The broken hierarchy of galaxy formation

Abstract

Recent observations of the distant Universe suggest that much of the stellar mass of bright galaxies was already in place at $z>1$. This presents a challenge for models of galaxy formation because massive halos are assembled late in hierarchical cosmologies such as cold dark matter (CDM). In this paper, we discuss a new implementation of the Durham semi-analytic model in which feedback due to active galactic nuclei (AGN) is assumed to quench cooling flows in massive halos. This mechanism naturally creates a break in the local galaxy luminosity function at bright magnitudes. The model is implemented within the Millennium N-body simulation; the accurate dark matter merger trees and large number of realizations of the galaxy formation process that the simulation provides results in highly accurate statistics. After adjusting the values of the physical parameters in the model by reference to the properties of local galaxies, we use it to investigate the evolution of the K-band luminosity and galaxy stellar mass functions. We also calculate the volume averaged star formation rate density of the Universe as a function of redshift and the way in which this is apportioned amongst galaxies of different mass. The model robustly predicts a substantial population of massive galaxies out to redshift $z\sim 5$ and a star formation rate density which rises with increasing redshift in objects of all masses. Although observational data on these properties have been cited as evidence for ``anti-hierarchical'' galaxy formation, we find that when AGN feedback is taken into account, the fundamentally hierachical CDM model provides a very good match to these observations.

11 pages, 8 colour figures. Accepted for publication in MNRAS. Galaxy catalogues are available for down load from http://www.icc.dur.ac.uk/

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• The Herschel census of infrared SEDs through cosmic time
• Energetics of the molecular gas in the H_2 luminous radio galaxy 3C 326: Evidence for negative AGN feedback
• The Dawn of the Red: Star formation histories of group galaxies over the past 5 billion years
• The evolution of post-starburst galaxies from z=2 to z= 0.5
• A fundamental problem in our understanding of low mass galaxy evolution
• Predictions for the CO emission of galaxies from a coupled simulation of galaxy formation and photon dominated regions
• The Atomic to Molecular Transition and its Relation to the Scaling Properties of Galaxy Disks in the Local Universe
• The nature of star formation in distant ultraluminous infrared galaxies selected in a remarkably narrow redshift range
• On the role of AGN feedback on the thermal and chemodynamical properties of the hot intra-cluster medium
• Cosmic evolution of radio selected active galactic nuclei in the COSMOS field
• Strong lensing optical depths in a \LambdaCDM universe
• The baryon fraction of LambdaCDM haloes
• Black Hole Growth in Hierarchical Galaxy Formation
• The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model
• The ACS Fornax Cluster Survey. VI. The Nuclei of Early-Type Galaxies in the Fornax Cluster
• A Stochastic Model for the Luminosity Fluctuations of Accreting Black Holes
• Global structure and kinematics of stellar haloes in cosmological hydrodynamic simulations
• Cosmic evolution of stellar quenching by AGN feedback: clues from the Horizon-AGN simulation
• AGN-driven outflows without immediate quenching in simulations of high-redshift disk galaxies
• 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
• Inside the Bondi radius of M87
• A Ten Billion Solar Mass Outflow of Molecular Gas Launched by Radio Bubbles in the Abell 1835 Brightest Cluster Galaxy
• SDSS DR7 superclusters. The catalogues
• How supernova explosions power galactic winds
• The Different Physical Mechanisms that Drive the Star-Formation Histories of Giant and Dwarf Galaxies
• How do central and satellite galaxies quench? -- Insights from spatially resolved spectroscopy in the MaNGA survey
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters
• A new measurement of the evolving near-infrared galaxy luminosity function out to z~4: a continuing challenge to theoretical models of galaxy formation
• 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
• 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
• The evolution of the mass-size relation for early type galaxies from z~1 to the present: dependence on environment, mass-range and detailed morphology
• The VLA-COSMOS 3~GHz Large Project: Cosmic evolution of radio AGN and implications for radio-mode feedback since z~5
• Satellite abundances around bright isolated galaxies
• Is AGN feedback necessary to form red elliptical galaxies?
• Are galactic star formation and quenching governed by local, global or environmental phenomena?
• The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
• Star formation quenching in massive galaxies
• LoCuSS: The steady decline and slow quenching of star formation in cluster galaxies over the last four billion years
• Galaxy evolution in overdense environments at high redshift: passive early-type galaxies in a cluster at redshift 2
• Accelerating AGN jets to parsec scales using general relativistic MHD simulations
• The Star Formation Epoch of the Most Massive Early-Type Galaxies
• The role of mergers in driving morphological transformation over cosmic time
• Substructure of the galaxy clusters in the REXCESS sample: observed statistics and comparison to numerical simulations
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function to $z=0.1$ from the r-band selected equatorial regions
• Gravitational Heating Helps Make Massive Galaxies Red and Dead
• The formation and evolution of low-surface-brightness galaxies
• HBT+: an improved code for finding subhalos and building merger trees in cosmological simulations
• Evolution of the Stellar-to-Dark Matter Relation: Separating Star-Forming and Passive Galaxies from z=1 to 0
• The answer is blowing in the wind: Simulating the interaction of jets with dynamic cluster atmospheres
• The mass of the black hole in Centaurus A from SINFONI AO-assisted integral-field observations of stellar kinematics
• Host galaxies of luminous z$\sim$0.6 quasars: Major mergers are not prevalent at the highest AGN luminosities
• Dark-ages reionization and galaxy formation simulation - III. Modelling galaxy formation and the epoch of reionization
• The Concentration Dependence of the Galaxy-Halo Connection: Modeling Assembly Bias with Abundance Matching
• Confronting theoretical models with the observed evolution of the galaxy population out to z=4
• Virialization of the inner CGM in the FIRE simulations and implications for galaxy discs, star formation and feedback
• Downsizing by Shutdown in Red Galaxies
• On the SFR-M${}_{\ast }$ main sequence archetypal star-formation history and analytical models
• An X-ray survey of the 2Jy sample. I: is there an accretion mode dichotomy in radio-loud AGN?
• On the Origin of Cores in Simulated Galaxy Clusters
• Feedback from Active Galactic Nuclei in Galaxy Groups
• Resolving the Discrepancy of Galaxy Merger Fraction Measurements at z ~ 0 - 3
• AEGIS: New Evidence Linking Active Galactic Nuclei to the Quenching of Star Formation
• Two Conditions for Galaxy Quenching: Compact Centres and Massive Haloes
• The XMM Cluster Survey: Active Galactic Nuclei and Starburst Galaxies in XMMXCS J2215.9-1738 at z=1.46
• Galaxy Zoo: The Environmental Dependence of Bars and Bulges in Disc Galaxies
• The flip-side of galaxy formation: A combined model of Galaxy Formation and Cluster Heating
• Environmentally-Driven Evolution of Simulated Cluster Galaxies
• The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations
• Bulge-forming galaxies with an extended rotating disk at z~2
• SDSS IV MaNGA: The global and local stellar mass assemby histories of galaxies
• Numerical Relativity and Astrophysics
• Blowing cold flows away: the impact of early AGN activity on the formation of a brightest cluster galaxy progenitor
• Cluster Galaxies Die Hard
• The duty cycle of local radio galaxies
• Are Radio AGN Powered by Accretion or Black Hole Spin?
• Radio Jets in Galaxies with Actively Accreting Black Holes: new insights from the SDSS
• Evidence for a change in the dominant satellite galaxy quenching mechanism at z=1
• The Argo Simulation: I. Quenching of Massive Galaxies at High Redshift as a Result of Cosmological Starvation
• A mid-infrared spectroscopic study of submillimeter galaxies: luminous starbursts at high redshift
• The Parameter Space of Galaxy Formation
• Searching for Evidence of Energetic Feedback in Distant Galaxies: A Galaxy Wide Outflow in a z~2 Ultraluminous Infrared Galaxy
• Origin of the anti-hierarchical growth of black holes
• 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
• The Stellar Mass Density at z~6 from Spitzer Imaging of i-drop 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
• X-rays across the galaxy population - III. The incidence of AGN as a function of star formation rate
• On the Stellar Masses of IRAC detected Lyman Break Galaxies at z~3
• The 2dF-SDSS LRG and QSO survey: evolution of the clustering of luminous red galaxies since z = 0.6
• A submillimetre galaxy at z=4.76 in the LABOCA survey of the Extended Chandra Deep Field South
• A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole
• The (black hole)-bulge mass scaling relation at low masses
• How to quench a galaxy
• The SINS/zC-SINF Survey of z~2 Galaxy Kinematics: The Nature of Dispersion Dominated Galaxies
• Interactions, star formation and AGN activity
• Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach
• Galaxy And Mass Assembly (GAMA): The large scale structure of galaxies and comparison to mock universes
• Galaxies that Shine: radiation-hydrodynamical simulations of disk galaxies
• SDSS-IV MaNGA: Evidence of the importance of AGN feedback in low-mass galaxies
• Adding Environmental Gas Physics to the Semi-Analytic Method for Galaxy Formation: Gravitational Heating
• The influence of the environmental history on quenching star formation in a $\Lambda$CDM universe
• What Does Clustering Tell Us About the Buildup of the Red Sequence?
• Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift
• On the origin of radio-loudness in AGNs and its relationship with the properties of the central supermassive black hole
• Understanding the H2/HI Ratio in Galaxies
• The Dependence of the Mass Assembly History of Cold Dark Matter Halos on Environment
• The Energetics and Lifetimes of Local Radio Active Galactic Nuclei
• 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 splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• Clustering of obscured and unobscured quasars in the Bootes field: Placing rapidly growing black holes in the cosmic web
• H0LiCOW III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435-1223 through weighted galaxy counts
• Extended Hot Halos Around Isolated Galaxies Observed in the ROSAT All-Sky Survey
• Galaxy morphology in the LambdaCDM cosmology
• Stellar mass functions: methods, systematics and results for the local Universe
• AGN self-regulation in cooling flow clusters
• Evolution of the Most Massive Galaxies to z=0.6: I. A New Method for Physical Parameter Estimation
• The XMM Cluster Survey: The build up of stellar mass in Brightest Cluster Galaxies at high redshift
• 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
• MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3
• Estimating the dark matter halo mass of our Milky Way using dynamical tracers
• 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
• A Spectacular H$\alpha$ Complex in Virgo: Evidence for a Collision Between M86 and NGC 4438 and Implications for Collisional ISM Heating of Ellipticals
• Hot gas in massive halos drives both mass quenching and environment quenching
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• 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
• Approximate Bayesian Computation for Astronomical Model Analysis: A Case Study in Galaxy Demographics and Morphological Transformation at High Redshift
• Radio imaging of the Subaru/XMM-Newton Deep Field - III. Evolution of the radio luminosity function beyond z=1
• Barred galaxies in the EAGLE cosmological hydrodynamical simulation
• The Properties of Sub-mm Galaxies in Hierarchical Models
• 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
• A Bayesian approach to the semi-analytic model of galaxy formation: methodology
• Satellites of Simulated Galaxies: survival, merging, and their relation to the dark and stellar halos
• Evolution of the Radio Loud Galaxy Population
• Halo masses for optically-selected and for radio-loud AGN from clustering and galaxy-galaxy lensing
• A Connection Between Bulge Properties and the Bimodality of Galaxies
• The Demography of Super-Massive Black Holes: Growing Monsters at the Heart of Galaxies
• The Environments of Active Galactic Nuclei within the zCOSMOS Density Field
• The radial distribution of galaxies in groups and clusters
• Modelling galaxy clustering: halo occupation distribution versus subhalo matching
• The Fraction of Quiescent Massive Galaxies in the Early Universe
• AEGIS: The Morphologies of Green Galaxies at 0.4<z<1.2
• On the puzzling plateau in the specific star formation rate at z=2-7
• LoCuSS: The mid-infrared Butcher-Oemler effect
• The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $\Lambda$CDM
• Quenching as a Contest between Galaxy Halos and their Central Black Holes
• Diffuse stellar component in galaxy clusters and the evolution of the most massive galaxies at z<~1
• ALLSMOG: an APEX Low-redshift Legacy Survey for MOlecular Gas. I - molecular gas scaling relations, and the effect of the CO/H2 conversion factor
• The Co-Formation of Spheroids and Quasars Traced in their Clustering
• Direct Evidence for Termination of Obscured Star Formation by Radiatively Driven Outflows in Reddened QSOs
• Specific star-formation and the relation to stellar mass from 0<z<2 as seen in the far-infrared at 70 and 160mu
• Narrow associated QSO absorbers: clustering, outflows and the line-of-sight proximity effect
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• SDSS IV MaNGA - The spatially resolved transition from star formation to quiescence
• How is Star Formation Quenched in Massive Galaxies?
• Galaxy And Mass Assembly (GAMA): Linking Star Formation Histories and Stellar Mass Growth
• An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies
• Spatially resolved star formation and fuelling in galaxy interactions
• Galaxy evolution in the infra-red: comparison of a hierarchical galaxy formation model with SPITZER data
• Mergers Do Trigger AGNs out to z $\sim$ 0.6
• Galactic chemical evolution in hierarchical formation models - I. Early-type galaxies in the local Universe
• The properties of the extended warm ionised gas around low-redshift QSOs and the lack of extended high-velocity outflows
• 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
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• The multiphase gas structure and kinematics in the circumnuclear region of NGC 5728
• Line Emission in the Brightest Cluster Galaxies of the NOAO Fundamental Plane and Sloan Digital Sky Surveys
• The AMUSING++ Nearby Galaxy Compilation: I. Full Sample Characterization and Galactic--Scale Outflows Selection
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• A Spatially Resolved Map of the Kinematics, Star-Formation and Stellar Mass Assembly in a Star-Forming Galaxy at z=4.9
• Cluster galaxies in XMMU J2235-2557: galaxy population properties in most massive environments at z~1.4
• Radio Continuum Surveys with Square Kilometre Array Pathfinders
• ALMA observations of cold molecular gas filaments trailing rising radio bubbles in PKS0745-191
• 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
• The alignment of satellite galaxies and cosmic filaments: observations and simulations
• Optical Emission Line Nebulae in Galaxy Cluster Cores 1: The Morphological, Kinematic and Spectral Properties of the Sample
• The Hot Gas Content of Low-Luminosity Early-Type Galaxies and the Implications Regarding Supernova Heating and AGN Feedback
• The Luminosity Function of high-redshift QSOs - A combined analysis of GOODS and SDSS
• The radio AGN population dichotomy: Green valley Seyferts versus red sequence low-excitation AGN
• IFU observations of luminous type II AGN - I. Evidence for ubiquitous winds
• ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster
• Direct observational evidence for a large transient galaxy population in groups at 0.85<z<1
• Outflowing Galactic Winds in Post-starburst and AGN Host Galaxies at 0.2<z<0.8
• The clustering of H-alpha emitters at z=2.23 from HiZELS
• Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations
• 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
• Insight Into the Formation of the Milky Way Through Cold Halo Substructure. I. The ECHOS of Milky Way Formation
• Only the Lonely: H I Imaging of Void Galaxies
• Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies
• Spinning dark matter halos promote bar formation
• Galaxies hosting an AGN: a view from the CALIFA survey
• The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
• A spectroscopic survey of dwarf galaxies in the Coma Cluster: Stellar populations, environment and downsizing
• Environmental quenching and hierarchical cluster assembly: Evidence from spectroscopic ages of red-sequence galaxies in Coma
• Galaxy Formation Spanning Cosmic History
• AGN are cooler than you think: the intrinsic far-IR emission from QSOs
• Supermassive black holes as the regulators of star formation in central galaxies
• A review of elliptical and disc galaxy structure, and modern scaling laws
• Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
• The Relation Between Cool Cluster Cores and Herschel-Detected Star Formation in Brightest Cluster Galaxies
• A Comprehensive Study of the Radio Properties of Brightest Cluster Galaxies
• An Energetic AGN Outburst Powered by a Rapidly Spinning Supermassive Black Hole or an Accreting Ultramassive Black Hole
• The Pan-STARRS1 Medium-Deep Survey: The role of galaxy group environment in the star formation rate versus stellar mass relation and quiescent fraction out to $z\sim 0.8$
• Hot gas halos around disk galaxies: Confronting cosmological simulations with observations
• Improved Models for Cosmic Infrared Background Anisotropies: New Constraints on the IR Galaxy Population
• New Constraints on the Efficiencies of Ram-Pressure Stripping and the Tidal Disruption of Satellite Galaxies
• Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
• 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
• Powering galactic super-winds with small-scale AGN winds
• Radio galaxies in the 2SLAQ Luminous Red Galaxy Survey: I. The evolution of low-power radio galaxies to z~0.7
• First test of Verlinde's theory of Emergent Gravity using Weak Gravitational Lensing measurements
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• 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
• Constrained simulations of the Local Group: on the radial distribution of substructures
• The evolution of early and late type galaxies in the COSMOS up to z~1.2
• A simple model to link the properties of quasars to the properties of dark matter halos out to high redshift
• Luminosity and stellar mass functions of disks and spheroids in the SDSS and the supermassive black hole mass function
• Destruction of Molecular Gas Reservoirs in Early-Type Galaxies by Active Galactic Nucleus Feedback
• Connecting stellar mass and star-formation rate to dark matter halo mass out to z ~ 2
• The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations
• The Self-Regulated Growth of Supermassive Black Holes
• Spectral ageing in the lobes of cluster-centre FR-II radio galaxies
• Black Holes in the Early Universe
• Galaxy and Mass Assembly (GAMA): Fine filaments of galaxies detected within voids
• The M_BH - M_star relation for X-ray obscured, red QSOs at 1.2< z <2.6
• The impact of radio feedback from active galactic nuclei in cosmological simulations: Formation of disk galaxies
• How do galaxies acquire their mass?
• A fundamental metallicity relation for galaxies at z = 0.84 - 1.47 from HiZELS
• The mass assembly of galaxy groups and the evolution of the magnitude gap
• Intrinsic galaxy shapes and alignments II: Modelling the intrinsic alignment contamination of weak lensing surveys
• The Origin of the Intrinsic Scatter in the Relation Between Black Hole Mass and Bulge Luminosity for Nearby Active Galaxies
• Physical properties of SDSS satellite galaxies in projected phase-space
• Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
• GAMA/WiggleZ: The 1.4GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z=0.75
• What is the (Dark) Matter with Dwarf Galaxies?
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• Torque-Limited Growth of Massive Black Holes in Galaxies Across Cosmic Time
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• The impact of mergers on relaxed X-ray clusters - III. Effects on compact cool cores
• Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
• Selection effects in the black hole-bulge relation and its evolution
• 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
• The Fornax Deep Survey (FDS) with VST. VI. Optical properties of the dwarf galaxies in the Fornax cluster
• Black Hole -- Galaxy Correlations in Simba
• Star Formation Shut Down by Multiphase Gas Outflow in a Galaxy at a Redshift of 2.45
• The effects of a hot gaseous halo in galaxy major mergers
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• 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
• Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies
• AEGIS: The Nature of the Host Galaxies of Low-ionization Outflows at z < 0.6
• Kinematics and physical conditions of HI in nearby radio sources. The last survey of the old Westerbork Synthesis Radio Telescope
• Environmental Dependence of Galaxy Merger Rate in ΛCDM Universe
• On the baryonic, stellar, and luminous scaling relations of disk galaxies
• The rapid growth phase of supermassive black holes
• ALMA reveals optically thin, highly excited CO gas in the jet-driven winds of the galaxy IC5063
• Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering
• Satellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matter
• Which galaxies dominate the neutral gas content of the Universe?
• Satellite abundances around bright isolated galaxies II: radial distribution and environmental effects
• AGN-Driven Outflows in Dwarf Galaxies
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• 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
• The Mid-IR and X-ray Selected QSO Luminosity Function
• Sizes and Kinematics of Extended Narrow-Line Regions in Luminous Obscured AGN Selected by Broadband Images
• LoCuSS: A Dynamical Analysis of X-ray AGN in Local Clusters
• Fast cold gas in hot AGN outflows
• A Lensing Survey of X-ray Luminous Galaxy Clusters at Redshift z ~ 0.2: II: CFH12k Weak Lensing Analysis and Global Correlations
• Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
• Models for jet power in elliptical galaxies: A case for rapidly spinning black holes
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• The Rise and Fall of Galaxy Activity in Dark Matter Haloes
• Satellite Galaxies and Fossil Groups in the Millennium Simulation
• Clustering of Radio Galaxies and Quasars
• LLAMA: Normal star formation efficiencies of molecular gas in the centres of luminous Seyfert galaxies
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• 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
• Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the last 10 Gyr
• A dynamical model of supernova feedback: gas outflows from the interstellar medium
• Modelling Shock Heating in Cluster Mergers: I. Moving Beyond the Spherical Accretion Model
• Intrinsic galaxy shapes and alignments I: Measuring and modelling COSMOS intrinsic galaxy ellipticities
• Storm in a "Teacup": a radio-quiet quasar with ~10kpc radio-emitting bubbles and extreme gas kinematics
• Starburst-AGN mixing: II. Optically-selected active galaxies
• Quenching Massive Galaxies with On-the-fly Feedback in Cosmological Hydrodynamic Simulations
• Disc instabilities and semi-analytic modelling of galaxy formation
• Dwarf galaxy populations in present-day galaxy clusters: I. Abundances and red fractions
• Determination of masses of the central black holes in NGC524 and NGC2549 using Laser Guide Star Adaptive Optics
• Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe
• How common is the Milky Way - satellite system alignment?
• Starburst radio galaxies: general properties, evolutionary histories and triggering
• Dust-Corrected Colors Reveal Bimodality in AGN Host Galaxy Colors at z~1
• The Overdense Environment of a Large Lyman-alpha Nebula at z~2.7
• The origin of the atomic and molecular gas contents of early-type galaxies. I. A new test of galaxy formation physics
• Pahs, Ionized Gas, and Molecular Hydrogen in Brightest Cluster Galaxies of Cool Core Clusters of Galaxies
• A Systematic Analysis of Caustic Methods for Galaxy Cluster Masses
• The ages, metallicities and star formation histories of early-type galaxies in SDSS
• 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
• Global star formation revisited
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• The Origin of Line Emission in Massive z~2.3 Galaxies: Evidence for Cosmic Downsizing of AGN Host Galaxies
• AGN feedback in dwarf galaxies?
• Avoiding progenitor bias: The structural and mass evolution of Brightest Group and Cluster Galaxies in Hierarchical models since z~1
• Energy- and momentum-conserving AGN feedback outflows
• Redistributing hot gas around galaxies: do cool clouds signal a solution to the overcooling problem?
• The Cool ISM in Elliptical Galaxies. II. Gas Content in the Volume - Limited Sample and Results from the Combined Elliptical and Lenticular Surveys
• Shedding Light on the Galaxy Luminosity Function
• Ram pressure stripping in a galaxy formation model. I. A novel numerical approach
• The host dark matter halos of [OII] emitters at 0.5< z< 1.5
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• MultiDark-Galaxies: data release and first results
• 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
• Quasar Feedback Survey: Multi-phase outflows, turbulence and evidence for feedback caused by low power radio jets inclined into the galaxy disk
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• A new way to measure supermassive black hole spin in accretion disc dominated Active Galaxies
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• How robust are predictions of galaxy clustering?
• Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
• MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z=2.2
• The Varied Fates of z~2 Star-forming Galaxies
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• The Evolution of Assembly Bias
• Substructure in the stellar halos of the Aquarius simulations
• The evolution of Lyman-break galaxies in CDM
• Enrichment and Pre-Heating in Intragroup Gas from Galactic Outflows
• The colour of galaxies in distant groups
• $\text{Herschel}$-ATLAS:The connection between star formation and AGN activity in radio-loud and radio-quiet active galaxies
• The Galaxy Major Merger Fraction to z ~ 1
• Times, environments and channels of bulge formation in a LambdaCDM cosmology
• The XMM Cluster Survey: The interplay between the brightest cluster galaxy and the intra-cluster medium via AGN feedback
• JWST Reveals Widespread AGN-Driven Neutral Gas Outflows in Massive z ~ 2 Galaxies
• The statistical properties of LCDM halo formation
• Quenching timescales of galaxies in the EAGLE simulations
• Properties of the galaxy population in hydrodynamical simulations of clusters
• ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
• Faint Submillimeter Galaxies Revealed by Multifield Deep ALMA Observations: Number Counts, Spatial Clustering, and A Dark Submillimeter Line Emitter
• Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
• Quasar Black Hole Mass Estimates in the Era of Time Domain Astronomy
• AGN-driven outflows and the AGN feedback efficiency in young radio galaxies
• The first detection of near-infrared CN bands in active galactic nuclei: signature of star formation
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Galaxy Formation in WDM Cosmology
• The luminosity-dependent high-redshift turnover in the steep spectrum radio luminosity function: clear evidence for downsizing in the radio-AGN population
• Revisiting the Baryon Fractions of Galaxy Clusters: A Comparison with WMAP 3-year Results
• The VIMOS VLT Deep Survey: Tracing the galaxy stellar mass assembly history over the last 8Gyr
• Mass assembly of galaxies: Smooth accretion versus mergers
• The evolution of the galaxy Red Sequence in simulated clusters and groups
• The Dynamics of Galaxy Pairs in a Cosmological Setting
• Close entrainment of massive molecular gas flows by radio bubbles in the central galaxy of Abell 1795
• Hot Gas Halos in Early-Type Field Galaxies
• The evolution of the red sequence slope in massive galaxy clusters
• Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
• The origin of the atomic and molecular gas contents of early-type galaxies. II. Misaligned gas accretion
• Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5
• The Stellar Populations of Lyman Break Galaxies at z~5
• SDSS-IV MaNGA: Inside-out vs. outside-in quenching in different local environments
• Metals Removed by Outflows from Milky Way Dwarf Spheroidal Galaxies
• Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
• GMASS Ultradeep Spectroscopy of Galaxies at redshift z~2. I. The stellar metallicity
• Radio-Quiet Quasars in the VIDEO Survey: Evidence for AGN-powered radio emission at S_1.4GHz < 1 mJy
• The Close AGN Reference Survey (CARS). A massive multi-phase outflow impacting the edge-on galaxy HE1353-1917
• Modelling galaxy stellar mass evolution from z~0.8 to today
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• 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?
• An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
• Dynamical Study of A1689 from Wide-Field VLT/VIMOS Spectroscopy: Mass Profile, Concentration Parameter, and Velocity Anisotropy
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• The clustering of radio galaxies at z~0.55 from the 2SLAQ LRG survey
• 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
• The chemical evolution of galaxies within the IGIMF theory: the [alpha/Fe] ratios and downsizing
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• The MASSIVE survey - XI. What drives the molecular gas properties of early-type galaxies
• Empirical H-alpha emitter count predictions for dark energy surveys
• Mass Functions of Supermassive Black Holes Across Cosmic Time
• Rapid Coeval Black Hole and Host Galaxy Growth in MRC 1138-262: The Hungry Spider
• Galaxy And Mass Assembly (GAMA): The dependence of the galaxy luminosity function on environment, redshift and colour
• Searching for massive galaxies at z>=3.5 in GOODS-North
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• The Clustering Characteristics of HI-Selected Galaxies from the 40% ALFALFA Survey
• Reproducing the assembly of massive galaxies within the hierarchical cosmogony
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• Tidal Disruption of Satellite Galaxies in a Semi-Analytic Model of Galaxy Formation
• Clustering, Bias and the Accretion Mode of X-ray selected AGN
• Triggered star-formation in the inner filament of Centaurus A
• The nebular emission of star-forming galaxies in a hierarchical universe
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• Herschel-ATLAS: The link between accretion luminosity and star formation in quasar host galaxies
• Music from the heavens - Gravitational waves from supermassive black hole mergers in the EAGLE simulations
• The velocity function of gas-rich galaxies
• Toward precise constraints on growth of massive black holes
• The duty cycle of radio galaxies revealed by LOFAR: remnant and restarted radio source populations in the Lockman Hole
• LOFAR-Boötes: Properties of high- and low-excitation radio galaxies at $0.5<z<2.0$
• Multi-phase feedback processes in the Sy2 galaxy NGC 5643
• Evolution of faint radio sources in the VIDEO-XMM3 field
• Galaxy Formation: Bayesian History Matching for the Observable Universe
• Towards a physical picture of star-formation quenching: the photometric properties of recently-quenched galaxies in the Sloan Digital Sky Survey
• Massive and Red Objects predicted by a semianalytical model of galaxy formation
• The properties of (sub)millimetre-selected galaxies as revealed by CANDELS HST WFC3/IR imaging in GOODS-South
• The effect of stellar feedback and quasar winds on the AGN population
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• The Mass and Spin of The Extreme Narrow Line Seyfert 1 Galaxy 1H 0707-495 and Its Implications for The Trigger for Relativistic Jets
• The SCUBA-2 Cosmology Legacy Survey: Ultraluminous star-forming galaxies in a z=1.6 cluster
• 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
• Halo Shapes From Weak Lensing: The Impact of Galaxy--Halo Misalignment
• Probing recent star formation with absorption-line strengths in hierarchical models and observations
• Quasar outflows at $z\ge 6$: the impact on the host galaxies
• Unveiling the oldest and most massive galaxies at very high redshift
• The Effect of Star Formation on the Redshift Evolution of Interstellar Metals, Atomic and Molecular Gas in Galaxies
• Can galactic outflows explain the properties of Ly-alpha emitters?
• The origin of low-surface-brightness galaxies in the dwarf regime
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• The chemical enrichment of the ICM from hydrodynamical simulations
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• A semi-analytic model comparison - gas cooling and galaxy mergers
• Ultradeep Near-Infrared Observations of GOODS 850-5
• A flexible modelling of galaxy assembly bias
• Constraining the dark energy equation of state using LISA observations of spinning Massive Black Hole binaries
• 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
• Thermal plasma in the giant lobes of the radio galaxy Centaurus A
• Maximum Spin of Black Holes Driving Jets
• 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
• Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description
• A Comparison of Galaxy Merger History Observations and Predictions from Semi-Analytic Models
• SDSS-IV MaNGA: The Spatial Distribution of Star Formation and its Dependence on Mass, Structure and Environment
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• The clustering of galaxies as a function of their photometrically-estimated atomic gas content
• RAiSE II: resolved spectral evolution in radio AGN
• Numerical resolution limits on subhalo abundance matching
• How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE
• The imprint of cosmic reionisation on the luminosity function of galaxies
• A Pilot Survey for KX QSOs in the UKIDSS Ultra Deep Survey Field
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• Recurrent radio emission and gas supply: the case of the radio galaxy B2 0258+35
• External pressure-triggering of star formation in a disc galaxy: a template for positive feedback
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• The Hierarchical Origins of Observed Galaxy Morphology
• The similarity of the stellar mass fractions of galaxy groups and clusters
• The Cocoon Shocks of Cygnus A: Pressures and Their Implications for the Jets and Lobes
• The Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?
• 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
• BCG Mass Evolution in Cosmological Hydro-Simulations
• The Millennium Run Observatory: First Light
• Hot Outflows in Galaxy Clusters
• Black hole evolution: II. Spinning black holes in a supernova-driven turbulent interstellar medium
• The importance of black hole repositioning for galaxy formation simulations
• BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes
• The Growth of Central and Satellite Galaxies in Cosmological Smoothed Particle Hydrodynamics Simulations
• The evolution of SMBH spin and AGN luminosities for $z<6$ within a semi-analytic model of galaxy formation
• X-ray selected AGN Hosts are Similar to Inactive Galaxies out to z=3: Results from CANDELS/CDF-S
• Light breeze in the local Universe
• The growth of disks and bulges during hierarchical galaxy formation. I: fast evolution vs secular processes
• The evolution of the star forming sequence in hierarchical galaxy formation models
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• GalICS II: the [alpha/Fe]-mass relation in elliptical galaxies
• The Baryons in the Milky Way Satellites
• Gas Mass Fractions and Star Formation in Blue-Sequence E/S0 Galaxies
• On the formation time scale of massive cluster ellipticals based on deep near-IR spectroscopy at z~2
• The impact of quenching on galaxy profiles in the Simba simulation
• Cold gas in cluster cores: Global stability analysis and non-linear simulations of thermal instability
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• The Rise of Active Galactic Nuclei in the GAlaxy Evolution and Assembly semi-analytic model
• The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback
• Host galaxy-active galactic nucleus alignments in the SDSS-DR7
• Wide-field VLBA Observations of the Chandra Deep Field South
• The Lifetime of FRIIs in Groups and Clusters: Implications for Radio-Mode Feedback
• Two-Face(s): ionized and neutral gas winds in the local Universe
• The role of submillimetre galaxies in hierarchical galaxy formation
• On the connection between the intergalactic medium and galaxies: The HI-galaxy cross-correlation at z < 1
• Concurrent Supermassive Black Hole and Galaxy Growth: Linking Environment and Nuclear Activity in z = 2.23 H-alpha Emitters
• The effect of variations in the input physics on the cosmic distribution of metals predicted by simulations
• 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
• Environmentally Driven Global Evolution of Galaxies
• Substructure in the Most Massive GEEC Groups: Field-like Populations in Dynamically Active Groups
• An Extreme Starburst in Close Proximity to the Central Galaxy of a Rich Galaxy Cluster at z=1.7
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• PRIMUS: An observationally motivated model to connect the evolution of the AGN and galaxy populations out to z~1
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• 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
• Efficient satellite quenching at z~1 from the GEEC2 spectroscopic survey of galaxy groups
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• The age dependence of the size-stellar mass relation and some implications
• Jet-driven outflows of ionised gas in the nearby radio galaxy 3C293
• Tracing the Quenching Journey across Cosmic Time
• The faint radio sky: VLBA observations of the COSMOS field
• Another thread in the tapestry of stellar feedback: X-ray binaries
• The rest-frame UV luminosity function at $z\simeq 4$: a significant contribution of AGN to the bright-end of the galaxy population
• Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
• A new infrared color criterion for the selection of 0<z<7 AGN: application to deep fields and implications for JWST surveys
• Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations
• CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST
• The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues
• Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
• Heating of the molecular gas in the massive outflow of the local ultraluminous-infrared and radio-loud galaxy 4C12.50
• T-RaMiSu: The Two-meter Radio Mini Survey I. The Bootes Field
• Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
• Massive and old quiescent galaxies at high redshift
• Streams in the Aquarius stellar haloes
• A Flexible Method of Estimating Luminosity Functions
• On the Dynamical Origin of the ICM Metallicity Evolution
• A simple model for AGN feedback in nearby early-type galaxies
• Constraints on black hole fuelling modes from the clustering of X-ray AGN
• ZENS IV. Similar Morphological Changes associated with Mass- and Environment-Quenching, and the Relative importance of Bulge Growth versus the Fading of Disks
• Gravitational lensing reveals extreme dust-obscured star formation in quasar host galaxies
• ALMA Observations of a Candidate Molecular Outflow in an Obscured Quasar
• Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies
• A systematic search for X-ray cavities in galaxy clusters, groups, and elliptical galaxies
• Markarian 6: shocking the environment of an intermediate Seyfert
• Witnessing the assembly at z=1.6 of a galaxy cluster (GMASS ultradeep spectroscopy of galaxies at z~2 - V)
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Luminosity function of galaxies in groups in the SDSS DR7: the dependence on mass, environment and galaxy type
• Cold gas dynamics in Hydra-A: evidence for a rotating disk
• Compact Groups of Galaxies selected by stellar mass: The 2MASS Compact Group Catalogue
• The first 62 AGN observed with SDSS-IV MaNGA - I: their characterization and definition of a control sample
• The red-sequence of 72 WINGS local galaxy clusters
• The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field
• Damn You, Little h! (or, Real-World Applications Of The Hubble Constant Using Observed And Simulated Data)
• Constraints on the star formation histories of galaxies from z~1 to z~0
• Massive Star-Forming Host Galaxies of Quasars on Sloan Digital Sky Survey Stripe 82
• Evolution of blue E/S0 galaxies from z~1: merger remnants or disk rebuilding galaxies?
• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
• AGN Jet-induced Feedback in Galaxies. II. Galaxy colours from a multicloud simulation
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• 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
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Dwarf galaxy populations in present-day galaxy clusters - II. The history of early-type and late-type dwarfs
• Rapid early coeval star formation and assembly of the most massive galaxies in the universe
• 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
• Tracking Down a Critical Halo Mass for Killing Galaxies through the Growth of the Red-Sequence
• A near-infrared morphological comparison of high-redshift submm and radio galaxies: massive star-forming discs vs relaxed spheroids
• The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$
• A Powerful AGN Outburst in RBS 797
• Enriching the hot circumgalactic medium
• Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the "green valley"
• Two-Phase Galaxy Formation
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• SINFONI-HiZELS: The dynamics, merger rates & metallicity gradients of `typical' star-forming galaxies at $z$ = 0.8-2.2
• Properties of Dark Matter Haloes and their Correlations: the Lesson from Principal Component Analysis
• High Radio Frequency Properties and Variability of Brightest Cluster Galaxies
• Chandra evidence for AGN feedback in the spiral galaxy NGC 6764
• The Red Sequence of High-Redshift Clusters: a Comparison with Cosmological Galaxy Formation Models
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups
• 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
• The structural and photometric properties of early-type galaxies in hierarchical models
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• MUFASA: The assembly of the red sequence
• A Relationship Between Halo Mass, Cooling, AGN Heating, and the Coevolution of Massive Black Holes
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• Nature and evolution of powerful radio galaxies and their link with the quasar luminosity function
• The Formation and Evolution of Virgo Cluster Galaxies - II. Stellar Populations
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• On the formation of massive galaxies: A simultaneous study of number density, size and intrinsic colour evolution in GOODS
• 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
• The Effect of AGN on the Global HI Content of Isolated Low-Mass Galaxies
• What produces the far-infrared/submm emission in the most luminous QSOs?
• The Building Up of the Black Hole Mass - Stellar Mass Relation
• NIR spectroscopic observation of massive galaxies in the protocluster at z = 3.09
• Probing the star formation history using the redshift evolution of luminosity functions
• Compact groups in theory and practice - I. The spatial properties of compact groups
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• A Giant Metrewave Radio Telescope/Chandra view of IRAS 09104+4109: A type 2 QSO in a cooling flow
• FR-II radio galaxies at low frequencies II: spectral ageing and source dynamics
• Constraining the supermassive black holes evolution through the continuity equation
• No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
• The discovery of a significant sample of massive galaxies at redshifts 5 < z < 6 in the UKIDSS Ultra Deep Survey Early Data Release
• Radio galaxy feedback in X-ray selected groups from COSMOS: the effect on the ICM
• Tracing the evolution of Active Galactic Nuclei host galaxies over the last 9 Gyrs of Cosmic time
• Galaxy structure with strong gravitational lensing: decomposing the internal mass distribution of massive elliptical galaxies
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• The environments of high redshift radio galaxies and quasars: probes of protoclusters
• The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing
• Radio AGN in nearby dwarf galaxies: the important role of AGN in dwarf-galaxy evolution
• High Redshift Galaxy Populations and their Descendants
• Star formation in high-redshift quasars: excess [O II] emission in the radio-loud population
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• A radio jet drives a molecular and atomic gas outflow in multiple regions within one square kiloparsec of the nucleus of the nearby galaxy IC5063
• Extreme star formation events in quasar hosts over $0.5<\text{z}<4$
• Color Distributions, Number and Mass Densities of Massive Galaxies at 1.5 < z < 3: Comparing Observations with Merger Simulations
• Emission line gas ionisation in young radio galaxies
• Environmental dependence of AGN activity. I.: the effects of host galaxy
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• Rest-frame UV--Optically Selected Galaxies at 2.3<z<3.5: Searching for Dusty Star-forming and Passively-Evolving Galaxies
• Early-Type galaxies at z ~ 1.3. III. On the dependence of Formation Epochs and Star Formation Histories on Stellar Mass and Environment
• Galaxy interactions are the dominant trigger for local type 2 quasars
• A modified star formation law as a solution to open problems in galaxy evolution
• Observational constraints on the co-evolution of supermassive black holes and galaxies
• 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
• COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: III. Comparison with semi-analytic models of galaxy formation
• The impact of TP-AGB stars on hierarchical galaxy formation models
• The morphological evolution, AGN fractions, dust content, environments, and downsizing of massive green valley galaxies at 0.5<z<2.5 in 3D-HST/CANDELS
• Compact groups from the Millennium Simulations: I. Their Nature and the completeness of the Hickson sample
• Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• A simple model linking galaxy and dark matter evolution
• The radio properties of a complete, X-ray selected sample of nearby, massive elliptical galaxies
• Realistic galaxy image simulation via score-based generative models
• Galaxy evolution from strong lensing statistics: the differential evolution of the velocity dispersion function in concord with the LambdaCDM paradigm
• The Evolving Faint-End of the Luminosity Function
• AGN All the Way Down? AGN-like Line Ratios are Common In the Lowest-Mass Isolated Quiescent Galaxies
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• The Look-back Time Evolution of Far-Ultraviolet Flux from the Brightest Cluster Elliptical Galaxies at z < 0.2
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• Tools for computing the AGN feedback: radio-loudness distribution and the kinetic luminosity function
• Characterizing the formation history of Milky Way-like stellar haloes with model emulators
• A Large Population of Obscured AGN in Disguise as Low Luminosity AGN in Chandra Deep Field South
• Galaxy properties and the cosmic web in simulations
• The prevalence of AGN feedback in massive galaxies at z~1
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5<z<2$ from KMOS
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• Galaxy Zoo: The interplay of quenching mechanisms in the group environment
• Monolithic or hierarchical star formation? A new statistical analysis
• On the evidence for large-scale galactic conformity in the local Universe
• 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
• Black Hole Demography: From scaling relations to models
• Is there a relationship between AGN and star formation in IR-bright AGNs?
• Faint Submillimeter Galaxies identified through their optical/near-infrared colours I: spatial clustering and halo masses
• Kinematics of CIV and [OIII] emission in luminous high-redshift quasars
• The Deep SWIRE Field. IV. First properties of the sub-mJy galaxy population: redshift distribution, AGN activity and star formation
• Creating mock catalogues of stellar haloes from cosmological simulations
• Spatial kinematics of Brightest Cluster Galaxies and their close companions from Integral Field Unit spectroscopy
• Revealing components of the galaxy population through nonparametric techniques
• The KMOS${}^{3D}$ Survey: rotating compact star forming galaxies and the decomposition of integrated line widths
• The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to $\sim$10${}^6$ L${}_{\odot }$ and Comparisons with Galaxy Formation Models
• Ultimate age-dating method for galaxy groups; clues from the Millennium Simulations
• Characterising the Far-infrared Properties of Distant X-ray Detected AGNs: Evidence for Evolution in the Infrared--X-ray Luminosity Ratio
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• The role of thermal evaporation in galaxy formation
• A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades
• The many lives of active galactic nuclei-II: The formation and evolution of radio jets and their impact on galaxy evolution
• The evolution of the stellar mass versus halo mass relationship
• Study of star-forming galaxies in SDSS up to redshift 0.4 II. Evolution from the fundamental parameters: mass, metallicity & SFR
• Stellar population gradients in early-type cluster galaxies with VIMOS IFU
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• Delayed triggering of radio Active Galactic Nuclei in gas-rich minor mergers in the local Universe
• Triggering Active Galactic Nuclei in galaxy clusters
• The Host Galaxies of X-ray Quasars Are Not Strong Star Formers
• Bulges and disks in the local Universe. Linking the galaxy structure to star formation activity
• Formation of disk galaxies in preheated media: a preventative feedback model
• Probing multi-phase outflows and AGN feedback in compact radio galaxies: the case of PKSB 1934-63
• Unveiling the Important Role of Groups in the Evolution of Massive Galaxies: Insights from an Infrared Passive Sequence at Intermediate Redshift
• A spectroscopic measurement of galaxy formation timescales with ROLES
• The roles of star formation and AGN activity of IRS sources in the HerMES fields
• The bulk kinetic power of radio jets in active galactic nuclei
• Recent Arrival of Faint Cluster Galaxies on the Red-sequence: Luminosity Functions from 119 square degrees of CFHTLS
• An obscured AGN population hidden in the VIPERS galaxies: identification through spectral energy distribution decomposition
• Supernovae and AGN driven galactic outflows
• Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy
• Young and turbulent: the early life of massive galaxy progenitors
• The flickering nuclear activity of Fornax A
• The Cosmic Far-Infrared Background Buildup Since Redshift 2 at 70 and 160 microns in the COSMOS and GOODS fields
• Evolution of the galaxy stellar mass function: evidence for an increasing $M^{\ast }$ from $z=2$ to the present day
• The discovery of a typical radio galaxy at z = 4.88
• Accretion, Growth of Supermassive Black Holes, and Feedback in Galaxy Mergers
• Global and Local Effects of Rotation: Observational Aspects
• The impact of AGN feedback on the 1D power spectra from the Ly$\alpha$ forest using the Horizon-AGN suite of simulations
• Structural Analysis of the SDSS Cosmic Web I.Nonlinear Density Field Reconstructions
• Faint-end Quasar Luminosity Functions from Cosmological Hydrodynamic Simulations
• Star formation in the CDFS: observations confront simulations
• The A2667 Giant Arc at z=1.03: Evidence for Large-scale Shocks at High Redshift
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe I. - The Effect of the Group Environment on Star Formation in Spiral Galaxies
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• The Sloan Digital Sky Survey Reverberation Mapping Project: Post-Starburst Signatures in Quasar Host Galaxies at z < 1
• The black holes of radio galaxies during the "Quasar Era": Masses, accretion rates, and evolutionary stage
• A Measurement of the Millimeter Emission and the Sunyaev-Zel'dovich Effect Associated with Low-Frequency Radio Sources
• An X-ray Detected Group of Quiescent Early-type Galaxies at z=1.6 in the Chandra Deep Field South
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Pan-STARRS1: Galaxy Clustering in the Small Area Survey 2
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• Dynamically evolving Mg II broad absorption line flow in SDSS J133356.02+001229.1
• Detecting Radio-AGN signatures in Red geysers
• Isolated galaxies in hierarchical galaxy formation models - present-day properties and environmental histories
• Exploring the unusually high black hole-to-bulge mass ratios in NGC4342 and NGC4291: the asynchronous growth of bulges and black holes
• X-ray Observations of Luminous Dusty Quasars at z > 2
• On stellar mass loss from galaxies in groups and clusters
• Observing the first galaxies
• Substructure Lensing: Effects of Galaxies, Globular Clusters & Satellite Streams
• The Radio Galaxy Population in the SIMBA SImulations
• Radio source feedback in galaxy evolution
• The first Super Massive Black Holes: indications from models for future observations
• Star formation activity and gas stripping in the Cluster Projected Phase-Space (CPPS)
• The effect of dwarf galaxies disruption in semi-analytic models
• Subhaloes gone Notts: Spin across subhaloes and finders
• Spitzer Infrared Low-Resolution Spectroscopic Study of Buried AGNs in a Complete Sample of Nearby Ultraluminous Infrared Galaxies
• Luminosity and surface brightness distribution of K-band galaxies from the UKIDSS Large Area Survey
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Galaxy pairs align with galactic filaments
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties
• The minor role of gas-rich major mergers in the rise of intermediate-mass early types at z <~ 1
• The galaxies that reionized the Universe
• 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
• The Chandra COSMOS Legacy survey: the z>3 sample
• Is there enough star formation in simulated protoclusters?
• Identifying active galactic nuclei via brightness temperature with sub-arcsecond International LOFAR Telescope observations
• Black hole growth and AGN feedback under clumpy accretion
• Massive Dark Matter Halos around Bright Isolated Galaxies in the 2dFGRS
• Constraints on galaxy formation models from the galaxy stellar mass function and its evolution
• Luminous Red Galaxies in hierarchical cosmologies
• Mass and Redshift Dependence of Star Formation in Relaxed Galaxy Clusters
• The Relative Role of Galaxy Mergers and Cosmic Flows in Feeding Black Holes
• 4098 galaxy clusters to z~0.6 in the Sloan Digital Sky Survey equatorial Stripe 82
• Modelling supermassive black hole growth: towards an improved sub-grid prescription
• Supermassive Black Holes and Their Environments
• The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
• The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• The specific star formation rate and stellar mass fraction of low-mass central galaxies in cosmological simulations
• Do model emission line galaxies live in filaments at z~1?
• Galaxy And Mass Assembly (GAMA): The 325 MHz Radio Luminosity Function of AGN and Star Forming Galaxies
• Quantitative Morphology of Galaxies from the SDSS I: Luminosity in Bulges and Disks
• Shocks, Seyferts and the SNR connection: a Chandra observation of the Circinus galaxy
• Evidence of ongoing AGN-driven feedback in a quiescent post starburst E+A galaxy
• Fundamental differences in the radio properties of red and blue quasars: Insight from the LOFAR Two-metre Sky Survey (LoTSS)
• The mass assembly of high-redshift black holes
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• Herschel Far-Infrared Photometry of the Swift Burst Alert Telescope Active Galactic Nuclei Sample of the Local Universe. II. SPIRE Observations
• Isolated elliptical galaxies in the local Universe
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• Outflows from active galactic nuclei: The BLR-NLR metallicity correlation
• A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
• Evaluating and Improving Semi-analytic modeling of Dust in Galaxies based on Radiative Transfer Calculations II: Dust Emission in the Infrared
• Mass transport by buoyant bubbles in galaxy clusters
• The spatial distribution of cold gas in hierarchical galaxy formation models
• A Chandra X-ray Analysis of Abell 1664: Cooling, Feedback and Star Formation in the Central Cluster Galaxy
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• Galaxy Zoo: Evidence for rapid, recent quenching within a population of AGN host galaxies
• Tracing galaxy populations through cosmic time: A critical test of methods for connecting the same galaxies between different redshifts at $z<3$
• X-ray selected AGN in groups at redshifts z~1
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• Confirming the Quiescent Galaxy Population out to $z=3$: A Stacking Analysis of Mid-, Far-Infrared and Radio Data
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• Spatially resolved evidence of the impact of quasar driven outflows on recent star formation : The case of Mrk 34
• ALMA observations of AGN fuelling: the case of PKS B1718-649
• Black Holes in Pseudobulges: demography and models
• The formation of galaxy disks in a hierarchical universe
• Galaxy downsizing evidenced by hybrid evolutionary tracks
• The VLA-COSMOS 3 GHz Large Project: Star formation properties and radio luminosity functions of AGN with moderate-to-high radiative luminosities out to $z\sim 6$
• HST/COS observations of a new population of associated QSO absorbers
• CFHT Legacy Ultraviolet Extension (CLUE): Witnessing Galaxy Transformations up to 7 Mpc from Rich Cluster Cores
• Active galactic nucleus jet feedback in hydrostatic halos
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Statistics of galaxy mergers: bridging the gap between theory and observation
• (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies III. Environments
• Galaxy And Mass Assembly (GAMA): The environments of high- and low- excitation radio galaxies
• The Shapes of BCGs and normal Ellipticals in Nearby Clusters
• The Role of Ram Pressure Stripping in the Quenching of Cluster Star Formation
• On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
• 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
• Hierarchical models of high redshift galaxies with thermally pulsing asymptotic giant branch stars: comparison with observations
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• Properties of fossil groups in cosmological simulations and galaxy formation models
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• The role of AGN and its obscuration on the position of the host galaxy relative to Main Sequence
• The Magellanic Quasars Survey. I. Doubling the Number of Known AGNs Behind the Small Magellanic Cloud
• Molecular gas mass functions of normal star forming galaxies since z~3
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• Gemini NIFS survey of feeding and feedback in nearby Active Galaxies -- V. Molecular and Ionised Gas Kinematics
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Stellar Dynamics and Star-Formation Histories of z $\sim$ 1 Radio-loud Galaxies
• An improved quasar detection method in EROS-2 and MACHO LMC datasets
• Cosmic downsizing of powerful radio galaxies to low radio luminosities
• Detection of Quasar Feedback from the Thermal Sunyaev-Zel'dovich Effect in Planck
• Star Formation and Environmental Quenching of GEEC2 Group Galaxies at z~1
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• Determining the core radio luminosity function of radio AGNs via copula
• Investigating evidence for different black hole accretion modes since redshift z~1
• The imprints of AGN feedback within a supermassive black hole's sphere of influence
• Radio-AGN Feedback: When the Little Ones were Monsters
• A Huge Filamentary Structure at z=0.55 and Star Formation Histories of Galaxies at z<1
• COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at $0<z<5$ Revealed by X-ray and Radio Stacking
• RESOLVE and ECO: Finding Low-Metallicity $z\sim 0$ Dwarf AGN Candidates Using Optimized Emission-Line Diagnostics
• Anti-hierarchical evolution of the Active Galactic Nucleus space density in a hierarchical universe
• From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
• The impact of environment and mergers on the HI content of galaxies in hydrodynamic simulations
• Constraining star formation rates in cool-core brightest cluster galaxies
• From Star-Forming Spirals to Passive Spheroids: Integral Field Spectroscopy of E+A Galaxies
• What triggers black-hole growth? Insights from star formation rates
• A new search for distant radio galaxies in the Southern hemisphere -- III. Optical spectroscopy and analysis of the MRCR--SUMSS sample
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• ORCA: The Overdense Red-sequence Cluster Algorithm
• The role of the most luminous, obscured AGN in galaxy assembly at z~2
• Spectro-photometric close pairs in GOODS-S: major and minor companions of intermediate-mass galaxies
• The challenge of large and empty voids in the SDSS DR7 redshift survey
• Observing AGN feedback with CO intensity mapping
• The resolution bias: low resolution feedback simulations are better at destroying galaxies
• Spectral ageing in the era of big data: integrated vs resolved models
• How Does Radio AGN Feedback Feed Back?
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• Spatial and luminosity distributions of galactic satellites
• Selection bias in dynamically-measured supermassive black hole samples: Scaling relations and correlations between residuals in semi-analytic galaxy formation models
• A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the LMC
• A compact, metal-rich, kpc-scale outflow in FBQS J0209-0438: Detailed diagnostics from HST/COS extreme UV observations
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• A New Method to Measure Star Formation Rates in Active Galaxies Using Mid-infrared Neon Emission Lines
• Compaction-Driven Black Hole Growth
• The effects of a hot gaseous halo on disc thickening in galaxy minor mergers
• AGNs as main contributors to the UV ionizing emissivity at high redshifts: predictions from a Lambda-CDM model with linked AGN/galaxy evolution
• Host galaxy colour gradients and accretion disc obscuration in AEGIS z~1 X-ray-selected active galactic nuclei
• Ultra-Red Galaxies Signpost Candidate Proto-Clusters at High Redshift
• Group quenching and galactic conformity at low redshift
• Multi-wavelength observations of a rich galaxy cluster at z ~ 1: the HST/ACS colour-magnitude diagram
• Low-power radio galaxy environments in the Subaru/XMM-Newton Deep Field at z~0.5
• The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN
• Dust-Enshrouded AGN can Dominate Host-Galaxy-Scale Cold-Dust Emission
• Reionisation in sterile neutrino cosmologies
• The Molecular Gas Content of z<0.1 Radio Galaxies: Linking the AGN Accretion Mode to Host Galaxy Properties
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• Constraining AGN Feedback in Massive Ellipticals with South Pole Telescope Measurements of the Thermal Sunyaev-Zel'dovich Effect
• Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• Imaging Extended Emission-Line Regions of Obscured AGN with the Subaru Hyper Suprime-Cam Survey
• The dual role of starburst and active galactic nuclei in driving extreme molecular outflows
• Star formation of X-ray AGN in COSMOS: The role of AGN activity and galaxy stellar mass
• Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
• SPH Simulations of Black Hole Accretion: A Step to Model Black Hole Feedback in Galaxies
• Black hole feedback in a multiphase interstellar medium
• Satellite quenching was not important for z$\sim$1 clusters: most quenching occurred during infall
• ACCESS: NIR Luminosity Function and Stellar Mass Function of Galaxies in the Shapley Supercluster Environment
• The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
• Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups
• Testing Star Formation Laws on Spatially Resolved Regions in a $z\approx 4.3$ Starburst Galaxy
• Structures and components in galaxy clusters: observations and models
• The interaction-driven starburst contribution to the cosmic star formation rate density
• Modeling the effects of dust evolution on the SEDs of galaxies of different morphological type
• The environments of z~1 Active Galactic Nuclei at 3.6um
• Cosmic CARNage I: on the calibration of galaxy formation models
• Near-infrared adaptive optics imaging of high redshift quasars
• A population of galaxy-scale jets discovered using LOFAR
• Radio AGN in galaxy clusters: heating hot atmospheres and driving supermassive black hole growth over cosmic time
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes
• Do AGN triggering mechanisms vary with radio power? II. The importance of mergers as a function of radio power and optical luminosity
• Superradiance of charged black holes embedded in dark matter halos
• The role of massive halos in the Star Formation History of the Universe
• Further constraining galaxy evolution models through the Size Function of SDSS Early-type galaxies
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• ACCESS II: A Complete Census of Star Formation in the Shapley Supercluster - UV and IR Luminosity Functions
• Dissecting the Red Sequence. IV. The Role of Truncation in the Two-Dimensional Family of Early-Type Galaxy Star Formation Histories
• Large Scale Structure in Absorption: Gas within and around Galaxy Voids
• Resolving the baryon-fraction profile in lensing galaxies
• The physical drivers of the atomic hydrogen-halo mass relation
• I. Apples to apples $A^2$: realistic galaxy simulated catalogs and photometric redshift predictions for next-generation surveys
• The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: host galaxy properties and accretion rates of radio galaxies
• Evolution of active galactic nuclei
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• Anisotropic AGN Outflows and Enrichment of the Intergalactic Medium
• The VLA-COSMOS Survey: V. 324 MHz continuum observations
• The dependence of AGN activity on stellar and halo mass in Semi-Analytic Models
• What determines large scale galaxy clustering: halo mass or local density?
• HerMES: SPIRE/Sub-millimetre Emission from Radio Selected AGN
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• The host galaxies of active galactic nuclei with powerful relativistic jets
• Extreme host galaxy growth in powerful early-epoch radio galaxies
• Simulations of the Sunyaev-Zeldovich Effect from Quasars
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• The evolution of the galaxy content of dark matter haloes
• The Origin of the Hubble Sequence in Lambda-CDM Cosmology
• The Illustris Simulation: Supermassive Black Hole - Galaxy Connection Beyond the Bulge
• The cosmic evolution of massive black holes and galaxy spheroids: global constraints at redshift z<~1.2
• Reconstructing the galaxy density field with photometric redshifts: I. Methodology and validation on stellar mass functions
• The DEEP2 Galaxy Redshift Survey: The Red Sequence AGN Fraction and its Environment and Redshift Dependence
• The XXL Survey XVIII. ATCA 2.1 GHz radio source catalogue and source counts for the XXL-South field
• J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
• Is there a black hole in NGC 4382?
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Groups in the Millennium Simulation and in SDSS DR7
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• The influence of halo assembly on galaxies and galaxy groups
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• A new sample of southern radio galaxies: Host galaxy masses and star-formation rates
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• AGN environments at z<1.5 in the UKIDSS Ultra-Deep Survey
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• Active Galactic Nuclei and the Truncation of Star Formation in K+A Galaxies
• An upper limit to the dry merger rate at <z> ~ 0.55
• The first 62 AGN observed with SDSS-IV MaNGA -- III: stellar and gas kinematics
• Luminous Red Galaxies in Simulations: Cosmic Chronometers?
• Aging of galaxies along the morphological sequence, marked by bulge growth and disk quenching
• Massive, red galaxies in a hierarchical universe I. Counts of Extremely Red Objects and basic properties
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• Galactic magnetic fields and hierarchical galaxy formation
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
• On the algorithms of radiative cooling in semi-analytic models
• Local and global environmental effects on galaxies and active galactic nuclei
• The Orientation of Galaxies in Galaxy Clusters
• A magnified view of circumnuclear star formation and feedback around an AGN at z=2.6
• The UV-Optical Color Dependence of Galaxy Clustering in the Local Universe
• Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
• A model for the metallicity evolution of damped Lyman-alpha systems
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Probing multiphase gas in local massive elliptical galaxies via multiwavelength observations
• Green galaxies in the COSMOS field
• Joint XMM-Newton and Chandra Observations of the NGC 1407/1400 Complex: a Tail of an Early-Type Galaxy and a Tale of a Nearby Merging Group
• Galactic conformity measured in semi-analytic models
• Direct Detection of Quasar Feedback Via the Sunyaev-Zeldovich Effect
• Evolution of the Red Sequence Giant to Dwarf Ratio in Galaxy Clusters out to z ~ 0.5
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• A Fundamental Line for Elliptical Galaxies
• XXL-HSC: The link between AGN activity and star formation in the Early Universe ($z⩾3.5$)
• Interpreting the possible break in the Black Hole - Bulge mass relation
• Subaru/MOIRCS Near-Infrared Imaging in the Proto-Cluster Region at z=3.1
• A sample of mJy radio sources at 1.4 GHz in the Lynx and Hercules fields - II. Cosmic evolution of the space density of FRI radio sources
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• A Two-Point Correlation Function For Galactic Halo Stars
• Gravitational Stability of Circumnuclear Disks in Elliptical Galaxies
• How accurate is it to update the cosmology of your halo catalogues?
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• Cosmic evolution of radio-AGN feedback: confronting models with data
• Disk Assembly and the M_BH-sigma Relation of Supermassive Black Holes
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Post-Starburst Properties of Post-Merger Galaxies
• A Multiwavelength Study of Active Galactic Nuclei in Post-Merger Remnants
• A Stacked Analysis of Brightest Cluster Galaxies Observed with the Fermi Large Area Telescope
• A new search for distant radio galaxies in the southern hemisphere - I. Sample definition and radio properties
• On the stellar populations of massive galaxies
• The clustering amplitude of X-ray selected AGN at z=0.8: Evidence for a negative dependence on accretion luminosity
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• The properties of quasar hosts at the peak of the quasar activity
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• Lensed arc statistics: comparison of Millennium-simulation galaxy clusters to Hubble Space Telescope observations of an X-ray selected sample
• Evolution of compact and fossil groups of galaxies from semi-analytical models of galaxy formation
• Why are AGN found in High Mass Galaxies?
• Evolution of galaxy groups in the Illustris simulation
• The hierarchical build-up of the Tully-Fisher relation
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• A CO molecular gas wind 340 pc away from the Seyfert 2 nucleus in ESO 420-G13 probes an elusive radio jet
• The galaxy population in cold and warm dark matter cosmologies
• The VLT LBG Redshift Survey - VI. Mapping HI in the proximity of $z\sim 3$ LBGs with X-Shooter
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• VIS3COS: III. environmental effects on the star formation histories of galaxies at z~0.8 seen in [OII], H$\delta$, and Dn4000
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Rise and fall of post-starburst galaxies in Magneticum Pathfinder
• The Nuclear Outflows and Feedback in the Seyfert 2 Galaxy Markarian 573
• HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey
• The KMOS Cluster Survey (KCS) II - The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift $1.39<z<1.61$
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Galaxy star formation in different environments
• The orbital PDF: the dynamical state of Milky Way sized haloes and the intrinsic uncertainty in the determination of their masses
• Moderate Steepening of Galaxy Cluster Dark Matter Profiles by Baryonic Pinching
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• The cross-power spectrum between 21cm emission and galaxies in hierarchical galaxy formation models
• 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
• Numerical modelling of the lobes of radio galaxies in cluster environments -- IV. Remnant radio galaxies
• Stellar Population Trends in S0 Galaxies
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• Detection of a Multi-Phase Ultra-Fast Wind in the Narrow-Line Seyfert 1 Galaxy Mrk 1044
• Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?
• The association between gas and galaxies II: The 2-point correlation function
• The age dependence of galaxy clustering
• The Clustering Evolution of Dusty Star-Forming Galaxies
• Spatial Clustering of High Redshift Lyman Break Galaxies
• The Combined NVSS-FIRST Galaxies (CoNFIG) Sample - I. Sample Definition, Classification and Evolution
• Evolution of environment dependent galaxy properties in the Sloan Digital Sky Survey
• 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
• Evidence for AGN-driven Outflows in Young Radio Quasars
• On the Role of Hot Feedback Mode in Active Galactic Nuclei Feedback in an Elliptical Galaxy
• Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
• Brightest Group Galaxies: Stellar Mass and Star Formation Rate (paper I)
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• Is NGC 3108 transforming itself from an early to late type galaxy -- an astronomical hermaphrodite?
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Can galaxy outflows and re-accretion produce the downsizing in specific star formation rate of late-type galaxies?
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• Deep ALMA photometry of distant X-ray AGN: improvements in star formation rate constraints, and AGN identification
• Generating Synthetic Cosmological Data with GalSampler
• The Quasar Feedback Survey: Revealing the Interplay of Jets, Winds & Emission Line Gas in Type 2 Quasars with Radio Polarization
• Do AGN triggering mechanisms vary with radio power? I.Optical morphologies of radio-intermediate HERGs
• Empirical Constraints on the Evolution of the Relationship between Black Hole and Galaxy Mass: Scatter Matters
• How to Find Variable Active Galactic Nuclei with Machine Learning
• On the cosmological evolution of the black hole - host galaxy relation in quasars
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• Star formation quenching imprinted on the internal structure of naked red nuggets
• Probing AGN triggering mechanisms through the starburstiness of the host galaxies
• Galaxy And Mass Assembly: Estimating galaxy group masses via caustic analysis
• The XXL Survey: XXXVI. Evolution and black hole feedback of high-excitation and low-excitation radio galaxies in XXL-S
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• The Variation of the Galaxy Luminosity Function with Group Properties
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• WISDOM project -- VIII. Multi-scale feedback cycles in the brightest cluster galaxy NGC 0708
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• The WIRCam Deep Survey II: Mass Selected Clustering
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• The Atacama Cosmology Telescope: the stellar content of galaxy clusters selected using the Sunyaev-Zel'dovich effect
• Understanding the redshift evolution of the luminosity functions of Lyman-alpha emitters
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• Lyα emitters in a cosmological volume I: the impact of radiative transfer
• Star Formation and AGN Feedback in the Local Universe: Combining LOFAR and MaNGA
• The mass and environmental dependence on the secular processes of AGN in terms of morphology, colour, and specific star-formation rate
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• Observable consequences of kinetic and thermal AGN feedback in elliptical galaxies and galaxy clusters
• The Evolution and Environments of X-ray Emitting Active Galactic Nuclei in High-Redshift Large-Scale Structures
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• The 6C** sample of steep-spectrum radio sources: II - Redshift distribution and the space density of high-redshift radio galaxies
• Tracing star formation with non-thermal radio emission
• The scaling relation between the mass of supermassive black holes and the kinetic energy of random motions of the host galaxies
• The Structure of Reionization in Hierarchical Galaxy Formation Models
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• Two phase galaxy formation: The Gas Content of Normal Galaxies
• The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
• A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
• Quasar Host Environments: The view from Planck
• Active Galactic Nuclei outflows in galaxy discs
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• Intermittent AGN episodes drive outflows with a large spread of observable loading factors
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• [OII] emitters in MultiDark-Galaxies and DEEP2
• GOODS-ALMA 2.0: Last gigayear star formation histories of the so-called starbursts within the main sequence
• Evidence of wind signatures in the gas velocity profiles of Red Geysers
• Herschel-ATLAS: the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects
• Identifying the progenitor set of present-day early-type galaxies: a view from the standard model
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations
• Universal Merger Histories of Dark-Matter Haloes
• Sersic Properties of Disc Galaxy Mergers
• The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure
• RAiSE: simulation-based analytical model of AGN jets and lobes
• Violent quenching: molecular gas blown to 1000 km/s during a major merger
• An Analysis Framework for Understanding the Origin of Nuclear Activity in Low-Power Radio Galaxies
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• On the connection between the metal-enriched intergalactic medium and galaxies: an OVI-galaxy cross-correlation study at $z<1$
• Atomic-to-molecular gas phase transition triggered by the radio jet in Centaurus A
• Searching For Fossil Evidence of AGN Feedback in WISE-Selected Stripe-82 Galaxies By Measuring the Thermal Sunyaev-Zel'dovich Effect With the Atacama Cosmology Telescope
• The galaxy correlation function as a constraint on galaxy formation physics
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Emergences of C IV narrow absorption troughs in the quasar SDSS J095254.10+021932.8
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
• Radio Morphology of Red Geysers
• Luminosity bias: from haloes to galaxies
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• The Evolution of K* and the Halo Occupation Distribution since z=1.5: Observations vs. Simulations
• A Moderate Cooling Flow Phase at Galaxy Formation
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• MUSE discovers perpendicular arcs in the inner filament of Cen A
• Boosting hierarchical structure formation with scalar-interacting dark matter
• Massive Lyman Break Galaxies at z~3 in the Spitzer Extragalactic First Look Survey
• Termination of star formation by BH feedback in equal- and unequal-mass mergers of disk and elliptical galaxies
• Predictions for the detection of Tidal Streams with Gaia using Great Circle Methods
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• The LOFAR Two Metre Sky Survey: Deep Fields. II. The ELAIS-N1 LOFAR deep field
• Does jackknife scale really matter for accurate large-scale structure covariances?
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• Outflows, Inflows and Young Stars in the inner 200 pc of the Seyfert galaxy NGC 2110
• The HI mass function as a probe of photoionisation feedback on low mass galaxy formation
• Connecting radio emission to AGN wind properties with Broad Absorption Line Quasars
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IX. Identification of Two Red Quasars at z > 5.6
• Measuring the jet power of flat spectrum radio quasars
• Star formation trends in high-redshift galaxy surveys: the elephant or the tail?
• Observed versus modelled u,g,r,i,z-band photometry of local galaxies - Evaluation of model performance
• The submillimetre view of massive clusters at z~0.8-1.6
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• On the Interaction of the PKS B1358-113 Radio Galaxy with the Abell 1836 Cluster
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• On the dependence of galaxy morphologies on galaxy mergers
• Precessing winds from the nucleus of the prototype Red Geyser?
• The Galactic Environment of the NeVIII Absorber toward HE0226-4110
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• The Elephant in the Bathtub: when the physics of star formation regulate the baryon cycle of galaxies
• Wide and deep near-UV (360nm) galaxy counts and the extragalactic background light with the Large Binocular Camera
• Radio Galaxy Zoo: Observational evidence for environment as the cause of radio source asymmetry
• II. Apples to apples $A^2$: cluster selection functions for next-generation surveys
• Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
• 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
• Hiding in Plain Sight - Recovering Clusters of Galaxies with the Strongest AGN in Their Cores
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• HST emission-line images of nearby 3CR radio galaxies: two photoionization, accretion and feedback modes
• Automatic detection of peculiar galaxy pairs in Sloan Digital Sky Survey
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Are galaxies with AGN a transition population?
• Theoretical reevaluations of the black hole mass - bulge mass relation - I. Effect of the seed black hole mass
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• Remarks on the methods of investigations of alignment of galaxies
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• G.A.S. II: Dust extinction in galaxies; Luminosity functions and InfraRed eXcess
• Galaxies behind the Galactic plane: First results and perspectives from the VVV Survey
• The abundance of satellites depends strongly on the morphology of the host galaxy
• Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar halo
• Metal enrichment in a semi-analytical model, fundamental scaling relations, and the case of Milky Way galaxies
• SMBH accretion properties of radio-selected AGN out to z~4
• Constraints on a scale-dependent bias from galaxy clustering
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• Signatures of inflowing gas in red geyser galaxies hosting radio-AGN
• Satellite quenching and morphological transformation of galaxies in groups and clusters
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Molecular Flows in Contemporary Active Galaxies and the Efficacy of Radio-Mechanical Feedback
• Herschel and Hubble study of a lensed massive dusty starbursting galaxy at $z\sim 3$
• The evolution of radio sources in the UKIDSS-DXS XMM-LSS field
• The relation of cosmic environment and morphology with the star formation and stellar populations of AGN and non-AGN galaxies
• The Cosmic History of Hot Gas Cooling and Radio AGN Activity in Massive Early-Type Galaxies
• Modelling the dusty universe I: Introducing the artificial neural network and first applications to luminosity and colour distributions
• Highly Ionized Collimated Outflow from HE 0238 - 1904
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Radio loud AGN and the L_X - σrelation of galaxy groups and clusters
• QSOFEED: The relationship between star formation and AGN Feedback
• Cosmological Simulations of Massive Compact High-z Galaxies
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Imaging the environment of a z = 6.3 submillimeter galaxy with SCUBA-2
• Dissecting galaxy formation models with Sensitivity Analysis -- A new approach to constrain the Milky Way formation history
• Evolution of the Most Massive Galaxies to z ~ 0.6: II. The link between radio AGN activity and star formation
• Forensic reconstruction of galaxy colour evolution and population characterisation
• Maximum Likelihood Random Galaxy Catalogues and Luminosity Function Estimation
• Investigating the properties of AGN feedback in hot atmospheres triggered by cooling-induced gravitational collapse
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Physical constraints on the central mass and baryon content of satellite galaxies
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• The impact of black hole seeding in cosmological simulations
• The Spitzer Extragalactic Representative Volume Survey (SERVS): The Environments of High-z SDSS Quasi-Stellar-Objects
• The active and passive populations of Extremely Red Objects
• Inverse Compton X-ray halos around high-z radio galaxies: A feedback mechanism powered by far-infrared starbursts or the CMB?
• The SMBH mass versus M_G sigma^2 relation: A comparison between real data and numerical models
• Properties of Luminous Red Galaxies in the Sloan Digital Sky Survey
• Constraints on the velocity profiles of galaxies from strong lensing statistics and semi-analytical modelling of galaxy formation
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Towards an understanding of third-order galaxy-galaxy lensing
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• The XXL Survey: XXXI. Classification and host galaxy properties of 2.1 GHz ATCA XXL-S radio sources
• AGN and quasar science with aperture masking interferometry on the James Webb Space Telescope
• SALT spectroscopic observations of galaxy clusters detected by ACT and a Type II quasar hosted by a brightest cluster galaxy
• The Clusters Hiding in Plain Sight (CHiPS) survey: Complete sample of extreme BCG clusters
• The strong environmental dependence of black hole scaling relations
• Star formation in mergers with cosmologically motivated initial conditions
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Stellar Populations of Luminous Evolved Galaxies at z~1.5
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• A search of CO emission lines in blazars: the low molecular gas content of BL Lac objects compared to quasars
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Investigation of the orientation of galaxies in clusters: the importance, methods and results of research
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• Cosmological growth and feedback from supermassive black holes
• Evolution of gaseous disk viscosity driven by supernova explosion in star-forming galaxies at high redshift
• Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
• A single galaxy population? statistical evidence that the Star-Forming Main Sequence might be the tip of the iceberg
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• How feedback shapes galaxies: an analytic model
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Identifying dynamically young galaxy groups via wide-angle tail galaxies: A case study in the COSMOS field at z=0.53
• Is the observed high-frequency radio luminosity distribution of QSOs bimodal?
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• On the relation between Lya absorbers and local galaxy filaments
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Galaxy Clusters in the Line of Sight to Background Quasars: II. Environmental effects on the sizes of baryonic halo sizes
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Revealing a Highly-Dynamic Cluster Core in Abell 1664 with Chandra
• Searching for molecular outflows in Hyper-Luminous Infrared Galaxies
• Modeling active galactic nuclei: ongoing problems for the faint-end of the luminosity function
• Observations of the High Redshift Universe
• Merger Histories and Environments of Dwarf AGN in IllustrisTNG
• Role of ionizing background on the statistics of metal absorbers in hydrodynamical simulations
• The growth of typical star-forming galaxies and their super massive black holes across cosmic time since z~2
• No evidence for excess AGN activity in recently quenched massive galaxies at cosmic noon
• Testing galaxy formation models with galaxy stellar mass functions
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• Massive spheroids can form in single minor mergers
• Dark-ages reionization and galaxy formation simulation -- XVIII. The high-redshift evolution of black holes and their host galaxies
• Analytic and numerical realisations of a disk galaxy
• The Properties of Massive Star-forming galaxies with Outside-in Assembly Mode
• Characteristic mass in galaxy quenching: environmental versus internal effects
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• HiZELS: the High Redshift Emission Line Survey with UKIRT
• A SCUBA-2 survey of FeLoBAL QSOs: Are FeLoBALs in a `transition phase' between ULIRGs and QSOs?
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Physical properties of the CDFS X-ray sources through fitting spectral energy distributions
• AGNs at the cosmic dawn: predictions for future surveys from a $\Lambda$CDM cosmological model
• The Rest-frame $H$-band Luminosity Function of Red Sequence Galaxies in Clusters at $1.0<z<1.3$
• Galaxy formation with cold gas accretion and evolving stellar initial mass function
• Rest-frame ultra-violet spectra of massive galaxies at z=3: evidence of high-velocity outflows
• 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 dependency of AGN infrared color-selection on source luminosity and obscuration: An observational perspective in CDFS and COSMOS
• Timescales for Hi consumption and SFR depletion of satellite galaxies in groups
• LoTSS/HETDEX: Disentangling star formation and AGN activity in gravitationally-lensed radio-quiet quasars
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• The relation between galaxy density and radio jet power for 1.4 GHz VLA selected AGN in Stripe 82
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• Dynamical analysis of strong-lensing galaxy groups at intermediate redshift
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• The environment of radio galaxies: A signature of AGN feedback at high redshifts
• Feedback in Galaxy Formation
• CO in the ALMA Radio-Source Catalogue (ARC): the molecular gas content of radio galaxies as a function of redshift
• COSMOS-Web: A history of galaxy migrations over the stellar mass-star formation rate plane
• Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmology
• RAiSE X: searching for radio galaxies in X-ray surveys
• 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
• Infrared spectroscopy of nearby radio active elliptical galaxies
• A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
• Evolution of Supermassive Black Holes from Cosmological Simulations
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• Far-infrared emission in luminous quasars accompanied by nuclear outflows
• Variation in the escape fraction of ionising photons from galaxies and the redshifted 21-cm power spectrum during reionization
• Episodic activities of supermassive black holes at redshift $z\le 2$: driven by mergers?
• A new gas cooling model for semi-analytical galaxy formation models
• The Discovery of a Hidden Broad Line AGN in a Bulgeless Galaxy: Keck NIR Spectroscopic Observations of SDSS J085153.64+392611.76
• [OIII] emission in z=2 quasars with and without Broad Absorption Lines
• Consequences of dark matter self-annihilation for galaxy formation
• Formation of a barred galaxy in a major merger: The role of AGN feedback
• 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
• A Bayesian Monte-Carlo Analysis of the M-sigma Relation
• Galaxy evolution across the optical emission-line diagnostic diagrams?
• Neglecting Primordial non-Gaussianity Threatens Future Cosmological Experiment Accuracy
• A correlation between the stellar and [Fe II] velocity dispersions in Active Galaxies
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• Optical Properties of Peaked Spectrum Radio Sources
• Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Can We Detect the Color-Density Relation with Photometric Redshifts?
• Evolution of Dust-Obscured Star Formation and Gas to z=2.2 from HiZELS
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• The First Galaxy Cluster Discovered by the VISTA Variables in the Vía Láctea Survey
• An empirical model to form and evolve galaxies in dark matter halos
• The scale dependence of mass assembly in galaxies
• The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation
• Spectroastrometry of rotating gas disks for the detection of supermassive black holes in galactic nuclei. II. Application to the galaxy Centaurus A (NGC 5128)
• A spectroscopic measure of the star-formation rate density in dwarf galaxies at z~1
• AGN in the CALIFA survey: X-ray detection of nuclear sources
• Spectral age distribution for radio-loud active galaxies in the XMM-LSS field
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• Numerical simulations of bar formation in the Local Group
• 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
• Where Do Obscured AGN Fit in A Galaxy's Timeline?
• Modelling emission lines in star forming galaxies
• Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• The ALPINE-ALMA [CII] Survey: CGM pollution and gas mixing by tidal stripping in a merging system at z~4.57
• Early Quenching of Massive Protocluster Galaxies Around z=2.2 Radio Galaxies
• Star formation in high redshift galaxies including Supernova feedback: effect on stellar mass and luminosity functions
• The Science Case for PILOT III: the Nearby Universe
• Astrophysics in 2006
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• The Evolution of the Low-Frequency Radio AGN Population to $z\simeq 1.5$ in the ELAIS N1 Field
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• Bimodal AGNs in Bimodal Galaxies
• Revisiting the Color-Color Selection: Submillimeter and AGN Properties of NUV-r-J Selected Quiescent Galaxies
• Rapidly varying accretion and AGN feedback
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• The Quasar Feedback Survey: zooming into the origin of radio emission with e-MERLIN
• Modelling the evolution of galaxies as a function of environment
• Weighing neutrinos using high redshift galaxy luminosity functions
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• The Circumgalactic Medium in Massive Halos
• Efficient uniform designs for multi-wave computer experiments
• The Size Function of Galaxy Disks out to z ~ 1 from the Canada-France-Hawaii-Telescope Legacy Survey
• Spectroastrometry of rotating gas disks for the detection of supermassive black holes in galactic nuclei. III. CRIRES observations of the Circinus galaxy
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Using galaxy pairs as cosmological tracers
• Gravitational-wave event rates as a new probe for dark matter microphysics
• The bimodality of the 10k zCOSMOS-bright galaxies up to z ~ 1: a new statistical and portable classification based on the optical galaxy properties
• A sample of mJy radio sources at 1.4 GHz in the Lynx and Hercules fields - I. Radio imaging, multicolour photometry and spectroscopy
• Winds and feedback from supermassive black holes accreting at low rates: Hydrodynamical treatment
• Leaving the dark ages with AMIGA
• 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
• Luminosity Functions of XMM-LSS C1 Galaxy Clusters
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Thermal and Chemical Evolution of Collapsing Filaments
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• Jet-Feedback on kpc scales: a review
• Starburst galaxies in semi-analytic models of galaxy formation and evolution
• Lack of Correlations between Cold Molecular Gas and AGN Properties in Type 1 AGNs at $z\lesssim 0.5$
• Does a radio jet drive the massive multi-phase outflow in the ultra-luminous infrared galaxy IRAS 10565+2448?
• On merger bias and the clustering of quasars
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Recovering dark-matter clustering from galaxies with Gaussianization
• LARgE Survey. I. Dead Monsters: the Massive End of the Passive Galaxy Stellar Mass Function at Cosmic Noon
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Clustering and descendants of MUSYC galaxies at z<1.5
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• An Absence of Radio-Loud Active Galactic Nuclei in Geometrically Flat Quiescent Galaxies: Implications for Maintenance-Mode Feedback Models
• The Clusters Hiding in Plain Sight (CHiPS) survey: A first discovery of a massive nearby cluster around PKS1353-341
• Radial stellar populations of AGN-host dwarf galaxies in SDSS-IV MaNGA survey
• Physical Properties, Star Formation, and Active Galactic Nucleus Activity in Balmer Break Galaxies at 0 < z < 1
• Does the Compact Radio Jet in PG 1700+518 Drive a Molecular Outflow?
• Optical and X-ray profiles in the REXCESS sample of galaxy clusters
• On the Evolution of the Star Formation Rate Function of Massive Galaxies. Constraints at 0.4<z<1.8 from the GOODS-MUSIC Catalogue
• Stellar populations of galaxies in the ALHAMBRA survey up to $z\sim 1$. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass$-$colour and the $UVJ$ colour$-$colour diagrams
• Galaxy Formation and Dark Matter
• Are compact groups hostile towards faint galaxies?
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• The distribution of galaxies gravitational field stemming from their tidal interaction
• The abundance of satellite galaxies in the inner region of $\Lambda$CDM Milky Way sized haloes
• Luminous satellite galaxies in gravitational lenses
• Dust extinction map of the Galactic plane based on the VVV survey data
• Probing the link between quenching and morphological evolution
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• Dynamical friction of a massive black hole in a turbulent gaseous medium
• The VOICE Survey : VST Optical Imaging of the CDFS and ES1 Fields
• Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows III: Observability and Connection to Halo Globular Clusters
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Spatially Extended [P II]1.188um and [Fe II]1.257um Emission Lines in a Nearby Seyfert Galaxy NGC 1068 Observed with OAO/ISLE
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• A 100-kpc inverse Compton X-ray halo around 4C60.07 at z=3.79
• The Close AGN Reference Survey (CARS): No evidence of galaxy-scale hot outflows in two nearby AGN
• The changing ISM of massive elliptical galaxies and cosmic evolution of radio galaxies and quasars
• A deep learning approach to halo merger tree construction
• Multi-wavelength consensus of large-scale linear bias
• Active Galactic Nuclei signatures in Red Geyser galaxies from Gemini GMOS-IFU observations
• Positive and negative feedback by AGN jets in high-redshift galaxies
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• Radio Galaxy 3C 230 Observed with Gemini Laser-Adaptive-Optics Integral-Field Spectroscopy
• MaNGA AGN dwarf galaxies (MAD) -- II. AGN outflows in dwarf galaxies
• Exploring the Active Galactic Nuclei population with extreme X-ray to optical flux ratios (Fx/Fo >50)
• The Occurrence of Compact Groups of Galaxies Through Cosmic Time
• Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Evolution of black hole and galaxy growth in a semi-numerical galaxy formation model
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• A general approach to quenching and galactic conformity
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• The LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap I. The Spectroscopic Redshift Catalog
• Mid-infrared Spectral Properties of Post-Starburst Quasars
• A Model of the Cosmic Infrared Background Produced by Distant Galaxies
• Chemical evolution of elliptical galaxies I: supernovae and AGN feedback
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• The Evolution of Radio Galaxies and X-ray Point Sources in Coma Cluster Progenitors Since z~1.2
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• A Hubble Space Telescope Imaging Study of Four FeLoBAL Quasar Host Galaxies
• Tidal Dwarf Galaxies at Intermediate Redshifts
• Red bulgeless galaxies in SDSS DR7. Are there any AGN hosts?
• The Degeneracy of Galaxy Formation Models
• Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution
• The Nature of Star Formation at 24 microns in the Group Environment at 0.3 < z < 0.55
• On the star formation efficiency in high redshift Lyman-α emitters
• Observations of Ly$\alpha$ Emitters at High Redshift
• VLT-MUSE spectroscopy of AGNs misclassified by BPT diagnostic or with weak emission lines
• Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• Testing a prediction of the merger origin of early-type galaxies: a correlation between stellar populations and asymmetry
• Unveiling a new structure behind the Milky Way
• The kinematics of globular clusters systems in the outer halos of the Aquarius simulations
• A hybrid multi resolution scheme to efficiently model the structure of reionization on the largest scales
• Measuring galaxy-galaxy-galaxy-lensing with higher precision and accuracy
• A physical model for the redshift evolution of high-z Lyman-Break Galaxies
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Dynamics of Lyman Break Galaxies and Their Host Halos
• A multi-band AGN-SFG classifier for extragalactic radio surveys using machine learning
• Astrophysics with the Laser Interferometer Space Antenna
• The X-Ray Zurich Environmental Study (X-ZENS). II. X-ray Observations of the Diffuse Intragroup Medium in Galaxy Groups
• Galaxy luminosity function and its cosmological evolution: Testing a new feedback model depending on galaxy-scale dust opacity
• A mass threshold in the number density of passive galaxies at z$\sim$2
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Disk Galaxy Evolution Along the Hubble Sequence
• What is the origin of the JWST SMBHs?
• Extending PLE models into the mid-IR, far-IR & sub-mm
• A Census of Mid-Infrared Selected Active Galactic Nuclei in Massive Galaxy Clusters at 0 < z < 1.3
• Intracluster gas pressure, entropy injection and redshift evolution
• Infall Profiles for Supercluster-Scale Filaments
• Efficient Identification of Broad Absorption Line Quasars using Dimensionality Reduction and Machine Learning
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• Identifying type II quasars at intermediate redshift with few-shot learning photometric classification
• Suppression of Star Formation in the Hosts of Low-Excitation Radio Galaxies
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Connecting Star Formation Quenching with Galaxy Structure and Supermassive Black Holes through Gravitational Heating of Cooling Flows
• Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• Advection-dominated accretion, jets and the spectral energy distribution of LINERs
• The environments of the radio galaxy population in SIMBA
• Red riding on hood: Exploring how galaxy colour depends on environment
• The global energetics of radio AGN kinetic feedback in the local universe
• Galaxy formation from a timescale perspective
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• Quantifying the Projected Suppression of Cluster Escape Velocity Profiles
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• The Co-Evolution of Galaxies and Black Holes: Current Status and Future Prospects
• Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• On the exclusion of intra-cluster plasma from AGN-blown bubbles
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• Sensitivity analysis of a galaxy formation model
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• The other side of Bulge Formation in a Lambda-CDM cosmology: Bulgeless Galaxies in the Local Universe
• Quasar emission lines, radio structures and radio unification
• Massive Black Hole Mergers
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• A Large Massive Quiescent Galaxy Sample at z~1.2
• Formation of Compact Clusters from High Resolution Hybrid Cosmological Simulations
• The feedback of quasars on their galactic environment
• On the accuracy of the high redshift cluster luminosity function
• A detached double X-ray tail in the merging galaxy cluster Z8338 with a large double tail
• Insights into environmental quenching at $z\sim 1$: an enhancement of faint, low-mass passive galaxies in clusters
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Evolution of the real-space correlation function from next generation cluster surveys
• Jet-mode feedback in NGC 5972: insights from resolved MUSE, GMRT and VLA observations
• Radio Properties of Cavities in the ICM: Imprints of AGN Activity
• The impact of binary star yields on the spectra of galaxies
• The EDGE-CALIFA survey: The effect of active galactic nucleus feedback on the integrated properties of galaxies at different stages of their evolution
• An Improved Treatment of Cosmological Intergalactic Medium Evolution
• Simulations of the accreted stellar halos of low-mass field galaxies
• Rest-Frame Ultraviolet to Near Infrared Observations of an Interacting Lyman Break Galaxy at z = 4.42
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Solving the puzzle of subhalo spins
• Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
• Effect of generic dark matter halo on transonic accretion onto galactic black holes
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• Geometrical tests of cosmological models. III. The cosmology-evolution diagram at z=1
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Reconstructing the LISA massive black hole binary population via iterative kernel density estimation
• The Formation and Evolution of Massive Galaxies
• Model-independent Reconstruction of UV Luminosity Function and Reionization Epoch
• The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Galaxy Interactions, Star Formation History, and Bulgeless Galaxies
• Multiwavelength Analysis of a Nearby Heavily Obscured AGN in NGC 449
• Detection of H-alpha emission from z>3.5 submillimetre luminous galaxies with AKARI-FUHYU spectroscopy
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• The non-Gaussian distribution of galaxies gravitational fields
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• On the behaviour of streams in angle and frequency spaces in different potentials
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Highly ionized gas on galaxy scales: mapping the interacting Seyfert galaxy LEDA 135736
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• Environmental Effects on the Star Formation Activity at z~0.9 in the COSMOS Field
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• The star-formation history of the Milky Way Galaxy
• Beyond diagnostic-diagrams: A critical exploration on the classification of ionization processes
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
• The size and mass evolution of the massive galaxies over cosmic time
• The stellar and hot gas content of low-mass galaxy clusters
• The interaction between feedback from active galactic nuclei and supernovae
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• Cool gas accretion, thermal evaporation and quenching of star formation in elliptical galaxies
• The galaxy-environment connection revealed by constrained simulations
• Why and when is internally-driven AGN feedback energetically favoured?
• Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9
• Orientation of galaxies in structures
• LeMMINGs. V. Nuclear activity and bulge properties: a detailed multi-component decomposition of $e$-MERLIN Palomar galaxies with $HST$
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• The Baryonic and Dark Matter Properties of High Redshift Gravitationally Lensed Disk Galaxies
• Hydrostatic equilibrium of a porous intracluster medium: implications for mass fraction and X-ray luminosity
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Lower-Luminosity Obscured AGN Host Galaxies are Not Predominantly in Major-Merging Systems at Cosmic Noon
• Influences of galaxy interactions on AGN activity
• Photometric variability in star-forming galaxies as evidence for low-mass AGN and a precursor to quenching
• Estimating the mass of galactic components using machine learning algorithms
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• On the signature of black holes on the quenched stellar mass function
• The life of central radio galaxies in clusters: AGN-ICM studies of eRASS1 clusters in the ASKAP fields
• Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs
• Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
• The Shape of AGN-Driven Winds in the Seyfert Galaxy NGC 3516
• Morphological Feature Distances Among the Spectral Types of SDSS Galaxies
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• The progenitor galaxies of stellar haloes as "failed" Milky Ways
• Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• The landscape of massive black-hole spectroscopy with LISA and Einstein Telescope
• Atmospheric pressure and molecular cloud formation in early-type galaxies
• Extended Hernquist-Springel formalism for cosmic star formation
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• The Homogeneous Properties of Halpha-Selected Galaxies at (0.05<z<0.15)
• Establishing the impact of powerful AGN on their host galaxies
• A Halo Merger Tree Generation and Evaluation Framework
• Angular momentum and morphological sequence of massive galaxies through Dark Sage
• The impact of AGN on their host galaxies
• A neutrino model fit to the CMB power spectrum
• The nature of the variable millimetre-selected AGN in the Brightest Cluster Galaxy of Abell 851
• Cosmological evolution of the AGN Kinetic Luminosity Function
• Formation and evolution of disk galaxies
• Modelling the outskirts of galaxies in a cosmological context
• Fast and Slow Rotators: The build-up of the Red Sequence
• Mutual feedback between star formation and nuclear activity
• Growing supermassive black holes: sub-grid modelling and intermediate-scale processes
• Physical Drivers of Emission Line Diversity of SDSS Seyfert 2s and LINERs After Removal of Contributions by Star Formation
• Investigating the spectra and physical nature of galaxy scale jets
• Gravity at Work: How the Build-Up of Environments Shape Galaxy Properties
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• Red Galaxies from Hot Halos in Cosmological Hydro Simulations
• A GMRT 610 MHz radio survey of the North Ecliptic Pole (NEP, ADF-N) / Euclid Deep Field North
• Massive black holes and their galaxies
• Star formation activity in Balmer break galaxies at $z$ < 1.5
• A multiwavelength study of near- and mid-infrared selected galaxies at high redshift: ERGs, AGN-identification and the contribution from dust
• Dissecting the multiple-component outflow in NGC 5548 with absorption-line Variability
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• The nuclear to host galaxy relation of high redshift quasars
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• The splash beneath the largest radio bubble in a cluster core
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• The origin of ionized gas in retired galaxies: dynamical clues
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• An Estimate of the Impact of Reionization on Supermassive Black Hole Growth
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Physical conditions in Centaurus A's northern filaments II: Does the HCO${}^{+}$ emission highlight the presence of shocks?
• Implication of a galaxy-scale negative feedback by one of the most powerful multi-phase outflows in a hyper-luminous infrared galaxy at the intermediate redshift