Mass function of dark matter halos

Abstract

We combine data from a number of N-body simulations to predict the abundance of dark halos in Cold Dark Matter universes over more than 4 orders of magnitude in mass. A comparison of different simulations suggests that the dominant uncertainty in our results is systematic and is smaller than 10--30% at all masses, depending on the halo definition used. In particular, our ``Hubble Volume'' simulations of \tcdm and \lcdm cosmologies allow the abundance of massive clusters to be predicted with uncertainties well below those expected in all currently planned observational surveys. We show that for a range of CDM cosmologies and for a suitable halo definition, the simulated mass function is almost independent of epoch, of cosmological parameters, and of initial power spectrum when expressed in appropriate variables. This universality is of exactly the kind predicted by the familiar Press-Schechter model, although this model predicts a mass function shape which differs from our numerical results, overestimating the abundance of ``typical'' halos and underestimating that of massive systems.

14 pages, 12 figures, Minor changes. Accepted for publication in MNRAS

References in corpus (1)

• Clustering of Galaxy Clusters in CDM Universes

Cited by in corpus (1261)

• The cosmological simulation code GADGET-2
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• The broken hierarchy of galaxy formation
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Halo Models of Large Scale Structure
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• The Aquarius Project: the subhalos of galactic halos
• First results from the IllustrisTNG simulations: matter and galaxy clustering
• Toward a halo mass function for precision cosmology: the limits of universality
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
• Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
• Did LIGO detect dark matter?
• Concentrations of Dark Halos from their Assembly Histories
• Cosmological Parameters from Observations of Galaxy Clusters
• The New Galaxy: Signatures of its Formation
• Halo Formation in Warm Dark Matter Models
• The Mass Function of an X-Ray Flux-Limited Sample of Galaxy Clusters
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• The Inner Structure of LambdaCDM Halos I: A Numerical Convergence Study
• Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
• A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4
• The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
• An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
• Cosmology with the Sunyaev-Zel'dovich Effect
• A Survey of z>5.8 Quasars in the Sloan Digital Sky Survey I: Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z~6
• Challenges for $\Lambda$CDM: An update
• Resolving Cosmic Structure Formation with the Millennium-II Simulation
• What Shapes the Luminosity Function of Galaxies?
• Ahf: Amiga's Halo Finder
• A unified model for AGN feedback in cosmological simulations of structure formation
• Formation of Galaxy Clusters
• Tracing cosmic evolution with clusters of galaxies
• Triaxial Modeling of Halo Density Profiles with High-resolution N-body Simulations
• The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
• The Luminosity and Color Dependence of the Galaxy Correlation Function
• Primordial Black Holes - Perspectives in Gravitational Wave Astronomy -
• Large-Scale Galaxy Bias
• 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal
• Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
• The subhalo populations of LCDM dark haloes
• Transients from Initial Conditions in Cosmological Simulations
• Constraining Galaxy Formation and Cosmology with the Conditional Luminosity Function of Galaxies
• Halo concentrations in the standard LCDM cosmology
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Simulations of Early Structure Formation: Primordial Gas Clouds
• The history of star formation in a LCDM universe
• Precision Determination of the Mass Function of Dark Matter Halos
• A primer on hierarchical galaxy formation: the semi-analytical approach
• The 2dF Galaxy Redshift Survey: The dependence of galaxy clustering on luminosity and spectral type
• Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and Voids
• COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos
• Accurate universal models for the mass accretion histories and concentrations of dark matter halos
• Feedback and Recycled Wind Accretion: Assembling the z=0 Galaxy Mass Function
• Scaling relations for galaxy clusters in the Millennium-XXL simulation
• The Evolution of X-ray Clusters of Galaxies
• Sample Variance Considerations for Cluster Surveys
• Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys
• Cosmological Constraints from the SDSS maxBCG Cluster Catalog
• Efficient Simulations of Early Structure Formation and Reionization
• Gravitational Lensing
• The Sunyaev-Zel'dovich angular power spectrum as a probe of cosmological parameters
• The nature of faint submm-selected galaxies
• Haloes gone MAD: The Halo-Finder Comparison Project
• Simulating cosmic structure formation with the GADGET-4 code
• An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
• Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample
• Dark matter and cosmic structure
• Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue
• A catalog of 132,684 clusters of galaxies identified from Sloan Digital Sky Survey III
• On the Mass-to-Light Ratio of Large Scale Structure
• Clustering of High Redshift ($z\ge 2.9$) Quasars from the Sloan Digital Sky Survey
• Cosmological parameters from lensing power spectrum and bispectrum tomography
• Effects of Baryons and Dissipation on the Matter Power Spectrum
• Galaxy and Mass Assembly (GAMA): The GAMA Galaxy Group Catalogue (G3Cv1)
• Towards a realistic population of simulated galaxy groups and clusters
• Chemical enrichment of the intra-cluster and intergalactic medium in a hierarchical galaxy formation model
• The Growth and Structure of Dark Matter Haloes
• K-band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution and Halo Occupation Number
• The halo mass function from the dark ages through the present day
• Percolation Galaxy Groups and Clusters in the SDSS Redshift Survey: Identification, Catalogs, and the Multiplicity Function
• Testing the Hadronuclear Origin of PeV Neutrinos Observed with IceCube
• Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology
• The Physics of Galaxy Clustering I: A Model for Subhalo Populations
• Galaxy Clusters in Hubble Volume Simulations: Cosmological Constraints from Sky Survey Populations
• Low-Frequency Gravitational Waves from Massive Black Hole Binaries: Predictions for LISA and Pulsar Timing Arrays
• Escape fraction of ionizing photons during reionization: effects due to supernova feedback and runaway OB stars
• The Observed Growth of Massive Galaxy Clusters I: Statistical Methods and Cosmological Constraints
• Velocity and spatial biases in CDM subhalo distributions
• The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0
• The origin and implications of dark matter anisotropic cosmic infall on ~L* haloes
• Evolution of the Galaxy - Dark Matter Connection and the Assembly of Galaxies in Dark Matter Halos
• The evolution of massive black hole seeds
• ELVIS: Exploring the Local Volume in Simulations
• Numerical study of halo concentrations in dark-energy cosmologies
• The realm of the galaxy protoclusters
• New Relationships between Galaxy Properties and Host Halo Mass, and the Role of Feedbacks in Galaxy Formation
• Cosmic Structure Growth and Dark Energy
• Substructures in Cold Dark Matter Haloes
• On Departures From a Power Law in the Galaxy Correlation Function
• The abundance and clustering of dark haloes in the standard Lambda CDM cosmogony
• The Arecibo Legacy Fast ALFA Survey: X. The HI Mass Function and Omega_HI From the 40% ALFALFA Survey
• The C4 Clustering Algorithm: Clusters of Galaxies in the Sloan Digital Sky Survey
• The Universal Mass Accretion History of CDM Haloes
• Formation of z ~ 6 quasars from hierarchical galaxy mergers
• Measuring ${\Omega }_m$ with the ROSAT Deep Cluster Survey
• Generating Dark Matter Halo Merger Trees
• Unusually Large Fluctuations in the Statistics of Galaxy Formation at High Redshift
• Supermassive Black Hole Formation by Direct Collapse: Keeping Protogalactic Gas H_2--Free in Dark Matter Halos with Virial Temperatures T_vir >~ 10^4 K
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Weighing simulated galaxy clusters using lensing and X-ray
• The halo mass function through the cosmic ages
• Towards a Concordant Model of Halo Occupation Statistics
• The X-ray virial relations for relaxed lensing clusters observed with Chandra
• Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures
• A dynamical model for the distribution of dark matter and gas in galaxy clusters
• Detecting the Earliest Galaxies Through Two New Sources of 21cm Fluctuations
• The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
• What is the Highest Plausible Redshift of Luminous Quasars?
