5$
• The Energetics and Lifetimes of Local Radio Active Galactic Nuclei
• The local radio-galaxy population at 20 GHz
• Observational Evidence for the Co-evolution of Galaxy Mergers, Quasars, and the Blue/Red Galaxy Transition
• The cosmic evolution of radio-AGN feedback to z=1
• Driving massive molecular gas flows in central cluster galaxies with AGN feedback
• The stellar population histories of early-type galaxies. III. The Coma Cluster
• Stellar mass functions: methods, systematics and results for the local Universe
• Widespread and Hidden Active Galactic Nuclei in Star-Forming Galaxies at Redshift > 0.3
• The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?
• Galaxy morphology in the LambdaCDM cosmology
• First Results from the 3D-HST Survey: The Striking Diversity of Massive Galaxies at z>1
• Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{\ast ,sph}$ and $M_{BH}$-$M_{\ast ,gal}$
• Simulating the physical properties of dark matter and gas inside the cosmic web
• The Substructure Hierarchy in Dark Matter Haloes
• New Chandra observations of the jet in 3C273. I. Softer X-ray than radio spectra and the X-ray emission mechanism
• Evolution of the Most Massive Galaxies to z=0.6: I. A New Method for Physical Parameter Estimation
• Mergers, Starbursts, and Quenching in the Simba Simulation
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). A precise measurement of the galaxy stellar mass function and the abundance of massive galaxies at redshifts 0.5<z<1.3
• AGN self-regulation in cooling flow clusters
• The Dependence of Galaxy Morphology and Structure on Environment and Stellar Mass
• The Origins of AGN Obscuration: The 'Torus' as a Dynamical, Unstable Driver of Accretion
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• Bar quenching in gas-rich galaxies
• AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
• Satellite quenching timescales in clusters from projected phase space measurements matched to simulated orbits
• Modelling Element Abundances in Semi-analytic Models of Galaxy Formation
• Black Hole-Galaxy Correlations without Self-Regulation
• Radio imaging of the Subaru/XMM-Newton Deep Field - III. Evolution of the radio luminosity function beyond z=1
• The ATLAS3D project - XXII. Low-efficiency star formation in early-type galaxies: hydrodynamic models and observations
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• Hot gas in massive halos drives both mass quenching and environment quenching
• Gas Infall and Stochastic Star Formation in Galaxies in the Local Universe
• A Spectacular H$\alpha$ Complex in Virgo: Evidence for a Collision Between M86 and NGC 4438 and Implications for Collisional ISM Heating of Ellipticals
• The drop in the cosmic star formation rate below redshift 2 is caused by a change in the mode of gas accretion and by AGN feedback
• Evolution of spiral galaxies in modified gravity
• Dissecting the Red Sequence - III. Mass-to-Light Variations in 3D Fundamental Plane Space
• A Bayesian approach to the semi-analytic model of galaxy formation: methodology
• The link between the assembly of the inner dark matter halo and the angular momentum evolution of galaxies in the EAGLE simulation
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• Satellites of Simulated Galaxies: survival, merging, and their relation to the dark and stellar halos
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• From Starburst to Quiescence: Testing AGN feedback in Rapidly Quenching Post-Starburst Galaxies
• Halo masses for optically-selected and for radio-loud AGN from clustering and galaxy-galaxy lensing
• Evolution of the Radio Loud Galaxy Population
• Updated Mass Scaling Relations for Nuclear Star Clusters and a Comparison to Supermassive Black Holes
• The Demography of Super-Massive Black Holes: Growing Monsters at the Heart of Galaxies
• Host galaxy morphologies of X-ray selected AGN: assessing the significance of different black hole fueling mechanisms to the accretion density of the Universe at z~1
• An Alternative Origin for Hypervelocity Stars
• AGN feedback works both ways
• The zCOSMOS 20k Group Catalog
• The radial distribution of galaxies in groups and clusters
• The Cosmic Decline in the H2/HI-Ratio in Galaxies
• The Starburst in the Abell 1835 Cluster Central Galaxy: A Case Study of Galaxy Formation Regulated by an Outburst from a Supermassive Black Hole
• Modelling galaxy clustering: halo occupation distribution versus subhalo matching
• SDSS Galaxy Clustering: Luminosity & Colour Dependence and Stochasticity
• Metal-rich multi-phase gas in M87: AGN-driven metal transport, magnetic-field supported multi-temperature gas, and constraints on non-thermal emission observed with XMM-Newton
• The X-ray Jets of Active Galaxies
• Linking black-hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution
• Disentangling galaxy environment and host halo mass
• AEGIS: The Morphologies of Green Galaxies at 0.4<z<1.2
• The duty cycle of radio-mode feedback in complete samples of clusters
• The Rest-Frame Optical Luminosity Function of Cluster Galaxies at z<0.8 and the Assembly of the Cluster Red Sequence
• Revisiting the "Fundamental Plane" of Black Hole Activity at Extremely Low Luminosities
• Radio Sources in Galaxy Clusters: Radial Distribution, and 1.4 GHz and K-band Bivariate Luminosity Function
• Diffuse stellar component in galaxy clusters and the evolution of the most massive galaxies at z<~1
• Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2
• The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies
• Quenching as a Contest between Galaxy Halos and their Central Black Holes
• The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $\Lambda$CDM
• On the puzzling plateau in the specific star formation rate at z=2-7
• Kiloparsec Scale Properties of Star-Formation Driven Outflows at z~2.3 in the SINS/zC-SINF AO Survey
• Star Formation and Metallicity Gradients in Semi-analytic Models of Disk Galaxy Formation
• Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?
• The Co-Formation of Spheroids and Quasars Traced in their Clustering
• The role of AGN in the colour transformation of galaxies at redshifts z~1
• Massive black hole merger rates: the effect of kpc separation wandering and supernova feedback
• Peak star formation efficiency and no missing baryons in massive spirals
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• Molecular outflow and feedback in the obscured Quasar XID2028 revealed by ALMA
• Spitzer bright, UltraVISTA faint sources in COSMOS: the contribution to the overall population of massive galaxies at z=3-7
• Prospects for observing extreme-mass-ratio inspirals with LISA
• Measuring the Average Evolution of Luminous Galaxies at z<3: The Rest-frame Optical Luminosity Density, Spectral Energy Distribution, and Stellar Mass Density
• Multi-dimensional modelling of X-ray spectra for AGN accretion-disk outflows
• Direct Evidence for Termination of Obscured Star Formation by Radiatively Driven Outflows in Reddened QSOs
• On the Origin of the Galaxy Star-Formation-Rate Sequence: Evolution and Scatter
• The VIPERS Multi-Lambda Survey. II. Diving with massive galaxies in 22 square degrees since z = 1.5
• Narrow associated QSO absorbers: clustering, outflows and the line-of-sight proximity effect
• Specific star-formation and the relation to stellar mass from 0<z<2 as seen in the far-infrared at 70 and 160mu
• LCDM predictions for galaxy protoclusters I: the relation between galaxies, protoclusters and quasars at z~6
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• On the nature of the Milky Way satellites
• Galaxy And Mass Assembly (GAMA): Linking Star Formation Histories and Stellar Mass Growth
• SDSS IV MaNGA - The spatially resolved transition from star formation to quiescence
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: II. The clustering of quasars and their dark environment
• Galaxy evolution in the infra-red: comparison of a hierarchical galaxy formation model with SPITZER data
• How is Star Formation Quenched in Massive Galaxies?
• Superclusters of galaxies from the 2dF redshift survey. I. The catalogue
• Fast and slow paths to quiescence: ages and sizes of 400 quiescent galaxies from the LEGA-C survey
• Jekyll & Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang
• A Swift survey of accretion onto stellar-mass black holes
• Spatially resolved star formation and fuelling in galaxy interactions
• The real-space clustering of luminous red galaxies around z<0.6 quasars in the Sloan Digital Sky Survey
• Mergers Do Trigger AGNs out to z $\sim$ 0.6
• The Mass Assembly of Fossil Groups of Galaxies in the Millennium Simulation
• Hot Atmospheres, Cold Gas, AGN Feedback and the Evolution of Early Type Galaxies: a Topical Perspective
• Black Hole Mass Scaling Relations for Spiral Galaxies. I. $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{sph}}$
• Galaxy bulges and their massive black holes: a review
• The WiggleZ Dark Energy Survey: High Resolution Kinematics of Luminous Star-Forming Galaxies
• Decreased Specific Star Formation Rates in AGN Host Galaxies
• Galactic chemical evolution in hierarchical formation models - I. Early-type galaxies in the local Universe
• The evolution of the cold interstellar medium in galaxies following a starburst
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• Not too big, not too small: the dark halos of the dwarf spheroidals in the Milky Way
• Does a 'stochastic' background of gravitational waves exist in the pulsar timing band?
• The multiphase gas structure and kinematics in the circumnuclear region of NGC 5728
• A Simple Model for Quasar Demographics
• Line Emission in the Brightest Cluster Galaxies of the NOAO Fundamental Plane and Sloan Digital Sky Surveys
• Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
• AGN feedback: galactic-scale outflows driven by radiation pressure on dust
• NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
• The properties of the extended warm ionised gas around low-redshift QSOs and the lack of extended high-velocity outflows
• A Spatially Resolved Map of the Kinematics, Star-Formation and Stellar Mass Assembly in a Star-Forming Galaxy at z=4.9
• Unravelling the complex structure of AGN-driven outflows: I. Kinematics and sizes
• Radio Continuum Surveys with Square Kilometre Array Pathfinders
• Strong lensing optical depths in a LCDM universe II: the influence of the stellar mass in galaxies
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• The unexpectedly large dust and gas content of quiescent galaxies at z>1.4
• A correlation between central supermassive black holes and the globular cluster systems of early-type galaxies
• The Star Formation Demographics of Galaxies in the Local Volume
• Revealing the galaxy-halo connection in IllustrisTNG
• Quiescence correlates strongly with directly-measured black hole mass in central galaxies
• Galaxy bulges and their black holes: a requirement for the quenching of star formation
• Weak Lensing by Galaxies in Groups and Clusters: I.--Theoretical Expectations
• ALMA observations of cold molecular gas filaments trailing rising radio bubbles in PKS0745-191
• The massive black hole-velocity dispersion relation and the halo baryon fraction: a case for positive AGN feedback
• The Growth in Size and Mass of Cluster Galaxies since z=2
• Galaxy-scale Star Formation on the Red Sequence: the Continued Growth of S0s and the Quiescence of Ellipticals
• The radio AGN population dichotomy: Green valley Seyferts versus red sequence low-excitation AGN
• AGN host galaxy mass function in COSMOS: is AGN feedback responsible for the mass-quenching of galaxies?
• The evolution of Black Hole scaling relations in galaxy mergers
• Optical Emission Line Nebulae in Galaxy Cluster Cores 1: The Morphological, Kinematic and Spectral Properties of the Sample
• The Luminosity Function of high-redshift QSOs - A combined analysis of GOODS and SDSS
• Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations
• Ongoing Formation of Bulges and Black Holes in the Local Universe: New Insights from GALEX
• ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster
• Outflowing Galactic Winds in Post-starburst and AGN Host Galaxies at 0.2<z<0.8
• IFU observations of luminous type II AGN - I. Evidence for ubiquitous winds
• The Rest Frame Ultraviolet Spectra of UV-Selected Active Galactic Nuclei at z ~ 2-3
• Direct observational evidence for a large transient galaxy population in groups at 0.85<z<1
• The Hot Gas Content of Low-Luminosity Early-Type Galaxies and the Implications Regarding Supernova Heating and AGN Feedback
• Feedback under the microscope II: heating, gas uplift, and mixing in the nearest cluster core
• Scaling Relations of Dwarf Galaxies without Supernova-Driven Winds
• Colours, Star formation Rates, and Environments of Star forming and Quiescent Galaxies at the Cosmic Noon
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• Systematic infrared 2.5-5 micron spectroscopy of nearby ultraluminous infrared galaxies with AKARI
• The X-ray luminosity function of Active Galactic Nuclei in the redshift interval z=3-5
• Insight Into the Formation of the Milky Way Through Cold Halo Substructure. I. The ECHOS of Milky Way Formation
• Star Formation Signatures in Optically Quiescent Early-type Galaxies
• AGN are cooler than you think: the intrinsic far-IR emission from QSOs
• Recovering Redshift Distributions with Cross-Correlations: Pushing The Boundaries
• A Relationship between Supermassive Black Hole Mass and the Total Gravitational Mass of the Host Galaxy
• A review of elliptical and disc galaxy structure, and modern scaling laws
• Supermassive black holes as the regulators of star formation in central galaxies
• The 60-month all-sky BAT Survey of AGN and the Anisotropy of Nearby AGN
• The subhalo - satellite connection and the fate of disrupted satellite galaxies
• Erratum - The many lives of AGN: cooling flows, black holes and the luminosities and colours of galaxies
• Galaxies hosting an AGN: a view from the CALIFA survey
• Faraday Rotation Structure on Kiloparsec Scales in the Giant Radio Lobes of Centaurus A
• Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
• Studying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2
• Galaxy Formation Spanning Cosmic History
• The scale of homogeneity of the galaxy distribution in SDSS DR6
• Improved Models for Cosmic Infrared Background Anisotropies: New Constraints on the IR Galaxy Population
• An Energetic AGN Outburst Powered by a Rapidly Spinning Supermassive Black Hole or an Accreting Ultramassive Black Hole
• A Comprehensive Study of the Radio Properties of Brightest Cluster Galaxies
• Hot gas halos around disk galaxies: Confronting cosmological simulations with observations
• Supermassive Black Holes in the Hierarchical Universe: A General Framework and Observational Tests
• Spitzer Observations of the Brightest Galaxies in X-ray-Luminous Clusters
• Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
• A Systematic Search for X-ray Cavities in the Hot Gas of Galaxy Groups
• The gentle monster PDS 456: the kpc scale molecular outflow and its implications for QSO feedback
• New Constraints on the Efficiencies of Ram-Pressure Stripping and the Tidal Disruption of Satellite Galaxies
• Populating the galaxy velocity dispersion - supermassive black hole mass diagram: A catalogue of (M_bh, sigma) values
• The Growth of Red Sequence Galaxies in a Cosmological Hydrodynamic Simulation
• Radio galaxies in the 2SLAQ Luminous Red Galaxy Survey: I. The evolution of low-power radio galaxies to z~0.7
• A Virtual Sky with Extragalactic HI and CO Lines for the SKA and ALMA
• Color and Stellar Population Gradients in Passively Evolving Galaxies at z~2 from HST/WFC3 Deep Imaging in the Hubble Ultra Deep Field
• A simple model to link the properties of quasars to the properties of dark matter halos out to high redshift
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• Alignment between galaxies and large-scale structure
• The route to massive black hole formation via merger-driven direct collapse: a review
• Galaxy gas as obscurer: II. Separating the galaxy-scale and nuclear obscurers of Active Galactic Nuclei
• A comprehensive and uniform sample of broad-line active galactic nuclei from the SDSS DR7
• Extended Lyman alpha emission around bright quasars
• The Self-Regulated Growth of Supermassive Black Holes
• Galaxy-galaxy lensing constraints on the relation between baryons and dark matter in galaxies in the Red Sequence Cluster Survey 2
• The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations
• Destruction of Molecular Gas Reservoirs in Early-Type Galaxies by Active Galactic Nucleus Feedback
• The triggering probability of radio-loud AGN: A comparison of high and low excitation radio galaxies in hosts of different colors
• The diverse cold molecular gas contents, morphologies, and kinematics of type-2 quasars as seen by ALMA
• Connecting stellar mass and star-formation rate to dark matter halo mass out to z ~ 2
• The M_BH - M_star relation for X-ray obscured, red QSOs at 1.2< z <2.6
• Spectral ageing in the lobes of cluster-centre FR-II radio galaxies
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• Toward a comprehensive model for feedback by active galactic nuclei: new insights from M87 observations by LOFAR, Fermi and H.E.S.S
• Black Holes in the Early Universe
• Galaxy Cluster Mass Reconstruction Project: II. Quantifying scatter and bias using contrasting mock catalogues
• The impact of radio feedback from active galactic nuclei in cosmological simulations: Formation of disk galaxies
• The mass assembly of galaxy groups and the evolution of the magnitude gap
• The Origin of the Intrinsic Scatter in the Relation Between Black Hole Mass and Bulge Luminosity for Nearby Active Galaxies
• How do galaxies acquire their mass?
• H${}_2$-based star formation laws in hierarchical models of galaxy formation
• GAMA/WiggleZ: The 1.4GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z=0.75
• Observational Evidence for an Age Dependence of Halo Bias
• Connection Between Stellar Mass Distributions Within Galaxies and Quenching Since z =2
• Torque-Limited Growth of Massive Black Holes in Galaxies Across Cosmic Time
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• What is the (Dark) Matter with Dwarf Galaxies?
• Reconstructing the cosmic density field with the distribution of dark matter halos
• Black-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation Rate
• Galaxy Cluster Mass Reconstruction Project: I. Methods and first results on galaxy-based techniques
• Ionised gas outflow signatures in SDSS-IV MaNGA active galactic nuclei
• Connecting massive galaxies to dark matter halos in BOSS - I. Is galaxy color a stochastic process in high-mass halos?
• The Gemini Deep Deep Survey: VIII. When Did Early-type Galaxies Form?
• Spitzer mid-IR spectroscopy of powerful 2Jy and 3CRR radio galaxies. I. Evidence against a strong starburst-AGN connection in radio-loud AGN
• The most luminous quasars do not live in the most massive dark matter haloes at any redshift
• Selection effects in the black hole-bulge relation and its evolution
• Hyper Suprime-Cam Subaru Strategic Program: A Mass-Dependent Slope of the Galaxy Size-Mass Relation at $z<1$
• CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2
• Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies
• Mid-infrared Properties and Color Selection for X-ray Detected AGN in the MUSYC ECDF-S field
• AEGIS: The Nature of the Host Galaxies of Low-ionization Outflows at z < 0.6
• Black Hole -- Galaxy Correlations in Simba
• Conduction and the Star-Formation Threshold in Brightest Cluster Galaxies
• LoCuSS: Connecting the Dominance and Shape of Brightest Cluster Galaxies with the Assembly History of Massive Clusters
• The effects of a hot gaseous halo in galaxy major mergers
• Tidal dwarf galaxies in the nearby Universe
• Star Formation Shut Down by Multiphase Gas Outflow in a Galaxy at a Redshift of 2.45
• Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF
• Satellite abundances around bright isolated galaxies II: radial distribution and environmental effects
• Testing the binary hypothesis: pulsar timing constraints on supermassive black hole binary candidates
• Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes. I: Feedback-regulated Star Formation and Black Hole Growth
• Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering
• Is there an upper limit to black hole masses?
• Environmental Dependence of Galaxy Merger Rate in ΛCDM Universe
• The rapid growth phase of supermassive black holes
• The Population of High Redshift AGNs in the Chandra COSMOS survey
• Large-scale outflows in luminous QSOs revisited: The impact of beam smearing on AGN feedback efficiencies
• Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Sizes and Kinematics of Extended Narrow-Line Regions in Luminous Obscured AGN Selected by Broadband Images
• GASP III. JO36: a case of multiple environmental effects at play?
• Fast cold gas in hot AGN outflows
• The Mid-IR and X-ray Selected QSO Luminosity Function
• Isotropic AGN Heating with Small Radio Quiet Bubbles in the NGC 5044 Group
• Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS
• LoCuSS: A Dynamical Analysis of X-ray AGN in Local Clusters
• The Rise and Fall of Galaxy Activity in Dark Matter Haloes
• Dissecting and Modelling Galaxy Assembly Bias
• Prediction of the Cosmic Evolution of the CO-Luminosity Functions
• Clustering of Radio Galaxies and Quasars
• Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
• The Effect of Environment on the Formation of Halpha Filaments and Cool Cores in Galaxy Groups and Clusters
• Satellite Galaxies and Fossil Groups in the Millennium Simulation
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• Models for jet power in elliptical galaxies: A case for rapidly spinning black holes
• A dynamical model of supernova feedback: gas outflows from the interstellar medium
• The Ubiquitous Radio Continuum Emission from the Most Massive Early-Type Galaxies
• LLAMA: Normal star formation efficiencies of molecular gas in the centres of luminous Seyfert galaxies
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): A quiescent formation of massive red-sequence galaxies over the past 9 Gyr
• The location and impact of jet-driven outflows of cold gas: the case of 3C293
• Delayed or no feedback? - Gas outflows in Type 2 AGNs. III
• Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the last 10 Gyr
• Quenching Massive Galaxies with On-the-fly Feedback in Cosmological Hydrodynamic Simulations
• A clear and measurable signature of modified gravity in the galaxy velocity field
• Starburst-AGN mixing: II. Optically-selected active galaxies
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• Baryon Cycling in the Low-Redshift Circumgalactic Medium: A Comparison of Simulations to the COS-Halos Survey
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• Ultraviolet through Infrared Spectral Energy Distributions from 1000 SDSS Galaxies: Dust Attenuation
• Dwarf galaxy populations in present-day galaxy clusters: I. Abundances and red fractions
• The MOSDEF survey: a census of AGN-driven ionized outflows at $z=1.4-3.8$
• Dust-Corrected Colors Reveal Bimodality in AGN Host Galaxy Colors at z~1
• Determination of masses of the central black holes in NGC524 and NGC2549 using Laser Guide Star Adaptive Optics
• Which AGN Jets Quench Star Formation in Massive Galaxies?
• The optically unbiased GRB host (TOUGH) survey. VI. Radio observations at z<1 and consistency with typical star-forming galaxies
• The spatially resolved star formation history of CALIFA galaxies: Cosmic time scales
• The orientation of galaxy dark matter haloes around cosmic voids
• Pahs, Ionized Gas, and Molecular Hydrogen in Brightest Cluster Galaxies of Cool Core Clusters of Galaxies
• On the interdependence of galaxy morphology, star formation, and environment in massive galaxies in the nearby Universe
• Reconstructing Redshift Distributions with Cross-Correlations: Tests and an Optimized Recipe
• ALMA observations of molecular clouds in three group centered elliptical galaxies: NGC 5846, NGC 4636, and NGC 5044
• Origins and Demographics of Wandering Black Holes
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• Global star formation revisited
• Herschel far-infrared photometry of the Swift Burst Alert Telescope active galactic nuclei sample of the local universe - III. Global star-forming properties and the lack of a connection to nuclear activity
• Bondi flow from a slowly rotating hot atmosphere
• The Origin of Line Emission in Massive z~2.3 Galaxies: Evidence for Cosmic Downsizing of AGN Host Galaxies
• The ages, metallicities and star formation histories of early-type galaxies in SDSS
• Anisotropic Locations of Satellite Galaxies: Clues to the Orientations of Galaxies within their Dark Matter Halos
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• On the self-regulation of intense star-formation in galaxies at z=1-3
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design, Data Processing, and Spectral Analysis Methods
• A 10,000-solar-mass black hole in the nucleus of a bulgeless dwarf galaxy
• MAGIICAT III. Interpreting Self-Similarity of the Circumgalactic Medium with Virial Mass using MgII Absorption
• Energy- and momentum-conserving AGN feedback outflows
• Active Galactic Nuclei in Void Regions
• AGN feedback in dwarf galaxies?
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• MultiDark-Galaxies: data release and first results
• Ram pressure stripping in a galaxy formation model. I. A novel numerical approach
• The link between accretion mode and environment in radio-loud active galaxies
• Energy flows in thick accretion disks and their consequences for black hole feedback
• Galaxy Zoo: Bulgeless Galaxies With Growing Black Holes
• Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
• How robust are predictions of galaxy clustering?
• Feedback in low-mass galaxies in the early Universe
• The mass and angular momentum distribution of simulated massive early-type galaxies to large radii
• Dust scaling relations in a cosmological simulation
• Precipitation-Regulated Star Formation in Galaxies
• The 10k zCOSMOS: morphological transformation of galaxies in the group environment since z~1
• Stellar feedback as the origin of an extended molecular outflow in a starburst galaxy
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• The Halo Occupation Distribution of SDSS Quasars
• The cosmic star formation rate evolution from z=5 to z=0 from the VIMOS VLT Deep Survey
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• Massive Compact Galaxies with High-Velocity Outflows: Morphological Analysis and Constraints on AGN Activity
• Galaxy morphology, kinematics and clustering in a hydrodynamic simulation of a LambdaCDM universe
• The Evolution of Assembly Bias
• MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z=2.2
• $\text{Herschel}$-ATLAS:The connection between star formation and AGN activity in radio-loud and radio-quiet active galaxies
• The colour of galaxies in distant groups
• A Comparative Analysis of the Supernova Legacy Survey Sample with ΛCDM and the $R_{\mathrm{h}}=ct$ Universe
• On the observed distributions of black hole masses and Eddington ratios from radiation pressure corrected virial indicators
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• The Rise of Massive Red Galaxies: the color-magnitude and color-stellar mass diagrams for z < ~2 from the MUltiwavelength Survey by Yale-Chile (MUSYC)
• Insights into formation scenarios of massive Early-Type galaxies from spatially resolved stellar population analysis in CALIFA
• The Limited Impact of Outflows: Integral-Field Spectroscopy of 20 Local AGNs
• The long gamma-ray burst rate and the correlation with host galaxy properties
• Disk Growth and Quenching
• A Census of Gas Outflows in Type 2 Active Galactic Nuclei
• JWST Reveals Widespread AGN-Driven Neutral Gas Outflows in Massive z ~ 2 Galaxies
• ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
• Galactic Archaeology with Gaia
• Heavily Obscured AGN in Star-Forming Galaxies at z~2
• Properties of the galaxy population in hydrodynamical simulations of clusters
• A z=2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments
• Molecular Gas Contents and Scaling Relations for Massive Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
• The statistical properties of LCDM halo formation
• Quenching timescales of galaxies in the EAGLE simulations
• The XMM Cluster Survey: The interplay between the brightest cluster galaxy and the intra-cluster medium via AGN feedback
• Regulation of Black Hole Winds and Jets Across the Mass Scale
• Revealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratios
• Eight-Dimensional Mid-Infrared/Optical Bayesian Quasar Selection
• The luminosity-dependent high-redshift turnover in the steep spectrum radio luminosity function: clear evidence for downsizing in the radio-AGN population
• The first detection of near-infrared CN bands in active galactic nuclei: signature of star formation
• Galaxy Formation in WDM Cosmology
• The mid-life crisis of the Milky Way and M31
• Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
• Faint Submillimeter Galaxies Revealed by Multifield Deep ALMA Observations: Number Counts, Spatial Clustering, and A Dark Submillimeter Line Emitter
• Dark-ages Reionization and Galaxy Formation Simulation - X. The small contribution of quasars to reionization
• Quasar Black Hole Mass Estimates in the Era of Time Domain Astronomy
• The WISSH QSOs project IX. Cold gas content and environment of luminous QSOs at z~2.4-4.7
• Return to [Log-]Normalcy: Rethinking Quenching, The Star Formation Main Sequence, and Perhaps Much More
• CANDELS Observations of the Environmental Dependence of the Color-Mass-Morphology Relation at z = 1.6
• The Chandra survey of the COSMOS field II: source detection and photometry
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
• Dissecting the Evolution of Dark Matter Subhaloes in the Bolshoi Simulation
• A Total Molecular Gas Mass Census in z~2-3 Star-forming Galaxies: Low-J CO Excitation Probes of Galaxies' Evolutionary States
• Close entrainment of massive molecular gas flows by radio bubbles in the central galaxy of Abell 1795
• The spatially-resolved star formation histories of CALIFA galaxies: Implications for galaxy formation
• Mini-quenching of $z=4-8$ galaxies by bursty star formation
• SDSS-IV MaNGA: Inside-out vs. outside-in quenching in different local environments
• The Sphericalization of Dark Matter Halos by Galaxy Disks
• Mass assembly of galaxies: Smooth accretion versus mergers
• X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations
• Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5
• The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
• The Stellar Populations of Lyman Break Galaxies at z~5
• Near-ultraviolet Spectroscopy of Star-forming Galaxies from eBOSS: Signatures of Ubiquitous Galactic-scale Outflows
• Radio-Quiet Quasars in the VIDEO Survey: Evidence for AGN-powered radio emission at S_1.4GHz < 1 mJy
• Metal mixing by buoyant bubbles in galaxy clusters
• The Different Environmental Dependencies of Star-formation for Giant and Dwarf Galaxies
• Quasars: What turns them off?
• Suppression of electron thermal conduction in the high $\beta$ intracluster medium of galaxy clusters
• The Chandra-COSMOS survey IV: X-ray spectra of the bright sample
• An Empirical Model for the Star Formation History in Dark Matter Halos
• GMASS Ultradeep Spectroscopy of Galaxies at redshift z~2. I. The stellar metallicity
• ALMA captures feeding and feedback from the active galactic nucleus in NGC613
• The Close AGN Reference Survey (CARS). A massive multi-phase outflow impacting the edge-on galaxy HE1353-1917
• The Accretion Disc Particle Method for Simulations of Black Hole Feeding and Feedback
• The Mass Assembly History of Spheroidal Galaxies: Did Newly-Formed Systems Arise Via Major Mergers?
• The Mass of the Black Hole in Arp 151 from Bayesian Modeling of Reverberation Mapping Data
• Stellar Kinematics in the Complicated Inner Spheroid of M31: Discovery of Substructure Along the Southeastern Minor Axis and its Relationship to the Giant Southern Stream
• The X-ray Properties of Early-Type Galaxies in the Extended Chandra Deep Field-South
• Bayesian inference of galaxy formation from the K-band luminosity function of galaxies: tensions between theory and observation
• Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN
• The clustering of radio galaxies at z~0.55 from the 2SLAQ LRG survey
• Galaxy Zoo: Are Bars Responsible for the Feeding of Active Galactic Nuclei at 0.2 < z < 1.0?
• LOFAR discovery of a 700-kpc remnant radio galaxy at low redshift
• An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
• Painting galaxies into dark matter halos using machine learning
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• The X-ray luminous cluster underlying the bright radio-quiet quasar H1821+643
• Dark-matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions
• Galaxy And Mass Assembly (GAMA): The dependence of the galaxy luminosity function on environment, redshift and colour
• Mass Functions of Supermassive Black Holes Across Cosmic Time
• The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
• Hydrodynamical simulations of Galactic fountains II: evolution of multiple fountains
• RAiSE III: 3C radio AGN energetics and composition
• The Millennium Galaxy Catalogue: The $M_{bh}$--$L_{spheroid}$ derived supermassive black hole mass function
• The VIMOS Ultra Deep Survey: The reversal of the star-formation rate $-$ density relation at $2<z<5$
• Rapid Coeval Black Hole and Host Galaxy Growth in MRC 1138-262: The Hungry Spider
• A Spectroscopic Survey of Faint Quasars in the SDSS Deep Stripe: I. Preliminary Results from the Co-added Catalog
• The MASSIVE survey - XI. What drives the molecular gas properties of early-type galaxies
• Reproducing the assembly of massive galaxies within the hierarchical cosmogony
• Herschel-ATLAS: The link between accretion luminosity and star formation in quasar host galaxies
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• Tidal Disruption of Satellite Galaxies in a Semi-Analytic Model of Galaxy Formation
• Tracing outflows in the AGN forbidden region with SINFONI
• A mass threshold for galactic gas discs by spin flips
• Galaxy Zoo: building the low-mass end of the red sequence with local post-starburst galaxies
• Clustering, Bias and the Accretion Mode of X-ray selected AGN
• Why Are AGN and Host Galaxies Misaligned?
• Preventing Star Formation in Early-Type Galaxies with Late-Time Stellar Heating
• Galaxy Groups in the 2dFGRS: the number density of groups
• On ths assembly history of stellar components in massive galaxies
• Multi-phase feedback processes in the Sy2 galaxy NGC 5643
• The influence of environment on satellite galaxies in the GAEA semi-analytic model
• The duty cycle of radio galaxies revealed by LOFAR: remnant and restarted radio source populations in the Lockman Hole
• Toward precise constraints on growth of massive black holes
• Chandra Observations of Nuclear Outflows in the Elliptical Galaxy NGC4552 in the Virgo Cluster
• LOFAR-Boötes: Properties of high- and low-excitation radio galaxies at $0.5<z<2.0$
• Starburst-AGN mixing: I. NGC 7130
• Extragalactic Radio Continuum Surveys and the Transformation of Radio Astronomy
• SPIDER II - The Fundamental Plane of Early-type Galaxies in grizYJHK
• The properties of (sub)millimetre-selected galaxies as revealed by CANDELS HST WFC3/IR imaging in GOODS-South
• Compact radio sources and jet-driven AGN feedback in the early Universe: Constraints from integral-field spectroscopy
• Massive and Red Objects predicted by a semianalytical model of galaxy formation
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• The Dissipative Merger Progenitors of Elliptical Galaxies
• High-z Quasars in the R_h=ct Universe
• Evolution of faint radio sources in the VIDEO-XMM3 field
• Towards a physical picture of star-formation quenching: the photometric properties of recently-quenched galaxies in the Sloan Digital Sky Survey
• The effect of stellar feedback and quasar winds on the AGN population
• Absence of self-averaging and of homogeneity in the large scale galaxy distribution
• The environments of luminous radio galaxies and type-2 quasars
• The 1.4 GHz radio properties of hard X-ray selected AGN
• Probing recent star formation with absorption-line strengths in hierarchical models and observations
• The origin of dust in galaxies across cosmic time
• Episodic Random Accretion and the Cosmological Evolution of Supermassive Black Hole Spins
• Non-linearity and environmental dependence of the star forming galaxies Main Sequence
• Predictions for Herschel from LambdaCDM: unveiling the cosmic star formation history
• The Relation Between Galaxy Morphology and Environment in the Local Universe: An RC3-SDSS Picture
• Clustering of Dust-Obscured Galaxies at z ~ 2
• Halo Shapes From Weak Lensing: The Impact of Galaxy--Halo Misalignment
• Star formation in z>1 3CR host galaxies as seen by Herschel
• The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]-$\lambda$1908Å~emission 10.8 to 12.5 Gyr ago
• KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Quasar outflows at $z\ge 6$: the impact on the host galaxies
• The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way
• Future constraints on halo thermodynamics from combined Sunyaev-Zel'dovich measurements
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution?
• Superclusters of galaxies from the 2dF redshift survey. II. Comparison with simulations
• The impact of AGN feedback and baryonic cooling on galaxy clusters as gravitational lenses
• The clustering of SDSS galaxy groups: mass and color dependence
• The Effect of Star Formation on the Redshift Evolution of Interstellar Metals, Atomic and Molecular Gas in Galaxies
• Dependence of the BALQSO fraction on Radio Luminosity
• Bayesian AGN Decomposition Analysis for SDSS Spectra: A Correlation Analysis of [OIII]$\lambda 5007$ Outflow Kinematics with AGN and Host Galaxy Properties
• Thermal plasma in the giant lobes of the radio galaxy Centaurus A
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• Evidence of suppression of star formation by quasar-driven winds in gas-rich host galaxies at z<1?
• Characterising and Identifying Galaxy Protoclusters
• Detection of a High Brightness Temperature Radio Core in the AGN-Driven Molecular Outflow Candidate NGC 1266
• SDSS-IV MaNGA: Identification of active galactic nuclei in optical integral field unit surveys
• Mapping the Dynamics of a Giant Ly-alpha Halo at z=4.1 with MUSE: The Energetics of a Large Scale AGN-Driven Outflow around a Massive, High-Redshift Galaxy
• Exploring the limits of AGN feedback: black holes and the star formation histories of low-mass galaxies
• Similarity of ionized gas nebulae around unobscured and obscured quasars
• The chemical enrichment of the ICM from hydrodynamical simulations
• Systematic search for tidal features around nearby galaxies: I. Enhanced SDSS imaging of the Local Volume
• A flexible modelling of galaxy assembly bias
• Herschel-ATLAS/GAMA: a difference between star-formation rates in strong-line and weak-line radio galaxies
• Maximum Spin of Black Holes Driving Jets
• The baryonic Tully-Fisher relation and galactic outflows
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• The atomic Hydrogen content of the post-reionization Universe
• LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content
• The growth of the nuclear black holes in submillimeter galaxies
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Topology of structure in the Sloan Digital Sky Survey: model testing
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Properties of Active Galaxies Deduced from H I Observations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Downsizing of the blue cloud and the influence of galaxy size on mass quenching over the last eight billion years
• mJIVE-20: a survey for compact mJy radio objects with the Very Long Baseline Array
• The clustering of galaxies as a function of their photometrically-estimated atomic gas content
• Satellite Quenching and Galactic Conformity at 0.3 < z < 2.5
• RAiSE II: resolved spectral evolution in radio AGN
• Recurrent radio emission and gas supply: the case of the radio galaxy B2 0258+35
• A Confirmation of the Strong Clustering of Distant Red Galaxies at 2 < z <3
• Cosmic Evolution of Black Holes and Spheroids. V. The Relation Between Black Hole Mass and Host Galaxy Luminosity for a Sample of 79 Active Galaxies
• The radio continuum structure of Centaurus A at 1.4 GHz
• The similarity of the stellar mass fractions of galaxy groups and clusters
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• External pressure-triggering of star formation in a disc galaxy: a template for positive feedback
• The merger fraction of active and inactive galaxies in the local Universe through an improved non-parametric classification
• Seeding Black Holes in Cosmological Simulations
• On the depletion and accretion timescales of cold gas in local early-type galaxies
• The Weak Clustering of Gas-Rich Galaxies
• Very Light Magnetized Jets on Large Scales - I. Evolution and Magnetic Fields
• Quantifying the Cosmic Web I: The large-scale halo ellipticity-ellipticity and ellipticity-direction correlations
• The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey
• Supermassive Black Holes and Their Host Galaxies - II. The correlation with near-infrared luminosity revisited
• The Hierarchical Origins of Observed Galaxy Morphology
• The Millennium Run Observatory: First Light
• Nearly all Massive Quiescent Disk Galaxies have a Surprisingly Large Atomic Gas Reservoir
• Hot Outflows in Galaxy Clusters
• The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• A new population of recently quenched elliptical galaxies in the SDSS
• AGN contamination of galaxy-cluster thermal X-ray emission: predictions for eRosita from cosmological simulations
• Simulations of Metal Enrichment in Galaxy Clusters by AGN Outflows
• Photo-heating and supernova feedback amplify each other's effect on the cosmic star formation rate
• BCG Mass Evolution in Cosmological Hydro-Simulations
• The Cocoon Shocks of Cygnus A: Pressures and Their Implications for the Jets and Lobes
• Kinetic AGN Feedback Effects on Cluster Cool Cores Simulated using SPH
• The Small Scatter in BH-Host Correlations & The Case for Self-Regulated BH Growth
• Black hole evolution: II. Spinning black holes in a supernova-driven turbulent interstellar medium
• Glimpsing the Imprint of Local Environment on the Galaxy Stellar Mass Function
• BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• On the formation time scale of massive cluster ellipticals based on deep near-IR spectroscopy at z~2
• The Colors of Central and Satellite Galaxies in zCOSMOS out to z ~ 0.8 and Implications for Quenching
• The growth of disks and bulges during hierarchical galaxy formation. I: fast evolution vs secular processes
• Hierarchical Growth and Cosmic Star Formation: Enrichment, Outflows and Supernova Rates
• X-ray selected AGN Hosts are Similar to Inactive Galaxies out to z=3: Results from CANDELS/CDF-S
• The Growth of Central and Satellite Galaxies in Cosmological Smoothed Particle Hydrodynamics Simulations
• Light breeze in the local Universe
• The Rise of Active Galactic Nuclei in the GAlaxy Evolution and Assembly semi-analytic model
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• The impact of quenching on galaxy profiles in the Simba simulation
• ZFOURGE catalogue of AGN candidates: an enhancement of 160μm-derived star-formation rates in active galaxies to $z$ = 3.2
• The evolution of the star forming sequence in hierarchical galaxy formation models
• The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback
• Deep Chandra Observations of Edges and Bubbles in the NGC 5846 Galaxy Group
• Star Formation in Luminous Quasars at 2<z<3
• A Tale of Dwarfs and Giants: Using a z=1.62 Cluster to Understand How the Red Sequence Grew Over The Last 9.5 Billion Years
• GalICS II: the [alpha/Fe]-mass relation in elliptical galaxies
• Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
• Two-Face(s): ionized and neutral gas winds in the local Universe
• 3-D Radiative Transfer Calculations of Radiation Feedback from Massive Black Holes: Outflow of Mass from the Dusty "Torus"
• The Host Galaxies and Black Holes of Typical z~0.5-1.4 AGN
• MOKA: a new tool for Strong Lensing Studies
• Simulations of Jet Heating in Galaxy Clusters: Successes and Challenges
• The effect of variations in the input physics on the cosmic distribution of metals predicted by simulations
• Concurrent Supermassive Black Hole and Galaxy Growth: Linking Environment and Nuclear Activity in z = 2.23 H-alpha Emitters
• The Lifetime of FRIIs in Groups and Clusters: Implications for Radio-Mode Feedback
• Host galaxy-active galactic nucleus alignments in the SDSS-DR7
• Heating the IGM by X-rays from Population III Binaries in High Redshift Galaxies
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• The evolution of Brightest Cluster Galaxies in a hierarchical universe
• Cosmological Evolution of the Duty Cycle of Quasars
• Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2
• Galaxy gas as obscurer: I. GRBs x-ray galaxies and find a N_H ~ M* relation
• Gemini GMOS and WHT SAURON integral-field spectrograph observations of the AGN driven outflow in NGC 1266
• Connecting Dark Matter Halos with the Galaxy Center and the Supermassive Black Hole
• The evolution of galaxy cluster X-ray scaling relations
• An Extreme Starburst in Close Proximity to the Central Galaxy of a Rich Galaxy Cluster at z=1.7
• Luminous superclusters: remnants from inflation
• FR II radio galaxies at low frequencies I: morphology, magnetic field strength and energetics
• A constant limiting mass scale for flat early-type galaxies from z=1 to z=0: density evolves but shapes do not
• Environmentally Driven Global Evolution of Galaxies
• The CALIFA view on stellar angular momentum across the Hubble sequence
• Normal black holes in bulge-less galaxies: the largely quiescent, merger-free growth of black holes over cosmic time
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Another thread in the tapestry of stellar feedback: X-ray binaries
• Cosmological measure with volume averaging and the vacuum energy problem
• Mosaiced wide-field VLBI observations of the Lockman Hole/XMM
• Tracing the Quenching Journey across Cosmic Time
• Early-type galaxies in the PEARS survey: Probing the stellar populations at moderate redshift
• Jet-induced molecular gas excitation and turbulence in the Teacup
• The faint radio sky: VLBA observations of the COSMOS field
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• Thermal and radiative AGN feedback have a limited impact on star formation in high-redshift galaxies
• Jet-driven outflows of ionised gas in the nearby radio galaxy 3C293
• Role of Cosmic Ray Streaming and Turbulent Damping in Driving Galactic Winds
• Quasar induced galaxy formation: a new paradigm ?
• A new infrared color criterion for the selection of 0<z<7 AGN: application to deep fields and implications for JWST surveys
• Star formation history of galaxies from z=0 to z=0.7 A backward approach to the evolution of star-forming galaxies
• AGN-Host Galaxy Connection: Morphology and Colours of X-ray Selected AGN at z < 2
• Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
• Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations
• Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
• Enhancement of AGN in a protocluster at z=1.6
• The nuclear X-ray emission of nearby early-type galaxies
• The Survival of Multiphase Dusty Clouds in Hot Winds
• Chemical evolution of Local Group dwarf galaxies in a cosmological context -- I. A new modelling approach and its application to the Sculptor dwarf spheroidal galaxy
• Kinetic or thermal AGN feedback in simulations of isolated and merging disk galaxies calibrated by the M-sigma relation
• The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
• Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
• Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
• 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
• ALMA Observations of a Candidate Molecular Outflow in an Obscured Quasar
• CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST
• AGN-Host Connection at 0.5 < z < 2.5: A rapid evolution of AGN fraction in red galaxies during the last 10 Gyr
• A simple model for AGN feedback in nearby early-type galaxies
• Diffuse UV light associated with the Spiderweb Galaxy: evidence for in-situ star formation outside galaxies
• A systematic search for X-ray cavities in galaxy clusters, groups, and elliptical galaxies
• The Metallicity and Elemental Abundance Gradients of Simulated Galaxies, and their Environmental Dependence
• On the Dynamical Origin of the ICM Metallicity Evolution
• T-RaMiSu: The Two-meter Radio Mini Survey I. The Bootes Field
• Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• Feedback by massive stars and the emergence of superbubbles II. X-ray properties
• Markarian 6: shocking the environment of an intermediate Seyfert
• Properties of galaxies in SDSS Quasar environments at z < 0.2
• Cold gas dynamics in Hydra-A: evidence for a rotating disk
• Damn You, Little h! (or, Real-World Applications Of The Hubble Constant Using Observed And Simulated Data)
• Simulating galaxy clusters -- I. Thermal and chemical properties of the intra-cluster medium
• Host galaxies of high-redshift extremely red and obscured quasars
• AMUSE-Field I: Nuclear X-ray Properties of Local Field and Group Spheroids across the Stellar Mass Scale
• Luminosity function of galaxies in groups in the SDSS DR7: the dependence on mass, environment and galaxy type
• Compact Groups of Galaxies selected by stellar mass: The 2MASS Compact Group Catalogue
• Is cold gas fuelling the radio galaxy NGC 315?
• Constraints on the star formation histories of galaxies from z~1 to z~0
• The red-sequence of 72 WINGS local galaxy clusters
• Mock Lightcones and Theory Friendly Catalogs for the CANDELS Survey
• The redshift evolution of major merger triggering of luminous AGN: a slight enhancement at z$\sim$2
• Constraints on Quenching of $z\lesssim 2$ Massive Galaxies from the Evolution of the average Sizes of Star-Forming and Quenched Populations in COSMOS
• Galactic inflow and wind recycling rates in the EAGLE simulations
• The Complete Ultraviolet Spectrum of the Archetypal "Wind-Dominated" Quasar Mrk~231: Absorption and Emission from a High-Speed Dusty Nuclear Outflow
• Tracing the Quenching History in Galaxy Clusters in the EAGLE Simulation
• Massive Star-Forming Host Galaxies of Quasars on Sloan Digital Sky Survey Stripe 82
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• A unified solution to the small scale problems of the $\Lambda$CDM model
• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
• An infrared view of AGN feedback in a type-2 quasar: the case of the Teacup galaxy
• Spectral index properties of milliJansky radio sources
• 3D simulations of the early stages of AGN jets: geometry, thermodynamics and backflow
• AGN Jet-induced Feedback in Galaxies. II. Galaxy colours from a multicloud simulation
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
• Black hole spin and radio loudness in a LCDM universe
• The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
• YZiCS: Unveiling Quenching History of Cluster Galaxies Using Phase-space Analysis
• On the fast quenching of young low-mass galaxies up to z $\sim$ 0.6: new spotlight on the lead role of environment
• A Powerful AGN Outburst in RBS 797
• AGN feedback in the nucleus of M51
• Enriching the hot circumgalactic medium
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• The effect of thermally pulsating asymptotic giant branch stars on the evolution of the rest-frame near-infrared galaxy luminosity function
• Galaxy And Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies
• Cosmic evolution of low-excitation radio galaxies in the LOFAR Two-meter Sky Survey Deep Fields
• From outside-in to inside-out: galaxy assembly mode depends on stellar mass
• Two-Phase Galaxy Formation
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• The Australia Telescope Large Area Survey: Spectroscopic Catalogue and Radio Luminosity Functions
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• A search for 21 cm HI absorption in AT20G compact radio galaxies
• Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the "green valley"
• Chandra evidence for AGN feedback in the spiral galaxy NGC 6764
• On the thermodynamic self-similarity of the nearest, most relaxed, giant ellipticals
• High Radio Frequency Properties and Variability of Brightest Cluster Galaxies
• A Serendipitous XMM Survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z=0.8 to z=0.1
• Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies
• Resolution-independent modeling of environmental effects in semi-analytic models of galaxy formation that include ram-pressure stripping of both hot and cold gas
• Galaxy Clustering Topology in the Sloan Digital Sky Survey Main Galaxy Sample: a Test for Galaxy Formation Models
• Optical Properties of High-Frequency Radio Sources from the Australia Telescope 20 GHz (AT20G) Survey
• The Quiescent X-ray Spectrum of Accreting Black Holes
• The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei II: Kinematic Classifications for the Population at z < 0.1
• The Roles of Mass and Environment in the Quenching of Galaxies. II
• The Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS): Survey design, data catalogue and GAMA/WiggleZ spectroscopy
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• SDSS-IV MaNGA: Star formation cessation in low-redshift galaxies I. Dependence on stellar mass and structural properties
• MUFASA: The assembly of the red sequence
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• A Relationship Between Halo Mass, Cooling, AGN Heating, and the Coevolution of Massive Black Holes
• The Cusp/Core problem: supernovae feedback versus the baryonic clumps and dynamical friction model
• SPIDER X - Environmental effects in central and satellite early-type galaxies through the stellar fossil record
• Nature and evolution of powerful radio galaxies and their link with the quasar luminosity function
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• The migration of nearby spirals from the blue to red sequence: AGN feedback or environmental effects?
• Where do "red and dead" early-type void galaxies come from?
• Stellar Mass--Gas-phase Metallicity Relation at $0.5\le z\le 0.7$: A Power Law with Increasing Scatter toward the Low-mass Regime
• Radio galaxy feedback in X-ray selected groups from COSMOS: the effect on the ICM
• The specific star formation rate of high redshift galaxies: the case for two modes of star formation
• Red Sequence Cluster Finding in the Millennium Simulation
• The Building Up of the Black Hole Mass - Stellar Mass Relation
• Tracing the evolution of Active Galactic Nuclei host galaxies over the last 9 Gyrs of Cosmic time
• The environments of high redshift radio galaxies and quasars: probes of protoclusters
• FR-II radio galaxies at low frequencies II: spectral ageing and source dynamics
• Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7
• Radio-loud AGN: is there a link between luminosity and cluster environment?
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Measuring the giant radio galaxy length distribution with the LoTSS
• Constraining the supermassive black holes evolution through the continuity equation
• Compact groups in theory and practice - I. The spatial properties of compact groups
• No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• A Giant Metrewave Radio Telescope/Chandra view of IRAS 09104+4109: A type 2 QSO in a cooling flow
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• The Interstellar Medium of Quiescent Galaxies and its Evolution With Time
• The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing
• What produces the far-infrared/submm emission in the most luminous QSOs?
• Metallicity Gradients at Large Galactocentric Radii Using the Near-infrared Calcium Triplet
• Appreciating mergers for understanding the non-linear $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ and $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{galaxy}}$ relations, updated herein, and the implications for the (reduced) role of AGN feedback
• Probing the star formation history using the redshift evolution of luminosity functions
• Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging of a Growing Compact Galaxy at z=1.9
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Luminous and High Stellar Mass Candidate Galaxies at z ~ 8 Discovered in CANDELS
• Two Growing Modes and the Morphology-Quiescence Relation in Galaxies
• Rest-frame UV--Optically Selected Galaxies at 2.3<z<3.5: Searching for Dusty Star-forming and Passively-Evolving Galaxies
• Radio AGN in nearby dwarf galaxies: the important role of AGN in dwarf-galaxy evolution
• Sussing Merger Trees: the influence of the halo finder
• Environmental dependence of AGN activity. I.: the effects of host galaxy
• Towards a deeper understanding of the physics driving galaxy quenching -- inferring trends in the gas content via extinction
• Origin of the galaxy HI size-mass relation
• Star formation in high-redshift quasars: excess [O II] emission in the radio-loud population
• Emission line gas ionisation in young radio galaxies
• LOFAR Observations of X-ray Cavity Systems
• CO Emission in Infrared-Selected Active Galactic Nuclei
• High Redshift Galaxy Populations and their Descendants
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• Extreme star formation events in quasar hosts over $0.5<\text{z}<4$
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• Observational constraints on the co-evolution of supermassive black holes and galaxies
• The strong correlation between post-starburst fraction and environment
• COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: III. Comparison with semi-analytic models of galaxy formation
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• A modified star formation law as a solution to open problems in galaxy evolution
• Jets blowing bubbles in the young radio galaxy 4C 31.04
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• The Optical-Radio Mapping: the kinetic efficiency of Radio-Loud AGNs
• X-ray properties of the Youngest Radio Sources and their Environments
• Compact groups from the Millennium Simulations: I. Their Nature and the completeness of the Hickson sample
• The effects of the cluster environment on the galaxy mass-size relation in MACSJ J1206.2-0847
• Galaxy interactions are the dominant trigger for local type 2 quasars
• A near-IR study of the host galaxies of 2Jy radio sources at 0.03 < z < 0.5: I - the data
• The impact of TP-AGB stars on hierarchical galaxy formation models
• Building a control sample for galaxy pairs
• Luminous buried AGNs as a function of galaxy infrared luminosity revealed through Spitzer low-resolution infrared spectroscopy
• Sizes and ages of SDSS ellipticals: Comparison with hierarchical galaxy formation models
• A Link Between Ram Pressure Stripping and Active Galactic Nuclei
• A Large Population of Obscured AGN in Disguise as Low Luminosity AGN in Chandra Deep Field South
• A simple model linking galaxy and dark matter evolution
• Stars, Dust, and the Growth of UV-Selected Sub-L* Galaxies at Redshift z~2
• Very large scale correlations in the galaxy distribution
• A Comprehensive GALEX Ultraviolet Catalog of Star Clusters in M31 and a Study of the Young Clusters
• Tools for computing the AGN feedback: radio-loudness distribution and the kinetic luminosity function
• On the galaxy-halo connection in the EAGLE simulation
• Radiative Transfer and Radiative driving of Outflows in AGN and Starbursts
• Galaxy Zoo: The interplay of quenching mechanisms in the group environment
• The radio properties of a complete, X-ray selected sample of nearby, massive elliptical galaxies
• On the Scatter in the Radius - Luminosity Relationship for Active Galactic Nuclei
• Galaxy evolution from strong lensing statistics: the differential evolution of the velocity dispersion function in concord with the LambdaCDM paradigm
• Measuring the Dark Matter Halo Mass of X-ray AGN at z~1 using photometric redshifts
• Gas Content Regulates the Lifecycle of Star Formation and Black Hole Accretion in Galaxies
• The early-type galaxies NGC 1407 and NGC 1400 - II: star formation and chemical evolutionary history
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Bottom-heavy initial mass function in a nearby compact L*-galaxy
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei. IV. Association with Galaxy Mergers
• WISDOM project - IV. A molecular gas dynamical measurement of the supermassive black hole mass in NGC 524
• The prevalence of AGN feedback in massive galaxies at z~1
• AGN All the Way Down? AGN-like Line Ratios are Common In the Lowest-Mass Isolated Quiescent Galaxies
• Realistic galaxy image simulation via score-based generative models
• Powerful winds in high-redshift obscured and red quasars
• Spatial kinematics of Brightest Cluster Galaxies and their close companions from Integral Field Unit spectroscopy
• The KMOS${}^{3D}$ Survey: rotating compact star forming galaxies and the decomposition of integrated line widths
• A comparison of black hole growth in galaxy mergers with Gasoline and Ramses
• Monolithic or hierarchical star formation? A new statistical analysis
• Herschel-ATLAS: Far-infrared properties of radio-loud and radio-quiet quasars
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• The EDGE-CALIFA survey: The role of spiral arms and bars in driving central molecular gas concentrations
• The Halo Occupation Distribution of Active Galactic Nuclei
• MIGHTEE: Are giant radio galaxies more common than we thought?
• Evidence for the Thermal Sunyaev-Zel'dovich Effect Associated with Quasar Feedback
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• On the evidence for large-scale galactic conformity in the local Universe
• The Deep SWIRE Field. IV. First properties of the sub-mJy galaxy population: redshift distribution, AGN activity and star formation
• Deep 21-cm HI Observations at z~0.1: The Precursor to the Arecibo Ultra Deep Survey
• Cusps and Cores in the presence of galactic bulges
• The Evolution of the Rest-frame V-band Luminosity Function from z=4: A Constant Faint-end Slope over the Last 12 Gyr of Cosmic History
• Revealing components of the galaxy population through nonparametric techniques
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• NGC1266 as a Local Candidate for Rapid Cessation of Star Formation
• SPIDER IX - Classifying Galaxy Groups according to their Velocity Distribution
• A Giant Metrewave Radio Telescope search for associated H{\sc i} 21\,cm absorption in GHz-peaked-spectrum sources
• Triggering Active Galactic Nuclei in galaxy clusters
• The many lives of active galactic nuclei-II: The formation and evolution of radio jets and their impact on galaxy evolution
• Radio Jet Feedback and Star Formation in Heavily Obscured Quasars at Redshifts ~0.3-3, I: ALMA Observations
• J1649+2635: A Grand-Design Spiral with a Large Double-Lobed Radio Source
• Simulating the Cooling Flow of Cool-Core Clusters
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• Timing the evolution of quiescent and star-forming local galaxies
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Delayed triggering of radio Active Galactic Nuclei in gas-rich minor mergers in the local Universe
• The role of thermal evaporation in galaxy formation
• Chemical enrichment in very low-metallicity environments: Bootes I
• On the AGN radio luminosity distribution and the black hole fundamental plane
• Tidal Disruption of Stellar Objects by Hard Supermassive Black Hole Binaries
• Galaxies Probing Galaxies at High Resolution: Co-Rotating Gas Associated with a Milky Way Analog at z=0.4
• The triggering of local AGN and their role in regulating star formation
• A tale of two populations: the stellar mass of central and satellite galaxies
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Multi-flavour SMBH seeding and evolution in cosmological environments
• Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
• A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• Young and turbulent: the early life of massive galaxy progenitors
• Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy
• Determining star-formation rates in Active Galactic Nuclei hosts via stellar population synthesis
• Formation of disk galaxies in preheated media: a preventative feedback model
• Rapid Quenching of Galaxies at Cosmic Noon
• The roles of star formation and AGN activity of IRS sources in the HerMES fields
• The Size-Luminosity Relationship of Quasar Narrow-Line Regions
• Supernovae and AGN driven galactic outflows
• Bulges and disks in the local Universe. Linking the galaxy structure to star formation activity
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• The Host Galaxies of X-ray Quasars Are Not Strong Star Formers
• HIghMass -- High HI Mass, HI-rich Galaxies at z~0: Sample Definition, Optical and Halpha Imaging, and Star Formation Properties
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• The picture of BLR in 2.5-D FRADO: Dynamics & Geometry
• X-ray Bright Active Galactic Nuclei in Massive Galaxy Clusters I: Number Counts and Spatial Distribution
• The flickering nuclear activity of Fornax A
• The bulk kinetic power of radio jets in active galactic nuclei
• Clocking the formation of today's largest galaxies: Wide field integral spectroscopy of Brightest Cluster Galaxies and their surroundings
• Finding Galaxy Groups In Photometric Redshift Space: the Probability Friends-of-Friends (pFoF) Algorithm
• Unveiling the Important Role of Groups in the Evolution of Massive Galaxies: Insights from an Infrared Passive Sequence at Intermediate Redshift
• The Cosmic Evolution of Faint Satellite Galaxies as a Test of Galaxy Formation and the Nature of Dark Matter
• A Break in Spiral Galaxy Scaling Relations at the Upper Limit of Galaxy Mass
• Fanaroff-Riley classification of radio galaxies using group-equivariant convolutional neural networks
• The Galaxy Stellar Mass Function of X-ray detected groups: environmental dependence of galaxy evolution in the COSMOS survey
• A spectroscopic measurement of galaxy formation timescales with ROLES
• The black holes of radio galaxies during the "Quasar Era": Masses, accretion rates, and evolutionary stage
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Satellite Alignment: I. Distribution of Substructures and Their Dependence On Assembly History From N-Body Simulations
• Moderate-Luminosity Growing Black Holes From 1.25 < z < 2.7: Varied Accretion In Disk-Dominated Hosts
• Fossil Groups in the Millennium Simulation. Evolution of the Brightest Galaxies
• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• An X-ray Detected Group of Quiescent Early-type Galaxies at z=1.6 in the Chandra Deep Field South
• Spatially Resolved Stellar Populations of $0.3<z<6.0$ Galaxies in WHL0137-08 and MACS0647+70 Clusters as Revealed by JWST: How do Galaxies Grow and Quench Over Cosmic Time?
• A Measurement of the Millimeter Emission and the Sunyaev-Zel'dovich Effect Associated with Low-Frequency Radio Sources
• Properties of Submillimeter Galaxies in a Semi-analytic Model using the "Count Matching" Approach: Application to the ECDF-S
• Faint-end Quasar Luminosity Functions from Cosmological Hydrodynamic Simulations
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• The Sloan Digital Sky Survey Reverberation Mapping Project: Post-Starburst Signatures in Quasar Host Galaxies at z < 1
• The discovery of a typical radio galaxy at z = 4.88
• HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
• Evolution of the galaxy stellar mass function: evidence for an increasing $M^{\ast }$ from $z=2$ to the present day
• Morphological Properties of Superclusters of Galaxies
• The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS
• Feedback from galactic stellar bulges and hot gaseous haloes of galaxies
• Red but not dead : Unveiling the Star-forming Far-infrared Spectral Energy Distribution of SpARCS Brightest Cluster Galaxies at 0 < z < 1.8
• The ELIXR Galaxy Survey. II: Baryons and Dark Matter in an Isolated Elliptical Galaxy
• Stellar Masses of Lyman Break Galaxies, Lyman Alpha Emitters and Radio Galaxies in Overdense Regions at z=4-6
• The Dearth of Difference between Central and Satellite Galaxies I. Perspectives on star formation quenching and AGN activities
• The first Super Massive Black Holes: indications from models for future observations
• Subhaloes gone Notts: Spin across subhaloes and finders
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• On stellar mass loss from galaxies in groups and clusters
• Towards a comprehensive picture of powerful quasars, their host galaxies and quasar winds at z ~ 0.5
• Morphologies of Galaxies in and around a Protocluster at z=2.300
• Luminosity and surface brightness distribution of K-band galaxies from the UKIDSS Large Area Survey
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• Hidden Starbursts and Active Galactic Nuclei at 0<z<4 from the Herschel-VVDS-CFHTLS-D1 Field: Inferences on Coevolution and Feedback
• An accurate low-redshift measurement of the cosmic neutral hydrogen density
• PRIMUS: One- and Two-Halo Galactic Conformity at $0.2<z<1$
• The Radio Galaxy Population in the SIMBA SImulations
• Computation of synthetic spectra from simulations of relativistic shocks
• Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales
• The effect of dwarf galaxies disruption in semi-analytic models
• Radio source feedback in galaxy evolution
• Supermassive black holes in disk-dominated galaxies outgrow their bulges and co-evolve with their host galaxies
• Detecting Radio-AGN signatures in Red geysers
• Satellite Quenching, Galaxy Inner Density and the Halo Environment
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• The Environment of Galaxies at Low Redshift
• Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations
• Is there enough star formation in simulated protoclusters?
• Bias from gas inhomogeneities in the pressure profiles as measured from X-ray and SZ observations
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• The rocky road to quiescence: compaction and quenching of quasar host galaxies at z~2
• Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• On the common mass scale of the Milky Way satellites
• SDSS-IV MaNGA: Faint quenched galaxies I- Sample selection and evidence for environmental quenching
• Galaxy-scale Bars in Late-type Sloan Digital Sky Survey Galaxies Do Not Influence the Average Accretion Rates of Supermassive Black Holes
• Intensity Mapping Cross-Correlations: Connecting the Largest Scales to Galaxy Evolution
• Multiscale cosmic web detachments, connectivity, and preprocessing in the supercluster SClA2142 cocoon
• Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties
• A tale of two feedbacks: star-formation in the host galaxies of radio-AGN
• The diverse formation histories of simulated disc galaxies
• The galaxies that reionized the Universe
• Black hole growth and AGN feedback under clumpy accretion
• The dependence of the pairwise velocity dispersion on galaxy properties
• Multi-phase outflows in post starburst E+A galaxies -- I. General sample properties and the prevalence of obscured starbursts
• A near-infrared study of the multi-phase outflow in the type-2 quasar J1509+0434
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• Supermassive Black Holes and Their Environments
• The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• Mass and Redshift Dependence of Star Formation in Relaxed Galaxy Clusters
• AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts, and evidence for large-scale structure
• Identifying active galactic nuclei via brightness temperature with sub-arcsecond International LOFAR Telescope observations
• Probing the Radio Loud/Quiet AGN dichotomy with quasar clustering
• Massive Dark Matter Halos around Bright Isolated Galaxies in the 2dFGRS
• Modelling supermassive black hole growth: towards an improved sub-grid prescription
• Luminous Red Galaxies in hierarchical cosmologies
• Galaxy And Mass Assembly (GAMA): The 325 MHz Radio Luminosity Function of AGN and Star Forming Galaxies
• A Census of Broad-Line Active Galactic Nuclei in Nearby Galaxies: Coeval Star Formation and Rapid Black Hole Growth
• A journey from the outskirts to the cores of groups I: Color- and mass-segregation in 20K-zCOSMOS groups
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• Scaling Relations for Galaxies Prior to Reionization
• The Ages of Passive Galaxies in a z=1.62 Protocluster
• A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
• The Galaxy Activity, Torus, and Outflow Survey (GATOS). V: Unveiling PAH survival and resilience in the circumnuclear regions of AGN with JWST
• Herschel Far-Infrared Photometry of the Swift Burst Alert Telescope Active Galactic Nuclei Sample of the Local Universe. II. SPIRE Observations
• Multiwavelength characterization of faint Ultra Steep Spectrum radio sources : A search for high-redshift radio galaxies
• Star Formation Quenching in High-redshift Large-scale Structure: Post-starburst Galaxies in the Cl1604 Supercluster at $z\sim 0.9$
• Evaluating and Improving Semi-analytic modeling of Dust in Galaxies based on Radiative Transfer Calculations II: Dust Emission in the Infrared
• Brighter galaxy bias: underestimating the velocity dispersions of galaxy clusters
• Evidence of ongoing AGN-driven feedback in a quiescent post starburst E+A galaxy
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• Isolated elliptical galaxies in the local Universe
• Mass transport by buoyant bubbles in galaxy clusters
• The spatial distribution of cold gas in hierarchical galaxy formation models
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• Galaxy Zoo: major galaxy mergers are not a significant quenching pathway
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• An environmental dependence of the physical and structural properties in the Hydra Cluster galaxies
• The mass assembly of high-redshift black holes
• Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
• Outflows from active galactic nuclei: The BLR-NLR metallicity correlation
• The clustering of X-ray selected AGN at z=0.1
• Shocks, Seyferts and the SNR connection: a Chandra observation of the Circinus galaxy
• A Chandra X-ray Analysis of Abell 1664: Cooling, Feedback and Star Formation in the Central Cluster Galaxy
• Tracing galaxy populations through cosmic time: A critical test of methods for connecting the same galaxies between different redshifts at $z<3$
• The VLA-COSMOS 3 GHz Large Project: Star formation properties and radio luminosity functions of AGN with moderate-to-high radiative luminosities out to $z\sim 6$
• The Formation of S0 Galaxies with Counter-Rotating Neutral and Molecular Hydrogen
• Galaxy Zoo: Evidence for rapid, recent quenching within a population of AGN host galaxies
• Mergers and Star Formation: The environment and Stellar Mass Growth of the Progenitors of Ultra-Massive Galaxies since z = 2
• Dependence of the Local Reionization History on Halo Mass and Environment: Did Virgo Reionize the Local Group?
• Confirming the Quiescent Galaxy Population out to $z=3$: A Stacking Analysis of Mid-, Far-Infrared and Radio Data
• Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster?
• Measuring AGN Feedback with the Sunyaev-Zel'dovich Effect
• X-ray selected AGN in groups at redshifts z~1
• ALMA observations of AGN fuelling: the case of PKS B1718-649
• The Largest X-ray Selected Sample of z>3 AGNs: C-COSMOS & ChaMP
• The spatial clustering of mid-IR selected star forming galaxies at z ~ 1 in the GOODS fields
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• MgII Line Variability of High Luminosity Quasars
• Spatially resolved evidence of the impact of quasar driven outflows on recent star formation : The case of Mrk 34
• Active galactic nucleus jet feedback in hydrostatic halos
• Stellar Populations of UV-Selected Active Galactic Nuclei Host Galaxies at z ~ 2 - 3
• NIHAO-XXIII: Dark Matter density shaped by Black Hole feedback
• Numerical Simulations of Hot Halo Gas in Galaxy Mergers
• Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation
• Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey - Data Release Six
• Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space
• The complex jet- and bar-perturbed kinematics in NGC 3393 as revealed with ALMA and GEMINI-GMOS/IFU
• Evidence for Black Hole Growth in Local Analogs to Lyman Break Galaxies
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• AGN Feedback in SDSS-IV MaNGA: AGNs have Suppressed Central Star Formation Rates
• On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
• Hierarchical models of high redshift galaxies with thermally pulsing asymptotic giant branch stars: comparison with observations
• Warm molecular and ionized gas kinematics in the Type-2 quasar J0945+1737
• AGN feedback in elliptical galaxies: numerical simulations
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• The Size, Shape and Orientation of Cosmological Voids in the Sloan Digital Sky Survey
• The Role of Ram Pressure Stripping in the Quenching of Cluster Star Formation
• Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA
• AGN feedback drives the colour evolution of local galaxies
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Probing the assembly history and dynamical evolution of massive black hole binaries with pulsar timing arrays
• A Multi-wavelength Study of the Turbulent Central Engine of the Low-mass AGN hosted by NGC404
• The First Large Absorption Survey in HI (FLASH): I. Science Goals and Survey Design
• Properties of fossil groups in cosmological simulations and galaxy formation models
• A deep / wide 1-2 GHz snapshot survey of SDSS Stripe 82 using the Karl G. Jansky Very Large Array in a compact hybrid configuration
• Galaxy And Mass Assembly (GAMA): The environments of high- and low- excitation radio galaxies
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• The Impact of Gas Stripping and Stellar Mass Loss on Satellite Galaxy Evolution
• Testing cold dark matter with the low mass Tully-Fisher relation
• Quiescent galaxies at $z\gtrsim 2.5$: observations vs. models
• Galaxy wide radio induced feedback in a radio quiet quasar
• Stellar Dynamics and Star-Formation Histories of z $\sim$ 1 Radio-loud Galaxies
• Physics of Coevolution of Galaxies and Supermassive Black Holes
• A Huge Filamentary Structure at z=0.55 and Star Formation Histories of Galaxies at z<1
• Infrared Contributions of X-Ray Selected Active Galactic Nuclei in Dusty Star-Forming Galaxies
• COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at $0<z<5$ Revealed by X-ray and Radio Stacking
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• The eMERGE Survey I: Very Large Array 5.5 GHz observations of the GOODS-North Field
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Supermassive Black Holes and Their Host Galaxies - I. Bulge luminosities from dedicated near-infrared data
• Radio-AGN Feedback: When the Little Ones were Monsters
• Population Synthesis Models for Late Build-Up of the Red Sequence
• Cosmic downsizing of powerful radio galaxies to low radio luminosities
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• The imprints of AGN feedback within a supermassive black hole's sphere of influence
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Multi-phase outflows in high redshift quasar host galaxies
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• Ionised Gas Kinematics in MaNGA AGN. Extents of the Narrow Line and Kinematically Disturbed regions
• Very High Angular Resolution Science with the Square Kilometre Array
• Determining the core radio luminosity function of radio AGNs via copula
• The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
• Brightest Cluster Galaxies: the centre can(not?) hold
• The peculiar radio galaxy 4C 35.06: a case for recurrent AGN activity?
• What triggers black-hole growth? Insights from star formation rates
• The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at $7<z<8$
• Spin alignment of dark matter haloes in the shells of the largest voids
• Constraining star formation rates in cool-core brightest cluster galaxies
• Dust reddening in star-forming galaxies
• Angular momentum transfer to a Milky Way disk at high redshift
• Observing AGN feedback with CO intensity mapping
• From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
• Effects of cosmological parameters and star formation models on the cosmic star formation history in LambdaCDM cosmological simulations
• SDSS-IV MaNGA: The Different Quenching Histories of Fast and Slow Rotators
• The role of the most luminous, obscured AGN in galaxy assembly at z~2
• xGASS: The Impact of Photometric Bulges on the Scatter of HI Scaling Relations
• Growing Massive Black Holes in a Local Group Environment: the Central Supermassive, Slowly Sinking, and Ejected Populations
• Connecting Compact Star-forming and Extended Star-forming Galaxies at Low-redshift: Implications for Galaxy Compaction and Quenching
• The resolution bias: low resolution feedback simulations are better at destroying galaxies
• A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\text{z}=0.6$ to $\text{z}=1.3$
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• A new search for distant radio galaxies in the Southern hemisphere -- III. Optical spectroscopy and analysis of the MRCR--SUMSS sample
• Spectral ageing in the era of big data: integrated vs resolved models
• Episodic Star Formation Coupled to Reignition of Radio Activity in 3C 236
• An extremely dense group of massive galaxies at the centre of the protocluster at z = 3.09 in the SSA22 field
• Anti-hierarchical evolution of the Active Galactic Nucleus space density in a hierarchical universe
• Galaxy and Mass Assembly (GAMA): Demonstrating the power of WISE in the study of Galaxy Groups to $z<0.1$
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C
• The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuiGGLE Survey
• Semi-analytic galaxy formation in f(R)-gravity cosmologies
• Selection bias in dynamically-measured supermassive black hole samples: Scaling relations and correlations between residuals in semi-analytic galaxy formation models
• Spectral Classification and Ionized Gas Outflows in $z\sim 2$ WISE-Selected Hot Dust-Obscured Galaxies
• Effects of Inclination on Measuring Velocity Dispersion and Implications for Black Holes
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN
• Group quenching and galactic conformity at low redshift
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• Compaction-Driven Black Hole Growth
• How Does Radio AGN Feedback Feed Back?
• The effect of cosmic web filaments on galaxy evolution
• Novel calibrations of virial black hole mass estimators in active galaxies based on X-ray luminosity and optical/NIR emission lines
• Host galaxy colour gradients and accretion disc obscuration in AEGIS z~1 X-ray-selected active galactic nuclei
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties derived from the SED Fitting with Optical, Infrared, and Radio Data
• Evidence for Widespread AGN Activity among Massive Quiescent Galaxies at z ~ 2
• Spatial and luminosity distributions of galactic satellites
• Dust-Enshrouded AGN can Dominate Host-Galaxy-Scale Cold-Dust Emission
• Strong lensing statistics in large, z~<0.2 surveys: bias in the lens galaxy population
• AGNs as main contributors to the UV ionizing emissivity at high redshifts: predictions from a Lambda-CDM model with linked AGN/galaxy evolution
• Multi-wavelength observations of a rich galaxy cluster at z ~ 1: the HST/ACS colour-magnitude diagram
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• Investigating the spectral age problem with powerful radio galaxies
• Radio Detection of Radio-Quiet Galaxies
• A New Empirical Method to Infer the Starburst History of the Universe from Local Galaxy Properties
• Detecting Relativistic X-ray Jets in High-Redshift Quasars
• Evolution of the Stellar Mass--Metallicity Relation - I: Galaxies in the z~0.4 Cluster Cl0024
• Quenching Timescales in the IllustrisTNG Simulation
• Regulation of Star Formation by a Hot Circumgalactic Medium
• Hoag's Object: Evidence for Cold Accretion onto an Elliptical Galaxy
• Imaging Extended Emission-Line Regions of Obscured AGN with the Subaru Hyper Suprime-Cam Survey
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• The Density and Spectral Energy Distributions of Red Galaxies at z~3.7
• Milky Way Analogues in MaNGA: Multi-Parameter Homogeneity and Comparison to the Milky Way
• Three-dimensional Magnetohydrodynamic Simulations of Buoyant Bubbles in Galaxy Clusters
• Post-Newtonian Cosmological Modelling
• Delayed star formation in high-redshift stream-fed galaxies
• Physical properties of Herschel selected galaxies in a semi-analytic galaxy formation model
• Mapping Jet-ISM Interactions in X-ray Binaries with ALMA: A GRS 1915$+$105 Case Study
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
• Satellite quenching was not important for z$\sim$1 clusters: most quenching occurred during infall
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• The Diverse Nature of Optical Emission Lines in Brightest Cluster Galaxies: IFU Observations of the Central Kiloparsecs
• Cold-gas outflows in typical low-redshift galaxies are driven by star formation, not AGN
• Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies
• Correlation of Black Hole and Bulge Masses: Driven by Energy but Correlated with Momentum
• SPH Simulations of Black Hole Accretion: A Step to Model Black Hole Feedback in Galaxies
• The Molecular Gas Content of z<0.1 Radio Galaxies: Linking the AGN Accretion Mode to Host Galaxy Properties
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Large-scale fluctuations in the distribution of galaxies from the Two Degree Field Galaxy Redshift Survey
• Effects of large-scale environment on the assembly history of central galaxies
• Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin
• Feedback from central black holes in elliptical galaxies. II: Can purely mechanical energy feedback models work?
