Semi-Analytic Modelling of Galaxy Formation: The Local Universe

Abstract

Using semi-analytic models of galaxy formation, we investigate galaxy properties such as the Tully-Fisher relation, the B and K-band luminosity functions, cold gas contents, sizes, metallicities, and colours, and compare our results with observations of local galaxies. We investigate several different recipes for star formation and supernova feedback, including choices that are similar to the treatment in Kauffmann, White & Guiderdoni (1993) and Cole et al. (1994) as well as some new recipes. We obtain good agreement with all of the key local observations mentioned above. In particular, in our best models, we simultaneously produce good agreement with both the observed B and K-band luminosity functions and the I-band Tully-Fisher relation. Improved cooling and supernova feedback modelling, inclusion of dust extinction, and an improved Press-Schechter model all contribute to this success. We present results for several variants of the CDM family of cosmologies, and find that models with values of ${\Omega }_0\simeq 0.3$--0.5 give the best agreement with observations.

26 pages, LaTeX, MNRAS format, 23 inlined postscript figures. Accepted for publication in MNRAS. Revised version contains substantial changes including improved models. High resolution figures, original version, and summary of changes may be found at http://www.fiz.huji.ac.il/~rachels/papers/sp.html

References in corpus (15)

• Large scale bias and the peak background split
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Starburst-driven Mass Loss from Dwarf Galaxies: Efficiency and Metal Ejection
• Properties of the Intracluster Medium in an Ensemble of Nearby Galaxy Clusters
• Properties of Galactic Outflows: Measurements of the Feedback from Star Formation
• How to Plant a Merger Tree
• On Measuring Chemical Abundances in Distant Galaxies Using Global Emission Line Spectra
• Global Extinction in Spiral Galaxies
• The 2dF Galaxy Redshift Survey: Spectral Types and Luminosity Functions
• The cosmological origin of the Tully-Fisher relation
• Chemical Properties of Star-Forming Emission Line Galaxies at z=0.1 - 0.5
• CDM-Variant Cosmological Models - I: Simulations and Preliminary Comparisons
• The Assembly of Matter in Galaxy Clusters
• The Near-Infrared Number Counts and Luminosity Functions of Local Galaxies
• The Deuterium Abundance at z=0.701 towards QSO 1718+4807

Cited by in corpus (811)

• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Cosmic Star Formation History
• The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
• Populating a cluster of galaxies - I. Results at z=0
• The broken hierarchy of galaxy formation
• Profiles of dark haloes: evolution, scatter, and environment
• How Do Galaxies Get Their Gas?
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Halo Models of Large Scale Structure
• Hierarchical Galaxy Formation
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• Stellar mass-to-light ratios and the Tully-Fisher relation
• Mass function of dark matter halos
• The epochs of early-type galaxy formation as a function of environment
• Galactic Winds
• A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
• Metallicity Calibrations and the Mass-Metallicity Relation for Star-Forming Galaxies
• Physical Models of Galaxy Formation in a Cosmological Framework
• Nearly 5000 Distant Early-Type Galaxies in COMBO-17: a Red Sequence and its Evolution since z~1
• From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
• Constraints on the relationship between stellar mass and halo mass at low and high redshift
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation
• Virial shocks in galactic haloes?
• Tracing Galaxy Formation with Stellar Halos I: Methods
• Halo occupation numbers and galaxy bias
• Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
• Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
• Structure and Formation of Elliptical and Spheroidal Galaxies
• What Shapes the Luminosity Function of Galaxies?
• Environmental Effects on Late-Type Galaxies in Nearby Clusters
• The Two Phases of Galaxy Formation
• The Connection between Galaxies and their Dark Matter Halos
• Dusty Star-Forming Galaxies at High Redshift
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• The SAURON project -- IX. A kinematic classification for early-type galaxies
• Galaxy Star-Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey
• The Cosmic Infrared Background: Measurements and Implications
• Galaxies in a simulated $\Lambda$CDM Universe I: cold mode and hot cores
• The 2dF Galaxy Redshift Survey: The environmental dependence of galaxy star formation rates near clusters
• Theoretical Challenges in Galaxy Formation
• Extragalactic Background Light Inferred from AEGIS Galaxy SED-type Fractions
• Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
• The Nature of High-Redshift Galaxies
• How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
• Mapping Large-Scale Gaseous Outflows in Ultraluminous Galaxies with Keck II ESI Spectra: Variations in Outflow Velocity with Galactic Mass
• Constraining Galaxy Formation and Cosmology with the Conditional Luminosity Function of Galaxies
• Ubiquitous outflows in DEEP2 spectra of star-forming galaxies at z=1.4
• AGN wind scaling relations and the co-evolution of black holes and galaxies
• The COS-Halos Survey: Physical Conditions and Baryonic Mass in the Low-Redshift Circumgalactic Medium
• Stellar Feedback in Galaxies and the Origin of Galaxy-scale Winds
• A primer on hierarchical galaxy formation: the semi-analytical approach
• The Evolution of the Stellar Mass Function of Galaxies from z=4.0 and the First Comprehensive Analysis of its Uncertainties: Evidence for Mass-dependent Evolution
• A Direct Measurement of Major Galaxy Mergers at z < 3
• Understanding Galaxy Evolution through Emission Lines
• Semi-analytic modeling of the EBL and consequences for extragalactic gamma-ray spectra
• The size evolution of galaxies since z~3: combining SDSS, GEMS and FIRES
• Connecting Galaxies, Halos, and Star Formation Rates Across Cosmic Time
• Towards an understanding of the rapid decline of the cosmic star formation rate
• The effect of galaxy mass ratio on merger--driven starbursts
• Feedback and Recycled Wind Accretion: Assembling the z=0 Galaxy Mass Function
• Self-Regulated Star Formation in Galaxies via Momentum Input from Massive Stars
• Multi-Phase Galaxy Formation: High Velocity Clouds and the Missing Baryon Problem
• The Secular Evolution of Disk Structural Parameters
• The Importance of Satellite Quenching for the Build-Up of the Red Sequence of Present Day Galaxies
• The 2dF Galaxy Redshift Survey: The b_J-band galaxy luminosity function and survey selection function
• A Halo-Based Galaxy Group Finder: Calibration and Application to the 2dFGRS
• The Effects of Photoionization on Galaxy Formation - I: Model and Results at z=0
• Modelling the Galaxy Bimodality: Shutdown Above a Critical Halo Mass
• Can Photoionization Squelching Resolve the Sub-structure Crisis?
• Simulations of Galaxy Formation in a Lambda CDM Universe I: Dynamical and Photometric Properties of a Simulated Disk Galaxy
• Making Galaxies in a Cosmological Context: The Need for Early Stellar Feedback
• Halo Substructure And The Power Spectrum
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• A unified multi-wavelength model of galaxy formation
• Dynamical Friction and Galaxy Merging Timescales
• On the fraction of star formation occurring in bound stellar clusters
• GEMS: Galaxy Evolution from Morphologies and SEDs
• On Extending the Mass-Metallicity Relation of Galaxies by 2.5 Decades in Stellar Mass
• Starburst-driven galactic winds: I. Energetics and intrinsic X-ray emission
• Streams, substructures and the early history of the Milky Way
• The Halo Occupation Distribution and the Physics of Galaxy Formation
• A White Paper on keV Sterile Neutrino Dark Matter
• Chemical enrichment of the intra-cluster and intergalactic medium in a hierarchical galaxy formation model
• The Growth and Structure of Dark Matter Haloes
• The Size Evolution of High Redshift Galaxies
• Evidence for Ubiquitous Collimated Galactic-Scale Outflows along the Star-Forming Sequence at z~0.5
• A Revised Parallel-Sequence Morphological Classification of Galaxies: Structure and Formation of S0 and Spheroidal Galaxies
• The origin of angular momentum in dark matter halos
• The Role of Cold Flows in the Assembly of Galaxy Disks
• Galaxy Formation Theory
• The SAURON project - XVII. Stellar population analysis of the absorption line strength maps of 48 early-type galaxies
• UV-optical colours as probes of early-type galaxy evolution
• The K20 survey. VI. The Distribution of the Stellar Masses in Galaxies up to z~2
• The accretion of galaxies into groups and clusters
• The Initial-Final Mass Relation: Direct Constraints at the Low Mass End
• GALICS I: A hybrid N-body semi-analytic model of hierarchical galaxy formation
• Dry Mergers in GEMS: The Dynamical Evolution of Massive Early-Type Galaxies
• Galaxies in LCDM with Halo Abundance Matching: luminosity-velocity relation, baryonic mass-velocity relation, velocity function and clustering
• The Colours of Satellite Galaxies in Groups and Clusters
• Optical Star-Formation Rate Indicators
• The Universal Mass Accretion History of CDM Haloes
• The Structure of the Interstellar Medium of Star Forming Galaxies
• AGN-controlled cooling in elliptical galaxies
• Quasar Feedback: the Missing Link in Structure Formation
• A Model of Supernovae Feedback in Galaxy Formation
• Turbulent Structure of a Stratified Supernova-Driven Interstellar Medium
• z~7-10 Galaxies in the HUDF and GOODS fields, and their UV Luminosity Functions
• The formation of disc galaxies in a LCDM universe
• On the onset of galactic winds in quiescent star forming galaxies
• The infrared side of galaxy formation. I. The local universe in the semi-analytical framework
• A Revised Model for the Formation of Disk Galaxies: Low Spin and Dark-Halo Expansion
• The Non-Parametric Model for Linking Galaxy Luminosity with Halo/Subhalo Mass
• Angular momentum and galaxy formation revisited
• A fitting formula for the merger timescale of galaxies in hierarchical clustering
• The evolution of massive black holes and their spins in their galactic hosts
• The Assembly History of Field Spheroidals: Evolution of Mass-to-light Ratios and Signatures of Recent Star Formation
• Revisiting the Cosmic Cooling Crisis
• The History of the Baryon Budget: Cosmic Logistics in a Hierarchical Universe
• Shredded Galaxies as the Source of Diffuse Intrahalo Light On Varying Scales
• Linking Early and Late Type Galaxies to their Dark Matter Haloes
• The DEEP2 Galaxy Redshift Survey: The Relationship Between Galaxy Properties and Environment at z ~ 1
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Building Merger Trees from Cosmological N-body Simulations
• Galaxies-Intergalactic Medium Interaction Calculation --I. Galaxy formation as a function of large-scale environment
• The stellar halo of the Galaxy
• A Turnover in the Galaxy Main Sequence of Star Formation at $M_{\ast }\sim 10^{10}{M}_{\odot }$ for Redshifts $z<1.3$
• The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth
• The Nearly Universal Merger Rate of Dark Matter Haloes in Lambda-CDM Cosmology
• The dust content of galaxies from z = 0 to z = 9
• The velocity dispersion function of early-type galaxies
• The MORGANA model for the rise of galaxies and active nuclei
• A Catalogue and Analysis of Local Galaxy Ages and Metallicities
• The merger rate of massive galaxies
• History of Galaxy Interactions and their Impact on Star Formation over the Last 7 Gyr from GEMS
• Testing Tidal-Torque Theory: I. Spin Amplitude and Direction
• Galaxy Properties from the Ultra-violet to the Far-Infrared: Lambda-CDM models confront observations
• The correlation between black hole mass and bulge velocity dispersion in hierarchical galaxy formation models
• An analytical model for the history of cosmic star formation
• A marked correlation function analysis of halo formation times in the Millennium Simulation
• Mergers in Lambda-CDM: Uncertainties in Theoretical Predictions and Interpretations of the Merger Rate
• On the Formation of Globular Cluster Systems in a Hierarchical Universe
• Galaxy growth in the concordance $\Lambda$CDM cosmology
• The Mass-Metallicity and Luminosity-Metallicity Relation from DEEP2 at z ~ 0.8
• How stellar feedback simultaneously regulates star formation and drives outflows
• Galaxy-Induced Transformation of Dark Matter Halos
• The origin of dwarf ellipticals in the Virgo cluster
• Simulations of the galaxy population constrained by observations from z=3 to the present day: implications for galactic winds and the fate of their ejecta
• HACC: Simulating Sky Surveys on State-of-the-Art Supercomputing Architectures
• How To Model Supernovae in Simulations of Star and Galaxy Formation
• Stellar masses of SDSS-III BOSS galaxies at z~0.5 and constraints to galaxy formation models
• The Dynamics of Sinking Satellites Around Disk Galaxies: A Poor Man's Alternative to High-Resolution Numerical Simulations
• Bars in Disk-Dominated and Bulge-Dominated Galaxies at z~0: New Insights from ~3600 SDSS Galaxies
• Galaxies in a Simulated $\Lambda$CDM Universe II: Observable Properties and Constraints on Feedback
• The Launching of Cold Clouds by Galaxy Outflows I: Hydrodynamic Interactions with Radiative Cooling
• The effects of feedback on the morphology of galaxy discs
• Near-infrared imaging and the K-z relation for radio galaxies in the 7C Redshift Survey
• A Global Model For Circumgalactic and Cluster-Core Precipitation
• Semi-analytical model of galaxy formation with high-resolution N-body simulations
• On the Life and Death of Satellite Haloes
• Structure of Disk Dominated Galaxies: II. Color Gradients and Stellar Population Models
• The Effects of Gas on Morphological Transformation in Mergers: Implications for Bulge and Disk Demographics
• Outflows in Infrared-Luminous Starbursts at z < 0.5. I. Sample, NaI D Spectra, and Profile Fitting
• Non-Gravitational Heating in the Hierarchical Formation of X-ray Clusters
• Star Formation in Semi-Analytic Galaxy Formation Models with Multiphase Gas
• Stellar populations of early-type galaxies in different environments II. Ages and metallicities
• A calibration of the relation between the abundance of close galaxy pairs and the rate of galaxy mergers
• Galactic accretion and the outer structure of galaxies in the CDM model
• Estimating photometric redshifts with artificial neural networks
• Cosmic ray feedback in hydrodynamical simulations of galaxy formation
• Luminosity function and radial distribution of Milky Way Satellites in a LCDM Universe
• Evolution of the atomic and molecular gas content of galaxies
• Virial masses of galactic halos from galaxy-galaxy lensing: theoretical modeling and application to SDSS
• The Dark Side of Galaxy Color
• The Tully-Fisher Relation and Its Residuals for a Broadly Selected Sample of Galaxies
• PTHalos: A fast method for generating mock galaxy distributions
• Chemical Evolution in Hierarchical Models Of Cosmic Structure I: Constraints on the Early Stellar Initial Mass Function
• But What About... Cosmic Rays, Magnetic Fields, Conduction, & Viscosity in Galaxy Formation
• Star formation histories of early-type galaxies. I: Higher order Balmer lines as age indicators
• Minor Galaxy Interactions: Star Formation Rates and Galaxy Properties
• N-body Dark Matter Haloes with simple Hierarchical Histories
• The Luminosity-Metallicity relation in the local universe from the 2dF Galaxy Redshift Survey
• Reproducing the Stellar Mass/Halo Mass Relation in Simulated LCDM Galaxies: Theory vs Observational Estimates
• The Importance of Dry and Mixed Mergers for Early-Type Galaxy Formation
• Effects of Preheating on X-ray Scaling Relations in Galaxy Clusters
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• The Correlation of Star Formation Quenching with Internal Galaxy Properties and Environment
• The VIMOS VLT Deep Survey: The build-up of the colour-density relation
• The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations
• Dependence of Interstellar Turbulent Pressure on Supernova Rate
• An Explanation for the Observed Weak Size Evolution of Disk Galaxies
• Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction, and metal diffusion on galaxy formation
• Morphologies of z~0.7 AGN Host Galaxies in CANDELS: No trend of merger incidence with AGN luminosity
• Extragalactic Background Light from Hierarchical Galaxy Formation: Gamma-ray Attenuation up to the Epoch of Cosmic Reionization and the First Stars
• Modeling the formation and evolution of star cluster populations in galaxy simulations
• Non-linear Stochastic Galaxy Biasing in Cosmological Simulations
• How well can we really estimate the stellar masses of galaxies from broadband photometry?
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes I: Basic Dynamics
• The abundance of (not just) dark matter haloes
• Spatially resolved spectroscopy of early-type galaxies over a range in mass
• Essential physics of early galaxy formation
• Photometric scaling relations of lenticular and spiral galaxies
• The Kinematic Connection Between Galaxies and Dark Matter Haloes
• The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands
• The local space density of Sb-Sdm galaxies as function of their scalesize, surface brightness and luminosity
• Squelched Galaxies and Dark Halos
• X-ray coronae in simulations of disc galaxy formation
• The Most Dark Matter Dominated Galaxies: Predicted Gamma-ray Signals from the Faintest Milky Way Dwarfs
• Galaxy Halo Occupation at High Redshift
• GeV Gamma-Ray Attenuation and the High-Redshift UV Background
• On the origin of the galaxy luminosity function
• Improved Cosmological Constraints from Gravitational Lens Statistics
• A fundamental problem in our understanding of low mass galaxy evolution
• The Atomic to Molecular Transition and its Relation to the Scaling Properties of Galaxy Disks in the Local Universe
• The importance of minor-merger-driven star formation and black-hole growth in disk galaxies
• Measuring Galaxy Environments with Deep Redshift Surveys
• The baryon fraction of LambdaCDM haloes
• The Impact of Feedback on Disk Galaxy Scaling Relations
• The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model
• The Bimodal Galaxy Stellar Mass Function in the COSMOS Survey to z~1: A Steep Faint End and a New Galaxy Dichotomy
• The Abundance of Distant and Extremely Red Galaxies: The Role of AGN Feedback in Hierarchical Models
• Galaxy Merger Statistics and Inferred Bulge-to-Disk Ratios in Cosmological SPH Simulations
• Suppression of star formation in early-type galaxies by feedback from supermassive black holes
• Gravitational Waves from Supermassive Black Hole Coalescence in a Hierarchical Galaxy Formation Model
• SHARDS: an optical spectro-photometric survey of distant galaxies
• Towards Cosmological Concordance on Galactic Scales
• Satellite abundances around bright isolated galaxies
• FIRE-3: Updated Stellar Evolution Models, Yields, & Microphysics and Fitting Functions for Applications in Galaxy Simulations
• The effect of non--gravitational gas heating in groups and clusters of galaxies
• The evolution of the galaxy distribution
• The role of mergers in driving morphological transformation over cosmic time
• Cooling and heating the ICM in hydrodynamical simulations
• The formation and evolution of low-surface-brightness galaxies
• The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
• The dark matter halos of dwarf galaxies: a challenge for the LCDM paradigm?
• The virialized mass of dark matter haloes
• The growth of galaxies in cosmological simulations of structure formation
• Downsizing by Shutdown in Red Galaxies
• 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
• The Formation of a Disk Galaxy within a Growing Dark Halo
• Implications of Cosmological Gamma-Ray Absorption - I.Evolution of the Metagalactic Radiation Field
• Modeling Angular-Momentum History in Dark-Matter Halos
• The Intrinsic Properties of SDSS Galaxies
• The dependence on environment of Cold Dark Matter Halo properties
• The Parameter Space of Galaxy Formation
• The Most Massive Galaxies at 3.0<z<4.0 in the NEWFIRM Medium-Band Survey: Properties and Improved Constraints on the Stellar Mass Function
• AGN Feedback Causes Downsizing
• Stellar populations of early-type galaxies in different environments I. Line-strength indices
• Tidally Triggered Star Formation in Close Pairs of Galaxies: Major and Minor Interactions
• The metal enrichment of elliptical galaxies in hierarchical galaxy formation models
• A Closer look at Bursty Star Formation with $L_{H\alpha }$ and $L_{UV}$ Distributions
• Halo Profiles and the Concentration-Mass Relation for a ΛCDM Universe
• Mismatch and Misalignment: Dark Haloes and Satellites of Disc Galaxies
• The matallicities of star-forming galaxies at intermediate redshifts 0.47 < z < 0.92
• How to quench a galaxy
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• Halos around edge-on disk galaxies in the SDSS
• Orbital structure of merger remnants: Trends with gas fraction in 1:1 mergers
• Massive Coronae of Galaxies
• Physical Conditions in the Low-Ionization Component of Starburst Outflows: The Shape of Near-Ultraviolet and Optical Absorption-Line Troughs in Keck Spectra of ULIRGs
• Dark halo properties from rotation curves
• Adding Environmental Gas Physics to the Semi-Analytic Method for Galaxy Formation: Gravitational Heating
• Abundance of Field Galaxies
• Beyond Halo Mass: Galactic Conformity as a Smoking Gun of Central Galaxy Assembly Bias
• Deep Extragalactic VIsible Legacy Survey (DEVILS): SED Fitting in the D10-COSMOS Field and the Evolution of the Stellar Mass Function and SFR-$M_{\star }$ relation
• 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
• Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
• X-ray Clusters of Galaxies as Tracers of Structure in the Universe
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?
• Radiative Stellar Feedback in Galaxy Formation: Methods and Physics
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• Galaxy formation in pre-processed dark halos
• Interpreting Debris from Satellite Disruption In External Galaxies
• The Fate of Substructures in Cold Dark Matter Haloes
• The metal enrichment of the intracluster medium in hierarchical galaxy formation models
• Global Probes of the Impact of Baryons on Dark Matter Halos
• Metallicity of the intergalactic medium using pixel statistics: IV. Oxygen
• The Evolution of the Optical and Near-Infrared Galaxy Luminosity Functions and Luminosity Densities to z~2
• The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies
• Models of the ICM with Heating and Cooling: Explaining the Global and Structural X-ray Properties of Clusters
• The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $\Lambda$CDM
• Effects of dust grains on early galaxy evolution
• First spectroscopic measurements of [OIII] emission from Lyman-alpha selected field galaxies at z ~ 3.1
• On the Origin of the Galaxy Star-Formation-Rate Sequence: Evolution and Scatter
• Massive black hole merger rates: the effect of kpc separation wandering and supernova feedback
• The Impact of Galaxy Formation on the X-ray Evolution of Clusters
• The Dark Side of Galaxy Color: evidence from new SDSS measurements of galaxy clustering and lensing
• The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution
• The Robustness of Dark Matter Density Profiles in Dissipationless Mergers
• Formation of the Galactic stellar halo I. Structure and kinematics
• The halo model and numerical simulations
• The B-Band Luminosity Function of Red and Blue Galaxies up to z=3.5
• Galactic chemical evolution in hierarchical formation models - I. Early-type galaxies in the local Universe
• Simulating the Formation of the Local Galaxy Population
• Cosmic Emulation: Fast Predictions for the Galaxy Power Spectrum
• Disc galaxy evolution models in a hierarchical formation scenario: structure and dynamics
• The Phase-Space Parameters of Brightest Halo Galaxies
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• Shocked Superwinds from the z~2 Clumpy Star-forming Galaxy, ZC406690
• The Beginning and Evolution of the Universe
• Kinematic Constraints on Evolutionary Scenarios for Blue Compact Dwarf Galaxies : I. Neutral Gas Dynamics
• On The Assembly History of Dark Matter Haloes
• The Impact of Cooling and Feedback on Disc Galaxies
• Gas cooling in simulations of the formation of the galaxy population
• 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
• Cosmic evolution of the galaxy mass and luminosity functions by morphological type from multi-wavelength data in the CDF-South
• Molecular Gas in the Lensed Lyman Break Galaxy cB58
• Simulations of galaxy formation in a cosmological volume
• Scaling Relations of Dwarf Galaxies without Supernova-Driven Winds
• Galaxy Formation Spanning Cosmic History
• Pre-heating the ICM in high resolution simulations: the effect on the gas entropy
• Predicting the number, spatial distribution and merging history of dark matter haloes
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• The DEEP Groth Strip Survey VII: The Metallicity of Field Galaxies at 0.26<z<0.82 and the Evolution of the Luminosity-Metallicity Relation
• What Causes The Formation of Disks and End of Bursty Star Formation?
• Dependence of Halo Properties on Interaction History, Environment and Cosmology
• The Redshift Distribution of Near-IR Selected Galaxies in the Great Observatories Origins Deep Survey as a Test of Galaxy Formation Scenarios
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• Luminosity and stellar mass functions of disks and spheroids in the SDSS and the supermassive black hole mass function
• Active Galactic Nuclei In Cosmological Simulations - I. Formation of black holes and spheroids through mergers
• The route to massive black hole formation via merger-driven direct collapse: a review
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• The Evolution of Stellar Exponential Discs
• The properties of the interstellar medium of galaxies across time as traced by the neutral atomic carbon [CI]
• A Galactic Wind at z = 5.190
• The density of very massive evolved galaxies to z~1.7
• Chemical evolution of local galaxies in a hierarchical model
• The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations
• Evaluating Semi-Analytic Halo Merging Histories
• Halo Substructure and Disk Heating in a Lambda CDM Universe
• The Dependence of Velocity and Clustering Statistics on Galaxy Properties
• Tidally-Triggered Star Formation in Close Pairs of Galaxies 2: Constraints on Burst Strengths and Ages
• The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
• Reconstructing the cosmic density field with the distribution of dark matter halos
• A Comparison of Semi-Analytic and Smoothed Particle Hydrodynamics Galaxy Formation
• Spectral Templates Optimal for Selecting Galaxies at z > 8 with JWST
• Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies
• CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2
• On the Distribution of Haloes, Galaxies and Mass
• Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes. I: Feedback-regulated Star Formation and Black Hole Growth
• Preheating by Previrialization and its Impact on Galaxy Formation
• Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
• Binary Aggregations in Hierarchical Galaxy Formation: The Evolution of the Galaxy Luminosity Function
• How Do Galaxies Get Their Gas?
• Semi-analytic forecasts for JWST -- IV. Implications for cosmic reionization and LyC escape fraction
• Galaxy formation in semi-analytic models and cosmological hydrodynamic zoom simulations
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• The Masses, Ancestors and Descendents of Extremely Red Objects: Constraints from Spatial Clustering
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. II. The star formation properties of galaxies in the Virgo cluster and surroundings
• Bulge Formation via Mergers in Cosmological Simulations
• Dark Matter Halos of Disk Galaxies: Constraints from the Tully-Fisher Relation
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design, Data Processing, and Spectral Analysis Methods
• Biases and Uncertainties in Physical Parameter Estimates of Lyman Break Galaxies from Broad-band Photometry
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• Lyman Alpha Emitters in the Hierarchically Clustering Galaxy Formation
• The art of modeling CO, [CI], and [CII] in cosmological galaxy formation models
• The observability of gamma-rays from neutralino annihilations in Milky Way substructure
• Evolution of field early-type galaxies: The view from GOODS/CDFS
• Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey
• The Epoch of Reionization in Models with Reduced Small Scale Power
• The host dark matter halos of [OII] emitters at 0.5< z< 1.5
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• Galaxy Formation at z~3: Constraints from Spatial Clustering
• The ALMA Spectroscopic Survey in the HUDF: the molecular gas content of galaxies and tensions with IllustrisTNG and the Santa Cruz SAM
• Star Formation History and Stellar Metallicity Distribution in a Cold Dark Matter Universe
• Early Hierarchical Formation of Massive Galaxies Triggered By Interactions
• The Varied Fates of z~2 Star-forming Galaxies
• The Dependence of the Galaxy Luminosity Function on Large-Scale Environment
• The maximum accretion rate of hot gas in dark matter halos
• A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
• Evidence that powerful radio jets have a profound influence on the evolution of galaxies
• Properties of the galaxy population in hydrodynamical simulations of clusters
• Galaxy Formation in WDM Cosmology
• Quasar Evolution Driven by Galaxy Encounters in Hierarchical Structures
• The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
• Simulations of Dust in Interacting Galaxies I: Dust Attenuation
• An Empirical Model for the Star Formation History in Dark Matter Halos
• On the morphologies, gas fractions, and star formation rates of small galaxies
• Massive star formation in Wolf-Rayet galaxies. V: Star formation rates, masses and the importance of galaxy interactions
• Non-uniform reionization by galaxies and its effect on the cosmic microwave backgroun
• A Revised LCDM Mass Model For The Andromeda Galaxy
• Sub-mm Emission Line Deep Fields: CO and [CII] Luminosity Functions out to z = 6
• Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN
• Effects of dynamical evolution on the distribution of substructures
• Formation of S0 galaxies through mergers. Morphological properties: tidal relics, lenses, ovals, and other inner components
• A Transition Mass in the Local Tully-Fisher Relation
• Momentum transfer across shear flows in Smoothed Particle Hydrodynamic simulations of galaxy formation
• On the supernovae heating of intergalactic medium
• The Millennium Galaxy Catalogue: Exploring the Color-Concentration Bimodality via Bulge-Disc Decomposition
• Formation of S0 galaxies through mergers. Bulge-disc structural coupling resulting from major mergers
• An empirical initial-final mass relation from hot, massive white dwarfs in NGC 2168 (M35)
• Clues for the origin of the fundamental metallicity relations. I: The hierarchical building up of the structure
• Massive and Red Objects predicted by a semianalytical model of galaxy formation
• Towards a physical picture of star-formation quenching: the photometric properties of recently-quenched galaxies in the Sloan Digital Sky Survey
• Quantitative Morphological Analysis of the HDF--North and HDF-South. I. Early- and Late-type Luminosity-Size Relations of galaxies out to z~1
• Probing recent star formation with absorption-line strengths in hierarchical models and observations
• GALICS -- VI. Modelling Hierarchical Galaxy Formation in Clusters
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Insights on the Formation, Evolution, and Activity of Massive Galaxies From Ultra-Compact and Disky Galaxies at z=2-3
• The elliptical colour-magnitude relation as a discriminant between the monolithic and merger paradigms: the importance of progenitor bias
• The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: II. The red bands
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution?
• Hierarchical Formation of Galaxies with Dynamical Response to Supernova-Induced Gas removal
• Evaluating and Improving Semi-analytic modelling of Dust in Galaxies based on Radiative Transfer Calculations
• The evolution of the galaxy luminosity function in the rest frame blue band up to z=3.5
• Constraining evolution in the Halo Model using galaxy redshift surveys
• Resolving The Generation of Starburst Winds in Galaxy Mergers
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• The Group Evolution Multiwavelength Study (GEMS): bimodal luminosity functions in galaxy groups
• The angular momentum of dark halos: merger and accretion effects
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• A Bridge from Optical to Infrared Galaxies: Explaining Local Properties, Predicting Galaxy Counts and the Cosmic Background Radiation
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• Coupled spheroid and black-hole formation, and the multifrequency detectability of active galactic nuclei and submillimetre sources
• Numerical Galaxy Catalog -I. A Semi-analytic Model of Galaxy Formation with N-body simulations
• The Millennium Run Observatory: First Light
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Spatially Resolved Gas-Phase Metallicity Distributions in Barred and Unbarred Spirals
• Breaking the Disk/Halo Degeneracy with Gravitational Lensing
• Gas Mass Fractions and Star Formation in Blue-Sequence E/S0 Galaxies
• Contribution from Star-Forming Galaxies to the Cosmic Gamma-Ray Background Radiation
• Galaxy Formation in Preheated Intergalactic Media
• The abundance of Lyman-(α) emitters in hierarchical models
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• Modelling SCUBA sources in a Lambda-CDM cosmology: hot starbursts or cold extended galactic dust?
• The DEEP2 Galaxy Redshift Survey: Spectral classification of galaxies at z~1
• Galaxy spectral parameterisation in the 2dF Galaxy Redshift Survey as a diagnostic of star formation history
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• Disentangling the Cosmic Web Towards FRB 190608
• Empirical constraints on the formation of early-type galaxies
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• Electromagnetic Counterparts to Black Hole Mergers
• Environmental Effects on Evolution of Cluster Galaxies in a LCDM Universe
• Post-merger Signatures of Red-sequence Galaxies in Rich Abell Clusters at $z\lesssim 0.1$
• The Ursa Major Cluster of Galaxies. III. Optical observations of dwarf galaxies and the luminosity function down to M_R=-11
• A simple model for AGN feedback in nearby early-type galaxies
• How well do cosmological simulations reproduce individual-halo properties?
• The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
• Morphology-Density Relation for Simulated Clusters of Galaxies in Cold Dark Matter Dominated Universe
• Distinguishing Local and Global Influences on Galaxy Morphology: An HST Comparison of High and Low X-ray Luminosity Clusters
• High redshift quasars and the supermassive black hole mass budget: constraints on quasar formation models
• Objective Classification of Galaxy Spectra using the Information Bottleneck Method
• Neutral Gas Outflows and Inflows in Infrared-Faint Seyfert Galaxies
• Resolution-independent modeling of environmental effects in semi-analytic models of galaxy formation that include ram-pressure stripping of both hot and cold gas
• Two-Phase Galaxy Formation
• The Formation and Evolution of Virgo Cluster Galaxies - II. Stellar Populations
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• Semi-analytic forecasts for JWST -- III. Intrinsic production efficiency of Lyman-continuum radiation
• Mock Catalogs for the DEEP2 redshift survey
• Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• Observational tests of the evolution of spheroidal galaxies
• Quantifying the Drivers of Star Formation on Galactic Scales. I. The Small Magellanic Cloud
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• The Properties of Spiral Galaxies: Confronting Hierarchical Galaxy Formation Models with Observations
• Probing the star formation history using the redshift evolution of luminosity functions
• Mass Function of Low Mass Dark Halos
• Newborn spheroids at high redshift: when and how did the dominant, old stars in today's massive galaxies form?
• The metallicity-luminosity relation at medium redshift based on faint CADIS emission line galaxies
• Sizing up Partially-Depleted Galaxy Cores
• Evolution of the Luminosity Function and Colors of Galaxies in a Lambda-CDM Universe
• Turbulent dissipation in the ISM: the coexistence of forced and decaying regimes and implications for galaxy formation and evolution
• The Observed Evolution of Galaxy Clustering Vs. Epoch-Dependent Biasing Models
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• The Ages of Dwarf Ellipticals
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• HST Photometry for the Halo Stars in the Leo Elliptical NGC 3377
• A simple model linking galaxy and dark matter evolution
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Realistic galaxy image simulation via score-based generative models
• Star Formation at the Twilight of the Dark Ages: Which Stars Reionized the Universe?
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Galaxy Number Counts in the Subaru Deep Field: Multi-band Analysis in a Hierarchical Galaxy Formation Model
• Infrared Luminosity Function of the Coma Cluster
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• Relations Between Environments of Quasars and Galaxy Formation
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• A Dimensional study of Disk Galaxies
• New multi-zoom method for N-body simulations: application to galaxy growth by accretion
• On the origin of the angular momentum properties of gas and dark matter in galactic halos and its implications
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• Multiple Merging Events in the Double Cluster A3128/A3125
• Young and turbulent: the early life of massive galaxy progenitors
• X-Ray Evolution of Active Galactic Nuclei and Hierarchical Galaxy Formation
• Measuring the Nonlinear Biasing Function from a Galaxy Redshift Survey
• Metals in the z~3 intergalactic medium: results from an ultra-high signal-to-noise ratio UVES quasar spectrum
• $\text{Mangrove}$: Learning Galaxy Properties from Merger Trees
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• The Tully-Fisher Relation as a Measure of Luminosity Evolution: A Low Redshift Baseline for Evolving Galaxies
• Luminosity Density of Galaxies and Cosmic Star Formation Rate from Lambda-CDM Hydrodynamical Simulations
• On stellar mass loss from galaxies in groups and clusters
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Marked clustering statistics in $f(R)$ gravity cosmologies
• 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
• Multitracer cosmological line intensity mapping mock lightcone simulation
• Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties
• The Role of Cold Flows and Reservoirs in Galaxy Formation With Strong Feedback
• The DEEP Groth Strip Galaxy Redshift Survey. VIII. The Evolution of Luminous Field Bulges at Redshift z ~ 1
• The dependence of the pairwise velocity dispersion on galaxy properties
• Status of Cold Dark Matter Cosmology
• Catastrophic Cooling in Superwinds: Line Emission and Non-equilibrium Ionization
• The Expected Mass Function for Low Mass Galaxies in a CDM Cosmology: Is There a Problem?
• Reliability of the dark matter clustering in cosmological N-body simulation on scales below the mean separation length of particles
• The environmental dependence of clustering in hierarchical models
• Evolutionary paths among different red galaxy types at 0.3 < z < 1.5 and the late buildup of massive E-S0's through major mergers
• Simulating Supersonic Turbulence in Galaxy Outflows
• Damped Lyman alpha systems and galaxy formation models - II. High ions and Lyman limit systems
• Detection of satellite remnants in the Galactic Halo with Gaia - I. The effect of the Galactic background, observational errors and sampling
• The formation of galaxy disks in a hierarchical universe
• Modeling Galaxy Clustering by Color
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• Model for Gravitational Interaction between Dark Matter and Baryons
• The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman 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
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• A Prescription for Galaxy Biasing Evolution as a Nuisance Parameter
• The Cluster Galaxy Circular Velocity Function
• Completeness in Photometric and Spectroscopic Searches for Clusters
• The pairwise velocity dispersion of galaxies: luminosity dependence and a new test of galaxy formation models
• The Cold Dark Matter crisis on galactic and subgalactic scales
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• Dust reddening in star-forming galaxies
• Models of Disk Evolution: Confrontation with Observations
• Spatial and luminosity distributions of galactic satellites
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Strong lensing statistics in large, z~<0.2 surveys: bias in the lens galaxy population
• Physical properties of Herschel selected galaxies in a semi-analytic galaxy formation model
• Simultaneous Modelling of the Stellar Halo and Globular Cluster System of NGC 5128
• The angular momentum of disc galaxies: implications for gas accretion, outflows, and dynamical friction
• Regulation of Star Formation by a Hot Circumgalactic Medium
• The evolution of Ks-selected galaxies in the GOODS/CDFS deep ISAAC field
• Discs in early-type lensing galaxies: effects on magnification ratios and measurements of $H_0$
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Patchy He II reionization and the physical state of the IGM
• Disk Galaxy Scaling Relations in the SFI++: Intrinsic Scatter and Applications
• Cosmic CARNage I: on the calibration of galaxy formation models
• A deeper view of Extremely Red Galaxies: the redshift distribution in the GOODS/CDFS ISAAC field
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Empirical Constraints for the Magnitude and Composition of Galactic Winds
• Galaxy number counts in the Hubble Deep Field as a strong constraint on a hierarchical galaxy formation model
• Merger relics of cluster galaxies
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• The Metallicity of Diffuse Intrahalo Light
• Testing homogeneity in the Sloan Digital Sky Survey Data Release Twelve with Shannon entropy
• Gravitational Lensing by a Compound Population of Halos: Standard Models
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• How does gas cool in DM halos?
• Formation of Supermassive Black Holes in Galactic Bulges: A Rotating Collapse Model Consistent with the $\mbh-σ$ Relation
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• NIHAO III: The constant disc gas mass conspiracy
• The contribution of HI-bearing ultra-diffuse galaxies to the cosmic number density of galaxies
• A backwards approach to the formation of disk galaxies I. Stellar and gas content
• Dynamical self-friction: how mass loss slows you down
• Composition of Low Redshift Halo Gas
• Evolution along the sequence of S0 Hubble types induced by dry minor mergers. II - Bulge-disk coupling in the photometric relations through merger-induced internal secular evolution
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• On the algorithms of radiative cooling in semi-analytic models
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Testing the Halo Model Against the SDSS Photometric Survey
• 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?
• The red and blue galaxy populations in the GOODS field: evidence for an excess of red dwarfs
• An analytic model for the epoch of halo creation
• Numerical simulations of the cosmic star formation history
• Schechter vs. Schechter: Sub-Arcsecond Gravitational Lensing and Inner Halo Profiles
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• Early Preheating and Galaxy Formation
• Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
• A NOEMA molecular line scan of the Hubble Deep Field North: Improved constraints on the CO luminosity functions and cosmic density of molecular gas
• Exploring the evolution of spiral galaxies
• A cosmological study of the star formation history in the solar neighbourhood
• Flux-limited strong gravitational lensing and dark energy
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• 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
• Testing the Modified Press-Schechter Model against N-Body Simulations
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• A Unique View of AGN-Driven Molecular Outflows: The Discovery of a Massive Galaxy Counterpart to a $z=2.4$ High-Metallicity Damped Lyman-$\alpha$ Absorber
• Empirically-motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations
• Galactosynthesis: Halo Histories, Star Formation, and Disks
• Spatial Clustering of High Redshift Lyman Break Galaxies
• The Evolution of Field Early-Type Galaxies in the FDF and WHDF
• Suppressing cosmic variance with paired-and-fixed cosmological simulations: average properties and covariances of dark matter clustering statistics
• Numerical simulations of buoyancy instabilities in galaxy cluster plasmas with cosmic rays and anisotropic thermal conduction
• Temperature and Entropy Fields of Baryonic Gas in the Universe
• Galaxy Outflows Without Supernovae
• Is NGC 3108 transforming itself from an early to late type galaxy -- an astronomical hermaphrodite?
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• On an Analytical Framework for Voids: Their abundances, density profiles and local mass functions
• Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• Forming stars on a viscous timescale: the key to exponential stellar profiles in disk galaxies?
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• 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
• The Radius of Baryonic Collapse in Disc Galaxy Formation
• Recent galaxy mergers and residual star formation of red sequence galaxies in galaxy clusters
• Precision Cosmology: Successes and Challenges
• High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair
• The Origin of the 24-micron Excess in Red Galaxies
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• The peculiar velocities of satellites of external disk galaxies
• Violent quenching: molecular gas blown to 1000 km/s during a major merger
• Number Counts of Bright Extremely Red Objects: Evolved Massive Galaxies at z~1
• The Fundamental Plane of Spiral Galaxies: Theoretical Expectations
• Identifying the progenitor set of present-day early-type galaxies: a view from the standard model
• The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
• Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
• The concentration-velocity dispersion relation in galaxy groups
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• DSPS: Differentiable Stellar Population Synthesis
• Massive galaxy formation caught in action at z~5 with JWST
• The Upper Asymptotic Giant Branch of the Elliptical Galaxy Maffei 1, and Comparisons with M32 and NGC 5128
• A simple model for the evolution of super-massive black holes and the quasar population
• The descendents of Lyman Break Galaxies in galaxy clusters: spatial distribution and orbital properties
• The mass loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts
• The Group Evolution Multiwavelength Study (GEMS): The near-infrared luminosity function of nearby galaxy groups
• The cosmic spectral energy distribution in the EAGLE simulation
• Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• Diffuse Far-UV Line Emission from the Low-Redshift Lyman Break Galaxy Analog KISSR242
• Virial halo mass function in the $Planck$ cosmology
• Chemical Enrichment in Damped Lyman Alpha Systems From Hierarchical Galaxy Formation Models
• Molecular Outflows in z > 6 QSO Hosts Driven by Star Formation
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Far-Ultraviolet Number Counts of Field Galaxies
• Statistics of Magnification Perturbations by Substructure in the Cold Dark Matter Cosmological Model
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• The effect of the environment on the Faber Jackson relation
• Strong Evolution in the Luminosity-Velocity Relation at z>1?
• Rosella: A mock catalogue from the P-Millennium simulation
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• Star Formation Histories Across the Interacting Galaxy NGC 6872, the Largest-Known Spiral
• On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations
• Constraints on the velocity profiles of galaxies from strong lensing statistics and semi-analytical modelling of galaxy formation
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• High-redshift radio galaxies: at the crossroads
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• The mass-dependent star formation histories of disk galaxies: infall model versus observations
• The Evolution of the ISM in the Mildly Disturbed Spiral Galaxy NGC 4647
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• A new method for testing isotropy with Shannon entropy
• Observations of the High Redshift Universe
• Massive spheroids can form in single minor mergers
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Galaxy interactions in filaments and sheets: effects of the large-scale structures versus the local density
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• The z ~ 4 Lyman Break Galaxies: Colors and Theoretical Predictions
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• The photoionization effect of the ultraviolet background on the colour-magnitude relation of elliptical galaxies
• Extragalactic Science with the Experiment for Cryogenic Large-aperture Intensity Mapping
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• The star-forming progenitors of massive red galaxies
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
• A physical model for the origin of the diffuse cosmic infrared background
• Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function
• Galaxy morphology and evolution from SWAN Adaptive Optics imaging
• The SZ Effect as a Probe of Non-Gravitational Entropy in Groups and Clusters of Galaxies
• Unravelling the Cosmic Web: An analysis of the SDSS DR14 with the Local Dimension
• Type Ia supernovae in a hierarchical galaxy formation model: the Milky Way
• Feedback Processes in Early-Type Galaxies
• Stellar populations of massive elliptical galaxies in very rich clusters
• Consequences of dark matter self-annihilation for galaxy formation
• The Origin and Evolution of the Mass-Metallicity Relation using GalICS
• Dynamical response to supernova-induced gas removal in two-component spherical galaxies
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium II: Effect of Turbulence within a Stratified Medium
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• Star formation in high redshift galaxies including Supernova feedback: effect on stellar mass and luminosity functions
• Lyman-break galaxies: high mass or low?
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Simulating the formation of cosmic structure
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• Ionised gas kinematics in bipolar H II regions
• On the Detectability of the SZ Effect of Massive Young Galaxies
• An empirical model to form and evolve galaxies in dark matter halos
• Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim 9-17$
• Self-similar collapse of collisional gas in an expanding Universe
• A consistent model for both the HI and stellar mass functions of galaxies
• Modelling the dynamical friction timescale of sinking satellite
• Bimodal AGNs in Bimodal Galaxies
• A VLT/FORS2 Narrowband Imaging Search for MgII Emission Around z ~ 0.7 Galaxies
• Relating galaxies across different redshift to study galaxy evolution
• Abundance matching for low mass galaxies in the CDM and FDM models
• Leaving the dark ages with AMIGA
• The progenitors of magnetic white dwarfs in open clusters
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• Exploring the Correlation between $\mathrm{H}\alpha$-to-UV Ratio and Burstiness for Typical Star-forming Galaxies at $z\sim 2$
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Number Density Evolution of Ks -band Selected High Redshift Galaxy Populations in the AKARI North Ecliptic Pole Field
• The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Luminous Matter Distribution, Bulk Flows and Baryon Contents in Cosmological Models with a Local Void
• Satellite survival in cold dark matter cosmology
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• A simple analytical model for the abundance of damped Ly-αabsorbers
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• An Overdensity of Extremely Red Objects Around Faint Mid-IR galaxies
• Chemical evolution of elliptical galaxies I: supernovae and AGN feedback
• Dissipative phenomena in extended-bodies interactions I: Methods Dwarf galaxies of the Local Group and their synthetic CMDs
• Interacting dark energy collapse with matter components separation
• Do minor interactions trigger star formation in galaxy pairs?
• A deep learning approach to halo merger tree construction
• The correlations between galaxy properties in different environments of the cosmic web
• From Gas to Stars Over Cosmic Time
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• OMEGA - OSIRIS Mapping of Emission-line Galaxies in A901/2: IV. - Extinction of Star-Formation Estimators with Inclination
• Nonlinear structure formation in Bound Dark Energy
• Understanding Galaxy Formation and Evolution
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• Secular evolution versus hierarchical merging: galaxy evolution along the Hubble sequence, in the field and rich environments
• Reliability of merger tree realizations of dark halos in the Monte-Carlo modeling of galaxy formation
• The quantity of dark matter in early-type galaxies and its relation to the environment
• The Degeneracy of Galaxy Formation Models
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Discovery of a double ring in the dwarf galaxy Mrk409
• Stellar kinematics and populations out to 1.5 effective radius in the elliptical galaxy NGC4636
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• Probing baryonic processes and gastrophysics in the formation of the Milky Way dwarf satellites: I. metallicity distribution properties
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Tracing the green valley with entropic thresholding
• Galaxy formation from a timescale perspective
• JWST Discovery of a Very Fast Biconical Outflow of Warm Molecular Gas in the Nearby Ultra-Luminous Infrared Galaxy F08572+3915 NW
• On the theory of mass loss in dwarf galaxies: I - basic equations and the case of wave/thermal driven winds
• Hierarchical Bayesian inference of the Initial Mass Function in Composite Stellar Populations
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Massive Black Hole Mergers
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• The Qz5 Survey (I): How the HI Mass Density of the Universe Evolves With Cosmic Time
• 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 Evolution of Spheroidal Galaxies in Different Environments
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• Thermodynamic evolution of the cosmological baryonic gas : II. Galaxy formation
• Metallicity and HI Column Density Properties of Damped Lyman-$\alpha$ Systems
• Star Formation and Chemical Evolution of DLAs with Semi-Analytical Model
• Galaxy Interactions, Star Formation History, and Bulgeless Galaxies
• Fast radiative transfer of dust reprocessing in semi-analytic models with artificial neural networks
• The Origin of the Stellar Mass-Stellar Metallicity Relation in the Milky Way Satellites and beyond
• The stellar mass - physical effective radius relation for dwarf galaxies in low-density environments
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Quantifying stochasticity-driven uncertainties in H II region metallicities
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
• Cosmology with One Galaxy: Auto-Encoding the Galaxy Properties Manifold
• Extended Enriched Gas in a Multi-Galaxy Merger at Redshift 6.7
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• The Influence of Subhaloes on Host Halo Properties
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• VEGA: Voids idEntification using Genetic Algorithm
• AGN Host Galaxies
• From Gas to Stars over Cosmic Time
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Galactosynthesis Predictions at High Redshift
• Constraints on the Epoch of Reionization with Roman Space Telescope and the Void Probability Function of Lyman-Alpha Emitters
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• Detailed modelling of the EBL along VHE γ-ray paths
• The progenitor galaxies of stellar haloes as "failed" Milky Ways
• Extended Hernquist-Springel formalism for cosmic star formation
• A physically-motivated template set for high-z galaxy SED fitting
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• The long road to the Green Valley: Tracing the evolution of the Green Valley galaxies in the EAGLE simulation
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Resolved Neutral Outflow from a Lensed Dusty Star Forming Galaxy at z=2.09
• Disk galaxy evolution: from the Milky Way to high-redshift disks
• The Optical Extragalactic Background Light from Resolved Galaxies
• Momentum deposition of supernovae with cosmic rays
• Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
• Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
• Stellar Populations of Spectroscopically Decomposed Bulge-Disk for S0 Galaxies from the CALIFA survey
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• The NIBLES bivariate luminosity--HI mass distribution function revised using Arecibo follow-up observations
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos