Clustering of Galaxies in a Hierarchical Universe: I. Methods and Results at z=0

Abstract

We introduce a new technique for following the formation and evolution of galaxies in cosmological N-body simulations. Dissipationless simulations are used to track the formation and merging of dark matter halos as a function of redshift. Simple prescriptions, taken directly from semi-analytic models of galaxy formation, are adopted for cooling, star formation, supernova feedback and the merging of galaxies within the halos. This scheme enables us to study the clustering properties of galaxies and to investigate how selection by type, colour or luminosity influences the results. In this paper, we study properties of the galaxy distribution at z=0. These include luminosity functions, colours, correlation functions, pairwise peculiar velocities, cluster M/L ratios and star formation rates. We focus on two variants of a CDM cosmology: a high- density model with Gamma=0.21 (TCDM) and a low-density model with Omega=0.3 and Lambda=0.7 (LCDM). Both are normalized to reproduce the I-band Tully-Fisher relation near a circular velocity of 220 km/s. Our results depend strongly both on this normalization and on the prescriptions for star formation and feedback. Very different assumptions are required to obtain an acceptable model in the two cases. For TCDM, efficient feedback is required to suppress the growth of galaxies low-mass field halos. Without it, there are too many galaxies and the correlation function turns over below 1 Mpc. For LCDM, feedback must be weak, otherwise too few L* galaxies are produced and the correlation function is too steep. Given the uncertainties in modelling some of the key physical processes, we conclude that it is not yet possible to draw conclusions about the values of cosmological parameters from studies of this kind. Further work on global star formation and feedback effects is required to narrow the range of possibilities

43 pages, Latex, 16 figures included, 2 additional GIF format figures, submitted to MNRAS

References in corpus (9)

• The Global Schmidt Law in Star Forming Galaxies
• The Formation of Galactic Disks
• Dark Matter Halos within Clusters
• Survival of Substructure within Dark Matter Haloes
• Southern Sky Redshift Survey: Clustering of Local Galaxies
• The seeds of rich galaxy clusters in the Universe
• The K-band Hubble diagram for the brightest cluster galaxies: a test of hierarchical galaxy formation models
• The Near-Infrared Number Counts and Luminosity Functions of Local Galaxies
• Merging History Trees of Dark Matter Haloes: a Tool for Exploring Galaxy Formation Models

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• A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protocluster at $z=6.01$
• The Group Evolution Multiwavelength Study (GEMS): bimodal luminosity functions in galaxy groups
• The Virial Mass Function of Nearby SDSS Galaxy Clusters
• Spatial distribution of galactic halos and their merger histories
• Accurate determination of the Lagrangian bias for the dark matter halos
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes II: Global Properties
• Locally Biased Galaxy Formation and Large Scale Structure
• Numerical Galaxy Catalog -I. A Semi-analytic Model of Galaxy Formation with N-body simulations
• The Millennium Run Observatory: First Light
• Modelling SCUBA sources in a Lambda-CDM cosmology: hot starbursts or cold extended galactic dust?
• Galaxy Formation in Preheated Intergalactic Media
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• The evolution of SMBH spin and AGN luminosities for $z<6$ within a semi-analytic model of galaxy formation
• The Luminosity Distribution of Local Group Galaxies
• Mass-to-Light Ratios of 2dF Galaxies
• Central stellar populations of early-type galaxies in low-density environments
• Another thread in the tapestry of stellar feedback: X-ray binaries
• The rest-frame UV luminosity function at $z\simeq 4$: a significant contribution of AGN to the bright-end of the galaxy population
• The Lensed Arc Production Efficiency of Galaxy Clusters: A Comparison of Matched Observed and Simulated Samples
• Tracing the Quenching Journey across Cosmic Time
• Measurement of the bias parameter from weak lensing
• Massive and old quiescent galaxies at high redshift
• Universal Scaling Relations in Scale-Free Structure Formation
• A simple model for AGN feedback in nearby early-type galaxies
• The halo-model description of marked statistics
• The Redshift Evolution of Clustering in the HDF
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Early Starbursts and Magnetic Field Generation in Galaxy Clusters
• Formation of S0 galaxies through mergers. Evolution in the Tully-Fisher relation since $z\sim 1$
• Statistics of Weak Lensing at Small Angular Scales: Analytical Predictions for Lower Order Moments
• Resolution-independent modeling of environmental effects in semi-analytic models of galaxy formation that include ram-pressure stripping of both hot and cold gas
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• Mock Catalogs for the DEEP2 redshift survey
• Chemical enrichment of Damped Lyman Alpha systems as a direct constraint on Population III star formation
• Mass and Light in the Supercluster of galaxies : MS0302+17
• The Properties of Spiral Galaxies: Confronting Hierarchical Galaxy Formation Models with Observations
• The specific star formation rate of high redshift galaxies: the case for two modes of star formation
• Infrared Luminous Lyman Break Galaxies: A Population that Bridges LBGs and SCUBA Galaxies
• Observational tests of the evolution of spheroidal galaxies
• Mass Function of Low Mass Dark Halos
• Substructure and the halo model of large-scale structure
• H alpha emitting galaxies and the star formation rate density at z~0.24
• Overmerging and M/L ratios in phenomenological galaxy formation models
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• High Redshift Galaxy Populations and their Descendants
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• Evolution of the Luminosity Function and Colors of Galaxies in a Lambda-CDM Universe
• Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
• The Observed Evolution of Galaxy Clustering Vs. Epoch-Dependent Biasing Models
• A modified star formation law as a solution to open problems in galaxy evolution
• A simple model linking galaxy and dark matter evolution
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• Star Formation at the Twilight of the Dark Ages: Which Stars Reionized the Universe?
• Galaxy Zoo: The interplay of quenching mechanisms in the group environment
• Simulations of Deep Pencil-Beam Redshift Surveys
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes III: Comparison with Simulations
• Reionization History from Coupled CMB/21cm Line Data
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• On the origin of the angular momentum properties of gas and dark matter in galactic halos and its implications
• The Distribution of Satellite Galaxies in a Lambda-CDM Universe
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• Simulating galaxy Clusters -II: global star formation histories and galaxy populations
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• Measuring the Nonlinear Biasing Function from a Galaxy Redshift Survey
• Probing the cosmic web: inter-cluster filament detection using gravitational lensing
• Multiple Merging Events in the Double Cluster A3128/A3125
• Morphologies of Galaxies in and around a Protocluster at z=2.300
• Survey of Water and Ammonia in Nearby galaxies (SWAN): Resolved Ammonia Thermometry, Water and Methanol Masers in the Nuclear Starburst of NGC 253
• Cosmological Density and Power Spectrum from Peculiar Velocities: Nonlinear Corrections and PCA
• Radio source feedback in galaxy evolution
• Large Scale Structure of the Universe
• Luminosity Density of Galaxies and Cosmic Star Formation Rate from Lambda-CDM Hydrodynamical Simulations
• Warm dark matter and the ionization history of the Universe
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• Large scale motions in superclusters: their imprint in the CMB
• The redshift-space two-point correlation functions of galaxies and groups in the Nearby Optical Galaxy sample
• The DEEP Groth Strip Galaxy Redshift Survey. VIII. The Evolution of Luminous Field Bulges at Redshift z ~ 1
• Gemini and Chandra observations of Abell 586, a relaxed strong-lensing cluster
• The dependence of the pairwise velocity dispersion on galaxy properties
• Discovery of a very extended X-ray halo around a quiescent spiral galaxy - the "missing link" of galaxy formation
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• Brighter galaxy bias: underestimating the velocity dispersions of galaxy clusters
• Probing for Dark Matter within Spiral Galaxy Disks
• The Environment of Active Galaxies in the SDSS-DR4
• Substructure in dark matter halos: Towards a model of the abundance and spatial distribution of subclumps
• Modeling Galaxy Clustering by Color
• The Effect of radiative cooling on the scale-dependence of global stellar and gas contents of groups and clusters of galaxies
• The luminosity dependence of clustering and higher order correlations in the PSCz survey
• Galaxy Clustering and Large-Scale Structure from z = 0.2 to z = 0.5 in Two Norris Redshift Surveys
• The impact of halo shapes on the bispectrum in cosmology
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• On the Continuous Formation of Field Spheroidal Galaxies in Hierarchical Models of Structure Formation
• The Impact of Gas Stripping and Stellar Mass Loss on Satellite Galaxy Evolution
• The Role of Ram Pressure Stripping in the Quenching of Cluster Star Formation
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The pairwise velocity dispersion of galaxies: luminosity dependence and a new test of galaxy formation models
• Completeness in Photometric and Spectroscopic Searches for Clusters
• Galaxy mergers up to z<2.5 I : The star formation properties of merging galaxies at separations 3-15 kpc
• On Recovering the Nonlinear Bias Function from Counts in Cells Measurements
• Power law correlations in galaxy distribution and finite volume effects from the Sloan Digital Sky Survey Data Release Four
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• The bright end of the colour-magnitude relation of cluster galaxies
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• Dust reddening in star-forming galaxies
• Energy, entropy and mass scaling relations for elliptical galaxies. Towards a physical understanding of their photometric properties
• Predicting the Clustering of X-Ray Selected Galaxy Clusters in Flux-Limited Surveys
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Spatial and luminosity distributions of galactic satellites
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• Patchy He II reionization and the physical state of the IGM
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• An Unbiased Measurement of Ho through Cosmic Background Imager Observations of the Sunyaev-Zel'dovich Effect in Nearby Galaxy Clusters
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
• Stellar-to-halo mass relation of cluster galaxies
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Collisional dynamics around binary black holes in galactic centers
• Biased Galaxy Formation And Measurements Of Beta
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• Spatial and Dynamical Biases in Velocity Statistics of Galaxies
• A Parametrized Galaxy Catalog Simulator For Testing Cluster Finding, Mass Estimation and Photometric Redshift Estimation in Optical and Near Infrared Surveys
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
• How covariant is the galaxy luminosity function?
• Understanding the Results of Galaxy-Galaxy Lensing using Galaxy-Mass Correlation in Numerical Simulations
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• The Physical Origin of Galactic Conformity: From Theory to Observation
• On the orbital and internal evolution of cluster galaxies
• Completely dark galaxies: their existence, properties, and strategies for finding them
• Dynamical self-friction: how mass loss slows you down
• A search for distant radio galaxies from SUMSS and NVSS: II. Optical Spectroscopy
• Gas cooling in semi-analytic models and SPH simulations: are results consistent?
• A Tunable Lyot Filter at Prime Focus: a Method for Tracing Supercluster Scales at z ~ 1
• A backwards approach to the formation of disk galaxies I. Stellar and gas content
• WMAP5 and the Cluster Mass Function
• Probing The Gravity Induced Bias with Weak Lensing: Test of Analytical results Against Simulations
• Joint XMM-Newton and Chandra Observations of the NGC 1407/1400 Complex: a Tail of an Early-Type Galaxy and a Tale of a Nearby Merging Group
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Testing the Halo Model Against the SDSS Photometric Survey
• Early Preheating and Galaxy Formation
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Understanding the PSCz Galaxy Power Spectrum with N-body Simulations
• Survey of Water and Ammonia in Nearby galaxies (SWAN): Resolved Ammonia Thermometry, and Water and Methanol Masers in IC 342, NGC 6946 and NGC 2146
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Quantifying the evolution of higher-order clustering
• The correlation function of X-ray galaxy clusters in the RASS1 Bright Sample
• Spectroscopic Confirmation of two Extremely Massive Protoclusters BOSS1244 and BOSS1542 at $z=2.24$
• Lensed arc statistics: comparison of Millennium-simulation galaxy clusters to Hubble Space Telescope observations of an X-ray selected sample
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• GalICS V : Low and high order clustering in mock SDSS's
• Testing the Modified Press-Schechter Model against N-Body Simulations
• Hierarchical build-up of galactic bulges and the merging rate of supermassive binary black holes
• A Unique View of AGN-Driven Molecular Outflows: The Discovery of a Massive Galaxy Counterpart to a $z=2.4$ High-Metallicity Damped Lyman-$\alpha$ Absorber
• The effects of halo alignment and shape on the clustering of galaxies
• 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
• Numerical simulations of buoyancy instabilities in galaxy cluster plasmas with cosmic rays and anisotropic thermal conduction
• The Host Haloes of Lyman Break Galaxies and Sub-millimeter Sources
• The segregation of baryons and dark matter during halo assembly
• Measuring the Distribution of Galaxies Between Halos
• The loss-cone problem in dense nuclei
• Colour Evolution of Disk Galaxy Models from z=4 to z=0
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• Environmental Enhancement of DM Haloes
• 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
• Generating Synthetic Cosmological Data with GalSampler
• Kinematics of the local universe IX. The Perseus-Pisces supercluster and the Tolman-Bondi model
• The mass function and distribution of velocity dispersions for UZC groups of galaxies
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair
• Universal Merger Histories of Dark-Matter Haloes
• Tuning Gravitationally Lensed Standard Sirens
• Dynamical Effect of the Turbulence of IGM on the Baryon Fraction Distribution
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• Topology and Geometry of the CfA2 Redshift Survey
• Ellipticals at $z=0$ from Self-Consistent Hydrodynamical Simulations: Comparison with SDSS Structural and Kinematical Data
• Figure rotation of dark halos in CDM simulations
• Identifying the progenitor set of present-day early-type galaxies: a view from the standard model
• The peculiar velocities of satellites of external disk galaxies
• Luminosity bias: from haloes to galaxies
• The Evolution of K* and the Halo Occupation Distribution since z=1.5: Observations vs. Simulations
• The galaxy correlation function as a constraint on galaxy formation physics
• DSPS: Differentiable Stellar Population Synthesis
• Chemical constraints on the contribution of Population III stars to cosmic reionization
• The Group Evolution Multiwavelength Study (GEMS): The near-infrared luminosity function of nearby galaxy groups
• The descendents of Lyman Break Galaxies in galaxy clusters: spatial distribution and orbital properties
• Higher Order Clustering in the Durham/UKST and Stromlo-APM Galaxy Redshift Surveys
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
• Tracing the Nature of Dark Energy with Galaxy Distribution
• A finer view of the conditional galaxy luminosity function and magnitude-gap statistics
• Stochastic gravitational wave background from cold dark matter halos
• Photometric Properties of the Most Massive High-Redshift Galaxies
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Dynamical flows through Dark Matter Haloes II: one and two points statistics at the virial radius
• Direct-collapse black hole formation induced by internal radiation of host halos
• Luminosity and Stellar Mass Functions of Local Star-Forming Galaxies
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Towards optimal estimation of the galaxy power spectrum
• The contribution of the IGM and minihalos to the 21 cm signal of reionization
• Compact groups in theory and practice - II. Comparing the observed and predicted nature of galaxies in compact groups
• Spin and structural halo properties at high redshift in a LCDM Universe
• Galaxy Correlation Statistics of Mock Catalogs for the DEEP2 Survey
• Mass of clusters in simulations
• Tracing early structure formation with massive starburst galaxies and their implications for reionization
• Statistical properties of dark matter mini-haloes at z >= 15
• The effect of gas-dynamics on semi-analytic modeling of cluster galaxies
• Constraining CMB-consistent primordial voids with cluster evolution
• Estimating the Correlation Length r_0 from the Number of Galaxy Pairs with Similar Redshifts
• Observations of the High Redshift Universe
• Analytic and numerical realisations of a disk galaxy
• The lensing efficiencies of MACS X-ray selected versus RCS optically selected galaxy clusters
• An analytic model for the galactic winds and mass outflows
• Predictions for the FAST telescope's CRAFTS Extra-Galactic HI Survey
• Cosmological Parameters 2000
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• The mass function of the Las Campanas loose groups of galaxies
• Testing galaxy formation models with galaxy stellar mass functions
• On the complexity and the information content of cosmic structures
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• NGC 6240 Supermassive Black Hole Binary dynamical evolution based on Chandra data
• Clusters of galaxies: setting the stage
• Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
• Dynamical consequences of CDM merger trees
• Dipole anisotropies of IRAS galaxies and the contribution of a large-scale local void
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• Feedback Processes in Early-Type Galaxies
• Analysis of the Spatial Distribution of Galaxies by Multiscale Methods
• Consequences of dark matter self-annihilation for galaxy formation
• Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• The redshift evolution of bias and baryonic matter distribution
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
• The dynamic stage of clusters and its influence on the stellar populations of galaxies
• The evolution of galaxy clustering since z=1 from the Calar Alto Deep Imaging Survey
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Dark Matter annihilation energy output and its effects on the high-z IGM
• Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
• A Multivariate Analysis of Galaxies in the Hubble Deep Field North
• Spatially Resolved Spectroscopy of Passive Spiral Galaxies
• An IllustrisTNG View of the Caustic Technique for Galaxy Cluster Mass Estimation
• The galaxy luminosity function around groups
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Evolution of the cosmological mass function in a moving barrier model
• Cosmological constraints from the masses and abundances of L* galaxies
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• The Size Evolution of Elliptical Galaxies
• Radio views of cosmic reionization
• The mass and temperature functions in a moving barrier model
• Leaving the dark ages with AMIGA
• Modelling the dynamical friction timescale of sinking satellite
• High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
• The Distribution of [OII] Equivalent Widths of LCRS Galaxies
• Point field models for the galaxy point pattern. Modelling the singularity of the two-point correlation function
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Photometric and clustering properties of hydrodynamical galaxies in a cosmological volume: results at z=0
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Active Galaxies and Cluster Gas
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• Interpreting the galaxy group CG J1720-67.8 through evolutionary synthesis models
• GABE: Galaxy Assembly with Binary Evolution
• Distortion of Infall Regions in Redshift Space-I
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• VST-GAME: Galaxy Assembly as a function of Mass and Environment with VST. Photometric assessment and density field of MACSJ0416
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• Merging History Trees for Dark Matter Halos: Tests of the Merging Cell Model in a CDM Cosmology
• CG J1720-67.8: A Detailed Analysis of Optical and Infrared Properties of a New Ultracompact Group of Galaxies
• Luminous Matter Distribution, Bulk Flows and Baryon Contents in Cosmological Models with a Local Void
• Do minor interactions trigger star formation in galaxy pairs?
• Semi-Numerical Simulation of Reionization with Semi-Analytical Modeling of Galaxy Formation
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• The impact of the cosmological constant on past and future star formation
• A deep learning approach to halo merger tree construction
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution
• Satellite galaxies in the Illustris-1 simulation: anisotropic locations around relatively isolated hosts
• Reliability of merger tree realizations of dark halos in the Monte-Carlo modeling of galaxy formation
• Simulating Kilonovae in the ΛCDM Universe
• Understanding Galaxy Formation and Evolution
• Alpha Shape Topology of the Cosmic Web
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• Cross-Correlation between Damped Ly-alpha Systems and Ly-break Galaxies in Cosmological SPH Simulations
• The Beylkin-Cramer Summation Rule and A New Fast Algorithm of Cosmic Statistics for Large Data Sets
• Nonlinear Velocity-Density Coupling: Analysis by Second-Order Perturbation Theory
• Modeling the accretion history of supermassive black holes
• Large scale correlations in gas traced by MgII absorbers around low mass galaxies
• Clusters and Groups of Galaxies in the Simulated Local Universe
• What is the optimal way to measure the galaxy power spectrum?
• Scaling of the 1-halo terms with bias
• The Orbital Structure of Dark Matter Halos with Gas
• Building Blocks of the Milky Way's Accreted Spheroid
• Testing Theoretical Models for the Higher-Order Moments of Dark Halo Distribution
• The formation and evolution of field massive galaxies
• Fast radiative transfer of dust reprocessing in semi-analytic models with artificial neural networks
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Building Halo Merger Trees from the Q Continuum Simulation
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• Thermodynamic evolution of the cosmological baryonic gas : II. Galaxy formation
• FLORAH: A generative model for halo assembly histories
• Star formation losses due to tidal debris in `hierarchical' galaxy formation
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Determination of the Linear Mass Power Spectrum From the Mass Function of Galaxy Clusters
• VEGA: Voids idEntification using Genetic Algorithm
• Star formation and chemical evolution of damped Lyman $\alpha$ systems
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Fred Hoyle: Contributions to the Theory of Galaxy Formation
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• Contamination of Cluster Radio Sources in the Measurement of the Thermal Sunyaev-Zel'dovich Angular Power Spectrum
• Evidence for Coupling of Evolved Star Atmospheres and Spiral Arms of the Milky Way
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• The Complexity and Information Content of Simulated Universes
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Angular momentum and morphological sequence of massive galaxies through Dark Sage
• The status of isochrony in the formation and evolution of self-gravitating systems
• Dark Energy Simulations
• Numerical Analyses of Weakly Nonlinear Velocity-Density Coupling
• Sunyaev-Zeldovich Cluster Counts as a Probe of Intra-Supercluster Gas
• Galaxies at the edges: a complete census of MACS J0416.1-2403 cluster
• The non-thermal secondary CMB anisotropies from a cosmic distribution of radio galaxy lobes
• Gaia GraL: Gaia gravitational lens systems IX. Using XGBoost to explore the Gaia Focused Product Release GravLens catalogue
• Two categories of UV-upturn galaxies revealed by semi-analytic models
• Extended Hernquist-Springel formalism for cosmic star formation
• A Halo Merger Tree Generation and Evaluation Framework
• The Cluster of Galaxies Abell 970
• White dwarfs in the building blocks of the Galactic spheroid
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• The spatial clustering of radio sources in NVSS and FIRST; implications for galaxy clustering evolution
• Cosmological constraints from clustering properties of galaxy clusters
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• Achieving Convergence in Galaxy Formation Models by Augmenting N-body Merger Trees
• The hierarchical build-up of bulges in CDM
• Ab Initio Formation of Galaxies, Groups and Large-Scale Structure
• The Nature of Hyperluminous Infrared Galaxies