• Foreground simulations for the LOFAR - Epoch of Reionization Experiment
• The universality of the virial halo mass function and models for non-universality of other halo definitions
• Revisiting the Cosmic Cooling Crisis
• The History of the Baryon Budget: Cosmic Logistics in a Hierarchical Universe
• Linking Early and Late Type Galaxies to their Dark Matter Haloes
• Gas Physics, Disk Fragmentation, and Bulge Formation in Young Galaxies
• Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces
• Groups of Galaxies in the Two Micron All-Sky Redshift Survey
• Photoionization Feedback in Low--Mass Galaxies at High Redshift
• Galaxies-Intergalactic Medium Interaction Calculation --I. Galaxy formation as a function of large-scale environment
• Non-linear Evolution of f(R) Cosmologies III: Halo Statistics
• Cosmological Constraints from Sunyaev-Zel'dovich-Selected Clusters with X-ray Observations in the First 178 Square Degrees of the South Pole Telescope Survey
• Too Big to Fail in the Local Group
• 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 velocity dispersion function of early-type galaxies
• The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
• Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology
• The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
• The mass function
• Catalog Extraction in SZ Cluster Surveys: a matched filter approach
• An analytical model for the history of cosmic star formation
• Lensing and X-ray mass estimates of clusters (SIMULATION)
• Fossil HII Regions: Self-Limiting Star Formation at High Redshift
• The Halo Mass Function: High-Redshift Evolution and Universality
• The Reionization History at High Redshifts I: Physical Models and New Constraints from CMB Polarization
• PINOCCHIO: pinpointing orbit-crossing collapsed hierarchical objects in a linear density field
• Evolution of the Mass Function of Dark Matter Haloes
• Redshifting Rings of Power
• Constraints on Omega_m, Omega_L, and Sigma_8, from Galaxy Cluster Redshift Distributions
• Planck Early Results XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
• Self Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum and Mass Measurements
• Correlation of CMB with large-scale structure: II. Weak lensing
• Hydrodynamical N-body simulations of coupled dark energy cosmologies
• On the Cluster Physics of Sunyaev-Zel'dovich Surveys II: Deconstructing the Thermal SZ Power Spectrum
• Halo Occupation Distribution Modeling of Clustering of Luminous Red Galaxies
• The DEEP2 Galaxy Redshift Survey: Evolution of the Color-Density Relation at 0.4 < z < 1.35
• Simulations of the Microwave Sky
• Hubble expansion & Structure Formation in Time Varying Vacuum Models
• Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution
• Probing Primordial Non-Gaussianity with Large-Scale Structure
• Halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditions
• Baryonic acoustic oscillations in simulated galaxy redshift surveys
• The Cut & Enhance method : selecting clusters of galaxies from the SDSS commissioning data
• Hydrodynamical simulations of cluster formation with central AGN heating
• Moving mesh cosmology: numerical techniques and global statistics
• The structure of voids
• Virial masses of galactic halos from galaxy-galaxy lensing: theoretical modeling and application to SDSS
• PTHalos: A fast method for generating mock galaxy distributions
• Properties of Galaxy Groups in the SDSS: II.- AGN Feedback and Star Formation Truncation
• The Evolution of Galaxy Number Density at z < 8 and its Implications
• Simulating the Universe with MICE: The abundance of massive clusters
• Cosmology with the shear-peak statistics
• Mass Function Predictions Beyond LCDM
• The Mass-To-Light Function of Virialized Systems and the Relationship Between Their Optical and X-ray Properties
• Red Galaxy Growth and the Halo Occupation Distribution
• Inside-out or Outside-in: The topology of reionization in the photon-starved regime suggested by Lyman-alpha forest data
• Measurement of Galaxy Cluster Sizes, Radial Profiles, and Luminosity Functions from SDSS Photometric Data
• Calibrating the Nonlinear Matter Power Spectrum: Requirements for Future Weak Lensing Surveys
• N-body Dark Matter Haloes with simple Hierarchical Histories
• Large scale bias and stochasticity of halos and dark matter
• Power spectrum normalization from the local abundance of rich clusters of galaxies
• Measurements of Secondary Cosmic Microwave Background Anisotropies with the South Pole Telescope
• Optical and X-ray clusters as tracers of the supercluster-void network. I Superclusters of Abell and X-ray clusters
• The impact of galaxy formation on the total mass, mass profile and abundance of haloes
• The MultiDark Database: Release of the Bolshoi and MultiDark Cosmological Simulations
• Self-similar scaling and evolution in the galaxy cluster X-ray Luminosity-Temperature relation
• SDSS galaxy bias from halo mass-bias relation and its cosmological implications
• Constraints on Warm Dark Matter from Cosmological Reionization
• The XMM-LSS survey: the Class 1 cluster sample over the initial 5 square degrees and its cosmological modelling
• Physical Implications of the X-ray Properties of Galaxy Groups and Clusters
• The REFLEX Galaxy Cluster Survey VII: Omega_m and sigma_8 from cluster abundance and large-scale clustering
• Analytic models of plausible gravitational lens potentials
• Cosmological constraints from the local X-ray luminosity function of the most X-ray luminous galaxy clusters
• Large-scale dark matter simulations
• Halo Model at Its Best: Constraints on Conditional Luminosity Functions from Measured Galaxy Statistics
• Constraining primordial non-Gaussianity with future galaxy surveys
• New constraints on dark energy from the observed growth of the most X-ray luminous galaxy clusters
• Searching for massive clusters in weak lensing surveys
• Assembly History and Structure of Galactic Cold Dark Matter Halos
• Voids in a $\Lambda$CDM Universe
• Fast Large Volume Simulations of the 21 cm Signal from the Reionization and pre-Reionization Epochs
• The overdensity and masses of the friends-of-friends halos and universality of the halo mass function
• Gravitational probes of dark matter physics
• Galaxy clusters identified from the SDSS DR6 and their properties
• N-body simulations for coupled dark energy: halo mass function and density profiles
• Large-scale non-Gaussian mass function and halo bias: tests on N-body simulations
• Three-Point Correlations in Weak Lensing Surveys: Model Predictions and Applications
• The Kinetic Sunyaev-Zel'dovich Effect from Reionization
• Constraining the WDM Particle Mass with Milky Way Satellites
• The X-Ray Luminosity--Mass Relation for Local Clusters of Galaxies
• The growth of dark matter halos: evidence for significant smooth accretion
• The X-ray Cluster Normalization of the Matter Power Spectrum
• Galaxy Halo Occupation at High Redshift
• On the origin of the galaxy luminosity function
• Improved Cosmological Constraints from Gravitational Lens Statistics
• Galaxy Groups: A 2MASS Catalog
• Separating the Early Universe from the Late Universe: cosmological parameter estimation beyond the black box
• Constraints from Gravitational Recoil on the Growth of Supermassive Black Holes at High Redshift
• Microwave Background Constraints on Mixing of Photons with Hidden Photons
• Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
• Cosmic Evolution of Size and Velocity Dispersion for Early Type Galaxies
• On determining the cluster abundance normalization
• Structure formation from non-Gaussian initial conditions: multivariate biasing, statistics, and comparison with N-body simulations
• The Cluster Mass Function from Early SDSS Data: Cosmological Implications
• Importance of Cluster Structural Evolution in Using X-ray and SZE Galaxy Cluster Surveys to Study Dark Energy
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters
• Cluster Alignments and Ellipticities in LCDM Cosmology
• An Optical Catalog of Galaxy Clusters Obtained from an Adaptive Matched Filter Finder Applied to SDSS DR6
• Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters
• The Extraordinary Amount of Substructure in the Hubble Frontier Fields Cluster Abell 2744
• The Evolution of Primordial Black Holes and their Final Observable Spins
• Towards Cosmological Concordance on Galactic Scales
• The COpernicus COmplexio: Statistical Properties of Warm Dark Matter Haloes
• Constraining cosmological parameters using Sunyaev-Zel'dovich cluster surveys
• NIHAO XV: The environmental impact of the host galaxy on galactic satellite and field dwarf galaxies
• Galaxy-galaxy Lensing: Dissipationless Simulations Versus the Halo Model
• Outskirts of Galaxy Clusters
• On the Origin of Stars in Bulges and Elliptical Galaxies
• The evolution of the galaxy distribution
• Cosmological structure formation in a homogeneous dark energy background
• Keck Deep Fields. II. The UV Galaxy Luminosity Function at z~4, 3, and 2
• On the Incidence and Kinematics of Strong Mg II Absorbers
• Probing Cosmology with Weak Lensing Peak Counts
• An accurate tool for the fast generation of dark matter halo catalogs
• Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
• Environmental Dependence of Dark Matter Halo Growth I: Halo Merger Rates
• An overdensity of galaxies at z=5.9 +/-0.2 in the Ultra Deep Field confirmed using the ACS grism
• Self-Calibration of Cluster Dark Energy Studies: Counts in Cells
• The dark matter halos of dwarf galaxies: a challenge for the LCDM paradigm?
• The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys
• Cosmological Constraints from the Red-Sequence Cluster Survey
• The nature of the Diffuse Gamma-Ray Background
• Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
• The Formation of a Disk Galaxy within a Growing Dark Halo
• Sensitivity Projections for Dark Matter Searches with the Fermi Large Area Telescope
• Characteristic Scales During Reionization
• Antitruncated Stellar Disks via Minor Mergers
• The halo merger rate in the Millennium Simulation and implications for observed galaxy merger fractions
• The Cosmic Code Comparison Project
• The Aemulus Project II: Emulating the Halo Mass Function
• Cross-correlation Weak Lensing of SDSS Galaxy Clusters I: Measurements
• Evolution of the cluster X-ray scaling relations since z>0.4
• (Mis-)Interpreting supernovae observations in a lumpy universe
• Cosmic Rays Above the Second Knee from Clusters of Galaxies and Associated High-Energy Neutrino Emission
• The environment of bright QSOs at z ~ 6: Star forming galaxies and X-ray emission
• Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter
• Dark Matter Annihilation in Substructures Revised
• Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics
• The first generation of stars in LCDM cosmology
• Halo Profiles and the Concentration-Mass Relation for a ΛCDM Universe
• Simultaneous Falsification of LCDM and Quintessence with Massive, Distant Clusters
• Scaling Relations and Overabundance of Massive Clusters at z>~1 from Weak-Lensing Studies with HST
• Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays
• Giant Arc Statistics In Concordance With A Concordance LCDM Universe
• Cosmic shear statistics in the Suprime-Cam 2.1 sq deg field: Constraints on Omega_m and sigma_8
• The Effect of Merger Boosts on the Luminosity, Temperature, and Inferred Mass Functions of Clusters of Galaxies
• Properties of cluster satellites in hydrodynamical simulations
• The FLAMINGOS Extragalactic Survey
• Time dependent couplings in the dark sector: from background evolution to nonlinear structure formation
• X-ray Temperatures for the EMSS High Redshift Cluster Sample: Constraints on Cosmology and the Dark Energy Equation of State
• The Next Generation Fornax Survey (NGFS): II. The Central Dwarf Galaxy Population
• The redshift evolution of massive galaxy clusters in the MACSIS simulations
• Cluster Galaxy Dynamics and the Effects of Large Scale Environment
• The 21 cm Forest: Radio Absorption Spectra as Probes of Minihalos Before Reionization
• Galaxy formation using halo merger histories taken from N-body simulations
• The Halo Mass Function from Excursion Set Theory. II. The Diffusing Barrier
• The Dark Universe
• Hubble Space Telescope Weak-lensing Study of the Galaxy Cluster XMMU J2235.3-2557 at z=1.4: A Surprisingly Massive Galaxy Cluster when the Universe is One-third of its Current Age
• Constraining Primordial Magnetism
• The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes
• The Rise of the First Stars: Supersonic Streaming, Radiative Feedback, and 21-cm Cosmology
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• Observations and Theoretical Implications of the Large Separation Lensed Quasar SDSS J1004+4112
• The Mean and Scatter of the Velocity Dispersion-Optical Richness Relation for maxBCG Galaxy Clusters
• Simulating nonlinear cosmological structure formation with massive neutrinos
• Simulating the physical properties of dark matter and gas inside the cosmic web
• Early structure in LCDM
• Clustering of obscured and unobscured quasars in the Bootes field: Placing rapidly growing black holes in the cosmic web
• The Cluster Mass Function from Weak Gravitational Lensing
• The Formation of the First Stars in the Universe
• Simulations of cosmic ray feedback by AGN in galaxy clusters
• Observational Constraints on General Relativistic Energy Conditions, Cosmic Matter Density and Dark Energy from X-Ray Clusters of Galaxies and Type-Ia Supernovae
• The metal enrichment of the intracluster medium in hierarchical galaxy formation models
• Small-Angle CMB Temperature Anisotropies Induced by Cosmic Strings
• MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an Extremely Massive Overdensity BOSS1441 at $z=2.32$
• Cluster Density Profiles as a Test of Modified Gravity
• The effects of baryons on the halo mass function
• Global Probes of the Impact of Baryons on Dark Matter Halos
• The effect of radiative cooling on scaling laws of X-ray groups and clusters
• Tidal stripping and the structure of dwarf galaxies in the Local Group
• Cluster abundance normalization from observed mass-temperature relation
• The Imprint of Warm Dark Matter on the Cosmological 21-cm Signal
• The Atacama Cosmology Telescope: Dynamical Masses and Scaling Relations for a Sample of Massive Sunyaev-Zel'dovich Effect Selected Galaxy Clusters
• Mass Accretion and its Effects on the Self-Similarity of Gas Profiles in the Outskirts of Galaxy Clusters
• Constraining dark energy with Sunyaev-Zel'dovich cluster surveys
• Tests for primordial non-Gaussianity
• Redshift-Space Distortions with the Halo Occupation Distribution II: Analytic Model
• Nonlinear Stochastic Biasing of Galaxies and Dark Halos in Cosmological Hydrodynamic Simulations
• Hubble expansion and structure formation in the "running FLRW model" of the cosmic evolution
• Precision cosmology defeats void models for acceleration
• Predicting the cosmological constant with the scale-factor cutoff measure
• Semi-Analytical Models for Lensing by Dark Halos: I. Splitting Angles
• The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $\Lambda$CDM
• The accretion history of dark matter halos II: The connections with the mass power spectrum and the density profile
• Templates for the Sunyaev-Zel'dovich Angular Power Spectrum
• Clusters of galaxies in the local universe
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?
• Dark Energy from the Thermal Sunyaev Zeldovich Power Spectrum
• On the radiative efficiencies, Eddington ratios, and duty cycles of luminous high-redshift quasars
• The stellar-to-halo mass relation for Local Group galaxies
• The effect of AGN feedback on the halo mass function
• The L_X--M relation of Clusters of Galaxies
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• Future Galaxy Cluster Surveys: The Effect of Theory Uncertainty on Constraining Cosmological Parameters
• Interpreting the Observed Clustering of Red Galaxies at z~3
• The Outer Rim Simulation: A Path to Many-Core Supercomputers
• The formation of compact massive self-gravitating discs in metal-free haloes with virial temperatures of ~ 13000-30000 K
• The Halo Distribution of 2dF Galaxies
• Neutrino physics from precision cosmology
• Collapse Barriers and Halo Abundance: Testing the Excursion Set Ansatz
• Simulating the Formation of the Local Galaxy Population
• Cosmological Information in Weak Lensing Peaks
• Star Formation and AGN Activity in Galaxy Clusters from $z=1-2$: a Multi-wavelength Analysis Featuring $Herschel$/PACS
• Constraining the Matter Power Spectrum Normalization using the SDSS/RASS and REFLEX Cluster surveys
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• Shear Selected Cluster Cosmology I: Tomography and Optimal Filtering
• Nonlinear clustering during the cosmic Dark Ages and its effect on the 21-cm background from minihalos
• Galaxy Voids in Cold Dark Matter Universes
• Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
• The Effects of Photoionization on Galaxy Formation -- III: Environmental Dependence in the Luminosity Function
• On The Assembly History of Dark Matter Haloes
• Galaxy Halo Masses from Galaxy-Galaxy Lensing
• The Evidence of Absence: Galaxy Voids in the Excursion Set Formalism
• Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors
• Dark energy and the evolution of spherical overdensities
• The universal nature of subhalo accretion
• JKCS041: a colour-detected galaxy cluster at z_phot=1.9 with deep potential well as confirmed by X-ray data
• Propagation of ultrahigh energy nuclei in clusters of galaxies: resulting composition and secondary emissions
• Metal Absorption Lines as Probes of the Intergalactic Medium Prior to the Reionization Epoch
• Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties
• Was Star-Formation Suppressed in High-Redshift Minihalos?
• The Abundance and Radial Distribution of Satellite Galaxies
• The imprints of local superclusters on the Sunyaev-Zel'dovich signals and their detectability with Planck
• An optimal filter for the detection of galaxy clusters through weak lensing
• Simulations of galaxy formation in a cosmological volume
• Self-Consistency and Calibration of Cluster Number Count Surveys for Dark Energy
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time
• Supermassive Black Holes in the Hierarchical Universe: A General Framework and Observational Tests
• The Accuracy of Subhalo Detection
• Predicting the number, spatial distribution and merging history of dark matter haloes
• Dependence of Halo Properties on Interaction History, Environment and Cosmology
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• A generalized local ansatz and its effect on halo bias
• Cosmological Origin of the Stellar Velocity Dispersions in Massive Early-Type Galaxies
• The thermal Sunyaev Zel'dovich effect power spectrum in light of Planck
• The Role of the Dust in Primeval Galaxies: A Simple Physical Model for Lyman Break Galaxies and Lyman Alpha Emitters
• Effects of asphericity and substructure on the determination of cluster mass with weak gravitational lensing
• A Subaru Weak Lensing Survey I: Cluster Candidates and Spectroscopic Verification
• Imprint of Intergalactic Shocks on the Radio Sky
• The First Stars in The Universe
• The Reionization History at High Redshifts II: Estimating the Optical Depth to Thomson Scattering from CMB Polarization
• SCORCH I: The Galaxy-Halo Connection in the First Billion Years
• The Structure of Halos: Implications for Group and Cluster Cosmology
• A simple model to link the properties of quasars to the properties of dark matter halos out to high redshift
• Hydrodynamic Simulation of the Cosmological X-ray Background
• Halo-model signatures from 380,000 SDSS Luminous Red Galaxies with photometric redshifts
• The New Horizon Run Cosmological N-Body Simulations
• Early Formation and Late Merging of the Giant Galaxies
• Three-Dimensional Identification and Reconstruction of Galaxy Systems within Deep Redshift Surveys
• The Ultimate Halo Mass in a LCDM Universe
• The MillenniumTNG Project: The galaxy population at $z\ge 8$
• GOTPM: A Parallel Hybrid Particle-Mesh Treecode
• Closing the Loop: A Self-Consistent Model of Optical, X-ray, and SZ Scaling Relations for Clusters of Galaxies
• Modeling halo mass functions in chameleon f(R) gravity
• On the use of semi-numerical simulations in predicting the 21-cm signal from the epoch of reionization
• The importance of dry and wet merging on the formation and evolution of elliptical galaxies
• The Formation of the First Massive Black Holes
• Secondary anisotropies of the CMB
• Redshift-Space Distortions with the Halo Occupation Distribution I: Numerical Simulations
• The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group
• The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos
• Reasoning From Fossils: Learning From the Local Black Hole Population About the Evolution of Quasars
• The early-type dwarf galaxy population of the Hydra I cluster
• Dark Energy Constraints from Galaxy Cluster Peculiar Velocities
• \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities
• Weighing Neutrinos with Galaxy Cluster Surveys
• Effects of Triaxiality on the Statistics of Large-Separation Gravitational Lenses
• Dark matter-radiation interactions: the impact on dark matter haloes
• Properties of host haloes of Lyman-break galaxies and Lyman-alpha Emitters from their number densities and angular clustering
• Searching for dark matter halos in the Suprime-Cam 2 sq deg field
• Testing Sunyaev-Zel'dovich measurements of the hot gas content of dark matter haloes using synthetic skies
• Gemini/GMOS Spectroscopy of 26 Strong Lensing Selected Galaxy Cluster Cores
• What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses
• Constraining amplitude and slope of the mass fluctuation spectrum using cluster baryon mass function
• Physical viscosity in smoothed particle hydrodynamics simulations of galaxy clusters
• Binary Aggregations in Hierarchical Galaxy Formation: The Evolution of the Galaxy Luminosity Function
• Dark Sky Simulations: Early Data Release
• The Masses, Ancestors and Descendents of Extremely Red Objects: Constraints from Spatial Clustering
• Large scale bias and the inaccuracy of the peak-background split
• Electromagnetic counterparts of supermassive black hole binaries resolved by pulsar timing arrays
• N-body simulations with generic non-Gaussian initial conditions I: Power Spectrum and halo mass function
• Dark Matter Halos of Disk Galaxies: Constraints from the Tully-Fisher Relation
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• HeII Recombination Lines From the First Luminous Objects
• The Effect of Gas Physics on the Halo Mass Function
• An analytic model for the bispectrum of galaxies in redshift space
• Cosmological constraints from evolution of cluster baryon mass function at z~0.5
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• The Build-Up of the Hubble Sequence in the COSMOS Field
• High-Redshift Galaxies from Early JWST Observations: Constraints on Dark Energy Models
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• The Spatial Clustering of ROSAT All-Sky Survey AGNs II. Halo Occupation Distribution Modeling of the Cross Correlation Function
• CosmoBolognaLib: C++ libraries for cosmological calculations
• Early Structure Formation and Reionization in a Cosmological Model with a Running Primordial Power Spectrum
• A Model for Multi-property Galaxy Cluster Statistics
• The Epoch of Reionization in Models with Reduced Small Scale Power
• Modeling Intra-Cluster Gas in Triaxial Dark Halos : An Analytical Approach
• The imprint of inhomogeneous HeII reionization on the HI and HeII Ly-alpha forest
• Self-Consistent Theory of Halo Mergers
• The integrated Sachs-Wolfe Effect -- Large Scale Structure Correlation
• The Halo Occupation Distribution of SDSS Quasars
• Large-Scale Structure in Brane-Induced Gravity II. Numerical Simulations
• Cosmology from the Thermal Sunyaev-Zel'dovich Power Spectrum: Primordial non-Gaussianity and Massive Neutrinos
• Large-Scale Structure Shocks at Low and High Redshifts
• Probing dark energy with baryonic oscillations and future radio surveys of neutral Hydrogen
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• Galactic Archaeology with Gaia
• The statistical properties of LCDM halo formation
• Non-linear evolution of the cosmic neutrino background
• The DEEP2 Galaxy Redshift Survey: Clustering Dependence on Galaxy Stellar Mass and Star Formation Rate at z~1
• Chameleon f(R) gravity in the virialized cluster
• The merger history of clusters and its effect on the X-ray properties of the intracluster medium
• A Comparison of Gas Dynamics in SPH and Semi-analytic Models of Galaxy Formation
• Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
• LoCuSS: Hydrostatic Mass Measurements of the High-$L_X$ Cluster Sample -- Cross-calibration of Chandra and XMM-Newton
• The Anisotropic Distribution of Satellite Galaxies
• A simulation pipeline for the Planck mission
• Spherical collapse and halo mass function in f(R) theories
• The impact of Early Dark Energy on non-linear structure formation
• The early-type dwarf galaxy population of the Centaurus cluster
• A new model to predict weak-lensing peak counts II. Parameter constraint strategies
• Effective Screening due to Minihalos During the Epoch of Reionization
• The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys
• A new model to predict weak-lensing peak counts I. Comparison with $N$-body Simulations
• The Non-Gaussian Halo Mass Function with fNL, gNL and tauNL
• The 21cm Signature of the First Stars
• Strong Gravitational Lensing and Dark Energy
• A Lyman-α protocluster at redshift 6.9
• UV Radiative Feedback on High-Redshift Proto-Galaxies
• Shapes of clusters and groups of galaxies: Comparison of model predictions with observations
• The nature of dark matter from the global high redshift HI 21 cm signal
• Mass functions in coupled Dark Energy models
• A Model For Infall Around Virialized Halos
• Galaxy Groups in the 2dFGRS: the number density of groups
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Dark matter halo abundances, clustering and assembly histories at high redshift
• The First Generation of Star-Forming Haloes
• The abundance of dark galaxies
• Do Distinct Cosmological Models Predict Degenerate Halo Populations?
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• The halo model for cosmology: a pedagogical review
• Searching for galaxy clusters using the aperture mass statistics in 50 VLT fields
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• Focusing on Warm Dark Matter with Lensed High-redshift Galaxies
• On the Self-Similar Appearance of Galaxy Clusters in X-rays
• On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion
• Unveiling the three-dimensional structure of galaxy clusters: resolving the discrepancy between X-ray and lensing masses
• Hierarchical Formation of Galaxies with Dynamical Response to Supernova-Induced Gas removal
• The 2dF Galaxy Redshift Survey: The clustering of galaxy groups
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Machine learning cosmological structure formation
• Halo modelling in chameleon theories
• Constraining halo occupation properties of X-ray AGNs using clustering of Chandra sources in the Bootes survey region
• Universal at last? The splashback mass function of dark matter halos
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Semi-analytic Simulations of Galactic Winds: Volume Filling Factor, Ejection of Metals and Parameter Study
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• Primordial non-Gaussianity from the covariance of galaxy cluster counts
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• A Lightcone Catalogue from the Millennium-XXL Simulation
• The scatter and evolution of the global hot gas properties of simulated galaxy cluster populations
• The Virial Mass Function of Nearby SDSS Galaxy Clusters
• Dwarf Dark Matter Halos
• Modelling Void Abundance in Modified Gravity
• Gravitational Waves from the First Stars
• Six More Ultra-Faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
• The early-type dwarf galaxy population of the Fornax cluster
• Cosmic Neutron Star Merger Rate and Gravitational Waves constrained by the R Process Nucleosynthesis
• Proto-groups at 1.8<z<3 in the zCOSMOS-deep sample
• Numerical Galaxy Catalog -I. A Semi-analytic Model of Galaxy Formation with N-body simulations
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Precision cosmology with a wide area XMM cluster survey
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• Studying the Lyman-$\alpha$ optical depth fluctuations at $z\sim 5.5$ using fast semi-numerical methods
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• The imprint of the interaction between dark sectors in galaxy clusters
• Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
• Detection and extraction of signals from the epoch of reionization using higher order one-point statistics
• Accurate and Efficient Halo-based Galaxy Clustering Modelling with Simulations
• The potential of X-ray cluster surveys to constrain primordial non-Gaussianity
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• Searching for diffuse light in the M96 Group
• Hierarchical Growth and Cosmic Star Formation: Enrichment, Outflows and Supernova Rates
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• Toward an accurate mass function for precision cosmology
• Future Evolution of Bound Superclusters in an Accelerating Universe
• Implications of multiple high-redshift galaxy clusters
• The phase-space distribution of infalling dark matter subhalos
• Observing simulated galaxy clusters with PHOX: a novel X-ray photon simulator
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy Studies
• The XMM--NEWTON Omega Project: I. The X-ray Luminosity - Temperature Relation at z>0.4
• A Snapshot Survey for Gravitational Lenses Among z>=4.0 Quasars: I. The z>5.7 Sample
• BLOX: The Bonn Lensing, Optical, and X-ray selected galaxy clusters -- I. Cluster catalog construction
• Dissipationless Merging and the Assembly of Central Galaxies
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Non-Gaussian halo assembly bias
• Distinguishing models of reionization using future radio observations of 21-cm 1-point statistics
• A simluated TCDM cosmology cluster catalogue: the NFW profile and the temperature-mass scaling relations
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• Combined analysis of weak lensing and X-ray blind surveys
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Deriving an Accurate Formula of Scale-dependent Bias with Primordial Non-Gaussianity: An Application of the Integrated Perturbation Theory
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• A New Halo Finding Method for N-Body Simulations
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Star formation in galaxies along the Pisces-Cetus Supercluster filaments
• Star formation in galaxies falling into clusters along supercluster-scale filaments
• An Analytical Approach to Inhomogeneous Structure Formation
• Modeling the Counts of Faint Radio Loud Quasars: Constraints on the Supermassive Black Hole Population and Predictions for High Redshift
• The Radio Luminosity Function of Cluster Radio Halos
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• Sharpening the Precision of the Sunyaev-Zel'dovich Power Spectrum
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Accurate Modeling of Weak Lensing with the sGL Method
• Accurate mass and velocity functions of dark matter halos
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• Imprints of the Early Universe on Axion Dark Matter Substructure
• Group finding in the stellar halo using M-giants in 2MASS: An extended view of the Pisces Overdensity?
• How well do cosmological simulations reproduce individual-halo properties?
• Modelling the post-reionization neutral Hydrogen (\HI) bias
• An XMM-Newton observation of the massive, relaxed galaxy cluster ClJ1226.9+3332 at z=0.89
• Unveiling the Dynamics of the Universe
• High redshift quasars and the supermassive black hole mass budget: constraints on quasar formation models
• Bayesian joint analysis of cluster weak lensing and Sunyaev-Zel'dovich effect data
• The role of HD cooling in primordial star formation
• Constraints on the small-scale power spectrum of density fluctuations from high-redshift gamma-ray bursts
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• TheHaloMod: An online calculator for the halo model
• Constraining primordial magnetic fields through large scale structure
• The discovery of a massive supercluster at z=0.9 in the UKIDSS DXS
• Capturing Halos at High Redshifts
• Cosmological Constraints from Galaxy Cluster Velocity Statistics
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Red Galaxy Clustering in the NOAO Deep Wide-Field Survey
• An Effective Model for the Cosmic-Dawn 21-cm Signal
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• Gravitational Lensing Statistics in Universes Dominated by Dark Energy
• The Mass Function of Void Galaxies in the SDSS Data Release 2
• High-redshift JWST Observations and Primordial Non-Gaussianity
• Unveiling the composition of radio plasma bubbles in galaxy clusters with the Sunyaev-Zel'dovich effect
• Imprints of mass accretion on properties of galaxy clusters
• How well do we know the Halo Mass Function?
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• The impact of spin temperature fluctuations on the 21-cm moments
• Cosmological constraints with weak lensing peak counts and second-order statistics in a large-field survey
• Mass Function of Low Mass Dark Halos
• Impact of baryons on the cluster mass function and cosmological parameter determination
• A blind HI survey in the Canes Venatici region
• Light-cone anisotropy in 21cm fluctuations during the epoch of reionization
• Probing the Core Structure of Dark Halos with Tangential and Radial Arc Statistics
• Circular velocity profiles of dark matter haloes
• Dark energy constraints from lensing-detected galaxy clusters
• Mass-temperature relation of galaxy clusters: implications from the observed luminosity-temperature relation and X-ray temperature function
• The strongest gravitational lenses: I. The statistical impact of cluster mergers
• The XMM--NEWTON Omega Project: II.Cosmological implications from the high redshift L-T relation of X-ray clusters
• Measuring Sigma8 with Cluster Lensing : Biases from Unrelaxed Clusters
• Reviewing the frequency and central depletion of Ultra-Diffuse Galaxies in galaxy clusters from the KIWICS survey
• The nonlinear matter power spectrum
• What is the best way to measure baryonic acoustic oscillations?
• Coupled Quintessence and the Halo Mass Function
• Mass Function of Rich Galaxy Clusters and Its Constraint on sigma_8
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• Bayesian modelling of clusters of galaxies from multi-frequency pointed Sunyaev--Zel'dovich observations
• Population III Generated Cosmic Rays and the Production of Li6
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• The journey of QSO haloes from z=6 to the present
• Integrated Sachs Wolfe Effect and Rees Sciama Effect
• Richness-mass relation self-calibration for galaxy clusters
• Monolithic or hierarchical star formation? A new statistical analysis
• Sensitivity of galaxy cluster dark energy constraints to halo modeling uncertainties
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Constraining warm dark matter with cosmic shear power spectra
• High-Redshift Galaxies in Cold Dark Matter Models
• Local stochastic non-Gaussianity and N-body simulations
• HI content and other structural properties of galaxies in the Virgo cluster from the Arecibo Legacy Fast ALFA Survey
• Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe
• The Accelerated Build-up of the Red Sequence in High Redshift Galaxy Clusters
• Nature of Lyman Alpha Blobs: Powered by Extreme Starbursts
• Redshift Accuracy Requirements for Future Supernova and Number Count Surveys
• Exploring the liminality: properties of haloes and subhaloes in borderline $f(R)$ gravity
• Cosmological and Astrophysical Implications of the Sunyaev-Zel'dovich Effect
• Can large-scale structure probe CMB-constrained non-Gaussianity?
• The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population
• On the Nonspherical Nature of Halo Formation
• X-Ray Evolution of Active Galactic Nuclei and Hierarchical Galaxy Formation
• A high precision semi-analytic mass function
• Likelihood Methods for Cluster Dark Energy Surveys
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function
• An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters
• Constraining the Redshift z=6 Quasar Luminosity Function Using Gravitational Lensing
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• Evolution of the Cluster Mass Function: Gpc^3 Dark Matter Simulations
• The Line-of-Sight Proximity Effect and the Mass of Quasar Host Halos
• Weak-Lensing Halo Numbers and Dark-Matter Profiles
• Constraining large scale HI bias using redshifted 21-cm signal from the post-reionization epoch
• Testing anthropic predictions for Lambda and the CMB temperature
• Non-universality of the mass function: dependence on the growth rate and power spectrum shape
• Excursion Set Theory for generic moving barriers and non-Gaussian initial conditions
• Galaxy Clusters as Reservoirs of Heavy Dark Matter and High-Energy Cosmic Rays: Constraints from Neutrino Observations
• Higher-order moments of the lensing shear and other spin two fields
• Accurate Weak Lensing of Standard Candles. II. Measuring sigma8 with Supernovae
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• Can Early Dark Energy be Detected in Non-Linear Structure?
• Weak Lensing as a Calibrator of the Cluster Mass-Temperature Relation
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• Radio source feedback in galaxy evolution
• Strong lensing statistics and the power spectrum normalisation
• Warm dark matter and the ionization history of the Universe
• Cluster mass functions in the quintessential Universe
• Primordial non-Gaussianity and Dark Energy constraints from Cluster Surveys
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Microwave-Sky Simulations and Projections for Galaxy Cluster Detection with the Atacama Cosmology Telescope
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: II. Foreground components and optimised filtering schemes
• Statistical and systematic errors in redshift-space distortion measurements from large surveys
• A low-scatter survey-based mass proxy for clusters of galaxies
• Nonlinear Bias of Cosmological Halo Formation in the Early Universe
• Halo abundances within the cosmic web
• The Sunyaev-Zeldovich Background
• Galaxy groups in the 2dF galaxy redshift survey: Luminosity and Mass Statistics
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Powellsnakes II: a fast Bayesian approach to discrete object detection in multi-frequency astronomical data sets
• Minimum size of 21-cm simulations
• The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
• The halo mass function in interacting Dark Energy models
• Substructure in dark matter halos: Towards a model of the abundance and spatial distribution of subclumps
• Decaying Cold Dark Matter and the Evolution of the Cluster Abundance
• Effects of the initial conditions on cosmological $N$-body simulations
• Reliability of the dark matter clustering in cosmological N-body simulation on scales below the mean separation length of particles
• Cross-Calibration of Cluster Mass-Observables
• Supermassive Black Hole Formation at High Redshifts Through a Primordial Magnetic Field
• Relativistic numerical cosmology with Silent Universes
• Most massive halos with Gumbel Statistics
• The Emergence of the First Star-free Atomic Cooling Haloes in the Universe
• Towards a general parametrization of the warm dark matter halo mass function
• Are Clusters Standard Candles? Galaxy Cluster Scaling Relations With the Sunyaev-Zeldovich Effect
• The REFLEX II galaxy cluster survey: power spectrum analysis
• A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
• Testing cold dark matter with the low mass Tully-Fisher relation
• Statistics of Sunyaev-Zel'dovich Cluster Surveys
• GMOS Spectroscopy of SCUBA Galaxies Behind A851
• Weak Lensing Observables in the Halo Model
• The Effects of Massive Substructures on Image Multiplicities in Gravitati onal Lenses
• The impact of halo shapes on the bispectrum in cosmology
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: I. Construction of all-sky thermal and kinetic SZ-maps
• Evolution of the Clustering of Photometrically Selected SDSS Galaxies
• Constraining Cosmology with High Convergence Regions in Weak Lensing Surveys
• The Selection Function of SZ Cluster Surveys
• Halo Mass Functions in Early Dark Energy Cosmologies
• How Unusual is the Milky Way's Assembly History?
• The Cluster Galaxy Circular Velocity Function
• Strong gravitational lensing and galactic bulges
• Cosmography using strongly lensed gravitational waves from binary black holes
• A measurement of galaxy halo mass from the surrounding HI Lyα absorption
• Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps
• CMB-Cluster Lensing
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• The rise and fall of a challenger: the Bullet Cluster in $\Lambda$ Cold Dark Matter simulations
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• On the reliability of merger-trees and the mass growth histories of dark matter haloes
• The intergalactic medium temperature and Compton y parameter
• On the Spatial Correlations of Lyman Break Galaxies
• Hydrodynamical simulations of coupled and uncoupled quintessence models I: Halo properties and the cosmic web
• Constraining Quasar and IGM Properties Through Bubble Detection in Redshifted 21-cm Maps
• Influence of Population III stars on cosmic chemical evolution
• Weak lensing in the second post-Newtonian approximation: Gravitomagnetic potentials and the integrated Sachs-Wolfe effect
• Cluster scaling relations from cosmological hydrodynamic simulations in dark energy dominated universe
• A Simple Empirically Motivated Template for the Unresolved Thermal Sunyaev-Zeldovich Effect
• Reionisation in sterile neutrino cosmologies
• A Short Introduction to Reionization Physics
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• A general framework to test gravity using galaxy clusters I: Modelling the dynamical mass of haloes in $f(R)$ gravity
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Do dark matter halos explain lensing peaks?
• Keck Deep Fields. I. Observations, Reductions, and the Selection of Faint Star-Forming Galaxies at Redshifts z~4, 3, and 2
• Estimating f_NL and g_NL from Massive High-Redshift Galaxy Clusters
• Cosmology with clusters of galaxies
• Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs
• Comparing halo bias from abundance and clustering
• Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
• Small-scale galaxy clustering in the EAGLE simulation
• Probability of the most massive cluster under non-Gaussian initial conditions
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• Probing the existence of a rich galaxy overdensity at z=5.2
• Cluster Ellipticities as a Cosmological Probe
• First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions
• A new model to predict weak-lensing peak counts III. Filtering technique comparisons
• Toward Understanding Environmental Effects in SDSS Clusters
• A closer look at CMB constraints on WIMP dark matter
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• Supermassive Black Hole Merger Rates: Uncertainties from Halo Merger Theory
• Why Newton's gravity is practically reliable in the large-scale cosmological simulations
• Effects of the complex mass distribution of dark matter halos on weak lensing cluster surveys
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• The power spectrum amplitude from clusters revisited: σ_8 using simulations with preheating and cooling
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• On the Average Comoving Number Density of Halos
• Halo Concentration and the Dark Matter Power Spectrum
• An Optical Catalog of Galaxy Clusters Obtained from an Adaptive Matched Filter Finder Applied to SDSS DR9 Data
• The 400d Galaxy Cluster Survey Weak Lensing Programme: I: MMT/Megacam Analysis of CL0030+2618 at z=0.50
• Exact Extreme Value Statistics and the Halo Mass Function
• Constraining the inner density slope of massive galaxy clusters
• Cluster correlations in redshift space
• Mass functions and bias of dark matter halos
• Re-ionizing the Universe without Stars
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• The mass function dependence on the dynamical state of dark matter haloes
• The effects of primordial non-Gaussianity on the cosmological reionization
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• Can Non-Gaussian Cosmological Models Explain the WMAP's High Optical Depth for Reionization?
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Excursion set theory for modified gravity: Eulerian versus Lagrangian environments
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• Constraints on the Inner Cluster Mass Profile and the Power Spectrum Normalization from Strong Lensing Statistics
• Constraining cosmology with shear peak statistics: tomographic analysis
• The effects of massive neutrinos on the linear point of the correlation function
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Groups in the Millennium Simulation and in SDSS DR7
• The Most Massive Black Holes in the Universe: Effects of Mergers in Massive Galaxy Clusters
• Clustering of dark matter halos on the light-cone: scale-, time- and mass-dependence of the halo biasing in the Hubble volume simulations
• Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• WMAP5 and the Cluster Mass Function
• On Physical Scales of Dark Matter Halos
• A Snapshot Survey for Gravitational Lenses Among z>=4.0 Quasars: II. Constraints on the 4.0<z<4.5 Quasar Population
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• The Goldilocks problem of the quasar contribution to reionization
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• Keck spectroscopy of z=1-3 ULIRGs from the Spitzer SWIRE survey
• Radio Point Sources and the Thermal SZ Power Spectrum
• Constraining cosmological parameters with the clustering properties of galaxy clusters in optical and X-ray bands
• Tests of Gravity with Galaxy Clusters
• Composition of Low Redshift Halo Gas
• Southern Cosmology Survey I: Optical Cluster Detections and Predictions for the Southern Common-Area Millimeter-Wave Experiments
• Constraining the halo mass function with observations
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• A Comparison of Simulated and Analytic Major Merger Counts
• Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters
• Gravitational Redshifts in Simulated Galaxy Clusters
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VII The Mass Function of Galaxy Clusters
• Some improvements to the spherical collapse model
• On the abundance of collapsed objects
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Conditional Probabilities in the Excursion Set Theory. Generic Barriers and non-Gaussian Initial Conditions
• Sunyaev-Zel'dovich Predictions for the Planck Surveyor Satellite using the Hubble Volume Simulations
• Schechter vs. Schechter: Sub-Arcsecond Gravitational Lensing and Inner Halo Profiles
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Fast Identification of Bound Structures in Large N-body Simulations
• Lensing Sunyaev-Zel'dovich Clusters
• Mass Variance from Archival X-ray Properties of Dark Energy Survey Year-1 Galaxy Clusters
• On the starting redshift for cosmological simulations: Focusing on halo properties
• Dark energy parameterizations and their effect on dark halos
• Flux-limited strong gravitational lensing and dark energy
• Searching for Intergalactic Shocks with the SKA
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: III. Properties of the expected SZ-cluster sample
• The clustering of the first galaxy halos
• Baryons: What, When and Where?
• The halo light cone catalogues of \Abacus{AbacusSummit}
• Photon Number Conserving Models of H II Bubbles during Reionization
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Galaxy Evolution and Cosmology with the Square Kilometre Array
• Richness-based masses of rich and famous galaxy clusters
• Gamma-ray probe of cosmic-ray pressure in galaxy clusters and cosmological implications
• Testing the Modified Press-Schechter Model against N-Body Simulations
• Changes in the halo formation rates due to features in the primordial spectrum
• Turning noise into signal: learning from the scatter in the Hubble diagram
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• Imprints of quasar duty cycle on the 21cm signal from the Epoch of Reionization
• Neutrino Signatures from the First Stars
• Electromagnetic signatures of supermassive black hole binaries resolved by PTAs
• Gravitational lensing magnification without multiple imaging
• The Total Mass of Dark Matter Haloes
• Cluster counts: calibration issue or new physics?
• CMB constraints on a physical model of reionization
• On an Analytical Framework for Voids: Their abundances, density profiles and local mass functions
• Galaxy Luminosity Functions in WINGS clusters
• The hybrid SZ power spectrum: Combining cluster counts and SZ fluctuations to probe gas physics
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• Cosmological parameter constraints from CMB lensing with cosmic voids
• Will Multiple Probes of Dark Energy find Modified Gravity?
• A new model for the full shape of the large-scale power spectrum
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• Detecting Reionization in the Star Formation Histories of High-Redshift Galaxies
• Physical component analysis of galaxy cluster weak gravitational lensing data
• Influence of Projection in Cluster Cosmology Studies
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• Euclid: Effect of sample covariance on the number counts of galaxy clusters
• Pairwise velocities in the Halo Model: Luminosity and Scale Dependence
• A Solution to the Missing Link in the Press-Schechter Formalism
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• Constraints on shear and rotation with massive galaxy clusters
• X-ray Cluster Constraints on Non-Gaussianity
• Are Simulations of CDM Consistent with Galactic-Scale Observations at High Redshift?
• Into the Lyα jungle: exploring the circumgalactic medium of galaxies at z ~ 4-5 with MUSE
• Dark Matter-baryon segregation in the non-linear evolution of coupled Dark Energy model
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• The Epoch of Reionization 21-cm Bispectrum: The impact of light-cone effects and detectability
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• The mass function and distribution of velocity dispersions for UZC groups of galaxies
• Galaxy Clusters as a probe of early dark energy
• How many arcminute-separation lenses are expected in the 2dF QSO survey?
• Universal Merger Histories of Dark-Matter Haloes
• Vector dark energy and high-z massive clusters
• The peculiar velocities of satellites of external disk galaxies
• Taming assembly bias for primordial non-Gaussianity
• The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• The build-up of halos within Press-Schechter theory
• Figure rotation of dark halos in CDM simulations
• Probing Population III Initial Mass Functions with He II/H$\alpha$ Intensity Mapping
• Non-Gaussian Scatter in Cluster Scaling Relations
• The Formation and Evolution of the First Massive Black Holes
• Can We Detect the Anisotropic Shapes of Quasar HII Regions During Reionization Through The Small-Scale Redshifted 21cm Power Spectrum?
• Detecting the gravitational wave background from primordial black hole dark matter
• The clustering of baryonic matter. I: a halo-model approach
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Measuring Bulk Flow of Galaxy Clusters using Kinematic Sunyaev-Zel'dovich effect: Prediction for Planck
• Statistical Properties of Radio Halos in Galaxy Clusters and Origin of Seed Electrons for Reacceleration
• Stochastic background of gravitational waves generated by pre-galactic black holes
• Measurements of the Cosmological Evolution of Magnetic Fields with the Square Kilometre Array
• A determination of dark matter bispectrum with a large set of N-body simulations
• Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
• The Effect of Radiative Cooling on the Sunyaev-Zel'dovich Cluster Counts and Angular Power Spectrum: Analytic Treatment
• The Cosmological History of Accretion onto Dark Halos and Supermassive Black Holes
• Passive Evolution of Galaxy Clustering
• Precision cosmology with a combination of wide and deep Sunyaev-Zeldovich cluster surveys
• On the cosmological mass function theory
• The Size Distribution of Void Filaments in a LCDM Cosmology
• A Phenomenological Model for the Intracluster Medium that matches X-ray and Sunyaev-Zel'dovich observations
• Detection and Fundamental Applications of Individual First Galaxies
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• Cluster Lensing of QSOs as a Probe of LCDM and Dark Energy Cosmologies
• Extending Recovery of the Primordial Matter Power Spectrum
• Cold dark energy constraints from the abundance of galaxy clusters
• Weak lensing by triaxial galaxy clusters
• A high-resolution cosmological simulation of a strong gravitational lens
• Counts of galaxy clusters as cosmological probes: the impact of baryonic physics
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Extreme value statistics of weak lensing shear peak counts
• Constraining quasar host halo masses with the strength of nearby Lyman-alpha forest absorption
• A Baryonic Effect on the Merger Timescale of Galaxy Clusters
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• On the equivalence between the effective cosmology and excursion set treatments of environment
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• The Diffuse Gamma-Ray Flux from Clusters of Galaxies
• Halo Occupation Distribution of Massive Galaxies since z = 1
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Tracing the Nature of Dark Energy with Galaxy Distribution
• Statistics of Quasars Multiply Imaged by Galaxy Clusters
• The Mass Function of Void Groups as a Probe of the Primordial non-Gaussianity
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Effects of Completeness and Purity on Cluster Dark Energy Constraints
• Anthropic predictions for vacuum energy and neutrino masses in the light of WMAP-3
• The evolution of star formation activity in galaxy groups
• Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
• The distribution of two-dimensional eccentricity of Sunyaev-Zeldovich Effect and X-ray surface brightness profiles
• The most massive Population III stars
• Competitive Accretion in Sheet Geometry and the Stellar IMF
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• A Better Way to Define Dark Matter Haloes
• Optical Galaxy Clusters in the Deep Lens Survey
• The Race Between Stars and Quasars in Reionizing Cosmic Hydrogen
• Large Scale Structure Forecast Constraints on Particle Production During Inflation
• Validation of Selection Function, Sample Contamination and Mass Calibration in Galaxy Cluster Samples
• Are the 2dFGRS superstructures a problem for hierarchical models?
• Probing dark energy with the next generation X-ray surveys of galaxy clusters
• Virial halo mass function in the $Planck$ cosmology
• The abundance of dark matter haloes down to Earth mass
• Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect
• Optimizing measurements of cluster velocities and temperatures for CCAT-prime and future surveys
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• Properties of High Redshift Quasars-I: Evolution of the super-massive black-hole to halo mass ratio
• Pure Density Evolution of the Ultraviolet Quasar Luminosity Function at $2\lesssim z\lesssim 6$
• Galaxy clustering at cosmic dawn from JWST/NIRCam observations to redshift z$\sim$11
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Superclusters with thermal SZ effect surveys
• Probing a cosmological model with a $\Lambda ={\Lambda }_0+3\beta H^2$ decaying-vacuum
• Dynamics and constraints of the dissipative Liouville cosmology
• Neutrino Mass Inference from SZ Surveys
• Sunyaev-Zel'dovich Cluster Survey Simulations for Planck
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• The Effect of Formation Redshifts on the Cluster Mass-Temperature Relation
• Pregalactic LiBeB Production by Supernova Cosmic Rays
• Halo Mass Definition and Multiplicity Function
• Massive, red galaxies in a hierarchical universe-II Clustering of Extremely Red Objects
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Cosmological Perturbations and the Running Cosmological Constant Model
• Constraining CMB-consistent primordial voids with cluster evolution
• Testing model independent modified gravity with future large scale surveys
• The Halo Occupation Distribution of HI from 21cm Intensity Mapping at Moderate Redshifts
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Discriminating power of milli-lensing observations for dark matter models
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• How far are the sources of IceCube neutrinos? Constraints from the diffuse TeV gamma-ray background
• Detailed theoretical predictions of the outskirts of dark matter halos
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Stacking Clusters in the ROSAT All-Sky Survey
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• Number Counts and Dynamical Vacuum Cosmologies
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
• Cluster Probes of Dark Energy Clustering
• Statistics of gravitational potential perturbations: A novel approach to deriving the X-ray temperature function
• Bumpy Power Spectra and Galaxy Clusters
• On the Angular Correlation Function of SZ Clusters : Extracting cosmological information from a 2D catalog
• High-redshift voids in the excursion set formalism
• The mass function of the Las Campanas loose groups of galaxies
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Cusp-core problem and strong gravitational lensing
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• Evidence for new physics from clusters ?
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• Expected properties of the Two-Point Autocorrelation Function of the IGM
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• 21-cm signatures of residual HI inside cosmic HII regions during reionization
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• Constraining thawing and freezing models with cluster number counts
• Cluster-Cluster Lensing and the Case of Abell 383
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• Biases on cosmological parameter estimators from galaxy cluster number counts
• A prescription for the conditional mass function of dark matter haloes
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function
• Toward an Improved Analytical Description of Lagrangian Bias
• Comparing cosmic shear measures - Optimizing the Information content of cosmic shear data vectors
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• Implications of the Lyman alpha Emission Line from a Candidate z=10 Galaxy
• Nonlinear stochastic biasing of halos: Analysis of cosmological N-body simulations and perturbation theories
• Testing the accuracy of likelihoods for cluster abundance cosmology
• Probing dark energy via galaxy cluster outskirts
• Unveiling cosmological information on small scales with line intensity mapping
• Dynamical quintessence fields Press-Schechter mass function: detectability and effect on dark haloes
• Multiply-imaged time-varying sources behind galaxy clusters - Comparing FRBs to QSOs, SNe, and GRBs
• Semi-numeric simulations of helium reionization and the fluctuating radiation background
• Spherical collapse of dark matter haloes in tidal gravitational fields
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• The ALFALFA HI velocity width function
• The Properties of X-ray Cold Fronts in a Statistical Sample of Simulated Galaxy Clusters
• Modelling the stochasticity of high-redshift halo bias
• Variation in the escape fraction of ionising photons from galaxies and the redshifted 21-cm power spectrum during reionization
• Nonsingular density profiles of dark matter halos and Strong gravitational lensing
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Constraining Cosmological Models by the Cluster Mass Function
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• A novel approach to cosmological non-linearities as an effective fluid
• Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ΛCDM
• On the primordial information available to galaxy redshift surveys
• Constraining stellar assembly and AGN feedback at the peak epoch of star formation
• Simulating the formation of cosmic structure
• The mass and temperature functions in a moving barrier model
• CMB-Normalized Predictions for Sunyaev-Zel'dovich effect fluctuations
• Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy
• The galaxy luminosity function around groups
• Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Evolution of the cosmological mass function in a moving barrier model
• Strong-lensing cosmography using third-generation gravitational-wave detectors
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• The U-band Galaxy Luminosity Function of Nearby Clusters
• Predicting the clustering properties of galaxy clusters detectable for the Planck satellite
• Gravitational Collapse of Baryonic and Dark matter
• The amplitude of mass fluctuations and mass density of the Universe constrained by strong gravitational lensing
• Halo abundances and shear in void models
• Using clusters in SZE + x-ray surveys as an ensemble of rulers to constrain cosmology
• Cosmological constraints from the masses and abundances of L* galaxies
• Deep learning insights into cosmological structure formation
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• Setting the Stage: Structures from Gaussian Random Fields
• Halo Model Analysis of Cluster Statistics
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• The virialization density of peaks with general density profiles under spherical collapse
• Gravitational wave constraints on extended dark matter structures
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Recovering the Tidal Field in the Projected Galaxy Distribution
• A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• A blind detection of a large, complex, Sunyaev--Zel'dovich structure
• Sunyaev-Zel'dovich power spectrum with decaying cold dark matter
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• Uncertainties in the S-Z selected cluster angular power spectrum
• Scale Dependence of the Halo Bias in General Local-Type Non-Gaussian Models I: Analytical Predictions and Consistency Relations
• Extended Press-Schechter theory and the density profiles of dark matter haloes
• An Introduction into the Theory of Cosmological Structure Formation
• The spherical collapse model with shell crossing
• Do all QSOs have the same black hole mass?
• Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
• Systematic errors in the determination of Hubble constant due to the asphericity and non-isothermality of clusters of galaxies
• X-ray Clusters of Galaxies as Cosmological Tools
• X-ray galaxy clusters abundance and mass temperature scaling
• Third-order cosmological perturbations of zero-pressure multi-component fluids: Pure general relativistic nonlinear effects
• Efficient simulation of discrete galaxy populations and associated radiation fields during the first billion years
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• Numerical action reconstruction of the dynamical history of dark matter haloes in N-body simulations
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• The rms peculiar velocity of galaxy clusters for different cluster masses and radii
• Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius
• Understanding the Cosmic Mass Function High Mass Behaviour
• Dark matter halo mass functions and density profiles from mass and energy cascade
• The Impact of Secondary non-Gaussianities in the CMB on Cosmological Parameter Estimation
• Studying Dark Energy with Galaxy Cluster Surveys
• Galaxy flows within 8,000 km/s from Numerical Action methods
• An Extended Zel'dovich Model for the Halo Mass Function
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• A new test for the stable clustering hypothesis
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Dust obscuration studies along quasar sight lines using simulated galaxies
• Detection of a CMB decrement towards a cluster of mJy radiosources
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• An Evolving Entropy Floor in the Intracluster Gas?
• Predictions for the Counts of Faint, High-Redshift Galaxies in the Mid-Infrared
• Imprint of massive neutrinos on Persistent Homology of large-scale structure
• Cosmic expansion and structure formation in running vacuum cosmologies
• Constraining the mass-concentration relation through weak lensing peak function
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Compact source detection in multi-channel microwave surveys: from SZ clusters to polarized sources
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• A Physical Model for the Quasar Luminosity Function Evolution between Cosmic Dawn and High Noon
• Maximum entropy distributions of dark matter in $\Lambda$CDM cosmology
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Biasing and Genus Statistics of Dark Matter Halos in the Hubble Volume Simulation
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• The Ursa Major Association of Galaxies. VI: A relative dearth of gas-rich dwarf galaxies
• Can we distinguish early dark energy from a cosmological constant?
• Self-Consistent Theory of Halo Mergers - II: CDM Power Spectra
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• Gravitational lensing effects on sub-millimetre galaxy counts
• Cosmological Implications and Physical Properties of an X-Ray Flux-Limited Sample of Galaxy Clusters
• Cross-correlation between the soft X-ray background and SZ Sky
• Probing the Primordial Power Spectrum with Cluster Number Counts
• Optimizing the yield of Sunyaev-Zel'dovich cluster surveys
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-Halo Lens Model
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• X-ray cluster cosmology
• Haloes at the ragged edge: The importance of the splashback radius
• The abundance and environment of dark matter haloes
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• The fractional Brownian motion and the halo mass function
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Non-Markov Excursion Set Model of Dark Matter Halo Abundances
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Halo mass function in scale invariant models
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
• Constraints on the warm dark matter model from gravitational lensing
• Tree-less 3d Friends-of-Friends using Spatial Hashing
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• The baryon mass function for galaxy clusters
• Cluster Assembly Times as a Cosmological Test
• Observations of Ly$\alpha$ Emitters at High Redshift
• Complementarity of Future Dark Energy Probes
• Deep learning insights into non-universality in the halo mass function
• Cluster contribution to the X-ray background as a cosmological probe
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Complementary Cosmological Simulations
• Improvements in the M-T relation and mass function and the measured Omega_m through clusters evolution
• The Effects of Relativistic Corrections on Cosmological Parameter Estimations from SZE Cluster Surveys
• An expanded merger-tree description of cluster evolution
• Anisotropies in the redshift-space correlations of galaxy groups and clusters I: Simulated catalogues
• Nonlinear structure formation in Bound Dark Energy
• Cosmic reionization constraints on the nature of cosmological perturbations
• On the reliability of initial conditions for dissipationless cosmological simulations
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
• Non-linear matter power spectrum without screening dynamics modelling in $f(R)$ gravity
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Evidence for Non-Linear Growth of Structure from an X-ray Selected Cluster Survey using a Novel Joint Analysis of the Chandra and XMM-Newton Archives
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Universality of the halo mass function in screened gravity theories
• DUET - The Dark Universe Exploration Telescope
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue
• Strong Lensing Probabilities in a Cosmological Model with a Running Primordial Power Spectrum
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Dark matter haloes: a multistream view
• An Empirical Mass Function Distribution
• An X-ray Galaxy Cluster Survey for Investigations of Dark Energy
• Accurate halo mass functions from the simplest excursion set theory
• Structural and Photometric Properties of the Andromeda Satellite Dwarf Galaxy Lacerta I from Deep Imaging with WIYN pODI
• Machine Learning and Structure Formation in Modified Gravity
• Stochastic backgrounds of gravitational waves from cosmological sources - The role of dark energy
• Bayesian analysis of spatially distorted cosmic signals from Poissonian data
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Measuring Omega_m using clusters evolution
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Massive Black Hole Mergers
• Evolution of Power Spectrum in Non-Gaussian Models
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• AMICO galaxy clusters in KiDS-1000: cosmological sample
• HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions
• The Halo Mass Function Redshift Dependence
• Stochastic Gravitational Wave Background originating from Halo Mergers
• Cosmological parameters from Galaxy Clusters: an Introduction
• Simulations and Observations of the Microwave Universe
• Statistical Properties of Supercluster-Like Filaments from Cosmological Simulations
• The Splashback Mass Function in the Presence of Massive Neutrinos
• Convergence of halo statistics: code comparison between Rockstar and CompaSO using scale-free simulations
• Simulating Binary Primordial Black Hole Mergers in Dark Matter Halos
• Thermodynamic evolution of the cosmological baryonic gas : II. Galaxy formation
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• The FAST Ursa Major supergroup HI survey (FUMaS): catalog and HI mass function
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• Global 21 cm signal: a promising probe of primordial features
• A Parameter-free Statistical Measurement of Halos with Power Spectra
• Systematic bias in the estimate of cluster mass and the fluctuation amplitude from cluster abundance statistics
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Characterising the optical properties of galaxy clusters with GMPhoRCC
• Sunyaev-Zel'dovich contribution in CMB analysis
• Galaxies and Cluster of Galaxies as Peak Patches of the Density Field
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• Determination of the Linear Mass Power Spectrum From the Mass Function of Galaxy Clusters
• The MeerKAT Fornax Survey VI. The collapse of the galaxy HI Mass Function in Fornax
• Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Directional miscentering dependence in weak lensing mass bias
• On Local Approximations to the Nonlinear Evolution of Large-Scale Structure
• Quinstant Dark Energy Predictions for Structure Formation
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• Probability distribution and statistical properties of spherically compensated cosmic regions in $\Lambda$CDM cosmology
• AMI-CL J0300+2613: a Galactic anomalous-microwave-emission ring masquerading as a galaxy cluster
• Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
• Cosmological constraints from the thermal Sunyaev Zeldovich power spectrum?
• Formation of Dark Matter Haloes in a Homogeneous Dark Energy Universe
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• The Contribution of Galaxies to the $3.4\mu \mathrm{m}$ Cosmic Infrared Background as Measured Using WISE
• Effect of the Cosmological Constant on Halo Size
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• Extended Hernquist-Springel formalism for cosmic star formation
• Searching for Clusters with SUMSS
• The haloes that reionized the Universe
• Effects of dynamical friction on perturbations for evolving dark energy
• Tracking through equality
• A flat faint end of the Fornax cluster galaxy luminosity function
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• Modeling Dark Matter Halos with Nonlinear Field Theories
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• Excursion Sets with a "Perfect" Collapse Model
• Measuring the baryon fraction in cluster of galaxies with Kinematic Sunyaev Zeldovich and a Standard Candle
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• The same with less: The cosmic web of warm versus cold dark matter dwarf galaxies
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Dark Energy Simulations
• BRIGHT lights, BIG city: Massive galaxies, giant Ly-a nebulae, and proto--clusters
• Particle Reacceleration by Turbulence and Radio Constraints on Multi-Messenger High-Energy Emission from the Coma Cluster
• The History of Galaxy Formation in Groups: An Observational Perspective
• Probing power spectrum enhancement at small scales with the SKA
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Mass functions from the excursion set model
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Using Dark Matter Haloes to Learn about Cosmic Acceleration: A New Proposal for a Universal Mass Function
• Cosmological constraints from clustering properties of galaxy clusters
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• Transition between order and chaos in a composite disk galaxy model with a massive nucleus and a dark matter halo
• Slicing cluster mass functions with a Bayesian razor
• Ginnungagap -- a massively parallel cosmological initial conditions generator
• The life and times of dark matter haloes: what will I be when I grow up?
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• Universality of the halo mass function in modified gravity cosmologies
• Clustering properties of TGSS radio sources
• A redshift distortion free correlation function at third order in the nonlinear regime
• The Relic Neutrino Backround from the First Stars
• The Mass Function of Dark Matter Haloes in a Cosmological Model with a Running Primordial Power Spectrum
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos