What Shapes the Luminosity Function of Galaxies?

Abstract

We investigate the physical mechanisms that shape the luminosity function. Beginning with the mass function of dark matter halos, we show how gas cooling, photoionization, feedback, merging and thermal conduction affect the shape of the luminosity function. We consider three processes whereby supernovae can affect the forming galaxy: (1) reheating of disk gas to the halo temperature; (2) expansion of the diffuse halo gas; (3) expulsion of cold disk gas from the halo. While feedback of form (1) is able to flatten the faint end of the luminosity function, this alone does not produce the sharp cut-off observed at large luminosities. Feedback of form (2) is also unable to solve this problem. The relative paucity of very bright galaxies can only be explained if cooling in massive halos is strongly suppressed. Conduction is a promising mechanism, but an uncomfortably high efficiency is required to suppress cooling to the desired level. If, instead, superwinds are responsible for the lack of bright galaxies, then the total energy budget required to obtain a good match to the galaxy luminosity function greatly exceeds the energy available from supernova explosions. The mechanism is only viable if the formation of central supermassive black holes play a crucial role in limiting the amount of stars that form in the host galaxy. (abridged)

10 pages, 5 figures. Submitted to ApJ

References in corpus (51)

• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Halo Models of Large Scale Structure
• Hierarchical Galaxy Formation
• Mass function of dark matter halos
• The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
• Halo occupation numbers and galaxy bias
• The 2dF Galaxy Redshift Survey: Near Infrared Galaxy Luminosity Functions
• X-ray Imaging Spectroscopy of Abell 1835
• Galaxies and Intergalactic Matter at Redshift z~3: Overview
• The K-Band Galaxy Luminosity Function
• Thermal Conduction in Clusters of Galaxies
• The Effects of Photoionization on Galaxy Formation - I: Model and Results at z=0
• New Observations of the Interstellar Medium in the Lyman Break Galaxy MS 1512-cB58
• Starburst-driven galactic winds: I. Energetics and intrinsic X-ray emission
• The Halo Occupation Distribution and the Physics of Galaxy Formation
• X-ray Spectroscopy of the Cluster of Galaxies Abell 1795 with XMM-Newton
• The Deuterium to Hydrogen Abundance Ratio Towards a Fourth QSO: HS0105+1619
• A Model of Supernovae Feedback in Galaxy Formation
• Discovery of Ghost Cavities in Abell 2597's X-ray Atmosphere
• Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA
• Modified-Entropy Models for the Intracluster Medium
• Weak Lensing Results from the 75 Square Degree CTIO Survey
• The New Emerging Model for the Structure of Cooling Cores in Clusters of Galaxies
• Constraints on Omega_m and sigma_8 from weak lensing in RCS fields
• Chandra observations of Abell 2199
• Bubbles, feedback and the intra-cluster medium: three-dimensional hydrodynamic simulations
• On the soft X-ray spectrum of cooling flows
• Cosmological constraints from the local X-ray luminosity function of the most X-ray luminous galaxy clusters
• Is cosmology consistent?
• Gravitating mass profiles of nearby galaxy clusters and relations with X-ray gas temperature, luminosity and mass
• Interaction of Radio Lobes with the Hot Intracluster Medium: Driving Convective Outflow in Hydra A
• Joint Cosmic Shear Measurements with the Keck and William Herschel Telescopes
• The growth of galaxies in cosmological simulations of structure formation
• Including star formation and supernova feedback within cosmological simulations of galaxy formation
• Magnetic fields in the Centaurus cluster
• Conduction and cooling flows
• The Impact of Galaxy Formation on the X-ray Evolution of Clusters
• Constraining the Matter Power Spectrum Normalization using the SDSS/RASS and REFLEX Cluster surveys
• Simulation of radio plasma in clusters of galaxies
• Chandra X-ray observations of the 3C295 cluster core
• Gas cooling in simulations of the formation of the galaxy population
• The Hawaii-AAO K-band Galaxy Redshift Survey -- Paper I: The Local K-band Luminosity Function
• Simulations of galaxy formation in a cosmological volume
• On conduction, cooling flows and galaxy formation
• A Comparison of Semi-Analytic and Smoothed Particle Hydrodynamics Galaxy Formation
• AGN Feedback on the Intracluster Medium
• A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
• Measuring Sigma8 with Cluster Lensing : Biases from Unrelaxed Clusters
• Cosmological Constraints from a Combined Analysis of the Cluster Mass Function and Microwave Background Anisotropies
• Implications of 2dFGRS results on cosmic structure

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• Direct evidence of AGN-feedback: a post starburst galaxy stripped of its gas by AGN-driven winds
• The evolution of the star forming sequence in hierarchical galaxy formation models
• X-ray selected AGN Hosts are Similar to Inactive Galaxies out to z=3: Results from CANDELS/CDF-S
• The abundance of Lyman-(α) emitters in hierarchical models
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• The Lifetime of FRIIs in Groups and Clusters: Implications for Radio-Mode Feedback
• The role of submillimetre galaxies in hierarchical galaxy formation
• Dissipationless Merging and the Assembly of Central Galaxies
• Galaxy-scale AGN Feedback - Theory
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• 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
• Another thread in the tapestry of stellar feedback: X-ray binaries
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• Tracing the Quenching Journey across Cosmic Time
• Impact of H_2-based star formation model on the z>=6 luminosity function and the ionizing photon budget for reionization
• Properties of ionized outflows in MaNGA DR2 galaxies
• Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies
• A simple model for AGN feedback in nearby early-type galaxies
• CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST
• On the origin of excess cool gas in quasar host halos
• Constraints on the star formation histories of galaxies from z~1 to z~0
• Luminosity function of galaxies in groups in the SDSS DR7: the dependence on mass, environment and galaxy type
• The Galaxy Luminosity Function from M_R = -25 to M_R = -9
• Evolution of blue E/S0 galaxies from z~1: merger remnants or disk rebuilding galaxies?
• AGN Jet-induced Feedback in Galaxies. II. Galaxy colours from a multicloud simulation
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• A Chandra study of the large-scale shock and cool filaments in Hydra A: Evidence for substantial gas dredge-up by the central outburst
• Massive galaxies on the road to quenching: ALMA observations of powerful high redshift radio galaxies
• Bivariate Galaxy Luminosity Functions in the Sloan Digital Sky Survey
• Kinematic constraints on the stellar and dark matter content of spiral and S0 galaxies
• Two-Phase Galaxy Formation
• High Radio Frequency Properties and Variability of Brightest Cluster Galaxies
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• O VI Emission Imaging of a Galaxy with the Hubble Space Telescope: a Warm Gas Halo Surrounding the Intense Starburst SDSS J115630.63+500822.1
• Evolution of X-ray cavities
• Galactic Winds in Cosmological Simulations of the Circumgalactic Medium
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• The structural and photometric properties of early-type galaxies in hierarchical models
• Where do "red and dead" early-type void galaxies come from?
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• 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 specific star formation rate of high redshift galaxies: the case for two modes of star formation
• The environments of high redshift radio galaxies and quasars: probes of protoclusters
• Observational tests of the evolution of spheroidal galaxies
• Rest-frame UV--Optically Selected Galaxies at 2.3<z<3.5: Searching for Dusty Star-forming and Passively-Evolving Galaxies
• First results from the JWST Early Release Science Program Q3D: The Warm Ionized Gas Outflow in z ~ 1.6 Quasar XID 2028 and its Impact on the Host Galaxy
• A modified star formation law as a solution to open problems in galaxy evolution
• The UV colours and dust attenuation of Lyman-break galaxies
• Characterizing the formation history of Milky Way-like stellar haloes with model emulators
• The ugrizYJHK luminosity distributions and densities from the combined MGC, SDSS and UKIDSS LAS datasets
• The Next Generation Virgo Cluster Survey. VII. The intrinsic shapes of low-luminosity galaxies in the core of the Virgo cluster, and a comparison with the Local Group
• How runaway stars boost galactic outflows
• Metal enriched gaseous halos around distant radio galaxies: Clues to feedback in galaxy formation
• The Evolving Faint-End of the Luminosity Function
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• A simple model linking galaxy and dark matter evolution
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Optical and Near-Infrared Integral Field Spectroscopy of the SCUBA Galaxy N2-850.4
• The Production of Cold Gas Within Galaxy Outflows
• Characterising the Far-infrared Properties of Distant X-ray Detected AGNs: Evidence for Evolution in the Infrared--X-ray Luminosity Ratio
• On the origin of the angular momentum properties of gas and dark matter in galactic halos and its implications
• The triggering of local AGN and their role in regulating star formation
• Galaxies Probing Galaxies at High Resolution: Co-Rotating Gas Associated with a Milky Way Analog at z=0.4
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Probing multi-phase outflows and AGN feedback in compact radio galaxies: the case of PKSB 1934-63
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• Evolution of the Stellar Mass Tully-Fisher Relation in Disk Galaxy Merger Simulations
• BASS XXXI: Outflow scaling relations in low redshift X-ray AGN host galaxies with MUSE
• Cold filaments in galaxy clusters: effects of heat conduction
• The ELIXR Galaxy Survey. II: Baryons and Dark Matter in an Isolated Elliptical Galaxy
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
• Detecting Radio-AGN signatures in Red geysers
• The MOSDEF survey: the prevalence and properties of galaxy-wide AGN-driven outflows at $z\sim 2$
• Deep spectroscopic luminosity function of Abell 85: no evidence for a steep upturn of the faint-end slope
• The first Super Massive Black Holes: indications from models for future observations
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• The galaxies that reionized the Universe
• Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties
• The specific star formation rate and stellar mass fraction of low-mass central galaxies in cosmological simulations
• Luminous Red Galaxies in hierarchical cosmologies
• Catastrophic Cooling in Superwinds: Line Emission and Non-equilibrium Ionization
• The Sunyaev-Zeldovich Background
• SINFONI/VLT 3D spectroscopy of massive galaxies: Evidence of rotational support at z~1.4
• Supernova-Driven Outflows in NGC 7552: A Comparison of H-alpha and UV Tracers
• Predictions for the intrinsic UV continuum properties of star forming galaxies and the implications for inferring dust extinction
• Simulating Supersonic Turbulence in Galaxy Outflows
• Multi-phase outflows in post starburst E+A galaxies -- II. A direct connection between the neutral and ionized outflow phases
• Mass transport by buoyant bubbles in galaxy clusters
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Disentangling the dark matter halo from the stellar halo
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$
• Evidence of ongoing AGN-driven feedback in a quiescent post starburst E+A galaxy
• A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• A weak lensing estimate from GEMS of the virial to stellar mass ratio in massive galaxies to z~0.8
• Properties of fossil groups in cosmological simulations and galaxy formation models
• The metallicity of galactic winds
• The Galaxy Activity, Torus, and Outflow Survey (GATOS). (IV): Exploring Ionized Gas Outflows in Central Kiloparsec Regions of GATOS Seyferts
• Testing cold dark matter with the low mass Tully-Fisher relation
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Hierarchical models of high redshift galaxies with thermally pulsing asymptotic giant branch stars: comparison with observations
• Multi-phase outflows in high redshift quasar host galaxies
• Gemini NIFS survey of feeding and feedback in nearby Active Galaxies -- V. Molecular and Ionised Gas Kinematics
• COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at $0<z<5$ Revealed by X-ray and Radio Stacking
• On the evolution of gas clouds exposed to AGN radiation. I. Three-dimensional radiation hydrodynamic simulations
• The Wide Area VISTA Extra-galactic Survey (WAVES)
• The baryonic mass-velocity relation; clues to feedback processes during structure formation and the cosmic baryon inventory
• Constraining star formation rates in cool-core brightest cluster galaxies
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• The Faint End of the Luminosity Function and Low Surface Brightness Galaxies
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Mid-infrared spectroscopy of high-redshift obscured quasars
• How Does Radio AGN Feedback Feed Back?
• The Close AGN Reference Survey (CARS): Locating the [O III] wing component in luminous local Type 1 AGN
• Dusty Cloud Acceleration by Radiation Pressure in Rapidly Star-Forming Galaxies
• A compact, metal-rich, kpc-scale outflow in FBQS J0209-0438: Detailed diagnostics from HST/COS extreme UV observations
• The mass fraction of AGN and the Fundamental Plane of black hole activity from a large X-ray selected sample of LINERs
• The dual role of starburst and active galactic nuclei in driving extreme molecular outflows
• 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
• Simulating the effect of photoheating feedback during reionization
• Regulation of Star Formation by a Hot Circumgalactic Medium
• Deep spectroscopy of nearby galaxy clusters: I. Spectroscopic luminosity function of Abell 85
• Jets in radio galaxies and quasars: an observational perspective
• Clustering Properties of restframe UV selected galaxies II: Migration of Star Formation sites with cosmic time from GALEX and CFHTLS
• 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
• A sensitive submillimetre survey of Broad Absorption Line quasars
• A deep Chandra observation of Abell 4059: a new face to radio-mode AGN feedback?
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows
• The Origin of the Hubble Sequence in Lambda-CDM Cosmology
• Galaxy Pairs in the Local Group
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• How covariant is the galaxy luminosity function?
• Measurement of the B-band Galaxy Luminosity Function with Approximate Bayesian Computation
• On the Environments of Giant Radio Galaxies
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation I: Introducing the Physically Evolved Winds (PhEW) Model
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• Models of the Cosmological 21 cm Signal from the Epoch of Reionization Calibrated with Lyman-alpha and CMB Data
• Composition of Low Redshift Halo Gas
• The accuracy of the UV continuum as an indicator of the star formation rate in galaxies
• The dwarf galaxy population in Abell 2218
• Massive, red galaxies in a hierarchical universe I. Counts of Extremely Red Objects and basic properties
• On the algorithms of radiative cooling in semi-analytic models
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• WISDOM Project -- VII. Molecular gas measurement of the supermassive black hole mass in NGC 7052
• The Ultraviolet Galaxy Luminosity Function from GALEX data: Color Dependent Evolution at Low Redshift
• 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
• The Ages of High Mass X-ray Binaries in NGC 2403 and NGC 300
• The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function
• Unveiling hidden active nuclei in MaNGA star-forming galaxies with HeII$\lambda$4686 line emission
• The UV-Optical Color Dependence of Galaxy Clustering in the Local Universe
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• 0.5 Mpc-scale extended X-ray emission in 4C 23.56
• Galaxy Luminosities in 2PIGG groups
• The Nuclear Outflows and Feedback in the Seyfert 2 Galaxy Markarian 573
• Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
• A Stacked Analysis of Brightest Cluster Galaxies Observed with the Fermi Large Area Telescope
• On the stellar populations of massive galaxies
• Observational constraints on the physics behind the evolution of AGN since z ~ 1
• The hierarchical build-up of the Tully-Fisher relation
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• Galaxy Evolution and Cosmology with the Square Kilometre Array
• Vertically Extended Neutral Gas in the Massive Edge-on Spiral NGC 5746
• A Unique View of AGN-Driven Molecular Outflows: The Discovery of a Massive Galaxy Counterpart to a $z=2.4$ High-Metallicity Damped Lyman-$\alpha$ Absorber
• Cool outflows in MaNGA: a systematic study and comparison to the warm phase
• Regulation of thermal conductivity in hot galaxy clusters by MHD turbulence
• The Stripe 82 Massive Galaxy Project III: A Lack of Growth Among Massive Galaxies
• Comparing Simulations of AGN Feedback
• Evolution in the Disks and Bulges of Group Galaxies since z=0.4
• Spatial Clustering of High Redshift Lyman Break Galaxies
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• The Clustering Evolution of Dusty Star-Forming Galaxies
• The association between gas and galaxies II: The 2-point correlation function
• Galaxy Outflows Without Supernovae
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• Can galaxy outflows and re-accretion produce the downsizing in specific star formation rate of late-type galaxies?
• Optical, near-IR and sub-mm IFU Observations of the nearby dual AGN Mrk 463
• Satellite Survival in Highly Resolved Milky Way Class Halos
• Suzaku Observations of the Outskirts of the Galaxy Cluster Abell 3395 including a Filament toward Abell 3391
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Modeling the red sequence: Hierarchical growth yet slow luminosity evolution
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• Swift XRT Observations of the Possible Dark Galaxy VIRGOHI 21
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• A UV study of nearby luminous infrared galaxies: star formation histories and the role of AGN
• Energetic Impact of Jet Inflated Cocoons in Relaxed Galaxy Clusters
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Observable consequences of kinetic and thermal AGN feedback in elliptical galaxies and galaxy clusters
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• The WIRCam Deep Survey II: Mass Selected Clustering
• Evolution of the galaxy luminosity function in progenitors of fossil groups
• The Variation of the Galaxy Luminosity Function with Group Properties
• The Origin of the 24-micron Excess in Red Galaxies
• A Massive Cluster at z = 0.288 Caught in the Process of Formation: The Case of Abell 959
• A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
• Dynamical Effect of the Turbulence of IGM on the Baryon Fraction Distribution
• Two phase galaxy formation: The Gas Content of Normal Galaxies
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• Violent quenching: molecular gas blown to 1000 km/s during a major merger
• The Interaction of 3C401 with the Surrounding Intracluster Medium
• The V-band luminosity function of galaxies in A2151
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• A WISE View of a Nearby Supercluster A2199
• From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5
• Kinematic signatures of AGN feedback in moderately powerful radio galaxies at z~2 observed with SINFONI
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Evolution of Galaxy Luminosity Function Using Photometric Redshifts
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Effects of Baryon Mass Loss on Profiles of Large Galactic Dark Matter Haloes
• Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
• Nearby Galaxies in the 2micron All Sky Survey I. K-band Luminosity Functions
• A simple model for the evolution of super-massive black holes and the quasar population
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• The Group Evolution Multiwavelength Study (GEMS): The near-infrared luminosity function of nearby galaxy groups
• Precessing winds from the nucleus of the prototype Red Geyser?
• Feedback by supermassive black holes in galaxy evolution: impacts of accretion and outflows on the star formation rate
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• Probing the hot X-ray gas in the narrow-line region of Mrk 3
• Resequencing the Hubble sequence and the quadratic (black hole mass)-(spheroid stellar mass) relation for elliptical galaxies
• Cold versus Warm Dark Matter simulations of a galaxy group
• Understanding Galaxy Outflows as the Product of Unstable Turbulent Support
• Correlations between bright submillimetre sources and low-redshift galaxies
• Assessing the Predictive Power of Galaxy Formation Models: A Comparison of Predicted and Observed Rest-Frame Optical Luminosity Functions at 2.0<z<3.3
• The influence of Red Spiral Galaxies on the Shape of the Local K-Band Luminosity Function
• Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
• SMBH accretion properties of radio-selected AGN out to z~4
• Systematic Survey for [OII], [OIII], and H$\alpha$ Blobs at $z=0.1-1.5$: The Implication for Evolution of Galactic-Scale Outflow
• Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• A Redshift Survey of the Nearby Galaxy Cluster Abell 2199: Comparison of the Spatial and Kinematic Distributions of Galaxies with the Intracluster Medium
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Investigating the properties of AGN feedback in hot atmospheres triggered by cooling-induced gravitational collapse
• Modelling the dusty universe I: Introducing the artificial neural network and first applications to luminosity and colour distributions
• One-Two Quench: A Double Minor Merger Scenario
• Invoking the virial theorem to understand the impact of (dry) mergers on the $M_{\mathrm{bh}}$-$\sigma$ relation
• Delayed Photoionization Feedback in a Super Star Cluster in SBS0335-052E
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Black holes, cuspy atmospheres, and galaxy formation
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• Extended Warm Gas in the ULIRG Mrk273: Galactic Outflows and Tidal Debris
• A Big Red Dot: Scattered light, host galaxy signatures and multi-phase gas flows in a luminous, heavily reddened quasar at cosmic noon
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• How feedback shapes galaxies: an analytic model
• Cosmological growth and feedback from supermassive black holes
• Searching for molecular outflows in Hyper-Luminous Infrared Galaxies
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• Bimodal morphologies of massive galaxies at the core of a protocluster at z=3.09 and the strong size growth of a brightest cluster galaxy
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• Massive spheroids can form in single minor mergers
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• The bright end of the galaxy luminosity function at $z\simeq 7$ from the VISTA VIDEO survey
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• Evolution of the Black Hole - Bulge Relationship in QSOs
• Observations of the High Redshift Universe
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• The environment of radio galaxies: A signature of AGN feedback at high redshifts
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Splitting the lentils: Clues to galaxy/black hole coevolution from the discovery of offset relations for non-dusty versus dusty (wet-merger-built) lenticular galaxies in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ diagram
• The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmology
• Host galaxies of luminous quasars: population synthesis of optical off-axis spectra
• Consequences of dark matter self-annihilation for galaxy formation
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• No evidence for feedback: Unexceptional Low-ionization winds in Host galaxies of Low Luminosity Active Galactic Nuclei at Redshift z ~1
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• Galaxy evolution across the optical emission-line diagnostic diagrams?
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Quenching star formation with low-luminosity AGN winds
• The scale dependence of mass assembly in galaxies
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• The galaxy luminosity function around groups
• Identification of a Fundamental Transition in a Turbulently-Supported Interstellar Medium
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• The interaction of the active nucleus with the host galaxy interstellar medium
• The Circumgalactic Medium in Massive Halos
• Deviations from the Infrared-Radio Correlation in Massive, Ultra-compact Starburst Galaxies
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Faint Dwarfs in Nearby Groups
• Leaving the dark ages with AMIGA
• The Infrared Luminosity Function of AKARI 90$\mu$m Galaxies in the Local Universe
• Gravity and the Nonlinear Growth of Structure in the Carnegie-Spitzer-IMACS Redshift Survey
• Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
• Deep UV Luminosity Functions at the Infall Region of the Coma Cluster
• Fe K lines in the nuclear region of M82
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• Dusty Cloud Acceleration with Multiband Radiation
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• The Ursa Major Association of Galaxies. VI: A relative dearth of gas-rich dwarf galaxies
• Simulated vs. observed UV emission at high redshift: a hint for a clumpy ISM?
• Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
• NIBLES - an HI census of stellar mass selected SDSS galaxies: II. Arecibo follow-up HI observations
• The Hot Interstellar Medium
• Chemical evolution of elliptical galaxies I: supernovae and AGN feedback
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• Spatially extended absorption around the z=2.63 radio galaxy MRC 2025-218: outflow or infall?
• Probing the interstellar medium of NGC1569 with Herschel
• A Giant Green Pea Identified in the Spectroscopy of Spatially Extended [OIII] Sources
• Radio Galaxy 3C 230 Observed with Gemini Laser-Adaptive-Optics Integral-Field Spectroscopy
• Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
• Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions
• The Degeneracy of Galaxy Formation Models
• Galaxy luminosity function and its cosmological evolution: Testing a new feedback model depending on galaxy-scale dust opacity
• Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
• Understanding Galaxy Formation and Evolution
• Stellar populations of galaxies in the ALHAMBRA survey up to $z\sim 1$. III. The stellar content of the quiescent galaxy population during the last $8$ Gyr
• Galaxy formation from a timescale perspective
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Causal Discovery in Astrophysics: Unraveling Supermassive Black Hole and Galaxy Coevolution
• Red riding on hood: Exploring how galaxy colour depends on environment
• The Circular Velocity Function of Group Galaxies
• The Performance of Photometric Reverberation Mapping at High Redshift and the Reliability of Damped Random Walk Models
• JWST Discovery of a Very Fast Biconical Outflow of Warm Molecular Gas in the Nearby Ultra-Luminous Infrared Galaxy F08572+3915 NW
• On the exclusion of intra-cluster plasma from AGN-blown bubbles
• Feedback Factory: Multiple faint radio-jets detected in a cluster at z=2
• Radio Properties of Cavities in the ICM: Imprints of AGN Activity
• Intermediate Mass Black Holes: A brief review
• Problems with the Current Cosmological Paradigm
• Bivariate luminosity-HI mass distribution function of galaxies based on the NIBLES survey
• The Formation and Evolution of Massive Galaxies
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• FLORAH: A generative model for halo assembly histories
• Model-independent Reconstruction of UV Luminosity Function and Reionization Epoch
• Revisiting the Galactic Winds in M82 II: Development of Multiphase Outflows in Simulations
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• The interaction between feedback from active galactic nuclei and supernovae
• Fred Hoyle: Contributions to the Theory of Galaxy Formation
• The MeerKAT Fornax Survey VI. The collapse of the galaxy HI Mass Function in Fornax
• Why and when is internally-driven AGN feedback energetically favoured?
• An ACA 1mm survey of HzRGs in the ELAIS-S1: survey description and first results
• The $K_s$-band luminosity function of the rich cluster VC04 in the Vela supercluster
• Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034
• Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
• A neutrino model fit to the CMB power spectrum
• How Does Feedback Affect Milky Way Satellite Formation?
• The impact of AGN on their host galaxies
• Resolved Neutral Outflow from a Lensed Dusty Star Forming Galaxy at z=2.09
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Intracluster globular clusters as tracers of the mass assembly of the Hydra I galaxy cluster
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• The influence of radio-galaxy activity on X-ray absorption lines from the intracluster medium
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• Ionized Gas Outflows and Shock-Heated Emission in the Highly Inclined Active Galaxy CGCG 012-070
• Mutual feedback between star formation and nuclear activity
• The most massive galaxies with large depleted cores: structural parameter relations and black hole masses
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• Feedback and the Initial Mass function
• 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
• AGN Heating of Cooling Flow Clusters: Problems with 3D Hydrodynamic Models
• The NIBLES bivariate luminosity--HI mass distribution function revised using Arecibo follow-up observations
• Gravity at Work: How the Build-Up of Environments Shape Galaxy Properties
• What best constrains galaxy evolution in the local Universe?