• Feedback from low-luminosity radio galaxies: B2 0258+35
• Measuring Gas Accretion and Angular Momentum near Simulated Supermassive Black Holes
• A population of galaxy-scale jets discovered using LOFAR
• Redshift Evolution in the Iron Abundance of the Intracluster Medium
• Radio AGN in 13,240 galaxy clusters from the Sloan Digital Sky Survey
• Do AGN triggering mechanisms vary with radio power? II. The importance of mergers as a function of radio power and optical luminosity
• Too dense to go through: The importance of low-mass clusters for satellite quenching
• A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: The Redshift Catalog
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• The environment of radio sources in the VLA-COSMOS Survey field
• Simulation-based inference of dynamical galaxy cluster masses with 3D convolutional neural networks
• Jets in radio galaxies and quasars: an observational perspective
• Brightest galaxies as halo centre tracers in SDSS DR7
• The environments of z~1 Active Galactic Nuclei at 3.6um
• Radio AGN in spiral galaxies
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Radio AGN in galaxy clusters: heating hot atmospheres and driving supermassive black hole growth over cosmic time
• A Chandra and ALMA Study of X-ray-irradiated Gas in the Central ~100 pc of the Circinus Galaxy
• Active galactic nucleus feedback in clusters of galaxies
• A Robust Estimator of the Small-Scale Galaxy Correlation Function
• Structures and components in galaxy clusters: observations and models
• A deep Chandra look at the low L_B elliptical NGC821: X-ray binaries, a galactic wind and emission at the nucleus
• A deep Chandra, VLA and Spitzer IRAC study of the very low luminosity nucleus of the elliptical NGC821
• Effect of local and large-scale environments on nuclear activity and star formation
• Convergence of Galaxy Properties with Merger Tree Temporal Resolution
• Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes
• Cosmic CARNage I: on the calibration of galaxy formation models
• The correlation of outflow kinematics with star formation rate -- Gas outflows in AGNs. VI
• The metallicity properties of simulated long-GRB galaxy hosts and the Fundamental Metallicity Relation
• Disk Galaxy Scaling Relations in the SFI++: Intrinsic Scatter and Applications
• Dynamics of relativistic radio jets in asymmetric environments
• Clustering Properties of restframe UV selected galaxies II: Migration of Star Formation sites with cosmic time from GALEX and CFHTLS
• Evolution of active galactic nuclei
• HerMES: SPIRE/Sub-millimetre Emission from Radio Selected AGN
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• The Origin of the Hubble Sequence in Lambda-CDM Cosmology
• The AGN-galaxy-halo connection: The distribution of AGN host halo masses to z=2.5
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• Dissecting the Red Sequence. IV. The Role of Truncation in the Two-Dimensional Family of Early-Type Galaxy Star Formation Histories
• Faraday rotation at low frequencies: magnetoionic material of the large FRII radio galaxy PKS J0636-2036
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• Linking haloes to galaxies: how many halo properties are needed?
• The cosmic evolution of massive black holes and galaxy spheroids: global constraints at redshift z<~1.2
• Properties and environment of Radio Emitting Galaxies in the VLA-zCOSMOS survey
• Resolving the baryon-fraction profile in lensing galaxies
• Observability of intermittent radio sources in galaxy groups and clusters
• Constraints on Feedback in the local Universe: The relation between star formation and AGN activity in early type galaxies
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• The dependence of AGN activity on stellar and halo mass in Semi-Analytic Models
• The evolution of the galaxy content of dark matter haloes
• The host galaxies of active galactic nuclei with powerful relativistic jets
• The VLA-COSMOS Survey: V. 324 MHz continuum observations
• Testing homogeneity in the Sloan Digital Sky Survey Data Release Twelve with Shannon entropy
• Simulations of the Sunyaev-Zeldovich Effect from Quasars
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• Ages and Metallicities of Early-Type Void Galaxies from Line Strength Measurements
• Anisotropic AGN Outflows and Enrichment of the Intergalactic Medium
• Radio Galaxy Zoo: Cosmological Alignment of Radio Sources
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• The physical drivers of the atomic hydrogen-halo mass relation
• The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: host galaxy properties and accretion rates of radio galaxies
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• Further constraining galaxy evolution models through the Size Function of SDSS Early-type galaxies
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• Dilution in elliptical galaxies: Implications for the relation between metallicity, stellar mass and star formation rate
• RHAPSODY-G simulations II - Baryonic growth and metal enrichment in massive galaxy clusters
• Galaxy Bias and ${\sigma }_8$ from Counts in Cells from the SDSS Main Sample
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• A new sample of southern radio galaxies: Host galaxy masses and star-formation rates
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Automated Morphological Classification of SDSS Red Sequence Galaxies
• Dark-ages Reionization & Galaxy Formation Simulation II: Spin and concentration parameters for dark matter haloes during the Epoch of Reionization
• The DEEP2 Galaxy Redshift Survey: The Red Sequence AGN Fraction and its Environment and Redshift Dependence
• The influence of halo assembly on galaxies and galaxy groups
• Revealing impacts of stellar mass and environment on galaxy quenching
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• The Origin of Double-Peaked Narrow Lines in Active Galactic Nuclei III: Feedback from Biconical AGN Outflows
• Active Galactic Nuclei and the Truncation of Star Formation in K+A Galaxies
• Prevalence of neutral gas in centres of merging galaxies
• The SPLASH survey: Quiescent galaxies are more strongly clustered but are not necessarily located in high-density environments
• Groups in the Millennium Simulation and in SDSS DR7
• The Properties of Radio Galaxies and the Effect of Environment in Large Scale Structures at $z\sim 1$
• The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• The XXL Survey XVIII. ATCA 2.1 GHz radio source catalogue and source counts for the XXL-South field
• The Physical Origin of Galactic Conformity: From Theory to Observation
• Large scale environments of z<0.4 active galaxies
• How covariant is the galaxy luminosity function?
• NIHAO III: The constant disc gas mass conspiracy
• In and out star formation in z~1.5 quiescent galaxies from rest-frame UV spectroscopy and the far-infrared
• The radio core of the Ultraluminous Infrared Galaxy F00183-7111: watching the birth of a quasar
• Classification and analysis of emission-line galaxies using mean field independent component analysis
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• The jet/wind outflow in Centaurus A: a local laboratory for AGN feedback
• Decoding the giant extragalactic radio sources
• The SEDs, Host Galaxies and Environments of Variability Selected AGN in GOODS-S
• Evidence of jet-clump interaction: a flip of the radio jet head of 3C~84
• A magnified view of circumnuclear star formation and feedback around an AGN at z=2.6
• Eddington's Demon: Inferring Galaxy Mass Functions and other Distributions from Uncertain Data
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). AGN feedback in [NeV] emitters
• Massive, red galaxies in a hierarchical universe I. Counts of Extremely Red Objects and basic properties
• Stellar age gradients and inside-out star formation quenching in galaxy bulges
• Aging of galaxies along the morphological sequence, marked by bulge growth and disk quenching
• The Role of Environment on the Formation of Early-Type Galaxies
• Galaxy groups in the 2MASS Redshift Survey
• Constraints on black hole duty cycles and the black hole-halo relation from SDSS quasar clustering
• Luminous Red Galaxies in Simulations: Cosmic Chronometers?
• A search for distant radio galaxies from SUMSS and NVSS: II. Optical Spectroscopy
• Welcome to the Twilight Zone: The Mid-Infrared Properties of Poststarburst Galaxies
• Determining the radio AGN contribution to the radio-FIR correlation using the black hole fundamental plane relation
• Black-hole masses, accretion rates and hot- and cold-mode accretion in radio galaxies at z~1
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• Star Formation, Radio Sources, Cooling X-ray Gas, and Galaxy Interactions in the Brightest Cluster Galaxy in 2A0335+096
• Star formation and quenching among the most massive galaxies at z~1.7
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• On Physical Scales of Dark Matter Halos
• Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
• Young AGN outburst running over older X-ray cavities
• HST NIR Snapshot Survey of 3CR Radio Source Counterparts II: An Atlas and Inventory of the Host Galaxies, Mergers and Companions
• The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity
• The impact of AGN on stellar kinematics and orbits in simulated massive galaxies
• A HR-like diagram for galaxies: the M_BH versus M_G sigma^2 relation
• How accurate is it to update the cosmology of your halo catalogues?
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• A Multiwavelength Spectral and Polarimetric Study of the Jet of 3C 264
• The eROSITA Final Equatorial-Depth Survey (eFEDS): LOFAR view of brightest cluster galaxies and AGN feedback
• Probing multiphase gas in local massive elliptical galaxies via multiwavelength observations
• SHARP -- VI. Evidence for CO (1-0) molecular gas extended on kpc-scales in AGN star forming galaxies at high redshift
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Direct Detection of Quasar Feedback Via the Sunyaev-Zeldovich Effect
• The Geometry of the Infrared and X-ray Obscurer in a Dusty Hyperluminous Quasar
• Optical colours of AGN in the Extended Chandra Deep Field South: Obscured black holes in early type galaxies
• Gravitational Stability of Circumnuclear Disks in Elliptical Galaxies
• The connection between star formation and supermassive Black Hole activity in the local Universe
• The UV-Optical Color Dependence of Galaxy Clustering in the Local Universe
• The weak imprint of environment on the stellar populations of galaxies
• Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
• Empirical Links between XRB and AGN accretion using the complete z<0.4 spectroscopic CSC/SDSS Catalog
• Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field
• Implications of the pulsar timing array detections for massive black hole mergers in the LISA band
• Galactic conformity measured in semi-analytic models
• Cosmic evolution of radio-AGN feedback: confronting models with data
• Evolution of superclusters in the cosmic web
• The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function
• Measuring cavity powers of active galactic nuclei in clusters using a hybrid X-ray-radio method -- A new window on feedback opened by subarcsecond LOFAR-VLBI observations
• Persistent fluctuations in the distribution of galaxies from the Two degree Field Galaxy Redshift Survey
• A model for the metallicity evolution of damped Lyman-alpha systems
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• Observational constraints on the physics behind the evolution of AGN since z ~ 1
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey
• Evolution of galaxy groups in the Illustris simulation
• Post-Starburst Properties of Post-Merger Galaxies
• The Nuclear Outflows and Feedback in the Seyfert 2 Galaxy Markarian 573
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• Why are AGN found in High Mass Galaxies?
• On the stellar populations of massive galaxies
• The Compact Structures of Massive $z\sim 0.7$ Post-Starburst Galaxies in the SQuIGG$\vec{L}$E Sample
• Decoding the spectra of SDSS early-type galaxies: New indicators of age and recent star formation
• A Multiwavelength Study of Active Galactic Nuclei in Post-Merger Remnants
• VIS3COS: III. environmental effects on the star formation histories of galaxies at z~0.8 seen in [OII], H$\delta$, and Dn4000
• Fueling the central engine of radio galaxies. III. Molecular gas and star formation efficiency of 3C 293
• WALLABY Pre-Pilot Survey: The effects of tidal interaction on radial distribution of color in galaxies of the Eridanus supergroup
• Disk Assembly and the M_BH-sigma Relation of Supermassive Black Holes
• A CO molecular gas wind 340 pc away from the Seyfert 2 nucleus in ESO 420-G13 probes an elusive radio jet
• Color-Magnitude Distribution of Face-on Nearby Galaxies in SDSS DR7
• The relative growth of Optical and Radio Quasars in SDSS
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• ALMA observations of the interaction of a radio jet with molecular gas in Minkowski's Object
• The clustering amplitude of X-ray selected AGN at z=0.8: Evidence for a negative dependence on accretion luminosity
• COSMOS2020: UV selected galaxies at $z\ge 7.5$
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI -- Stellar Populations
• The hierarchical build-up of the Tully-Fisher relation
• Suppressed star formation in circumnuclear regions in Seyfert galaxies
• The LOFAR view of giant, early-type galaxies: radio emission from active nuclei and star formation
• On Neutron Star Mergers as the Source of r-process Enhanced Metal Poor Stars in the Milky Way
• The Lives of High Redshift Mergers
• Obscured and powerful AGN and starburst activities at z~3.5
• Synthetic X-ray spectra for simulations of the dynamics of an accretion flow irradiated by a quasar
• Evolution of [OIII]5007 emission-line profiles in narrow emission-line galaxies
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• Measures of Galaxy Environment - III. Difficulties in identifying proto-clusters at z ~ 2
• Jet-Shocked H2 and CO in the Anomalous Arms of Molecular Hydrogen Emission Galaxy NGC 4258
• The Accretion and Cooling of Preheated Gas in Dark Matter Halos
• ULASJ1234+0907: The Reddest Type 1 Quasar at z=2.5 Revealed in the X-ray and Far Infra-red
• A Study of Outflows in Luminous Quasars at Redshift $\sim 0.4-0.8$
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• The GLEAM 4-Jy (G4Jy) Sample: II. Host-galaxy identification for individual sources
• A Unique View of AGN-Driven Molecular Outflows: The Discovery of a Massive Galaxy Counterpart to a $z=2.4$ High-Metallicity Damped Lyman-$\alpha$ Absorber
• The Evolution of Brightest Cluster Galaxies in the Nearby Universe I: Colours and Stellar Masses from the Sloan Digital Sky Survey and Wide Infrared Survey Explorer
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• Merging Galaxies with Tidal Tails in COSMOS to z=1
• Galaxy star formation in different environments
• Unveiling the origin of the gamma-ray emission in NGC 1068 with the Cherenkov Telescope Array
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: II -The sample and surface mass density profiles
• DM haloes in the fifth-force cosmology
• Enhanced Star Formation Efficiency in the Central Regions of Nearby Quasars Hosts
• Long Gamma-Ray Bursts and Their Host Galaxies at High Redshift
• Regulation of thermal conductivity in hot galaxy clusters by MHD turbulence
• Probing feedback in protogalaxies: Multiphase gas in a DLA at z~2.4
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Jet-Intracluster Medium interaction in Hydra A. II The Effect of Jet Precession
• Stellar Population Trends in S0 Galaxies
• The Source of Mass Accreted by the Central Black Hole in Cooling Flow Clusters
• Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
• The Type II AGN-host galaxy connection: insights from the VVDS and VIPERS surveys
• Strong spiral arms drive secular growth of pseudo bulges in disk galaxies
• The diverse X-ray properties of four truly isolated elliptical galaxies: NGC 2954, NGC 6172, NGC 7052, and NGC 7785
• Mapping the neutral atomic hydrogen gas outflow in the restarted radio galaxy 3C 236
• The Sloan Digital Sky Survey Reverberation Mapping Project: Quasar Host Galaxies at $z<0.8$ from Image Decomposition
• Circumnuclear and infalling HI gas in a merging galaxy pair at z=0.123
• Placing High-Redshift Quasars in Perspective: a Catalog of Spectroscopic Properties from the Gemini Near Infrared Spectrograph -- Distant Quasar Survey
• Color Magnitude Relation and Morphology of Low-Redshift ULIRGs in SDSS
• Properties of Long Gamma-Ray Burst Host Galaxies in Cosmological Simulation
• Evolution in the Disks and Bulges of Group Galaxies since z=0.4
• The Evolution of Field Early-Type Galaxies in the FDF and WHDF
• Deep Chandra X-ray Imaging of a Nearby Radio Galaxy 4C+29.30: X-ray/Radio Connection
• Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
• The GLEAM 4-Jy (G4Jy) Sample: I. Definition and the catalogue
• Evidence of different star formation histories for high- and low-luminosity radio galaxies
• Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25
• Fueling the central engine of radio galaxies. II. The footprints of AGN feedback on the ISM of 3C 236
• On the Role of Hot Feedback Mode in Active Galactic Nuclei Feedback in an Elliptical Galaxy
• Constructing high-fidelity halo merger trees in AbacusSummit
• Accurate Identification of Galaxy Mergers with Stellar Kinematics
• Spatial Clustering from GALEX-SDSS samples: Star Formation History and large-scale clustering
• Coevolution Between Supermassive Black Holes and Bulges Is Not Via Internal Feedback Regulation But By Rationed Gas Supply Due To Angular Momentum Distribution
• The evolution of the AGN content in groups up to z~1
• Evolution of environment dependent galaxy properties in the Sloan Digital Sky Survey
• Comparing Simulations of AGN Feedback
• The parsec-scale HI outflows in powerful radio galaxies
• Galaxy And Mass Assembly (GAMA): Bivariate functions of H$\alpha$ star forming galaxies
• The hydrodynamic stability of gaseous cosmic filaments
• The galaxy-halo size relation of low-mass galaxies in FIRE
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• Quenching or Bursting: the Role of Stellar Mass, Environment, and Specific Star Formation Rate to $z$ $\sim$ 1
• Confronting Cold Dark Matter Predictions with Observed Galaxy Rotations
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Quantifying the Thermal Sunyaev-Zel'dovich Effect and Excess Millimeter Emission in Quasar Environments
• Molecular Cloud Properties and CO Line Emission in z >~ 6 Galaxies
• Hosts and triggers of AGNs in the Local Universe
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Do AGN triggering mechanisms vary with radio power? I.Optical morphologies of radio-intermediate HERGs
• The XXL Survey: XXXVI. Evolution and black hole feedback of high-excitation and low-excitation radio galaxies in XXL-S
• The luminosity function of galaxies to $M_{BgVriz}\sim -14$ in $z\sim 0.3$ clusters
• B2 0902+34: A Collapsing Protogiant Elliptical Galaxy at z=3.4
• Generating Synthetic Cosmological Data with GalSampler
• The statistics of voids as a tool to constrain cosmological parameters: sigma_8 and Omega_m h
• How to Find Variable Active Galactic Nuclei with Machine Learning
• The filamentary radio lobes of the Seyfert-Starburst composite galaxy NGC3079
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• Empirical Constraints on the Evolution of the Relationship between Black Hole and Galaxy Mass: Scatter Matters
• Can galaxy outflows and re-accretion produce the downsizing in specific star formation rate of late-type galaxies?
• The XXL Survey: XXIX. GMRT 610 MHz continuum observations
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Optical, near-IR and sub-mm IFU Observations of the nearby dual AGN Mrk 463
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• Is NGC 3108 transforming itself from an early to late type galaxy -- an astronomical hermaphrodite?
• Brightest Group Galaxies: Stellar Mass and Star Formation Rate (paper I)
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• The host galaxy/AGN connection. Brightness profiles of early-type galaxies hosting Seyfert nuclei
• Influence of Projection in Cluster Cosmology Studies
• Ultra Steep Spectrum radio sources in the Lockman Hole: SERVS identifications and redshift distribution at the faintest radio fluxes
• On the cosmological evolution of the black hole - host galaxy relation in quasars
• Relation Between Globular Clusters and Supermassive Black Holes in Ellipticals as a Manifestation of the Black Hole Fundamental Plane
• Evolution of Group Galaxies from the First Red-Sequence Cluster Survey
• Probing AGN triggering mechanisms through the starburstiness of the host galaxies
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• Precision Cosmology: Successes and Challenges
• The Cosmic History of Black Hole Growth from Deep Multiwavelength Surveys
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• The Evolution and Environments of X-ray Emitting Active Galactic Nuclei in High-Redshift Large-Scale Structures
• Observable consequences of kinetic and thermal AGN feedback in elliptical galaxies and galaxy clusters
• The Origin of the 24-micron Excess in Red Galaxies
• A Massive Spiral Galaxy in the Zone of Avoidance
• Ultramassive black holes in the most massive galaxies: $M_{\mathrm{BH}}-\sigma$ versus $M_{\mathrm{BH}}-R_{\mathrm{b}}$
• A UV study of nearby luminous infrared galaxies: star formation histories and the role of AGN
• Improving Correlation Function Fitting with Ridge Regression: Application to Cross-Correlation Reconstruction
• The (black hole mass)-(color) relations for early- and late-type galaxies: red and blue sequences
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• The XMM-Newton survey of the ELAIS-S1 field II: optical identifications and multiwavelength catalogue of X-ray sources
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• Evolution of the galaxy luminosity function in progenitors of fossil groups
• Subaru Hyper Suprime-Cam View of Quasar Host Galaxies at z < 1
• Quenching by gas compression and consumption: A case study of a massive radio galaxy at z = 2.57
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• Star Formation and AGN Feedback in the Local Universe: Combining LOFAR and MaNGA
• Herschel-ATLAS: far-infrared properties of radio-selected galaxies
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• The State of the Molecular Gas in Post-Starburst Galaxies
• Exploring the Luminosity Evolution and Stellar Mass Assembly of 2SLAQ Luminous Red Galaxies Between Redshift 0.4 and 0.8
• WISDOM project -- VIII. Multi-scale feedback cycles in the brightest cluster galaxy NGC 0708
• The Magnetic Field and Polarization Properties of Radio Galaxies in Different Accretion States
• On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• The host galaxy properties of variability selected AGN in the Pan-STARRS1 Medium-Deep Survey
• The mass and environmental dependence on the secular processes of AGN in terms of morphology, colour, and specific star-formation rate
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Dark-ages Reionization and Galaxy Formation Simulation -- XVII. Sizes, angular momenta and morphologies of high redshift galaxies
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• Quasar Host Environments: The view from Planck
• Two phase galaxy formation: The Gas Content of Normal Galaxies
• Herschel-ATLAS: the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects
• H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
• The extent of ionization in simulations of radio-loud AGNs impacting kpc gas discs
• The stellar populations of early-type galaxies -- II. The effects of environment and mass
• Evidence of wind signatures in the gas velocity profiles of Red Geysers
• BH Accretion in Low-Mass Galaxies Since z~1
• Comparison of Observed Galaxy Properties with Semianalytic Model Predictions using Machine Learning
• Quasi-stellar objects in the ALHAMBRA survey. I. Photometric redshift accuracy based on a 23 optical-NIR filter photometry
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• Dust evolution with active galactic nucleus feedback in elliptical galaxies
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• Resolved HI Imaging of a Population of Massive HI-Rich Galaxies with Suppressed Star Formation
• AGN Feedback in Groups and Clusters of Galaxies
• Active Galactic Nuclei outflows in galaxy discs
• RAiSE: simulation-based analytical model of AGN jets and lobes
• Effect of dark matter annihilation on gas cooling and star formation
• Intermittent AGN episodes drive outflows with a large spread of observable loading factors
• The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• An Analysis Framework for Understanding the Origin of Nuclear Activity in Low-Power Radio Galaxies
• On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELS
• Violent quenching: molecular gas blown to 1000 km/s during a major merger
• The Cosmological History of Accretion onto Dark Halos and Supermassive Black Holes
• Radio observations of the CDF-South: a possible link between radio emission and star formation in X-ray selected AGN
• The galaxy correlation function as a constraint on galaxy formation physics
• Spatially-resolved NUV-r color of local star-forming galaxies and clues for quenching
• Atomic-to-molecular gas phase transition triggered by the radio jet in Centaurus A
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• VLA and ALMA observations of the lensed radio-quiet quasar SDSS J0924+0219: a molecular structure in a 3 microJy radio source
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Luminosity bias: from haloes to galaxies
• Galaxy And Mass Assembly (GAMA): 'No Smoking' zone for giant elliptical galaxies?
• X-ray properties and obscured fraction of AGN in the J1030 Chandra field
• A new model framework for circumgalactic Ly$\alpha$ radiative transfer constrained by galaxy-Ly$\alpha$ forest clustering
• A Moderate Cooling Flow Phase at Galaxy Formation
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• The role of galaxy mass on AGN emission: a view from the VANDELS survey
• Semi-analytic galaxy formation in early dark energy cosmologies
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• 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
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• M_BH - sigma relation in SDSS flat-spectrum radio quasars
• AGN triggering in the infall regions of distant X-ray luminous galaxy clusters at 0.9 < z <~ 1.6
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Expanding the Sample: The Relationship Between the Black Hole Mass of BCGs and the Total Mass of Galaxy Clusters
• Termination of star formation by BH feedback in equal- and unequal-mass mergers of disk and elliptical galaxies
• Investigating the relationship between AGN activity and stellar mass in zCOSMOS galaxies at 0<z<1 using emission line diagnostic diagrams
• The assembly bias of emission line galaxies
• WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
• Constraining the multi-scale dark-matter distribution in CASSOWARY 31 with strong gravitational lensing and stellar dynamics
• Galaxy Morphologies Revealed with Subaru HSC and Super-Resolution Techniques I: Major Merger Fractions of L_UV~3-15 L_UV* Dropout Galaxies at z~4-7
• Determine the galaxy bias factors on large scales using bispectrum method
• Radio Morphology of Red Geysers
• MUSE discovers perpendicular arcs in the inner filament of Cen A
• Galaxy Ecosystems: gas contents, inflows and outflows
• Broadband spectral energy distributions of SDSS-selected quasars and of their host galaxies: intense activity at the onset of AGN feedback
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• Probing the hot X-ray gas in the narrow-line region of Mrk 3
• Constraining the Noise-Free Distribution of Halo Spin Parameters
• The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
• Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
• Does jackknife scale really matter for accurate large-scale structure covariances?
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• On the Interaction of the PKS B1358-113 Radio Galaxy with the Abell 1836 Cluster
• Extending Recovery of the Primordial Matter Power Spectrum
• Nearby Galaxies in the 2micron All Sky Survey I. K-band Luminosity Functions
• Extension and estimation of correlations in Cold Dark Matter models
• Galaxy and Mass Assembly (GAMA): Small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• AEGIS: Chandra Observation of DEEP2 Galaxy Groups and Clusters
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
• Evolution of the Milky Way in Semi-Analytic Models: Detecting Cold Gas at z=3 with ALMA and SKA
• Radio Emission and AGN Feedback in Post-starburst Galaxies
• Nowhere to Hide: Radio-faint AGN in the GOODS-N field. II. Multi-wavelength AGN selection techniques and host galaxy properties
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The Elephant in the Bathtub: when the physics of star formation regulate the baryon cycle of galaxies
• Measuring the jet power of flat spectrum radio quasars
• Radio Galaxy Zoo: Observational evidence for environment as the cause of radio source asymmetry
• Connecting radio emission to AGN wind properties with Broad Absorption Line Quasars
• The effect of active galactic nuclei on the cold interstellar medium in distant star-forming galaxies
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• Death at watersheds: galaxy quenching in low-density environments
• Galaxy Clusters in the IRAC Dark Field II: Mid-IR Sources
• Wide and deep near-UV (360nm) galaxy counts and the extragalactic background light with the Large Binocular Camera
• Discovery of a red backsplash galaxy candidate near M81
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• The effect of environment on star formation activity and morphology at 0.5 < z < 2.5 in CANDELS
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• Compact Molecular Gas Distribution in Quasar Host Galaxies
• Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• On the slow quenching of M* galaxies: heavily-obscured AGNs clarify the picture
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• HST emission-line images of nearby 3CR radio galaxies: two photoionization, accretion and feedback modes
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Ubiquitous radio emission in quasars: predominant AGN origin and a connection to jets, dust and winds
• The LOFAR-eFEDS survey: The incidence of radio and X-ray AGN and the disk-jet connection
• Metal enrichment in a semi-analytical model, fundamental scaling relations, and the case of Milky Way galaxies
• Assessing the Predictive Power of Galaxy Formation Models: A Comparison of Predicted and Observed Rest-Frame Optical Luminosity Functions at 2.0<z<3.3
• The influence of Red Spiral Galaxies on the Shape of the Local K-Band Luminosity Function
• The GALEX Arecibo SDSS Survey VII: The Bivariate Neutral Hydrogen-Stellar Mass Function for Massive Galaxies
• The evolution of star formation activity in galaxy groups
• A new discovery space opened by eROSITA: Ionised AGN outflows from X-ray selected samples
• The $z\lesssim 1$ drop of cosmic dust abundance in a semi-analytic framework
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• The Spiderweb proto-cluster is being magnetized by its central radio jet
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• Do quasar broad-line velocity widths add any information to virial black hole mass estimates?
• The evolution of the Fundamental Plane of radio galaxies from z~0.5 to the present day
• A Modified Synchrotron Model for Knots in the M87 Jet
• The nuclear activity and central structure of the elliptical galaxy NGC 5322
• Clustering Properties of restframe UV selected galaxies I: the correlation length derived from GALEX data in the local Universe
• The kinetic power of jets magnetically accelerated from advection dominated accretion flows in radio galaxies
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• On the Stellar Populations in Faint Red Galaxies in the Hubble Ultra Deep Field
• Stellar populations, stellar masses and the formation of galaxy bulges and discs at $z<3$ in CANDELS
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• Radio Observations of the Hubble Deep Field South Region IV: Optical Properties of the Faint Radio Population
• The evolution of radio sources in the UKIDSS-DXS XMM-LSS field
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Radio loud AGN and the L_X - σrelation of galaxy groups and clusters
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• The MOSDEF-LRIS Survey: Connection between Galactic-scale Outflows and the Properties of $z$~2 star-forming Galaxies
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Dark-ages Reionization and Galaxy Formation Simulation - XIII. AGN quenching of high-redshift star formation in ZF-COSMOS-20115
• Evolution of the Most Massive Galaxies to z ~ 0.6: II. The link between radio AGN activity and star formation
• QSOFEED: The relationship between star formation and AGN Feedback
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• A practical guide to the massive black hole cosmic history
• Correlation of Black Hole-Bulge Masses by AGN Jets
• X-Ray Emitting Active Galactic Nuclei from z = 0.6-1.3 in the Intermediate and High-Density Environments of the ORELSE Survey
• Complex distribution and velocity field of molecular gas in NGC 1316 as revealed by Morita Array of ALMA
• The Cosmic History of Hot Gas Cooling and Radio AGN Activity in Massive Early-Type Galaxies
• Forensic reconstruction of galaxy colour evolution and population characterisation
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• The spatial distribution of X-ray selected AGN in the Chandra deep fields: a theoretical perspective
• Molecular Flows in Contemporary Active Galaxies and the Efficacy of Radio-Mechanical Feedback
• Milky Way type galaxies in a LCDM cosmology
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• SAGAN-II : Molecular gas content of giant radio galaxies
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). III. Discovery of a z = 4.72 Radio Galaxy with Lyman Break Technique
• Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Investigating the properties of AGN feedback in hot atmospheres triggered by cooling-induced gravitational collapse
• Signatures of inflowing gas in red geyser galaxies hosting radio-AGN
• A Redshift Survey of the Nearby Galaxy Cluster Abell 2199: Comparison of the Spatial and Kinematic Distributions of Galaxies with the Intracluster Medium
• The Effects of an AGN on Host Galaxy Colour and Morphology Measurements
• Galaxy and Mass Assembly (GAMA): A $\text{WISE}$ study of the activity of emission-line systems in G23
• Satellite quenching and morphological transformation of galaxies in groups and clusters
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
• Black Hole Growth in Disk Galaxies Mediated by the Secular Evolution of Short Bars
• The XXL Survey: XXXI. Classification and host galaxy properties of 2.1 GHz ATCA XXL-S radio sources
• Compact groups in theory and practice - II. Comparing the observed and predicted nature of galaxies in compact groups
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Searching for signs of jet-driven negative feedback in the nearby radio galaxy UGC 05771
• Constraints on the velocity profiles of galaxies from strong lensing statistics and semi-analytical modelling of galaxy formation
• Spectropolarimetry of the superwind filaments of the starburst galaxy M82 II: kinematics of the dust surrounding the nuclear starburst
• The large molecular gas fraction of post-starburst galaxies at z > 1
• Spin and structural halo properties at high redshift in a LCDM Universe
• {\em Herschel}-ATLAS/GAMA: The Environmental Density of Far-Infrared Bright Galaxies at $z\le 0.5$
• Constraining the Redshift Evolution of FIRST Radio Sources in RCS1 Galaxy Clusters
• CircleZ: Reliable Photometric redshifts for AGN computed using only photometry from Legacy Survey Imaging for DESI
• On the Reversal of SFR-Density Relation at z=1: Insights from Simulations
• The H$\alpha$ star formation main sequence in cluster and field galaxies at $z\sim 1.6$
• Synergies between low- and intermediate-redshift galaxy populations revealed with unsupervised machine learning
• Evolution of the infrared Tully-Fisher relation up to z=1.4
• KCWI observations of the extended nebulae in Mrk 273
• POLAR -- I: linking the 21-cm signal from the epoch of reionization to galaxy formation
• Radio jet-ISM interaction and positive radio-mechanical feedback in Abell 1795
• Hubble Space Telescope Images of Red Mergers: How Dry are They?
• Detecting the halo heating from AGN feedback with ALMA
• The Subaru/XMM-Newton Deep Field - II. The 37 brightest radio sources
• High-redshift galaxy groups as seen by Athena/WFI
• The SMBH mass versus M_G sigma^2 relation: A comparison between real data and numerical models
• Compactness of Cold Gas in High-Redshift Galaxies
• Observational evidence for AGNs feedback at parsec scale
• When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath$z\gtrsim 1$
• The Effect of Assembly Bias on Redshift Space Distortions
• Predictions of Quasar Clustering: Redshift, Luminosity and Selection Dependence
• The Impact of Environment on Late Time Evolution of the Stellar Mass - Halo Mass Relation
• Multi-Scale Morphological Analysis of SDSS DR5 Survey using the Metric Space Technique
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• Reproducible $k$-means clustering in galaxy feature data from the GAMA survey
• Non-Gaussianity of the Cosmic Infrared Background anisotropies II : Predictions of the bispectrum and constraints forecast
• The Relative Growth of Black Holes and of the Stellar Components of Galaxies
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• The mass-dependent star formation histories of disk galaxies: infall model versus observations
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• The Clusters Hiding in Plain Sight (CHiPS) survey: Complete sample of extreme BCG clusters
• Jet-Intracluster Medium interaction in Hydra A. I Estimates of jet velocity from inner knots
• A new method for testing isotropy with Shannon entropy
• Cosmological growth and feedback from supermassive black holes
• A search of CO emission lines in blazars: the low molecular gas content of BL Lac objects compared to quasars
• Identifying dynamically young galaxy groups via wide-angle tail galaxies: A case study in the COSMOS field at z=0.53
• The evolution of the gas fraction of quiescent galaxies modeled as a consequence of their creation rate
• Radio Source Evolution on Galactic Scales
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• SALT spectroscopic observations of galaxy clusters detected by ACT and a Type II quasar hosted by a brightest cluster galaxy
• Gas outflows in Seyfert galaxies: effects of star formation versus AGN feedbacks
• Why are classical bulges more common in S0 galaxies than in spiral galaxies?
• Star formation in mergers with cosmologically motivated initial conditions
• A 1-dimensional hydrodynamic model for accretion, cooling and heating of gas in dark matter halos from $z=6$ to $z=0$
• A rare example of low surface-brightness radio lobes in a gas-rich early-type galaxy: the story of NGC 3998
• Probing Plasma Physics with Spectral Index Maps of Accreting Black Holes on Event Horizon Scales
• Strongly lensed neutral hydrogen emission: detection predictions with current and future radio interferometers
• Faint, Evolving Radio AGN in SDSS Luminous Red Galaxies
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• The effect of gas-dynamics on semi-analytic modeling of cluster galaxies
• Dead or Alive? How Bursty Star Formation and Patchy Dust Can Cause Temporary Quiescence in High Redshift Galaxies
• The impact of a young radio galaxy: clues from the cosmic-ray electron population
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
• The [CII] 158 $\mu$m emission line as a gas mass tracer in high redshift quiescent galaxies
• The strong environmental dependence of black hole scaling relations
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Discovery of five low luminosity active galactic nuclei at the centre of the Perseus cluster
• Using Real and Simulated Measurements of the Thermal Sunyaev-Zel'dovich Effect to Constrain Models of AGN Feedback
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Fluctuation Spectroscopy: A New Probe of Old Stellar Populations
• Stellar Populations of Luminous Evolved Galaxies at z~1.5
• The Properties of Radio and Mid-infrared Detected Galaxies and the Effect of Environment on the Co-evolution of AGN and Star Formation at $z\sim 1$
• Exploring the AGN-Merger Connection in Arp 245 I: Nuclear Star Formation and Gas Outflow in NGC 2992
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Transitive X-ray spectrum and PeV gamma-ray cutoff in the M87 jet: Electron "Pevatron"
• Revealing a Highly-Dynamic Cluster Core in Abell 1664 with Chandra
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• The Massive and Distant Clusters of WISE Survey V: Extended Radio Sources in Massive Galaxy Clusters at z~1
• MeerKAT discovers a jet-driven bow shock near GRS 1915+105. How an invisible large-scale jet sculpts a microquasar's environment
• AGN feedback in clusters: shock and sound heating
• The Cosmic Evolution of Halo Pairs: I. Global Trends
• Chemo-dynamical simulations of dwarf galaxy evolution
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• Knot in Cen A: Stochastic Magnetic Field for Diffusive Synchrotron Radiation?
• The host galaxies of micro-Jansky radio sources
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• The evolution of the density of galaxy clusters and groups: denser environments at higher redshifts
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• Dark-ages reionization and galaxy formation simulation -- XVIII. The high-redshift evolution of black holes and their host galaxies
• X-Ray Bright Active Galactic Nuclei in Local Dwarf Galaxies: Insights from eROSITA
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) cluster survey IV: Superclusters in the local Universe at z <= 0.03
• Role of ionizing background on the statistics of metal absorbers in hydrodynamical simulations
• A group-galaxy cross-correlation function analysis in zCOSMOS
• Stellar populations in superclusters of galaxies
• Evaluating hydrodynamical simulations with green valley galaxies
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• No evidence for excess AGN activity in recently quenched massive galaxies at cosmic noon
• Modeling active galactic nuclei: ongoing problems for the faint-end of the luminosity function
• Investigating the impact of quasar-driven outflows on galaxies at redshift 0.3-0.4
• Heating and enriching the intracluster medium
• Characteristic mass in galaxy quenching: environmental versus internal effects
• Observations of the High Redshift Universe
• Correlation function: biasing and fractal properties of the cosmic web
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• The Role of Nuclear Star Clusters in Enhancing Supermassive Black Hole Feeding Rates During Galaxy Mergers
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Analytic and numerical realisations of a disk galaxy
• Examining transitional galaxies to understand the role of clusters and their dynamical status in galaxy quenching
• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• Multiwavelength radio observations of a Brightest Cluster Galaxy at z=1.71: Detection of a modest Active Galactic Nucleus and evidence for extended star formation
• Massive spheroids can form in single minor mergers
• Testing galaxy formation models with galaxy stellar mass functions
• Is the observed high-frequency radio luminosity distribution of QSOs bimodal?
• Early Science Result from the Japanese Virtual Observatory: AGN and Galaxy Clustering at z = 0.3 to 3.0
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• Searching for molecular outflows in Hyper-Luminous Infrared Galaxies
• Exploring the relation between dust mass and galaxy properties using Dusty SAGE
• Supernovae-induced accretion and star formation in the inner kiloparsec of a gaseous disk
• X-ray analysis of SDSS J165202.60+172852.4, an obscured quasar with outflows at peak galaxy formation epoch
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Gamma-ray emission from spectrally resolved cosmic rays in galaxies
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model. II. The colour-density relation up to z=1.5
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• Possible Evidence of a Universal Radio/X-ray Correlation in a near-Complete Sample of Hard X-ray Selected Seyfert Galaxies
• Massive Quiescent Galaxies at z>3 in The Millennium Simulation Populated by A Semi-analytic Galaxy Formation Model
• What has quenched the massive spiral galaxies?
• Physical Conditions and Extension of the Coronal Line Region in IC 5063
• Galaxy formation with cold gas accretion and evolving stellar initial mass function
• CO in the ALMA Radio-Source Catalogue (ARC): the molecular gas content of radio galaxies as a function of redshift
• Galaxy triplets in Sloan Digital Sky Survey Data Release 7 - III. Analysis of Configuration and Dynamics
• VLA 1.4 GHz Catalogs of the Abell 370 and Abell 2390 Cluster Fields
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• On the dark matter haloes inner structure and galaxy morphology
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• The Ursa Major cluster redefined as a `supergroup'
• Identifying AGN's Balmer-Absorptions and stratified NLR kinematics in SDSSJ112611.63+425246.4
• RAiSE X: searching for radio galaxies in X-ray surveys
• Rest-frame ultra-violet spectra of massive galaxies at z=3: evidence of high-velocity outflows
• Relic jet activity in "Hanny's Voorwerp" revealed by the LOFAR Two metre Sky Survey
• RAD@home citizen science discovery of an AGN spewing a large unipolar radio bubble onto its merging companion galaxy
• The dependency of AGN infrared color-selection on source luminosity and obscuration: An observational perspective in CDFS and COSMOS
• AGNs at the cosmic dawn: predictions for future surveys from a $\Lambda$CDM cosmological model
• The optically-selected 1.4-GHz quasar luminosity function below 1 mJy
• Semi-Analytic Galaxy Formation in Massive Neutrino Cosmologies
• A Novel Method to Identify AGNs Based on Emission Line Excess and the Nature of Low-luminosity AGNs in the Sloan Digital Sky Survey: II - Nature of Low-luminosity AGNs
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Selecting and Modelling Remnant AGNs with Limited Spectral Coverage
• The relation between galaxy density and radio jet power for 1.4 GHz VLA selected AGN in Stripe 82
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
• The XXL Survey XI: ATCA 2.1 GHz continuum observations
• COSMOS-Web: A history of galaxy migrations over the stellar mass-star formation rate plane
• Cospatial Star Formation and Supermassive Black Hole Growth in $z\sim 3$ Galaxies: Evidence for In-situ Co-evolution
• Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim 4$ gas-rich halo
• This is not the feedback you have been looking for: nearby optical AGN rarely drive kpc-scale cold-gas outflows
• Feeding and feedback in the powerful radio galaxy 3C 120
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• Soft clustering analysis of galaxy morphologies: A worked example with SDSS
• A super-linear "radio-AGN main sequence'' links mean radio-AGN power and galaxy stellar mass since z$\sim$3
• Evolution of Starburst Galaxies in the Illustris Simulation
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Gas Accretion and Angular Momentum
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• On the Anticorrelation Between Galaxy Light Concentration and X-ray-to-Optical Flux Ratio
• The imprint of the thick stellar disc in the mid-plane of three early-type edge-on galaxies in the Fornax cluster
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Constraints on the densities and temperature of Seyfert 2 NLR
• No evidence for feedback: Unexceptional Low-ionization winds in Host galaxies of Low Luminosity Active Galactic Nuclei at Redshift z ~1
• Clustering of MgII absorption line systems around massive galaxies: an important constraint on feedback processes in galaxy formation
• The Roles of Mass and Environment in the Quenching of Galaxies
• Demographics of Tidal Disruption Events with L-Galaxies: I. Volumetric TDE rates and the abundance of Nuclear Star Clusters
• The Discovery of a Hidden Broad Line AGN in a Bulgeless Galaxy: Keck NIR Spectroscopic Observations of SDSS J085153.64+392611.76
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Galaxy evolution across the optical emission-line diagnostic diagrams?
• Do current X-ray observations capture most of the black-hole accretion at high redshifts?
• Bulgeless disks, dark galaxies, inverted color gradients, and other expected phenomena at higher z. The chromatic surface brightness modulation (CMOD) effect
• Quenching, bursting and galaxy shapes: colour transformation as a function of morphology
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Faraday rotation study of NGC 612 (PKS 0131-36): a hybrid radio source and its magnetised circumgalactic environment
• Very Large Array observations of the mini-halo and AGN feedback in the Phoenix cluster
• Unraveling the complex structure of AGN-driven outflows: IV. Comparing AGNs with and without strong outflows
• Consequences of dark matter self-annihilation for galaxy formation
• A new gas cooling model for semi-analytical galaxy formation models
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4
• Compact Galaxies at Intermediate Redshifts Quench Faster than Normal-sized Galaxies
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• Rest-frame UV single-epoch black hole mass estimates of low-luminosity AGN at intermediate redshifts
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• Optical Properties of Peaked Spectrum Radio Sources
• Episodic activities of supermassive black holes at redshift $z\le 2$: driven by mergers?
• Quenching or Bursting: Star Formation Acceleration--A New Methodology for Tracing Galaxy Evolution
• The mass dependence of structure, star formation rate, and mass assembly mode at 0.5<z< 2.5
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• A catalogue of faint local radio AGN and the properties of their host galaxies
• Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared
• Constraining UV Continuum Slopes of Active Galactic Nuclei With CLOUDY Models of Broad Line Region EUV Emission Lines
• Outflow and metallicity in the broad-line region of low-redshift active galactic nuclei
• Where Do Obscured AGN Fit in A Galaxy's Timeline?
• G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
• Properties of Galaxies around AGNs with Most Massive Supermassive Black Hole Revealed by the Clustering Analysis
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• Studying Large and Small Scale Environments of Ultraviolet Luminous Galaxies
• The $M-\sigma$ relation between supermassive black holes and their host galaxies
• On the Evolution of the Bi-Modal Distribution of Galaxies in the Plane of Specific Star Formation Rate versus Stellar Mass
• Molecular gas excitation and outflow properties of obscured quasars at z$\sim$0.1
• The extraordinary radio galaxy MRC B1221-423: probing deeper at radio and optical wavelengths
• Non-thermal filaments and AGN recurrent activity in the galaxy group Nest200047: a LOFAR, uGMRT, MeerKAT, VLA radio spectral analysis
• Cold Dust Emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: Dependence on Luminosity, Obscuration & AGN Activity
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Spectral age distribution for radio-loud active galaxies in the XMM-LSS field
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Using the Star Forming Main Sequence To Explore Quiescent Galaxies Across Cosmic Time
• The Host Galaxies of Radio AGN: New Views from Combining LoTSS and MaNGA Observations
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• The Size Evolution of Elliptical Galaxies
• Shocks and Spatially Offset Active Galactic Nuclei Produce Velocity Offsets in Emission Lines
• JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H${}_2$ in the radio galaxy 3C 326 N
• Misalignment between cold gas and stellar components in early-type galaxies
• Balancing the Baryon Budget: The fraction of the IGM due to Galaxy Mergers
• The extremely X-ray luminous radio-loud quasar CFHQS J142952+544717 at $z=6.18$ under Chandra high-angular resolution lens
• An empirical model to form and evolve galaxies in dark matter halos
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics
• The scale dependence of mass assembly in galaxies
• The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation
• The Influence of Environment on the Chemical Evolution in Low-mass Galaxies
• Ionized Gas Kinematics along the Large-Scale Radio Jets in Type 2 AGNs
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VII. Redshift Evolution of Radio Galaxy Environments at z=0.3-1.4
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• Evolution of the Sérsic Index up to z=2.5 from JWST and HST
• Rapidly varying accretion and AGN feedback
• Revisiting the Color-Color Selection: Submillimeter and AGN Properties of NUV-r-J Selected Quiescent Galaxies
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Census of Gaseous Satellites around Local Spiral Galaxies
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Modelling the evolution of galaxies as a function of environment
• Deviations from the Infrared-Radio Correlation in Massive, Ultra-compact Starburst Galaxies
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• Bimodal AGNs in Bimodal Galaxies
• On the Evolution of High-Redshift Active Galactic Nuclei
• The Circumgalactic Medium in Massive Halos
• The role of environment in low-level active galactic nucleus activity: no evidence for cluster enhancement
• Hard X-ray Irradiation Potentially Drives Negative AGN Feedback by Altering Molecular Gas Properties
• Ultimate Merging at z~0.1
• Jet-Feedback on kpc scales: a review
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• The Evolution of the Low-Frequency Radio AGN Population to $z\simeq 1.5$ in the ELAIS N1 Field
• A consistent model for both the HI and stellar mass functions of galaxies
• Alignment in the orientation of LOFAR radio sources
• The Infrared Luminosity Function of AKARI 90$\mu$m Galaxies in the Local Universe
• Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxies
• Quenching in the Right Place at the Right Time: Tracing the Shared History of Starbursts, AGNs, and Post-starburst Galaxies Using Their Structures and Multiscale Environments
• Starburst galaxies in semi-analytic models of galaxy formation and evolution
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• Winds and feedback from supermassive black holes accreting at low rates: Hydrodynamical treatment
• Active Galactic Nuclei and their Role in Galaxy Evolution: The Infrared Perspective
• Hydrodynamic simulations of the Disk of Gas Around Supermassive black holes (HDGAS) -I; Molecular Gas Dynamics
• The XXL Survey: XXXIV. Double irony in XXL-North. A tale of two radio galaxies in a supercluster at z = 0.14
• Relating galaxies across different redshift to study galaxy evolution
• JCMT/SCUBA-2 uncovers an excess of $850\mu$m counts on megaparsec scales around high-redshift quasars. Characterization of the overdensities and their alignment with the quasars' Ly$\alpha$ nebulae
• Lack of Correlations between Cold Molecular Gas and AGN Properties in Type 1 AGNs at $z\lesssim 0.5$
• Stellar Mass Profiles of Quiescent Galaxies in Different Environments at $z\sim 0$
• Role of Feedback in AGN-HOST Coevolution: A Study from Partially Obscured Active Galactic Nuclei
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• Quantifying the effect of black hole feedback from the central galaxy on the satellite populations of groups and clusters
• Spatial density fluctuations and selection effects in galaxy redshift surveys
• JWST/NIRSpec spectroscopy of intermediate-mass quiescent galaxies at $z\sim 3-4$
• A close-pair analysis of damp mergers at intermediate redshifts
• Radio continuum and X-ray emission from the most extreme FIR-excess galaxy NGC 1377: An extremely obscured AGN revealed
• Leaving the dark ages with AMIGA
• Abundance matching for low mass galaxies in the CDM and FDM models
• A Novel Method to Identify AGNs Based on Emission Line Excess and the Nature of Low-luminosity AGNs in the Sloan Digital Sky Survey: I - A Novel Method
• X-Ray-to-Radio Offset Inference from Low-Count X-Ray Jets
• The Ly$\alpha$, CIV, and HeII nebulae around J1000+0234: a galaxy pair at the center of a galaxy overdensity at $z=4.5$
• Heavily Reddened z~2 Type 1 Quasars II: H-alpha Star Formation Constraints from SINFONI IFU Observations
• A Direct Linkage Between AGN Outflows in The Narrow-line Regions and The X-ray Emission From The Accretion disks
• On merger bias and the clustering of quasars
• The Clusters Hiding in Plain Sight (CHiPS) survey: A first discovery of a massive nearby cluster around PKS1353-341
• The Fundamental Manifold of spiral galaxies: ordered versus random motions and the morphology dependence of the Tully-Fisher relation
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319
• Sub-Eddington super-massive black hole activity in Fornax early type galaxies
• Autocorrelations of stellar light and mass in the low-redshift Universe
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• The evolution of high-redshift massive black holes
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Measuring Transverse Motions for Nearby Galaxy Clusters
• Are many radio-selected BL Lacs radio quasars in disguise?
• Quantifying jet-interstellar medium interactions in Cyg X-1: Insights from dual-frequency bow shock detection with MeerKAT
• A Multi-wavelength Survey of AGN in Massive Clusters: AGN Distribution and Host Galaxy Properties
• Stellar hardening of massive black hole binaries: the impact of the host rotation
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• Predictions for LISA and PTA based on SHARK galaxy simulations
• An Absence of Radio-Loud Active Galactic Nuclei in Geometrically Flat Quiescent Galaxies: Implications for Maintenance-Mode Feedback Models
• Does a radio jet drive the massive multi-phase outflow in the ultra-luminous infrared galaxy IRAS 10565+2448?
• Black hole virial masses from single-epoch photometry: the miniJPAS test case
• Ongoing Star Formation In AGN Host Galaxy Disks: A View From Core-collapse Supernovae
• Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
• GABE: Galaxy Assembly with Binary Evolution
• Collimation of the kiloparsec-scale radio jets in NGC 2663
• Spatially Resolved Stellar Populations of Eight GOODS-South AGN at z~1
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Interchanging Interactive 3-d Graphics for Astronomy
• Semi-analytic galaxy formation in coupled dark energy cosmologies
• Correlation functions in 2D and 3D as descriptors of the cosmic web
• A Markov Chain Monte Carlo approach for measurement of jet precession in radio-loud active galactic nuclei
• Global structure of the Local Universe according to 2MRS survey
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• Ageing and Quenching through the ageing diagram II: physical characterization of galaxies
• The Grism Lens-Amplified Survey from Space (GLASS). XII. Spatially Resolved Galaxy Star Formation Histories and True Evolutionary Paths at z > 1
• On the dwarf galaxies rotation curves diversity problem
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• Entropy Limit and the Cold Feedback Mechanism in Cooling Flow Clusters
• Co-evolution of supermassive black holes with galaxies from semi-analytic model: stochastic gravitational wave background and black hole clustering
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• Probing the roles of orientation and multi-scale gas distributions in shaping the obscuration of Active Galactic Nuclei through cosmic time
• Double Trouble: Two spectroscopically confirmed low-mass quiescent galaxies at z>5 in overdensities
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Tracking galaxy evolution through low frequency radio continuum observations using SKA and Citizen-science Research using Multi-wavelength data
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Angular Momentum Evolution in Dark Matter Halos
• Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• Galaxy Formation and Dark Matter
• The radiative transfer of synchrotron radiation through a compressed random magnetic field
• RAiSERed: radio continuum redshifts for lobed AGNs
• Dynamical friction of a massive black hole in a turbulent gaseous medium
• A fundamental equation for Supermassive Black Holes
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• On the connection between AGN radiative feedback and massive black hole spin
• The XXL survey: XLII. Detection and characterization of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety
• Quantifying parameter errors due to the peculiar velocities of type Ia supernovae
• Does the Compact Radio Jet in PG 1700+518 Drive a Molecular Outflow?
• Fundamental properties of Fanaroff-Riley II radio galaxies investigated via Monte Carlo simulations
• Mapping the Spatial Distribution of Dust Extinction in NGC 959 Using Broadband Visible and mid-IR Filters
• Active galactic nuclei cores in infrared-faint radio sources: Very long baseline interferometry observations using the Very Long Baseline Array
• X-ray properties of K-selected galaxies at 0.5<z<2.0: Investigating trends with stellar mass, redshift and spectral type
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• The changing ISM of massive elliptical galaxies and cosmic evolution of radio galaxies and quasars
• Probing the link between quenching and morphological evolution
• Are compact groups hostile towards faint galaxies?
• Luminous satellite galaxies in gravitational lenses
• A Fresh Look at AGN Spectral Energy Distribution Fitting with the XMM-SERVS AGN Sample
• Spatially Extended [P II]1.188um and [Fe II]1.257um Emission Lines in a Nearby Seyfert Galaxy NGC 1068 Observed with OAO/ISLE
• On the reliability of photometric and spectroscopic tracers of halo relaxation
• Discovery of a spatially and kinematically resolved 55~kpc-scale superbubble inflated by an intermediate redshift non-BAL quasar
• Measuring the thermal and ionization state of the low-$z$ IGM using likelihood free inference
• Radio continuum emission and HI gas accretion in the NGC 5903/5898 compact group of early-type galaxies
• From haloes to galaxies. III. The gas cycle of local galaxy populations
• Electron Energy Distributions in the Extended Gas Nebulae associated with High-z AGN: Maxwell-Boltzmann vs. kappa distributions
• A Physical Model for the Quasar Luminosity Function Evolution between Cosmic Dawn and High Noon
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• A plausible link between dynamically unsettled molecular gas and the radio jet in NGC 6328
• The impact of the cosmological constant on past and future star formation
• MaNGA AGN dwarf galaxies (MAD) -- II. AGN outflows in dwarf galaxies
• Mid-infrared Spectral Properties of Post-Starburst Quasars
• Exploring the Active Galactic Nuclei population with extreme X-ray to optical flux ratios (Fx/Fo >50)
• AGN feedback in an infant galaxy cluster: the LOFAR-Chandra view of the giant FRII radio galaxy J103025+052430 at z=1.7
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• A deep learning approach to halo merger tree construction
• Red bulgeless galaxies in SDSS DR7. Are there any AGN hosts?
• Active Galactic Nuclei signatures in Red Geyser galaxies from Gemini GMOS-IFU observations
• Chemical evolution of elliptical galaxies I: supernovae and AGN feedback
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Critical Stellar Central Densities Drive Galaxy Quenching in the Nearby Universe
• Radio Galaxy 3C 230 Observed with Gemini Laser-Adaptive-Optics Integral-Field Spectroscopy
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• Positive and negative feedback by AGN jets in high-redshift galaxies
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Classical bulges, supermassive blackholes and AGN feedback: Extension to low-mass galaxies
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• Identifications of FIRST radio sources in the NOAO Deep-Wide Field Survey
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• An Evolutionary Sequence of Young Radio Galaxies
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
• The Many Assembly Histories of Massive Void Galaxies as Revealed by Integral Field Spectroscopy
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Central gas entropy excess as a direct evidence for AGN feedback in galaxy groups and clusters
• The growth of disks and bulges during hierarchical galaxy formation. II: metallicity, stellar populations and dynamical evolution
• The Origin of Star Formation in Early-type Galaxies Inferred from Spatially Resolved Spectroscopy
• A Hubble Space Telescope Imaging Study of Four FeLoBAL Quasar Host Galaxies
• The mass-size relation of LRGs from BOSS and DECaLS
• Properties of AGN selected by their mid-IR colours: evidence for a physically distinct mode of black hole growth
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Spitzer IRS observations of k+a galaxies: A link between PAH emission properties and AGN feedback?
• The Occurrence of Compact Groups of Galaxies Through Cosmic Time
• A Model of the Cosmic Infrared Background Produced by Distant Galaxies
• A general approach to quenching and galactic conformity
• Evolution of black hole and galaxy growth in a semi-numerical galaxy formation model
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• The origin of redshift asymmetries: How LambdaCDM explains anomalous redshift
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Dark Matter Annihilation Feedback in cosmological simulations I: Code convergence and idealised halos
• The optical vs. mid-infrared spectral properties of 82 Type 1 AGNs: coevolution of AGN and starburst
• Universal bimodality in kinematic morphology and the divergent pathways to galaxy quenching
• Disk Galaxy Evolution Along the Hubble Sequence
• Deep spectroscopy of 9C J1503+4528: a very young CSS radio source at z=0.521
• Astraeus VII: The environmental-dependent assembly of galaxies in the Epoch of Reionization
• Infall Profiles for Supercluster-Scale Filaments
• Simulating Kilonovae in the ΛCDM Universe
• Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
• Feeding and Feedback in nearby AGN - Comparison with the Milky Way center
• An Ising model for galaxy bias
• Testing a prediction of the merger origin of early-type galaxies: a correlation between stellar populations and asymmetry
• The Physical Characteristics of Interstellar Medium in NGC 3665 with Herschel Observations
• The Degeneracy of Galaxy Formation Models
• Far-UV Emission Properties of FR1 Radio Galaxies
• What is the origin of the JWST SMBHs?
• The evolution of baryonic mass function of galaxies to z=3
• COSMOS2020: Disentangling the Role of Mass and Environment in Star Formation Activity of Galaxies at $0.4<z<4$
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• AGN STORM 2: I. First results: A Change in the Weather of Mrk 817
• Eight luminous early-type galaxies in nearby pairs and sparse groups I. Stellar populations spatially analysed
• A Census of Mid-Infrared Selected Active Galactic Nuclei in Massive Galaxy Clusters at 0 < z < 1.3
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Modeling the Alignment Profile of Satellite Galaxies in Clusters
• Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• Astrophysics with the Laser Interferometer Space Antenna
• Galaxy luminosity function and its cosmological evolution: Testing a new feedback model depending on galaxy-scale dust opacity
• Numerical Simulation of Star Formation by the Bow Shock of the Centaurus A Jet
• Does Feedback from Supermassive Blackhole Co-evolve With Host In Type 2 Quasars?
• NIHAO XXVII: Crossing the green valley
• M31 circum-nuclear region: a molecular survey with the IRAM-interferometer
• Machine Learning the Fates of Dark Matter Subhalos: A Fuzzy Crystal Ball
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• Clusters and Groups of Galaxies in the Simulated Local Universe
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Feeding and feedback from little monsters: AGN in dwarf galaxies
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Galaxy And Mass Assembly (GAMA): $\mathbf{z}\sim 0$ Galaxy Luminosity Function down to $\mathbf{L}\sim 10^6{\mathbf{L}}_{\odot }$ via Clustering Based Redshift Inference
• JWST Discovery of a Very Fast Biconical Outflow of Warm Molecular Gas in the Nearby Ultra-Luminous Infrared Galaxy F08572+3915 NW
• Connecting Star Formation Quenching with Galaxy Structure and Supermassive Black Holes through Gravitational Heating of Cooling Flows
• Temporal Self-Organization in Galaxy Formation
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• Large scale correlations in gas traced by MgII absorbers around low mass galaxies
• Dissecting the star-formation history of starburst galaxies: the case of NGC7673
• Magnetic fields in galaxies: I. Radio disks in local late-type galaxies
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Red Dragon: A Redshift-Evolving Gaussian Mixture Model for Galaxies
• Central star formation in an early-type galaxy I~Zw~81 in the Bootes void
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• Detecting quasars at very high redshift with next generation X-ray telescopes
• MEGADES: MEGARA Galaxy Discs Evolution Survey. Data Release I: central fields
• The environments of the radio galaxy population in SIMBA
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
• Spherical accretion in giant elliptical galaxies: multi-transonicity, shocks, and implications on AGN feedback
• Galaxy formation from a timescale perspective
• The Performance of Photometric Reverberation Mapping at High Redshift and the Reliability of Damped Random Walk Models
• Thinking outside the halo: Tracing the large-scale distribution of diffuse cosmic metals with semi-analytic models
• Gravitational fluctuations of the galaxy distribution
• The Active Nucleus of IC4970: A Nearby Example of Merger-Induced Cold-Gas Accretion
• The Co-Evolution of Galaxies and Black Holes: Current Status and Future Prospects
• Suppression of Star Formation in the Hosts of Low-Excitation Radio Galaxies
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• A study on the multicolour evolution of Red Sequence galaxy populations: insights from hydrodynamical simulations and semi-analytical models
• Virgo Filaments V: Disrupting the Baryon Cycle in the NGC 5364 Galaxy Group
• Disentangling the Dynamical Mechanisms for Cluster Galaxy Evolution
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• The global energetics of radio AGN kinetic feedback in the local universe
• Statistical and dynamical decoupling of the IGM from Dark Matter
• Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
• Quenching of Galaxies at Cosmic Noon: Understanding the Effect of Environment
• Red riding on hood: Exploring how galaxy colour depends on environment
• Insights into environmental quenching at $z\sim 1$: an enhancement of faint, low-mass passive galaxies in clusters
• Building Blocks of the Milky Way's Accreted Spheroid
• Spatial variations of magnetic field along active galactic nuclei jets on sub-pc to Mpc scales
• LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• On the exclusion of intra-cluster plasma from AGN-blown bubbles
• Central star formation in double-peak gas rich radio galaxies
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• Making use of sub-resolution halos in N-body simulations
• Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ~ 1.4
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• The Formation and Evolution of Massive Galaxies
• Massive Black Hole Mergers
• Quasar emission lines, radio structures and radio unification
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Polarization and variability of compact sources measured in Planck time-ordered data
• A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• Digging deeper into NGC\,6868 I: stellar population
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• HI 21-cm absorption in radio-loud AGN with double-peaked [OIII] emission
• Quasars Have Fewer Close Companions than Normal Galaxies
• An Improved Treatment of Cosmological Intergalactic Medium Evolution
• Reconstructing the LISA massive black hole binary population via iterative kernel density estimation
• Dynamical response to supernova-induced gas removal in spiral galaxies with dark matter halo
• Rest-Frame Ultraviolet to Near Infrared Observations of an Interacting Lyman Break Galaxy at z = 4.42
• Exploring the Dependence of Gas Cooling and Heating Functions on the Incident Radiation Field with Machine Learning
• Evidence for AGN-Regulated Cooling in Clusters at $z\sim 1.4$: A Multi-Wavelength View of SPT-CL J0607-4448
• The EDGE-CALIFA survey: The effect of active galactic nucleus feedback on the integrated properties of galaxies at different stages of their evolution
• Gaseous Flows in Galaxies
• A systematic study of AGN feedback in a disk galaxy I: global overview
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• A New Multi-Scale Structure Finding Algorithm to Identify Cosmological Structure
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Fast radio bursts as probes of feedback from active galactic nuclei
• The Impact of Baryons on the Large-Scale Structure of the Universe
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• The LOFAR view of massive early-type galaxies: Transition from radio AGN to host emission
• Using Machine Learning to Determine Morphologies of $z<1$ AGN Host Galaxies in the Hyper Suprime-Cam Wide Survey
• The Physical Properties of Galaxies with Unusually Red Mid-Infrared Colours
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Solving the puzzle of subhalo spins
• Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Black hole growth and stellar assembly at high-z
• Barions and $\Lambda$CDM Model Problems
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• Using dust to constrain dark matter models
• No Evidence of Quasar-Mode Feedback in a Four-Way Group Merger at z~0.84
• The first high-redshift cavity power measurements of cool-core galaxy clusters with the International LOFAR Telescope
• Exploring the Cosmic Web in the Sloan Digital Sky Survey Data Release Seven using the Local Dimension
• Beyond the Halo: Redefining environment with unbound matter in N-body simulations
• From Nearby Low Luminosity AGN to High Redshift Radio Galaxies: Science Interests with SKA
• Growth and Feedback from the First Black Holes
• A study of the scaling relation $M_{\bullet }\propto R_e{\sigma }^3$ for supermassive black holes and an update of the corresponding theoretical model
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• Star Formation in CALIFA survey perturbed galaxies. II. Star Formation Histories and Oxygen Abundances
• Seeking for the leading actor on the cosmic stage: Galaxies versus Supermassive Black Holes
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• Detection of H-alpha emission from z>3.5 submillimetre luminous galaxies with AKARI-FUHYU spectroscopy
• The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
• The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
• The Diversity of Environments Around Luminous Quasars at Redshift $z\sim 6$
• The physical properties and the evolution of the interacting system AM1204-292
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• Observations and Simulations of Radio Emission and Magnetic Fields in Minkowski's Object
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• Ultra-violet photo-ionisation in far-infrared selected sources
• The time evolution of bias
• Highly ionized gas on galaxy scales: mapping the interacting Seyfert galaxy LEDA 135736
• Black Hole masses for 14 gravitational lensed quasars
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• Method for Determining AGN Accretion Phase in Field Galaxies
• LeMMINGs. V. Nuclear activity and bulge properties: a detailed multi-component decomposition of $e$-MERLIN Palomar galaxies with $HST$
• Triplets of Quasars at high redshift I: Photometric data
• A Swift X-ray view of the SMS4 sample -- II: X-ray properties of 17 bright radio sources
• Does stellar mass assembly history vary with environment?
• Dust contribution to the panchromatic galaxy emission
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• The relation of galaxies and dark matter haloes to the filamentary cosmic web
• Automatic Machine Learning Framework to Study Morphological Parameters of AGN Host Galaxies within $z<1.4$ in the Hyper Supreme-Cam Wide Survey
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• The galaxy-environment connection revealed by constrained simulations
• Long-term implications of observing an expanding cosmological civilization
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Cool gas accretion, thermal evaporation and quenching of star formation in elliptical galaxies
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• Structural diversity of disc galaxies originating in the cold gas inflow from cosmic webs
• Lower-Luminosity Obscured AGN Host Galaxies are Not Predominantly in Major-Merging Systems at Cosmic Noon
• An ACA 1mm survey of HzRGs in the ELAIS-S1: survey description and first results
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• The Two-Point Correlation of 2QZ Quasars and 2SLAQ LRGs: From a Quasar Fueling Perspective
• A Bending in the Size-mass Relation of Star-forming Galaxies across $0.5<z<6.0$ at a Critical Stellar Mass of $10^{10}{M}_{\odot }$ Revealed by JWST
• Major merger fraction along the massive galaxy quenching channel at 0.2$<z<$0.7
• Photometric variability in star-forming galaxies as evidence for low-mass AGN and a precursor to quenching
• Why and when is internally-driven AGN feedback energetically favoured?
• The Quasar Candidates Catalogs of DESI Legacy Imaging Survey Data Release 9
• Witnessing the formation of a brightest cluster galaxy at z>2
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• Imaging and photometric studies of NGC 1316 (Fornax A) using Astrosat/UVIT
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• Constraints on the galaxy formation models during epoch of reionization with high redshift observations
• Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9
• The Sharpest Ultraviolet view of the star formation in an extreme environment of the nearest Jellyfish Galaxy IC 3418
• Influences of galaxy interactions on AGN activity
• Upcoming SKA precursor surveys and sensitivity to HI mass function
• Host galaxy and nuclear properties of IR-selected AGNs with and without outflow signatures
• Hydrostatic equilibrium of a porous intracluster medium: implications for mass fraction and X-ray luminosity
• Testing the role of AGN on the star formation and metal enrichment of "twin galaxies"
• Capivara: A Spectral-based Segmentation Method for IFU Data Cubes
• A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon
• Dynamical properties and star formation history of a low-mass quenched galaxy at Cosmic Noon
• The scientific potential of space-based gravitational wave detectors
• Formation and evolution of disk galaxies
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• The progenitor galaxies of stellar haloes as "failed" Milky Ways
• Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
• Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
• X-ray luminosity functions of different morphological and X-ray type AGN populations
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• Three-Dimensional Filamentation Analysis of SDSS DR5 Survey
• What halts the growth of galaxies?
• Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties
• The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim 1$
• Feeding and feedback in nuclei of galaxies
• Detection of helicoidal motion in the optical jet of PKS 0521-365
• Investigating possible unification of Seyfert galaxies and blazars in Fermi-LAT sample
• An isolated early-type dwarf galaxy that ran away from the group environment
• The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
• Predicting halo occupation and galaxy assembly bias with machine learning
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Properties of Interstellar Medium in the S0 Galaxy NGC 1222: Evidence for Shocked-enhanced Line Emission
• The nature of the variable millimetre-selected AGN in the Brightest Cluster Galaxy of Abell 851
• Cosmological evolution of the AGN Kinetic Luminosity Function
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• On the fairness of the main galaxy sample of SDSS
• Wide Field Multiband Imaging of Low Redshift Quasar Environments
• The AURORA Survey: Tracing Galactic Outflows at $z\gtrsim 2.5$ with JWST/NIRSpec NUV Absorption Lines
• Main sequence of star formation and colour bimodality considering galaxy environment
• The highly obscured Seyfert 2 nucleus in NGC 1448 observed with MUSE
• Dust removal timescale in galaxies across cosmic time
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• On the signature of black holes on the quenched stellar mass function
• Digging deeper into NGC 6868 II: ionized gas and excitation mechanism
• Extended Hernquist-Springel formalism for cosmic star formation
• The richest superclusters. I. Morphology
• The landscape of massive black-hole spectroscopy with LISA and Einstein Telescope
• The impact of AGN on their host galaxies
• Angular momentum and morphological sequence of massive galaxies through Dark Sage
• AGN Absorption Linked to Host Galaxies
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• ReveaLLAGN 1: JWST Emission-Line Spectra Reveal Low-Luminosity AGN with UV-Deficient SEDs and Warm Molecular Gas
• Blueberry and Green Pea galaxies live in low density environments
• Time-Dependent Cosmic Ray Halos from Bursty Star Formation and Active Galactic Nuclei: Semi-Analytic Formalism and Galaxy Formation Implications
• Ultra-fast model emulation with PRISM; analyzing the Meraxes galaxy formation model
• Red Galaxies from Hot Halos in Cosmological Hydro Simulations
• Mutual feedback between star formation and nuclear activity
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Physical Drivers of Emission Line Diversity of SDSS Seyfert 2s and LINERs After Removal of Contributions by Star Formation
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Quasar clustering at redshift 6
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• The Nature of Hyperluminous Infrared Galaxies
• Spheroid ages, kinematics and BH relations
• Ageing and Quenching: Influence of Galaxy Environment and Nuclear Activity in Transition Stage
• A Mass Dependent Density Profile from Dwarfs to Clusters
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• Physical conditions in Centaurus A's northern filaments II: Does the HCO${}^{+}$ emission highlight the presence of shocks?
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Capturing dual AGN activity and kiloparsec-scale outflows in IRAS 20210+1121
• Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers
• COSMOS2025: A Machine Learning Census of Massive Quiescent Galaxies at $2.5<\text{z}<5$
• The AGN content of deep radio surveys and radio emission in radio-quiet AGN. Why every astronomer should care about deep radio fields
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
• Suppression of galactic outflows by cosmological infall and circumgalactic medium
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• SMA Observations of the Archetypal Compact Steep-spectrum Radio Source 3C 303.1
• Now you see it, now you don't: Star formation truncation precedes the loss of molecular gas by ~100 Myr in massive post-starburst galaxies at z~0.6
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• The splash beneath the largest radio bubble in a cluster core
• GA-NIFS: AGN activity in a Lyα emitter within a triple-AGN system anchored by a passive galaxy at z=3
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• Galaxy catalogs from the SAGE Semi-Analytic Model calibrated on THE THREE HUNDRED hydrodynamical simulations: A method to push the limits toward lower mass galaxies in dark matter only clusters simulations
• The Star Formation History and Stellar Assembly of High Redshift Galaxies
• Citations to Australian Astronomy: 5 and 10 Year Benchmarks
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• Disk Sizes in a LCDM Universe
• An empirical model of the extragalactic radio background
• What excites the optical emission in X-ray-selected galaxies?
• Growing supermassive black holes: sub-grid modelling and intermediate-scale processes
• Using strong lensing to understand the microJy radio emission in two radio quiet quasars at redshift 1.7
• Investigating the spectra and physical nature of galaxy scale jets
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• The GLEAM 4-Jy (G4Jy) Sample: IV. Multiwavelength data and analysis
• The Baryon Budget of Galaxies across the First Billion Years
• Massive black holes and their galaxies
• The kinematic imprinting of environmental quenching in $z<0.2$ galaxies
• The origin of ionized gas in retired galaxies: dynamical clues
• Mentari: A pipeline to model the galaxy SED using semi analytic models
• Estimating Transient Rates from Cosmological Simulations and BPASS
• White dwarfs in the building blocks of the Galactic spheroid
• Star-forming S0 Galaxies in SDSS-MaNGA: fading spirals or rejuvenated S0s?
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Black Holes and Baryon Number Violation: Unveiling the Origins of Early Galaxies and the Low-Mass Gap
• Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies