Hierarchical Galaxy Formation

Abstract

We describe the GALFORM semi-analytic model for calculating the formation and evolution of galaxies in hierarchical models. It improves upon, and extends, the Cole et al 1994 model. The model employs a new Monte-Carlo algorithm to follow the merging evolution of dark matter halos with arbitrary mass resolution. It incorporates realistic descriptions of the density profiles of dark matter halos and their gas content; follows the chemical evolution of gas and stars, and the associated production of dust; and includes a detailed calculation of the sizes of disks and spheroids. Wherever possible, our prescriptions for modelling individual physical processes are based on results of numerical simulations. We apply our methods to the LCDM cosmology (Omega_0=0.3, Lambda_0=0.7), and find good agreement with a wide range of properties of the local galaxy population: the B-band and K-band luminosity functions, the distribution of colours for the population as a whole, the ratio of ellipticals to spirals, the distribution of disk sizes, and the current cold gas content of disks. (Abridged)

Accepted for publication in MNRAS

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• The Dawes Review 1: Kinematic studies of star-forming galaxies across cosmic time
• Evolution in the Halo Masses of Isolated Galaxies between z~1 and z~0: From DEEP2 to SDSS
• A Comparison of Independent Star Formation Diagnostics for a UV-Selected Sample of Nearby Galaxies
• Towards Cosmological Concordance on Galactic Scales
• FIRE-3: Updated Stellar Evolution Models, Yields, & Microphysics and Fitting Functions for Applications in Galaxy Simulations
• SHARDS: an optical spectro-photometric survey of distant galaxies
• The Origin and Properties of Intracluster Stars in a Rich Cluster
• The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
• On the Origin of Stars in Bulges and Elliptical Galaxies
• The effect of non--gravitational gas heating in groups and clusters of galaxies
• Cosmological structure formation in a homogeneous dark energy background
• The evolution of the galaxy distribution
• The role of mergers in driving morphological transformation over cosmic time
• Ultraluminous Infrared Galaxies
• Galactic outflow rates in the EAGLE simulations
• Spatial and Dynamical Properties of Voids in a LCDM Universe
• The formation and evolution of low-surface-brightness galaxies
• Cooling and heating the ICM in hydrodynamical simulations
• On the Evolutionary History of Stars and their Fossil Mass and Light
• Deep ACS Imaging of the Halo of NGC 5128: Reaching the Horizontal Branch
• The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
• Dissipationless Mergers of Elliptical Galaxies and the Evolution of the Fundamental Plane
• A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. I Method description
• Semi-Analytic Galaxies - I. Synthesis of environmental and star-forming regulation mechanisms
• Downsizing by Shutdown in Red Galaxies
• Evolution of the Near-Infrared Tully-Fisher Relation: Constraints on the Relationship Between the Stellar and Total Masses of Disk Galaxies since z=1
• Including star formation and supernova feedback within cosmological simulations of galaxy formation
• Confronting theoretical models with the observed evolution of the galaxy population out to z=4
• Dark-ages reionization and galaxy formation simulation - III. Modelling galaxy formation and the epoch of reionization
• The Evolution of Early-type Red Galaxies with the GEMS Survey: Luminosity-size and Stellar Mass-size Relations Since z=1
• On the SFR-M${}_{\ast }$ main sequence archetypal star-formation history and analytical models
• Feedback from Active Galactic Nuclei in Galaxy Groups
• The Formation of a Disk Galaxy within a Growing Dark Halo
• Modern yields per stellar generation: the effect of the IMF
• The flip-side of galaxy formation: A combined model of Galaxy Formation and Cluster Heating
• Modeling Angular-Momentum History in Dark-Matter Halos
• Cluster Galaxies Die Hard
• Merger Rates of Dark-Matter Haloes
• Stellar Ages and Metallicities of Central and Satellite Galaxies: Implications for Galaxy Formation and Evolution
• The Parameter Space of Galaxy Formation
• The Stellar Masses and Star Formation Histories of Galaxies at z ~ 6: Constraints from Spitzer Observations in the Great Observatories Origins Deep Survey
• The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
• The metal enrichment of elliptical galaxies in hierarchical galaxy formation models
• X-rays across the galaxy population - III. The incidence of AGN as a function of star formation rate
• Milky Way vs Andromeda: a tale of two disks
• The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope
• The evolution of early-type galaxies at z~1 from the K20 survey
• Galaxy And Mass Assembly (GAMA): The large scale structure of galaxies and comparison to mock universes
• Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman-$\alpha$ forest, and Milky Way satellites
• Orbital structure of merger remnants: Trends with gas fraction in 1:1 mergers
• Dwarf galaxy formation with H2-regulated star formation
• Predicting the Cosmological Constant from the Causal Entropic Principle
• The Las Campanas/AAT Rich Cluster Survey II: The Environmental Dependance of Galaxy Colours in Clusters at z~0.1
• Adding Environmental Gas Physics to the Semi-Analytic Method for Galaxy Formation: Gravitational Heating
• Two-dimensional kinematics of SLACS lenses: II. Combined lensing and dynamics analysis of early-type galaxies at z = 0.08 - 0.33
• The Dependence of the Mass Assembly History of Cold Dark Matter Halos on Environment
• Galaxy formation using halo merger histories taken from N-body simulations
• The History of Cosmological Star Formation: Three Independent Approaches and a Critical Test Using the Extragalactic Background Light
• Constructing Merger Trees that Mimic N-Body Simulations
• The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?
• Galaxy morphology in the LambdaCDM cosmology
• Heating of Galactic Disks by Infalling Satellites
• Radiative Stellar Feedback in Galaxy Formation: Methods and Physics
• Old and young stellar populations in DustPedia galaxies and their role in dust heating
• The hierarchical assembly of galaxies and black holes in the first billion years: predictions for the era of gravitational wave astronomy
• The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• The metal enrichment of the intracluster medium in hierarchical galaxy formation models
• Observing the Formation of the Hubble Sequence in the Great Observatories Origins Deep Survey
• Global Probes of the Impact of Baryons on Dark Matter Halos
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• Approximate Bayesian Computation for Astronomical Model Analysis: A Case Study in Galaxy Demographics and Morphological Transformation at High Redshift
• Lyman-break galaxies at z~5 -I. First significant stellar mass assembly in galaxies that are not simply z~3 LBGs at higher redshift
• Gas Infall and Stochastic Star Formation in Galaxies in the Local Universe
• A Bayesian approach to the semi-analytic model of galaxy formation: methodology
• The stellar accretion origin of stellar population gradients in massive galaxies at large radii
• The Subhalo Mass Function and Ultralight Bosonic Dark Matter
• Incidence of WISE-Selected Obscured AGNs in Major Mergers and Interactions from the SDSS
• Constraining the primordial initial mass function with stellar archaeology
• Barred galaxies in the EAGLE cosmological hydrodynamical simulation
• Satellites of Simulated Galaxies: survival, merging, and their relation to the dark and stellar halos
• The Properties of Sub-mm Galaxies in Hierarchical Models
• Galactic porosity and a star formation threshold for the escape of ionising radiation from galaxies
• Evolution of the Radio Loud Galaxy Population
• Unravelling obese black holes in the first galaxies
• Formation of the Black Holes in the Highest Redshift Quasars
• Spatial correlation between submillimetre and Lyman-alpha galaxies in the SSA 22 protocluster
• The radial distribution of galaxies in groups and clusters
• The K20 survey. IV. The redshift distribution of Ks<20 galaxies: a test of galaxy formation models
• Formation versus destruction: the evolution of the star cluster population in galaxy mergers
• The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses
• 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
• The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies
• On the puzzling plateau in the specific star formation rate at z=2-7
• keV Neutrino Model Building
• The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450um-selected galaxies and their contribution to the cosmic infrared background
• Effects of dust grains on early galaxy evolution
• Clusters of galaxies in the local universe
• Metal Enrichment of the ICM: a 3-D Picture of Chemical and Dynamical Properties
• HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
• On the Origin of the Galaxy Star-Formation-Rate Sequence: Evolution and Scatter
• Impact of star formation history on the measurement of star formation rates
• A 2dF spectroscopic study of globular clusters in NGC 5128: Probing the formation history of the nearest giant Elliptical
• Direct Evidence for Termination of Obscured Star Formation by Radiatively Driven Outflows in Reddened QSOs
• Galaxy And Mass Assembly (GAMA): Galaxy environments and star formation rate variations
• The Impact of Galaxy Formation on the X-ray Evolution of Clusters
• Galaxy And Mass Assembly (GAMA): Refining the Local Galaxy Merger Rate using Morphological Information
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution
• How is Star Formation Quenched in Massive Galaxies?
• Overconsumption, outflows and the quenching of satellite galaxies
• The Sloan Lens ACS Survey. XII. Extending Strong Lensing to Lower Masses
• The B-Band Luminosity Function of Red and Blue Galaxies up to z=3.5
• Bulges versus disks: the evolution of angular momentum in cosmological simulations of galaxy formation
• 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
• Probing cluster formation under extreme conditions: massive star clusters in blue compact galaxies
• Galactic chemical evolution in hierarchical formation models - I. Early-type galaxies in the local Universe
• The optical-to-radio spectral energy distributions of low-metallicity blue compact dwarf galaxies
• Simulating the Formation of the Local Galaxy Population
• Galaxy Voids in Cold Dark Matter Universes
• The UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the Lyman-Break Galaxy Population at z~5
• An Excursion-Set Model for the Structure of GMCs and the ISM
• Where are the stars?
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• Building disc structure and galaxy properties through angular momentum: The DARK SAGE semi-analytic model
• The Phase-Space Parameters of Brightest Halo Galaxies
• The Ages, Metallicities and Alpha Element Enhancements of Globular Clusters in the Elliptical NGC 5128: A Homogeneous Spectroscopic Study with Gemini/GMOS
• On The Assembly History of Dark Matter Haloes
• On the Interstellar Medium and Star Formation Demographics of Galaxies in the Local Universe
• Shocked Superwinds from the z~2 Clumpy Star-forming Galaxy, ZC406690
• The Effects of Photoionization on Galaxy Formation -- III: Environmental Dependence in the Luminosity Function
• Kinematic Constraints on Evolutionary Scenarios for Blue Compact Dwarf Galaxies : I. Neutral Gas Dynamics
• The low-end of the black hole mass function at cosmic dawn
• The Impact of Cooling and Feedback on Disc Galaxies
• Gas cooling in simulations of the formation of the galaxy population
• The Diversity of Extremely Red Objects
• Life and times of dwarf spheroidal galaxies
• Galaxy bulges and their black holes: a requirement for the quenching of star formation
• Weak Lensing by Galaxies in Groups and Clusters: I.--Theoretical Expectations
• Bimodal Color Distribution in Hierarchical Galaxy Formation
• Revealing the galaxy-halo connection in IllustrisTNG
• The clustering of H-alpha emitters at z=2.23 from HiZELS
• Molecular Gas in the Lensed Lyman Break Galaxy cB58
• Generating Merger Trees for Dark Matter Haloes: A Comparison of Methods
• Simulations of galaxy formation in a cosmological volume
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• Galaxy And Mass Assembly (GAMA): the Stellar Mass Budget by Galaxy Type
• Physical Properties of Spectroscopically-Confirmed Galaxies at z >= 6. II. Morphology of the Rest-Frame UV Continuum and Lyman-alpha Emission
• A review of elliptical and disc galaxy structure, and modern scaling laws
• A New Prescription for Protogalactic Feedback and Outflows: Where Have All the Baryons Gone?
• APOGEE DR16: a multi-zone chemical evolution model for the Galactic disc based on MCMC methods
• Galaxy Formation Spanning Cosmic History
• Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
• Pre-heating the ICM in high resolution simulations: the effect on the gas entropy
• Satellite Systems around Galaxies in Hydrodynamic Simulations
• The Environmental Dependence of the Infrared Luminosity and Stellar Mass Functions
• Chemical abundances in an UV-selected sample of galaxies
• Hot gas halos around disk galaxies: Confronting cosmological simulations with observations
• Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
• From the far-ultraviolet to the far-infrared -- galaxy emission at $0\le z\le 10$ in the Shark semi-analytic model
• VLT Spectroscopy of Globular Cluster Systems, II. Spectroscopic Ages, Metallicities, and [alpha/Fe] Ratios of Globular Clusters in Early-Type Galaxies
• Cosmological Origin of the Stellar Velocity Dispersions in Massive Early-Type Galaxies
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• Active Galactic Nuclei In Cosmological Simulations - I. Formation of black holes and spheroids through mergers
• 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
• The properties of Ly-alpha emitting galaxies in hierarchical galaxy formation models
• The UV colours of high-redshift early-type galaxies: evidence for recent star formation and stellar mass assembly over the last 8 billion years
• The low-mass end of the baryonic Tully-Fisher relation
• Substructure of fuzzy dark matter haloes
• The mass assembly of galaxy groups and the evolution of the magnitude gap
• VEGAS: A VST Early-type GAlaxy Survey. II. Photometric study of giant ellipticals and their stellar halos
• Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
• The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
• What is the (Dark) Matter with Dwarf Galaxies?
• The satellites of the Milky Way - Insights from semi-analytic modelling in a LambdaCDM cosmology
• Reconstructing the cosmic density field with the distribution of dark matter halos
• The most luminous quasars do not live in the most massive dark matter haloes at any redshift
• The Millennium Galaxy Catalogue: Dynamically Close Galaxy Pairs and the Global Merger Rate
• The 0.1<z<1.65 evolution of the bright end of the [OII] luminosity function
• When and where did GW150914 form?
• On the Distribution of Haloes, Galaxies and Mass
• Coming of Age in the Dark Sector: How Dark Matter Haloes grow their Gravitational Potential Wells
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• Which galaxies dominate the neutral gas content of the Universe?
• The Ages and Abundances of a Sample of Globular Clusters in M49 (NGC 4472)
• Triggered Star Formation in Galaxy Pairs at z=0.08-0.38
• Preheating by Previrialization and its Impact on Galaxy Formation
• Satellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matter
• Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
• Hiding in plain sight: An abundance of compact massive spheroids in the local Universe
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• Constraints on QSO models from a relation between the QSO luminosity function and the local black hole mass function
• Incorporating interactive 3-dimensional graphics in astronomy research papers
• Relations Between the Sizes of Galaxies and their Dark Matter Halos at Redshifts $0<z<3$
• Observational Properties of Ultra-Diffuse Galaxies in the Field: Field-UDGs are Predominantly Blue and Starforming
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- I. Survey motivation, design and data processing
• Binary Aggregations in Hierarchical Galaxy Formation: The Evolution of the Galaxy Luminosity Function
• The Evolution of the Dark Halo Spin Parameters lambda and lambda' in a LCDM Universe: The Role of Minor and Major Mergers
• Modelling Shock Heating in Cluster Mergers: I. Moving Beyond the Spherical Accretion Model
• Voids in the 2dFGRS and LCDM simulations: spatial and dynamical properties
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• A dynamical model of supernova feedback: gas outflows from the interstellar medium
• Intrinsic galaxy shapes and alignments I: Measuring and modelling COSMOS intrinsic galaxy ellipticities
• The Masses, Ancestors and Descendents of Extremely Red Objects: Constraints from Spatial Clustering
• Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe
• Southern GEMS Groups I: Dynamical Properties
• How common is the Milky Way - satellite system alignment?
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• Dwarf galaxy populations in present-day galaxy clusters: I. Abundances and red fractions
• Dependence of Galaxy Structure on Rest-frame Wavelength and Galaxy Type
• Bulge Formation via Mergers in Cosmological Simulations
• AzTEC/ASTE 1.1-mm Survey of the AKARI Deep Field South: source catalogue and number counts
• The origin of the atomic and molecular gas contents of early-type galaxies. I. A new test of galaxy formation physics
• Baryon Dynamics, Dark Matter Substructure, and Galaxies
• Clustering properties of BzK-selected galaxies in GOODS-N: environmental quenching and triggering of star formation at z ~ 2
• The Role of Dust in the Early Universe I : Protogalaxy Evolution
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• Avoiding progenitor bias: The structural and mass evolution of Brightest Group and Cluster Galaxies in Hierarchical models since z~1
• Self-Consistent Theory of Halo Mergers
• The host dark matter halos of [OII] emitters at 0.5< z< 1.5
• The Kinematics of the Globular Cluster System of NGC 5128 with a New, Large Sample of Radial Velocity Measurements
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• Metal-Poor Globular Clusters and Galaxy Formation
• The tidal evolution of dark matter substructure -- II. The impact of artificial disruption on subhalo mass functions and radial profiles
• Star Formation History and Stellar Metallicity Distribution in a Cold Dark Matter Universe
• Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
• How robust are predictions of galaxy clustering?
• Entropy Injection as a Global Feedback Mechanism
• Early Hierarchical Formation of Massive Galaxies Triggered By Interactions
• The Varied Fates of z~2 Star-forming Galaxies
• The colour of galaxies in distant groups
• The Epoch of Reionization
• The evolution of Lyman-break galaxies in CDM
• Do Mergers Spin up Dark Matter Halos?
• GEMS: which galaxies dominate the z~0.7 ultraviolet luminosity density?
• A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
• Properties of the galaxy population in hydrodynamical simulations of clusters
• The statistical properties of LCDM halo formation
• Galaxy Formation in WDM Cosmology
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Exploring the evolutionary paths of the most massive galaxies since z~2
• Galaxy Groups at 0.3 <= z <= 0.55. II. Evolution to z ~ 0
• The Anisotropic Distribution of Satellite Galaxies
• Dark-ages reionization & galaxy formation simulation IV: UV luminosity functions of high-redshift galaxies
• The evolution of the galaxy Red Sequence in simulated clusters and groups
• Quasar Evolution Driven by Galaxy Encounters in Hierarchical Structures
• Hot Gas Halos in Early-Type Field Galaxies
• The Stellar Populations of Lyman Break Galaxies at z~5
• Predicting the locations of possible long-lived low-mass first stars: Importance of satellite dwarf galaxies
• Mass assembly of galaxies: Smooth accretion versus mergers
• The origin of the atomic and molecular gas contents of early-type galaxies. II. Misaligned gas accretion
• Quenching star formation in cluster galaxies
• Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
• A Hubble Space Telescope Lensing Survey of X-ray Luminous Galaxy Clusters: II. A Search for Gravitationally Lensed EROs
• An Empirical Model for the Star Formation History in Dark Matter Halos
• Simulations of Dust in Interacting Galaxies I: Dust Attenuation
• Stellar Populations of Bulges in 14 Cluster Disc Galaxies
• Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN
• The angular momentum of cold dark matter haloes with and without baryons
• An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
• A Revised LCDM Mass Model For The Andromeda Galaxy
• Bayesian inference of galaxy formation from the K-band luminosity function of galaxies: tensions between theory and observation
• 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
• The GALEX-SDSS NUV & FUV Flux Density and Local Star-Formation Rate
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• Effects of dynamical evolution on the distribution of substructures
• Galaxy clustering from COMBO-17: The halo occupation distribution at <z>=0.6
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• Structure Formation Inside Triaxial Dark Matter Halos: Galactic Disks, Bulges and Bars
• Massive galaxies & EROs at z=1-3 in cosmological hydrodynamic simulations: near-IR properties
• Lyman Alpha Emitter Evolution in the Reionization Epoch
• Shapes of clusters and groups of galaxies: Comparison of model predictions with observations
• Herschel-ATLAS: The link between accretion luminosity and star formation in quasar host galaxies
• The Effect of Gravitational Recoil on Black Holes Forming in a Hierarchical Universe
• Momentum transfer across shear flows in Smoothed Particle Hydrodynamic simulations of galaxy formation
• Reproducing the assembly of massive galaxies within the hierarchical cosmogony
• The abundance of dark galaxies
• Toward precise constraints on growth of massive black holes
• Luminous Quasars Do Not Live in the Most Overdense Regions of Galaxies at z~4
• The Millennium Galaxy Catalogue: Exploring the Color-Concentration Bimodality via Bulge-Disc Decomposition
• Clues for the origin of the fundamental metallicity relations. I: The hierarchical building up of the structure
• Galaxy Groups in the 2dFGRS: the number density of groups
• Predictions for deep galaxy surveys with JWST from $\Lambda$CDM
• Constraining the Minimum Mass of High-Redshift Galaxies and Their Contribution to the Ionization State of the IGM
• Massive and Red Objects predicted by a semianalytical model of galaxy formation
• Eridanus - A Supergroup in the Local Universe?
• GALICS -- VI. Modelling Hierarchical Galaxy Formation in Clusters
• Galaxy And Mass Assembly (GAMA): the Stellar Mass Budget of Galaxy Spheroids and Disks
• The evolution of the mass function split by morphology up to redshift 1 in the FORS Deep and the GOODS-S Fields
• Insights on the Formation, Evolution, and Activity of Massive Galaxies From Ultra-Compact and Disky Galaxies at z=2-3
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Predictions for Herschel from LambdaCDM: unveiling the cosmic star formation history
• Modeling Tidal Streams in evolving dark matter halos
• {Chemo-spectrophotometric evolution of spiral galaxies: IV. Star formation efficiency and effective ages of spirals
• Halo Shapes From Weak Lensing: The Impact of Galaxy--Halo Misalignment
• The elliptical colour-magnitude relation as a discriminant between the monolithic and merger paradigms: the importance of progenitor bias
• Elliptical galaxies from mergers of discs
• The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: II. The red bands
• Signatures of reionization on Lyman alpha emitters
• Hierarchical Formation of Galaxies with Dynamical Response to Supernova-Induced Gas removal
• The K20 survey. II. The Different Spatial Clustering of z~1 Old and Dusty Star-Forming EROs
• Angular momentum distribution of hot gas and implications for disk galaxy formation
• The 2dF Galaxy Redshift Survey: The clustering of galaxy groups
• Can galactic outflows explain the properties of Ly-alpha emitters?
• Systematic search for tidal features around nearby galaxies: I. Enhanced SDSS imaging of the Local Volume
• Testing the predictions of the cold dark matter model for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
• Peculiar early-type galaxies in the SDSS Stripe82
• A semi-analytic model comparison - gas cooling and galaxy mergers
• Is There a Missing Galaxy Problem at High Redshift?
• The origin of low-surface-brightness galaxies in the dwarf regime
• Evaluating and Improving Semi-analytic modelling of Dust in Galaxies based on Radiative Transfer Calculations
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• Galactic Bulges from HST NICMOS Observations: Global Scaling Relations
• Resolving The Generation of Starburst Winds in Galaxy Mergers
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• A Lightcone Catalogue from the Millennium-XXL Simulation
• From blue star-forming to red passive: galaxies in transition in different environments
• The evolution of the galaxy luminosity function in the rest frame blue band up to z=3.5
• Deep near-infrared imaging of RDCS J1252.9-2927 at z=1.237: The colour-magnitude diagram
• A Bridge from Optical to Infrared Galaxies: Explaining Local Properties, Predicting Galaxy Counts and the Cosmic Background Radiation
• Exploring the Selection of Galaxy Clusters and Groups: An Optical Survey for X-ray Dark Clusters
• The imprint of cosmic reionisation on the luminosity function of galaxies
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE
• Stellar populations of Globular Clusters in the Elliptical galaxy NGC1407
• Multiwavelength Observations of the Low Metallicity Blue Compact Dwarf Galaxy SBS 0335-052
• Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
• Numerical Galaxy Catalog -I. A Semi-analytic Model of Galaxy Formation with N-body simulations
• 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
• An Empirical Study of the Relationship between Lyα and UV selected Galaxies: Do Theorists and Observers `Select' the Same Objects?
• Extended X-ray emission around 4C 41.17 at z=3.8
• The Millennium Run Observatory: First Light
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• A new population of recently quenched elliptical galaxies in the SDSS
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Spatially Resolved Gas-Phase Metallicity Distributions in Barred and Unbarred Spirals
• Star Formation in a Stellar Mass Selected Sample of Galaxies to z=3 from the GOODS NICMOS Survey (GNS)
• Modelling SCUBA sources in a Lambda-CDM cosmology: hot starbursts or cold extended galactic dust?
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• The evolution of the star forming sequence in hierarchical galaxy formation models
• The clustering of Ly-alpha emitters in a LambdaCDM Universe
• The abundance of Lyman-(α) emitters in hierarchical models
• The evolution of SMBH spin and AGN luminosities for $z<6$ within a semi-analytic model of galaxy formation
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• A Slippery Slope: Systematic Uncertainties in the Line Width Baryonic Tully-Fisher Relation
• IRS Spectroscopy and Multi-wavelength Study of Luminous Star-forming Galaxies at z~1.9
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• A Unifying Framework for Self-consistent Gravitational Lensing and Stellar Dynamics Analyses of Early-Type Galaxies
• Physical regimes for feedback in galaxy formation
• Introducing a new, robust galaxy finder algorithm for simulations
• The role of submillimetre galaxies in hierarchical galaxy formation
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• An analytical model for the accretion of dark matter subhalos
• Central stellar populations of early-type galaxies in low-density environments
• Environmental Effects on Evolution of Cluster Galaxies in a LCDM Universe
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• Disentangling the Cosmic Web Towards FRB 190608
• The Link Between SCUBA and Spitzer: Cold Galaxies at z<1
• How to Grow a Healthy Merger Tree
• Limits on the luminosity function of Ly-alpha emitters at z = 7.7
• The rest-frame UV luminosity function at $z\simeq 4$: a significant contribution of AGN to the bright-end of the galaxy population
• Retaining Black Holes with Very Large Recoil Velocities
• The ESO-Sculptor Survey: Luminosity functions of galaxies per spectral type at redshifts 0.1-0.5
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• A multiscale approach to environment and its influence on the colour distribution of galaxies
• A simple model for AGN feedback in nearby early-type galaxies
• The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last $\approx$10 Gyr
• Constraints on black hole fuelling modes from the clustering of X-ray AGN
• Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies
• Measuring the growth rate of structure with Type IA Supernovae from LSST
• The fundamental gas depletion and stellar-mass buildup times of star forming galaxies
• Feedback and Brightest Cluster Galaxy Formation: ACS Observations of the Radio Galaxy TN J1338--1942 at z=4.1
• Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
• Streams in the Aquarius stellar haloes
• Constraints on the star formation histories of galaxies from z~1 to z~0
• High redshift formation and evolution of central massive objects I: model description
• Spectroscopy of luminous z>7 galaxy candidates and sources of contamination in z>7 galaxy searches
• Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probe
• The Arecibo Galaxy Environment Survey: II. A HI view of the Abell cluster 1367 and its outskirts
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
• Evolution of blue E/S0 galaxies from z~1: merger remnants or disk rebuilding galaxies?
• Dwarf galaxy populations in present-day galaxy clusters - II. The history of early-type and late-type dwarfs
• Black hole spin and radio loudness in a LCDM universe
• Accurate mass and velocity functions of dark matter halos
• Characterization of Low Surface Brightness structures in annotated deep images
• High redshift quasars and the supermassive black hole mass budget: constraints on quasar formation models
• Dim galaxies and outer halos of galaxies missed by 2MASS ? The near-infrared luminosity function and density
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• The dependence of tidal stripping efficiency on the satellite and host galaxy morphology
• Enriching the hot circumgalactic medium
• The signature of dark energy on the local Hubble flow
• Atomic and Molecular Gas in Colliding Galaxy Systems: I. The Data
• Neutral Gas Outflows and Inflows in Infrared-Faint Seyfert Galaxies
• Galaxy Clustering Topology in the Sloan Digital Sky Survey Main Galaxy Sample: a Test for Galaxy Formation Models
• Resolution-independent modeling of environmental effects in semi-analytic models of galaxy formation that include ram-pressure stripping of both hot and cold gas
• SINFONI-HiZELS: The dynamics, merger rates & metallicity gradients of `typical' star-forming galaxies at $z$ = 0.8-2.2
• Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the "green valley"
• Quasars and galaxy formation
• Two-Phase Galaxy Formation
• A New Statistical Model for Population III Supernova Rates: Discriminating Between $\Lambda$CDM and WDM Cosmologies
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• The structural and photometric properties of early-type galaxies in hierarchical models
• Chemical enrichment of Damped Lyman Alpha systems as a direct constraint on Population III star formation
• Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies
• The Formation and Evolution of Virgo Cluster Galaxies - II. Stellar Populations
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• Mass Function of Low Mass Dark Halos
• The Properties of Spiral Galaxies: Confronting Hierarchical Galaxy Formation Models with Observations
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• Galaxy structure with strong gravitational lensing: decomposing the internal mass distribution of massive elliptical galaxies
• The environments of high redshift radio galaxies and quasars: probes of protoclusters
• Observational tests of the evolution of spheroidal galaxies
• The VLT LBG Redshift Survey I: Clustering and Dynamics of ~1000 Galaxies at z~3
• GASP. XII. The variety of physical processes occurring in a single galaxy group in formation
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• Newborn spheroids at high redshift: when and how did the dominant, old stars in today's massive galaxies form?
• An analytical model for galaxy metallicity: What do metallicity relations tell us about star formation and outflow?
• Strong-lensing Measurement of the Mass-density Profile out to 3 Effective Radii for $z\sim 0.5$ Early-type Galaxies
• Radio AGN in nearby dwarf galaxies: the important role of AGN in dwarf-galaxy evolution
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution
• The UV colours and dust attenuation of Lyman-break galaxies
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Sizes and ages of SDSS ellipticals: Comparison with hierarchical galaxy formation models
• Structural properties of discs and bulges of early-type galaxies
• A modified star formation law as a solution to open problems in galaxy evolution
• Understanding the nature of the optically faint radio sources and their connection to the submillimeter population
• Exploring the nature of the Lyman-$\alpha$ emitter CR7
• Deep mid-infrared observations of Lyman-break galaxies
• Realistic Event Rates for Detection of Supermassive Black Hole Coalescence by LISA
• Feedback from quasars in star-forming galaxies and the triggering of massive galactic winds
• Gravitational Lens Time Delays in CDM
• Galaxies Under the Cosmic Microscope: Resolved Spectroscopy and New Constraints on the z=1 Tully-Fisher relation
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• Star Formation at the Twilight of the Dark Ages: Which Stars Reionized the Universe?
• Realistic galaxy image simulation via score-based generative models
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Dark-matter decays and Milky Way satellite galaxies
• Galaxy properties and the cosmic web in simulations
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• HST Photometry for the Halo Stars in the Leo Elliptical NGC 3377
• Photometric characterization of a well defined sample of isolated galaxies in the context of the AMIGA project
• The ugrizYJHK luminosity distributions and densities from the combined MGC, SDSS and UKIDSS LAS datasets
• On the evolutionary status of early-type galaxies in clusters at z~0.2 - I. The Fundamental Plane
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• The Halos and Environments of Nearby Galaxies (HERON) I: Imaging, Sample Characteristics, and Envelope Diameters
• Creating mock catalogues of stellar haloes from cosmological simulations
• Relations Between Environments of Quasars and Galaxy Formation
• Infrared Luminosity Function of the Coma Cluster
• The Production of Cold Gas Within Galaxy Outflows
• Direct evidence for Ly$\alpha$ depletion in the protocluster core
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• New Horizon: On the origin of the stellar disk and spheroid of field galaxies at $z=0.7$
• Galaxy Number Counts in the Subaru Deep Field: Multi-band Analysis in a Hierarchical Galaxy Formation Model
• The Tully-Fisher relation of distant field galaxies
• Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Halo Occupation Number, Mass-to-Light Ratios and Omega_m
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• The visibility of Lyman Alpha Emitters: constraining reionization, ionizing photons and dust
• Chemical abundances in the polar disk of NGC4650A: implications for cold accretion scenario
• Predicting Hα emission line galaxy counts for future galaxy redshift surveys
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Stellar mass functions of galaxies, disks and spheroids at z~0.1
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• The triggering of local AGN and their role in regulating star formation
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• Star Formation Quenching Timescale of Central Galaxies in a Hierarchical Universe
• The evolution of the stellar mass versus halo mass relationship
• Stellar population gradients in early-type cluster galaxies with VIMOS IFU
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• Stellar populations in the bulges of isolated galaxies
• Metals in the z~3 intergalactic medium: results from an ultra-high signal-to-noise ratio UVES quasar spectrum
• The Structure of Galaxies: I. Surface Photometry Techniques
• X-Ray Evolution of Active Galactic Nuclei and Hierarchical Galaxy Formation
• Isolated compact elliptical galaxies: Stellar systems that ran away
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• NIR Luminosity Function of Galaxies in Close Major-Merger Pairs and Mass Dependence of Merger Rate
• Properties of Submillimeter Galaxies in a Semi-analytic Model using the "Count Matching" Approach: Application to the ECDF-S
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Predicting the Properties of the Remnants of Dissipative Galaxy Mergers
• Accretion, Growth of Supermassive Black Holes, and Feedback in Galaxy Mergers
• Spatially Resolved Stellar Populations of $0.3<z<6.0$ Galaxies in WHL0137-08 and MACS0647+70 Clusters as Revealed by JWST: How do Galaxies Grow and Quench Over Cosmic Time?
• Exploring the formation of spheroidal galaxies out to z~1.5 in GOODS
• The effect of Warm Dark Matter on galaxy properties: constraints from the stellar mass function and the Tully-Fisher relation
• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• Star formation in the CDFS: observations confront simulations
• The Fornax Cluster VLT Spectroscopic Survey II - Planetary Nebulae kinematics within 200 kpc of the cluster core
• Modelling Galaxy Merger Timescales and Tidal Destruction
• Iron in galaxy groups and clusters: Confronting galaxy evolution models with a newly homogenised dataset
• An accurate low-redshift measurement of the cosmic neutral hydrogen density
• The first Super Massive Black Holes: indications from models for future observations
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Radio source feedback in galaxy evolution
• Evolution of galactic magnetic fields
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Substructure Lensing: Effects of Galaxies, Globular Clusters & Satellite Streams
• The cosmic assembly of stellar haloes in massive Early-Type Galaxies
• The effect of differential accretion on the Gravitational Wave Background and the present day MBH Binary population
• Critical analysis of the luminosity functions per galaxy type measured from redshift surveys
• Subhaloes gone Notts: Spin across subhaloes and finders
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• The Munich Near-Infrared Cluster Survey (MUNICS) - Number density evolution of massive field galaxies to z ~ 1.2 as derived from the K-band selected survey
• An enhanced fraction of starbursting galaxies among high Eddington ratio AGNs
• The galaxies that reionized the Universe
• A duality in the origin of bulges and spheroidal galaxies
• Evolution of LMC/M33-mass dwarf galaxies in the EAGLE simulation
• Predictions for the intrinsic UV continuum properties of star forming galaxies and the implications for inferring dust extinction
• Catastrophic Cooling in Superwinds: Line Emission and Non-equilibrium Ionization
• First Results from the KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics of Lensed Galaxies at Cosmic Noon
• Massive Dark Matter Halos around Bright Isolated Galaxies in the 2dFGRS
• The Ks-band Luminosity and Stellar Mass Functions of Galaxies in z~1 Clusters
• Do model emission line galaxies live in filaments at z~1?
• Luminous Red Galaxies in hierarchical cosmologies
• Optical Line Emission from z$\sim$6.8 Sources with Deep Constraints on Ly$\alpha$ Visibility
• A journey from the outskirts to the cores of groups I: Color- and mass-segregation in 20K-zCOSMOS groups
• Status of Cold Dark Matter Cosmology
• The dependence of the pairwise velocity dispersion on galaxy properties
• Constraints on galaxy formation models from the galaxy stellar mass function and its evolution
• The DEEP Groth Strip Galaxy Redshift Survey. VIII. The Evolution of Luminous Field Bulges at Redshift z ~ 1
• Climbing Halo Merger Trees with TreeFrog
• The Stellar Haloes of Massive Elliptical Galaxies III: Kinematics at Large Radius
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• Discovery of a very extended X-ray halo around a quiescent spiral galaxy - the "missing link" of galaxy formation
• Evaluating and Improving Semi-analytic modeling of Dust in Galaxies based on Radiative Transfer Calculations II: Dust Emission in the Infrared
• Damped Lyman alpha systems and galaxy formation models - II. High ions and Lyman limit systems
• Modeling the gravitational potential of a cosmological dark matter halo with stellar streams
• Simulating Supersonic Turbulence in Galaxy Outflows
• The spatial distribution of cold gas in hierarchical galaxy formation models
• The cosmic evolution of the galaxy luminosity density
• The history of the dark and luminous side of Milky Way-like progenitors
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• The environmental dependence of clustering in hierarchical models
• Detection of satellite remnants in the Galactic Halo with Gaia - I. The effect of the Galactic background, observational errors and sampling
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• Tracing galaxy populations through cosmic time: A critical test of methods for connecting the same galaxies between different redshifts at $z<3$
• The formation of galaxy disks in a hierarchical universe
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Unveiling sub-parsec supermassive black hole binary candidates in active galactic nuclei
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• The Evolution of the Luminosity Function in Deep Fields: A Comparison with CDM Models
• Black Holes in Pseudobulges: demography and models
• CFHT Legacy Ultraviolet Extension (CLUE): Witnessing Galaxy Transformations up to 7 Mpc from Rich Cluster Cores
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• The galaxy luminosity - size relation and selection biases in the Hubble Ultra Deep Field
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• Globular Cluster Systems of Early-type Galaxies in Low-density Environments
• A new method to assign galaxy cluster membership using photometric redshifts
• On the Continuous Formation of Field Spheroidal Galaxies in Hierarchical Models of Structure Formation
• Testing cold dark matter with the low mass Tully-Fisher relation
• Modelling the Milky Way through adiabatic compression of cold dark matter halo
• Hierarchical models of high redshift galaxies with thermally pulsing asymptotic giant branch stars: comparison with observations
• Properties of fossil groups in cosmological simulations and galaxy formation models
• The Role of Ram Pressure Stripping in the Quenching of Cluster Star Formation
• Statistics of galaxy mergers: bridging the gap between theory and observation
• Numerical simulations of dwarf galaxy merger trees
• The Angular Momentum of Gas in Proto-Galaxies: II -- The Impact of Preheating
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• Lyman Break Galaxies and the Reionization of the Intergalactic Medium
• The pairwise velocity dispersion of galaxies: luminosity dependence and a new test of galaxy formation models
• Massive z ~ 1.3 evolved galaxies revealed
• A Hubble Space Telescope Lensing Survey of X-ray Luminous Galaxy Clusters: III. A Multiply-imaged Extremely Red Galaxy at z=1.6
• The Pristine survey XIII: Uncovering the very metal-poor tail of the thin disc
• Low-mass suppression of the satellite luminosity function due to the supersonic baryon--cold-dark-matter relative velocity
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Limits on the evolution of galaxies from the statistics of gravitational lenses
• The Cold Dark Matter crisis on galactic and subgalactic scales
• Kinematic and chemical evolution of early-type galaxies
• Recent star formation in local, morphologically disturbed spheroidal galaxies on the optical red sequence
• Exploring the astrophysics of dark atoms
• GRASIL-3D: an Implemention of Dust Effects in the SEDs of Simulated Galaxies
• The origin of bulges and discs in the CALIFA survey: I. Morphological evolution
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• The baryonic mass-velocity relation; clues to feedback processes during structure formation and the cosmic baryon inventory
• ORCA: The Overdense Red-sequence Cluster Algorithm
• Spatial and luminosity distributions of galactic satellites
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• Reionisation in sterile neutrino cosmologies
• Optical/near-infrared colours of early-type galaxies and constraints on their star formation histories
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• The HI Velocity Function: a test of cosmology or baryon physics?
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• Lyman break galaxy close and interacting pairs at z ~ 3
• GOYA Survey: U and B Number Counts in the Groth-Westphal Strip
• A Multiband Study of the Galaxy Populations of the First Four Sunyaev--Zeldovich Effect selected Galaxy Clusters
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• Models of Disk Evolution: Confrontation with Observations
• Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Simultaneous Modelling of the Stellar Halo and Globular Cluster System of NGC 5128
• Regulation of Star Formation by a Hot Circumgalactic Medium
• The origin of dispersion in DLA metallicities
• Charting Unexplored Dwarf Galaxy Territory With RR Lyrae
• The angular momentum of disc galaxies: implications for gas accretion, outflows, and dynamical friction
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• A search for low surface brightness dwarf galaxies in different environments
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Patchy He II reionization and the physical state of the IGM
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• Convergence of Galaxy Properties with Merger Tree Temporal Resolution
• Galaxy number counts in the Hubble Deep Field as a strong constraint on a hierarchical galaxy formation model
• Turbulence in the Intergalactic Medium
• Galaxies Under the Cosmic Microscope: A GMOS Study of the Lensed Disk-Galaxy #289 in A2218
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• Merger relics of cluster galaxies
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Further constraining galaxy evolution models through the Size Function of SDSS Early-type galaxies
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• On the Formation of Galaxy Halos: Comparing NGC 5128 and the Local Group Members
• The physical drivers of the atomic hydrogen-halo mass relation
• Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations
• The Origin of the Hubble Sequence in Lambda-CDM Cosmology
• Ages and Metallicities of Early-Type Void Galaxies from Line Strength Measurements
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• I. Apples to apples $A^2$: realistic galaxy simulated catalogs and photometric redshift predictions for next-generation surveys
• Testing homogeneity in the Sloan Digital Sky Survey Data Release Twelve with Shannon entropy
• The evolution of the galaxy content of dark matter haloes
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
• Interacting Galaxies in the A901/902 Supercluster with STAGES
• How does gas cool in DM halos?
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• The importance of preventive feedback: inference from observations of the stellar masses and metallicities of Milky Way dwarf galaxies
• How covariant is the galaxy luminosity function?
• The influence of halo assembly on galaxies and galaxy groups
• The Most Massive Black Holes in the Universe: Effects of Mergers in Massive Galaxy Clusters
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• The fraction of early-type galaxies in low redshift groups and clusters of galaxies
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• An Isochrone Database and a Rapid Model for Stellar Population Synthesis
• Spheroidal post-mergers in the local Universe
• An HST Morphological Survey of Faint EROs
• Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• The evolution of barred galaxies in the EAGLE simulations
• Reconstructing the galaxy density field with photometric redshifts: I. Methodology and validation on stellar mass functions
• Galactic magnetic fields and hierarchical galaxy formation
• The accuracy of the UV continuum as an indicator of the star formation rate in galaxies
• Local stellar formation history from the 40 pc white dwarf sample
• Massive, red galaxies in a hierarchical universe I. Counts of Extremely Red Objects and basic properties
• Identification of tidal features in deep optical galaxy images with Convolutional Neural Networks
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• Euclid preparation XXVI. The Euclid Morphology Challenge. Towards structural parameters for billions of galaxies
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• Dynamical self-friction: how mass loss slows you down
• On the algorithms of radiative cooling in semi-analytic models
• Keck spectroscopy of z=1-3 ULIRGs from the Spitzer SWIRE survey
• Active Galactic Nucleus and Extended Starbursts in a Mid-stage Merger VV114
• Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift Performance
• On Physical Scales of Dark Matter Halos
• Gas cooling in semi-analytic models and SPH simulations: are results consistent?
• Narrow-band surveys for very high redshift Lyman-alpha emitters
• Local and global environmental effects on galaxies and active galactic nuclei
• A backwards approach to the formation of disk galaxies I. Stellar and gas content
• Observational evidence for bar formation in disk galaxies via cluster-cluster interaction
• The MillenniumTNG Project: The large-scale clustering of galaxies
• An investigation of star formation and dust attenuation in major mergers using ultraviolet and infrared data
• Early Preheating and Galaxy Formation
• How accurate is it to update the cosmology of your halo catalogues?
• Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
• Luminosity Functions beyond the spectroscopic limit. I. Method and near-infrared LFs in the HDF-N and HDF-S
• A Catalog of Luminous Infrared Galaxies in the IRAS Survey and the Second Data Release of the SDSS
• Conditional Mass Functions and Merger Rates of Dark Matter Halos in the Ellipsoidal Collapse Model
• The spatial distribution of neutral hydrogen as traced by low HI mass galaxies
• Galactic conformity measured in semi-analytic models
• The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
• A tight relation between the age distributions of stellar clusters and the properties of the interstellar medium in the host galaxy
• Constraining galactic structures of mirror dark matter
• Evolution of the Galaxy Luminosity Function at z < 0.3
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• The Canada-UK Deep Submillimetre Survey VIII: Source Identifications in the 3-hour field
• The Bar Pattern Speed of NGC 1433 Estimated Via Sticky-Particle Simulations
• The properties of quasar hosts at the peak of the quasar activity
• Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Soliton Merger Rates and Enhanced Axion Dark Matter Decay
• Exploring the evolution of spiral galaxies
• A Candidate Kiloparsec-scale Quasar Pair at $z=5.66$
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• A Linear Perturbation Theory of Inhomogeneous Reionization
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• The GALAH Survey: Chemically tagging the Fimbulthul stream to the globular cluster $\omega$ Centauri
• A new search for distant radio galaxies in the southern hemisphere - I. Sample definition and radio properties
• The galaxy population in cold and warm dark matter cosmologies
• Rise and fall of post-starburst galaxies in Magneticum Pathfinder
• The HST/ACS Coma Cluster Survey - VII. Structure and Assembly of Massive Galaxies in the Center of the Coma Cluster
• The hierarchical build-up of the Tully-Fisher relation
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Testing the Modified Press-Schechter Model against N-Body Simulations
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• EMPRESS. VI. Outflows Investigated in Low-Mass Galaxies with $M_{\ast }=10^4-10^7{M}_{\odot }$: Weak Feedback in Low-Mass Galaxies?
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• The PAU Survey: Spectral features and galaxy clustering using simulated narrow band photometry
• Characterising the evolving $K$-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys
• Evolution of high-redshift quasar hosts and promotion of massive black hole seed formation
• The orbital PDF: the dynamical state of Milky Way sized haloes and the intrinsic uncertainty in the determination of their masses
• An ESO/VLT survey of NIR (Z<=25) selected galaxies at redshifts 4.5<z<6: constraining the cosmic star formation rate near the reionization epoch
• Polarization of the Cosmic Microwave Background from Non-Uniform Reionization
• Are Dry Mergers Dry, Moist, or Wet?
• 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
• Galaxy Evolution and Cosmology with the Square Kilometre Array
• Galaxy star formation in different environments
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• 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
• Connected structure in the 2dFGRS
• Modeling the Ages and Metallicities of Early-Type Galaxies in Fundamental Plane Space
• Numerical simulations of buoyancy instabilities in galaxy cluster plasmas with cosmic rays and anisotropic thermal conduction
• Modeling the QSO luminosity and spatial clustering at low redshifts
• The galaxy-halo size relation of low-mass galaxies in FIRE
• The Clustering Evolution of Dusty Star-Forming Galaxies
• Galaxy Outflows Without Supernovae
• Colour Evolution of Disk Galaxy Models from z=4 to z=0
• Measuring the Distribution of Galaxies Between Halos
• The Missing Satellite Problem Outside of the Local Group: I -- Pilot Observation
• On the Origin of the Dichotomy of Early-Type Galaxies: The Role of Dry Mergers and AGN Feedback
• Constructing high-fidelity halo merger trees in AbacusSummit
• Studying Cosmic Dawn using redshifted HI 21-cm signal: A brief review
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• Sizes, Half-Mass Densities, and Mass Functions of Star Clusters in the Merger Remnant NGC 1316: Clues to the Fate of Second-Generation Globular Clusters
• Galaxy clusters and groups in the ALHAMBRA Survey
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• Distinguishing `disks' from `mergers': tracing the kinematic asymmetries in local (U)LIRGs using `kinemetry'-based criteria
• The CFHT Legacy Survey: The Morphology-Density Relation of Galaxies out to Z~1
• What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• The Luminosity Function and Surface Brightness Distribution of HI Selected Galaxies
• Demographics of Isolated Galaxies Along the Hubble Sequence
• The Variation of the Galaxy Luminosity Function with Group Properties
• Lyα emitters in a cosmological volume I: the impact of radiative transfer
• A Two-Phase Chemical Enrichment Model for the Milky Way Globular Cluster System
• A Massive Spiral Galaxy in the Zone of Avoidance
• The Structure of Reionization in Hierarchical Galaxy Formation Models
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• The WIRCam Deep Survey II: Mass Selected Clustering
• The Resolved Stellar Populations of a Dwarf Spheroidal Galaxy in the Virgo Cluster
• Determining the Nature of the Extended HI Structure Around LITTLE THINGS Dwarf Galaxy NGC 1569
• The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
• The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey
• The HI mass function of star-forming galaxies at $\mathbf{z}\sim 0.35$
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
• The Expected Properties of Dark Lenses
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• The GALAH Survey: Accreted stars also inhabit the Spite Plateau
• The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
• An Accurate Cluster Selection Function for the J-PAS Narrow-Band wide-field survey
• The neutral hydrogen distribution in large-scale haloes from 21-cm intensity maps
• The Fundamental Plane of Spiral Galaxies: Theoretical Expectations
• Sersic Properties of Disc Galaxy Mergers
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• GOODS-ALMA 2.0: Last gigayear star formation histories of the so-called starbursts within the main sequence
• First Systematic Search for Oxygen-Line Blobs at High Redshift: Uncovering AGN Feedback and Star-Formation Quenching
• Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories
• Kinematics of the OVI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
• Substructure in the Andromeda Galaxy Globular Cluster System
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• Identifying the progenitor set of present-day early-type galaxies: a view from the standard model
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• What to expect from dynamical modelling of galactic haloes
• The galaxy correlation function as a constraint on galaxy formation physics
• The Upper Asymptotic Giant Branch of the Elliptical Galaxy Maffei 1, and Comparisons with M32 and NGC 5128
• Constraints on the Baryonic Compression and Implications for the Fraction of Dark Halo Lenses
• Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
• Luminosity bias: from haloes to galaxies
• The assembly bias of emission line galaxies
• On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
• The Cosmological History of Accretion onto Dark Halos and Supermassive Black Holes
• Cosmic evolution of metal densities: the enrichment of the Inter-Galactic Medium
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• Present-day scaling relations of submm galaxies: origin of spheroidal sytems
• Crash-testing the CAULDRON code for joint lensing and dynamics analysis of early-type galaxies
• II. Apples to apples $A^2$: cluster selection functions for next-generation surveys
• The Galactic Environment of the NeVIII Absorber toward HE0226-4110
• The role of Pop III stars and early black holes in the 21cm signal from Cosmic Dawn
• Lyman-alpha emitters in a cosmological volume II: the impact of the intergalactic medium
• The descendents of Lyman Break Galaxies in galaxy clusters: spatial distribution and orbital properties
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• The z=0 Galaxy Luminosity Function: I. Techniques for Identification of Dwarf Galaxies at ~10 Mpc
• Nearby Galaxies in the 2micron All Sky Survey I. K-band Luminosity Functions
• Star formation trends in high-redshift galaxy surveys: the elephant or the tail?
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IX. Identification of Two Red Quasars at z > 5.6
• The HI mass function as a probe of photoionisation feedback on low mass galaxy formation
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• The cosmic spectral energy distribution in the EAGLE simulation
• Astraeus VIII: A new framework for Lyman-$\alpha$ emitters applied to different reionisation scenarios
• Theoretical reevaluations of the black hole mass - bulge mass relation - I. Effect of the seed black hole mass
• Metal enrichment in a semi-analytical model, fundamental scaling relations, and the case of Milky Way galaxies
• Probing Outflows in z= 1~2 Galaxies through FeII/FeII* Multiplets
• Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
• The evolution of disc galaxies with and without classical bulges since z~1
• The star formation histories of early-type galaxies: insights from the rest-frame ultra-violet
• A Hybrid Fast Multipole Method for Cosmological N-body Simulations
• The intrinsic SFRF and sSFRF of galaxies: comparing SDSS observation with IllustrisTNG simulation
• 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
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• Galaxy source counts at 7.7 $\mu$m, 10 $\mu$m and 15 $\mu$m with the James Webb Space Telescope
• Morphology of Mock SDSS Catalogues
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar halo
• Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
• Modelling the dusty universe I: Introducing the artificial neural network and first applications to luminosity and colour distributions
• The Capodimonte Deep Field I - Presentation of the survey and first follow-up studies
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Discovery of a Supercluster at $z\sim$0.91 and Testing the $\Lambda$CDM Cosmological Model
• Galaxy And Mass Assembly (GAMA): Comparing Visually and Spectroscopically Identified Galaxy Merger Samples
• The ages of stellar populations in a warm dark matter universe
• Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• Probability Friends-of-Friends (PFOF) Group Finder: Performance Study and Observational Data Applications on Photometric Surveys
• Exploring binary black hole mergers and host galaxies with Shark and COMPAS
• POX 186: A Dwarf Galaxy in the Process of Formation?
• Chemical Enrichment in Damped Lyman Alpha Systems From Hierarchical Galaxy Formation Models
• Massive Early-Type Galaxies in the HSC-SSP: Flux Fraction of Tidal Features and Merger Rates
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• On the accretion of a new group of galaxies onto Virgo: II. The effect of pre-processing on the stellar population content of dEs
• Star formation activity of intermediate redshift cluster galaxies out to the infall regions
• Halo concentrations from extended Press-Schechter merger histories
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Cosmic Star Formation: Constraints on the Galaxy Formation Models
• The active and passive populations of Extremely Red Objects
• Physical constraints on the central mass and baryon content of satellite galaxies
• The Universal Specific Merger Rate of Dark Matter Halos
• A unique small-scale gravitational arc in Abell 1201
• Constraints on the velocity profiles of galaxies from strong lensing statistics and semi-analytical modelling of galaxy formation
• Effective Dark Matter Halo catalog in $f(R)$ gravity
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Influence of ~7 keV sterile neutrino dark matter on the process of reionization
• Rosella: A mock catalogue from the P-Millennium simulation
• BVRI Surface Photometry of Isolated Spiral Galaxies
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• A random-walk model for dark matter halo spins
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright sub-millimetre galaxies
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Chandra observations of NGC4342, an optically faint, X-ray gas-rich early-type galaxy
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters
• Cosmic star formation rate: a theoretical approach
• Abundance ratios in dwarf elliptical galaxies
• Bulge formation through disc instability -- I
• Merger history trees of dark matter haloes in moving barrier models
• Tracing early structure formation with massive starburst galaxies and their implications for reionization
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• The Phoenix Deep Survey: The star-formation rates and the stellar masses of EROs
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Star Formation Enhancement in Barred Disk Galaxies in Interacting Galaxy Clusters
• The mass-dependent star formation histories of disk galaxies: infall model versus observations
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Galaxy Peculiar Velocities and Infall onto Groups
• A new method for testing isotropy with Shannon entropy
• Bulges of disk galaxies at intermediate redshifts.II. Nuclear, disk and global colours in the Groth Strip
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Particle tagging and its implications for stellar population dynamics
• Massive spheroids can form in single minor mergers
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• Merger history of central galaxies in Semi-Analytic Models of galaxy formation
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Gaia-IGRINS synergy: Orbits of Newly Identified Milky Way Star Clusters
• Modelling the formation of today's massive ellipticals
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Constraining the Black Hole Mass Spectrum with LISA Observations II: Direct comparison of detailed models
• Analytic and numerical realisations of a disk galaxy
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• Galaxy Clusters in the Line of Sight to Background Quasars: II. Environmental effects on the sizes of baryonic halo sizes
• The cosmic atomic hydrogen mass density as a function of mass and galaxy hierarchy from spectral stacking
• Observations of the High Redshift Universe
• Keck Spectroscopy of Globular Clusters in the Virgo Cluster Dwarf Elliptical VCC 1386
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• The nature and descendants of Lyman-break galaxies in the LambdaCDM cosmology
• Clustering of galaxies at 3.6 microns in the Spitzer Wide-area Infrared Extragalactic legacy survey
• Fast and Accurate Fourier Series Solutions to Gravitational Lensing by A General Family of Two Power-Law Mass Distributions
• The environment of radio galaxies: A signature of AGN feedback at high redshifts
• The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates
• Revisiting the formation History of the minor-axis dust lane galaxy NGC1947
• The photoionization effect of the ultraviolet background on the colour-magnitude relation of elliptical galaxies
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• Star-Forming, Rotating Spheroidal Galaxies in the GAMA and SAMI Surveys
• The star-forming progenitors of massive red galaxies
• Merging of Low-Mass Systems and the Origin of the Fundamental Plane
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• Chemical abundances of the PRGs UGC7576 and UGC9796. I. Testing the formation scenario
• A Comparison of Galaxy Group Luminosity Functions from Semi-Analytic Models
• Broad-line region configuration of the supermassive binary black hole candidate PG1302-102 in the relativistic Doppler boosting scenario
• The SZ Effect as a Probe of Non-Gravitational Entropy in Groups and Clusters of Galaxies
• AGNs at the cosmic dawn: predictions for future surveys from a $\Lambda$CDM cosmological model
• A physical model for the origin of the diffuse cosmic infrared background
• Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
• Galaxy morphology and evolution from SWAN Adaptive Optics imaging
• Growing the First Galaxies' Merger Trees
• Type Ia supernovae in a hierarchical galaxy formation model: the Milky Way
• Variation in the escape fraction of ionising photons from galaxies and the redshifted 21-cm power spectrum during reionization
• Dynamical response to supernova-induced gas removal in two-component spherical galaxies
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Bulgeless Galaxies at Intermediate Redshift: Sample Selection, Colour Properties, and the Existence of Powerful AGN
• Colour pairs for constraining the age and metallicity of stellar populations
• Can We Detect the Color-Density Relation with Photometric Redshifts?
• On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
• A new gas cooling model for semi-analytical galaxy formation models
• A survey for dwarf galaxy remnants around fourteen globular clusters in the outer halo
• The central region of the enigmatic Malin 1
• The origin of star-gas misalignments in simulated galaxies
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• MOSFIRE and LDSS3 Spectroscopy for an [OII] Blob at z=1.18: Gas Outflow and Energy Source
• The scale dependence of mass assembly in galaxies
• The galaxy luminosity function around groups
• The Size Evolution of Elliptical Galaxies
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Surface photometry and structure of high redshift disk galaxies in the HDF-S NICMOS field
• Simulating the formation of cosmic structure
• Ionised gas kinematics in bipolar H II regions
• Effective dark matter power spectra in $f(R)$ gravity
• Numerical simulations of bar formation in the Local Group
• G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
• The puzzling origin of the 6Li plateau
• The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• An empirical model to form and evolve galaxies in dark matter halos
• Modelling emission lines in star forming galaxies
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Statistics of Neutral Regions During Hydrogen Re-Ionization
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Leaving the dark ages with AMIGA
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• Abundance matching for low mass galaxies in the CDM and FDM models
• Modelling the dynamical friction timescale of sinking satellite
• Bimodal AGNs in Bimodal Galaxies
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• Rapid Simulations of Halo and Subhalo Clustering
• Matrix Formalism of Excursion Set Theory: A new approach to statistics of dark matter halo counting
• Gravitational-wave event rates as a new probe for dark matter microphysics
• Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• The detection and X-ray evolution of galaxy groups at high redshift
• Groups of two galaxies in SDSS: implications of colours on star formation quenching time-scales
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Thermal and Chemical Evolution of Collapsing Filaments
• Number Density Evolution of Ks -band Selected High Redshift Galaxy Populations in the AKARI North Ecliptic Pole Field
• Recovering dark-matter clustering from galaxies with Gaussianization
• The effect of pressure-anisotropy-driven kinetic instabilities on magnetic field amplification in galaxy clusters
• Physical Properties, Star Formation, and Active Galactic Nucleus Activity in Balmer Break Galaxies at 0 < z < 1
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• Interpreting the galaxy group CG J1720-67.8 through evolutionary synthesis models
• SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
• Stellar populations of the bulges of four spiral galaxies
• Photometry and dynamics of the minor mergers AM\,1228-260 and AM\,2058-381
• On the population of primordial star clusters in the presence of UV background radiation
• An optimised tiling pattern for multi-object spectroscopic surveys: application to the 4MOST survey
• The SAMI Galaxy Survey: The contribution of different kinematic classes to the stellar mass function of nearby galaxies
• Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulations
• The Impact of Dust in Host Galaxies on Quasar Luminosity Functions
• Photometry and Dynamics of the Minor Merger AM1219-430 with Gemini GMOS-S
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Determining the systemic redshift of Lyman-alpha emitters with neural networks and improving the measured large-scale clustering
• Efficient simulation of discrete galaxy populations and associated radiation fields during the first billion years
• Interchanging Interactive 3-d Graphics for Astronomy
• Angular Momentum Evolution in Dark Matter Halos
• Self-Consistent Theory of Halo Mergers - II: CDM Power Spectra
• Binary Stellar Population Synthesis Study of Elliptical Galaxies
• The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
• Bulges of disk galaxies at intermediate redshifts. I. Samples with and without bulges in the Groth Strip Survey
• Selection and Mid-infrared Spectroscopy of Ultraluminous Star-Forming Galaxies at z~2
• An X-ray View of Star Formation in the Central 3 kpc of NGC 2403
• New photometric investigation of the double ringed galaxy ESO474-G26. Unveiling the formation scenario
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• The Evolutionary Status of Clusters of Galaxies at z ~ 1
• Limits on dust emission from z~5 LBGs and their local environments
• Bursting and quenching in satellite galaxies
• Luminous Matter Distribution, Bulk Flows and Baryon Contents in Cosmological Models with a Local Void
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• Low Surface Brightness structures from annotated deep CFHT images: effects of the host galaxy's properties and environment
• Mission Design for the TAIJI misson and Structure Formation in Early Universe
• Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows III: Observability and Connection to Halo Globular Clusters
• Ultra-fine dark matter structure in the Solar neighbourhood
• Radio properties of Green Pea galaxies
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• Measuring Detailed Chemical Abundances From Co-added Medium Resolution Spectra I. Tests using Milky Way dwarf spheroidal galaxies and globular clusters
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• The impact of the cosmological constant on past and future star formation
• Merging Tree Algorithm of Growing Voids in Self Similar and CDM Models
• Multi-wavelength consensus of large-scale linear bias
• A Random Walk Model for Dark Matter Halo Concentrations
• A Model of the Cosmic Infrared Background Produced by Distant Galaxies
• Host Galaxy Demographics Of Individually Detectable Supermassive Black-hole Binaries with Pulsar Timing Arrays
• The significant effects of stellar mass estimation on galaxy pair fractions
• Low Redshift QSO Lyman alpha Absorption Line Systems Associated with Galaxies
• Clues on Arp 142: The Spiral-Elliptical merger
• Interacting dark energy collapse with matter components separation
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Dissipative phenomena in extended-bodies interactions I: Methods Dwarf galaxies of the Local Group and their synthetic CMDs
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• Red bulgeless galaxies in SDSS DR7. Are there any AGN hosts?
• How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
• A deep learning approach to halo merger tree construction
• Cosmic happenstance: 24-$\mu$m selected, multi-component Herschel sources are line-of-sight projections
• Extending PLE models into the mid-IR, far-IR & sub-mm
• Testing a prediction of the merger origin of early-type galaxies: a correlation between stellar populations and asymmetry
• HI mapping of the Leo Triplet: Morphologies and kinematics of tails and bridges
• An expanded merger-tree description of cluster evolution
• The Degeneracy of Galaxy Formation Models
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• The effect of finite halo size on the clustering of neutral hydrogen
• Dynamics of Lyman Break Galaxies and Their Host Halos
• A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
• Are Lyα emitters segregated in protoclusters regions?
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• 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
• Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
• A hybrid multi resolution scheme to efficiently model the structure of reionization on the largest scales
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• The quantity of dark matter in early-type galaxies and its relation to the environment
• Reliability of merger tree realizations of dark halos in the Monte-Carlo modeling of galaxy formation
• Cross-Roads in Studies of Galaxy Evolution
• Disentangling the morpho-kinematic properties of a face-on merger at z~0.7
• SED-inferred properties and morphology of Lyman-break galaxies at $z\sim 1$ in the CDF-S
• Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
• The Galaxy Structure-Redshift Relationship
• The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Co-Interacting Dark Matter
• Interactions, Mergers and the Fundamental Mass Relations of Galaxies
• STRRINGS: STReams in Residual Images of Nearby GalaxieS
• Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• XXL-HSC: Host properties of X-ray detected AGNs in XXL clusters
• JWST Discovery of a Very Fast Biconical Outflow of Warm Molecular Gas in the Nearby Ultra-Luminous Infrared Galaxy F08572+3915 NW
• Low Metallicity Galaxies from the Dark Energy Survey
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• Reconstruction Analysis of the IRAS Point Source Catalog Redshift Survey
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• Sensitivity analysis of a galaxy formation model
• The Formation and Evolution of Massive Galaxies
• Bayesian analysis of spatially distorted cosmic signals from Poissonian data
• Solving the puzzle of subhalo spins
• Spatial clustering of USS sources and galaxies
• Rendezvous in CAVITY: Kinematics and gas properties of an isolated dwarf-dwarf merging pair in a cosmic void region
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Reconstructing the Milky Way chemical map with Galactic Chemical Evolution tool OMEGA+ from SDSS-MWM
• Simulations of the accreted stellar halos of low-mass field galaxies
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• Machine learning applications in astrophysics: Photometric redshift estimation
• Accurate halo mass functions from the simplest excursion set theory
• Formation of Compact Clusters from High Resolution Hybrid Cosmological Simulations
• Dynamical response to supernova-induced gas removal in spiral galaxies with dark matter halo
• Testing Theoretical Models for the Higher-Order Moments of Dark Halo Distribution
• The north-south asymmetry of the ALFALFA HI velocity width function
• On the accuracy of the high redshift cluster luminosity function
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Extracting Galaxy Merger Timescales II: A new fitting formula
• Massive Black Hole Mergers
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• Fast radiative transfer of dust reprocessing in semi-analytic models with artificial neural networks
• Metallicity and HI Column Density Properties of Damped Lyman-$\alpha$ Systems
• The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective
• Low-Mass Cluster Galaxies: A Cornerstone of Galaxy Evolution
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• The Origin of the Stellar Mass-Stellar Metallicity Relation in the Milky Way Satellites and beyond
• Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals
• Clustering of 2PIGG galaxy groups with 2dFGRS galaxies
• Star Formation and Chemical Evolution of DLAs with Semi-Analytical Model
• The formation and evolution of field massive galaxies
• Thermodynamic evolution of the cosmological baryonic gas : II. Galaxy formation
• The Dirt on Dry Mergers
• FLORAH: A generative model for halo assembly histories
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Supernova Feedback Keeps Galaxies Simple
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• VEGA: Voids idEntification using Genetic Algorithm
• The Baryonic and Dark Matter Properties of High Redshift Gravitationally Lensed Disk Galaxies
• Star Formation in a Cosmological Simulation of Reionization
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• From Gas to Stars over Cosmic Time
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Main-sequence Turnoff Stars as Probes of the Ancient Galactic Relic: Chemo-dynamical Analysis of a Pilot Sample
• The Nature of LoBAL QSOs: II. HST/WFC3 Observations Reveal Host Galaxies Dominated by Mergers
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• HELP project - a dreamed-of multiwavelength dataset for SED fitting: the influence of used models for the main physical properties of galaxies
• Fred Hoyle: Contributions to the Theory of Galaxy Formation
• Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods
• Extended Hernquist-Springel formalism for cosmic star formation
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• The self regulating star formation of gas rich dwarf galaxies in quiescent phase
• Interactions among intermediate redshift galaxies. The case of SDSSJ134420.86+663717.8
• GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• The progenitor galaxies of stellar haloes as "failed" Milky Ways
• The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers
• Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties
• A Halo Merger Tree Generation and Evaluation Framework
• Environmental Invariance of the Galaxy Size-Mass Relation
• Halo detection via large-scale Bayesian inference
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Disk galaxy evolution: from the Milky Way to high-redshift disks
• The NIBLES bivariate luminosity--HI mass distribution function revised using Arecibo follow-up observations
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Star formation activity in Balmer break galaxies at $z$ < 1.5
• Mutual feedback between star formation and nuclear activity
• Solving small-scale clustering problems in approximate lightcone mocks
• On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
• Modelling the outskirts of galaxies in a cosmological context
• Black Hole merger rates in the first billion years in light of JWST data
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• A multiwavelength study of near- and mid-infrared selected galaxies at high redshift: ERGs, AGN-identification and the contribution from dust
• Blanco DECam Bulge Survey (BDBS) IV: Metallicity Distributions and Bulge Structure from 2.6 Million Red Clump Stars
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• 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
• The dusty SF history of high-z galaxies, modelling tools and future prospects
• Observing the high redshift universe using the VIMOS-IFU
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• Observational tests of the galaxy formation process
• Hierarchal formation and growth of galaxies through dynamical friction
• From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
• The Nature of Hyperluminous Infrared Galaxies
• Ultra-fast model emulation with PRISM; analyzing the Meraxes galaxy formation model
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• What fraction of stars formed in infrared galaxies at high redshift?
• Clustering around radio galaxies at z~1.5
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies