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

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• 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
• LoCuSS: Hydrostatic Mass Measurements of the High-$L_X$ Cluster Sample -- Cross-calibration of Chandra and XMM-Newton
• The Anisotropic Distribution of Satellite Galaxies
• Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
• Simulations of Damped Lyman-Alpha and Lyman Limit Absorbers in Different Cosmologies: Implications for Structure Formation at High Redshift
• Spherical collapse and halo mass function in f(R) theories
• A simulation pipeline for the Planck mission
• The impact of Early Dark Energy on non-linear structure formation
• The early-type dwarf galaxy population of the Centaurus cluster
• The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys
• Effective Screening due to Minihalos During the Epoch of Reionization
• A new model to predict weak-lensing peak counts II. Parameter constraint strategies
• The Non-Gaussian Halo Mass Function with fNL, gNL and tauNL
• A new model to predict weak-lensing peak counts I. Comparison with $N$-body Simulations
• Strong Gravitational Lensing and Dark Energy
• A Lyman-α protocluster at redshift 6.9
• The 21cm Signature of the First Stars
• UV Radiative Feedback on High-Redshift Proto-Galaxies
• Shapes of clusters and groups of galaxies: Comparison of model predictions with observations
• Mass functions in coupled Dark Energy models
• The nature of dark matter from the global high redshift HI 21 cm signal
• Dark matter halo abundances, clustering and assembly histories at high redshift
• Do Distinct Cosmological Models Predict Degenerate Halo Populations?
• Galaxy Groups in the 2dFGRS: the number density of groups
• A Model For Infall Around Virialized Halos
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• The First Generation of Star-Forming Haloes
• The abundance of dark galaxies
• The halo model for cosmology: a pedagogical review
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Searching for galaxy clusters using the aperture mass statistics in 50 VLT fields
• 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
• On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion
• Focusing on Warm Dark Matter with Lensed High-redshift Galaxies
• The 2dF Galaxy Redshift Survey: The clustering of galaxy groups
• Hierarchical Formation of Galaxies with Dynamical Response to Supernova-Induced Gas removal
• On the Self-Similar Appearance of Galaxy Clusters in X-rays
• Unveiling the three-dimensional structure of galaxy clusters: resolving the discrepancy between X-ray and lensing masses
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Machine learning cosmological structure formation
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density
• Constraining halo occupation properties of X-ray AGNs using clustering of Chandra sources in the Bootes survey region
• Primordial non-Gaussianity from the covariance of galaxy cluster counts
• Halo modelling in chameleon theories
• A Lightcone Catalogue from the Millennium-XXL Simulation
• The scatter and evolution of the global hot gas properties of simulated galaxy cluster populations
• 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
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• Universal at last? The splashback mass function of dark matter halos
• The early-type dwarf galaxy population of the Fornax cluster
• Dwarf Dark Matter Halos
• Modelling Void Abundance in Modified Gravity
• Six More Ultra-Faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
• Cosmic Neutron Star Merger Rate and Gravitational Waves constrained by the R Process Nucleosynthesis
• The Virial Mass Function of Nearby SDSS Galaxy Clusters
• Gravitational Waves from the First Stars
• Studying the Lyman-$\alpha$ optical depth fluctuations at $z\sim 5.5$ using fast semi-numerical methods
• Proto-groups at 1.8<z<3 in the zCOSMOS-deep sample
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• Numerical Galaxy Catalog -I. A Semi-analytic Model of Galaxy Formation with N-body simulations
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Precision cosmology with a wide area XMM cluster survey
• 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
• The imprint of the interaction between dark sectors in galaxy clusters
• 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
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• Searching for diffuse light in the M96 Group
• Hierarchical Growth and Cosmic Star Formation: Enrichment, Outflows and Supernova Rates
• Implications of multiple high-redshift galaxy clusters
• Future Evolution of Bound Superclusters in an Accelerating Universe
• Observing simulated galaxy clusters with PHOX: a novel X-ray photon simulator
• The phase-space distribution of infalling dark matter subhalos
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• Toward an accurate mass function for precision cosmology
• Dissipationless Merging and the Assembly of Central Galaxies
• Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy Studies
• BLOX: The Bonn Lensing, Optical, and X-ray selected galaxy clusters -- I. Cluster catalog construction
• A Snapshot Survey for Gravitational Lenses Among z>=4.0 Quasars: I. The z>5.7 Sample
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• The XMM--NEWTON Omega Project: I. The X-ray Luminosity - Temperature Relation at z>0.4
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• 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
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• Combined analysis of weak lensing and X-ray blind surveys
• Deriving an Accurate Formula of Scale-dependent Bias with Primordial Non-Gaussianity: An Application of the Integrated Perturbation Theory
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Star formation in galaxies falling into clusters along supercluster-scale filaments
• An Analytical Approach to Inhomogeneous Structure Formation
• Star formation in galaxies along the Pisces-Cetus Supercluster filaments
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• The Radio Luminosity Function of Cluster Radio Halos
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• Sharpening the Precision of the Sunyaev-Zel'dovich Power Spectrum
• Modeling the Counts of Faint Radio Loud Quasars: Constraints on the Supermassive Black Hole Population and Predictions for High Redshift
• A New Halo Finding Method for N-Body Simulations
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• How well do cosmological simulations reproduce individual-halo properties?
• Accurate mass and velocity functions of dark matter halos
• Group finding in the stellar halo using M-giants in 2MASS: An extended view of the Pisces Overdensity?
• Accurate Modeling of Weak Lensing with the sGL Method
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Imprints of the Early Universe on Axion Dark Matter Substructure
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• 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
• An XMM-Newton observation of the massive, relaxed galaxy cluster ClJ1226.9+3332 at z=0.89
• Modelling the post-reionization neutral Hydrogen (\HI) bias
• The role of HD cooling in primordial star formation
• Bayesian joint analysis of cluster weak lensing and Sunyaev-Zel'dovich effect data
• Constraining primordial magnetic fields through large scale structure
• TheHaloMod: An online calculator for the halo model
• High redshift quasars and the supermassive black hole mass budget: constraints on quasar formation models
• Unveiling the Dynamics of the Universe
• The discovery of a massive supercluster at z=0.9 in the UKIDSS DXS
• An Effective Model for the Cosmic-Dawn 21-cm Signal
• Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization
• Capturing Halos at High Redshifts
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Red Galaxy Clustering in the NOAO Deep Wide-Field Survey
• Cosmological Constraints from Galaxy Cluster Velocity Statistics
• Quasars and galaxy formation
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Unveiling the composition of radio plasma bubbles in galaxy clusters with the Sunyaev-Zel'dovich effect
• 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
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• A blind HI survey in the Canes Venatici region
• Imprints of mass accretion on properties of galaxy clusters
• Mass Function of Low Mass Dark Halos
• How well do we know the Halo Mass Function?
• 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
• Impact of baryons on the cluster mass function and cosmological parameter determination
• Dark energy constraints from lensing-detected galaxy clusters
• Light-cone anisotropy in 21cm fluctuations during the epoch of reionization
• Circular velocity profiles of dark matter haloes
• The XMM--NEWTON Omega Project: II.Cosmological implications from the high redshift L-T relation of X-ray clusters
• Probing the Core Structure of Dark Halos with Tangential and Radial Arc Statistics
• 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 nonlinear matter power spectrum
• Measuring Sigma8 with Cluster Lensing : Biases from Unrelaxed Clusters
• Coupled Quintessence and the Halo Mass Function
• What is the best way to measure baryonic acoustic oscillations?
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• Reviewing the frequency and central depletion of Ultra-Diffuse Galaxies in galaxy clusters from the KIWICS survey
• Mass Function of Rich Galaxy Clusters and Its Constraint on sigma_8
• Population III Generated Cosmic Rays and the Production of Li6
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• 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
• Bayesian modelling of clusters of galaxies from multi-frequency pointed Sunyaev--Zel'dovich observations
• The journey of QSO haloes from z=6 to the present
• Sensitivity of galaxy cluster dark energy constraints to halo modeling uncertainties
• Monolithic or hierarchical star formation? A new statistical analysis
• HI content and other structural properties of galaxies in the Virgo cluster from the Arecibo Legacy Fast ALFA Survey
• Constraining warm dark matter with cosmic shear power spectra
• Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe
• High-Redshift Galaxies in Cold Dark Matter Models
• Richness-mass relation self-calibration for galaxy clusters
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Integrated Sachs Wolfe Effect and Rees Sciama Effect
• Local stochastic non-Gaussianity and N-body simulations
• Can large-scale structure probe CMB-constrained non-Gaussianity?
• On the Nonspherical Nature of Halo Formation
• Cosmological and Astrophysical Implications of the Sunyaev-Zel'dovich Effect
• Nature of Lyman Alpha Blobs: Powered by Extreme Starbursts
• Redshift Accuracy Requirements for Future Supernova and Number Count Surveys
• The Accelerated Build-up of the Red Sequence in High Redshift Galaxy Clusters
• Exploring the liminality: properties of haloes and subhaloes in borderline $f(R)$ gravity
• The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population
• Likelihood Methods for Cluster Dark Energy Surveys
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function
• Evolution of the Cluster Mass Function: Gpc^3 Dark Matter Simulations
• An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• A high precision semi-analytic mass function
• X-Ray Evolution of Active Galactic Nuclei and Hierarchical Galaxy Formation
• The Line-of-Sight Proximity Effect and the Mass of Quasar Host Halos
• Constraining the Redshift z=6 Quasar Luminosity Function Using Gravitational Lensing
• Higher-order moments of the lensing shear and other spin two fields
• Testing anthropic predictions for Lambda and the CMB temperature
• Galaxy Clusters as Reservoirs of Heavy Dark Matter and High-Energy Cosmic Rays: Constraints from Neutrino Observations
• Weak-Lensing Halo Numbers and Dark-Matter Profiles
• 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
• Constraining large scale HI bias using redshifted 21-cm signal from the post-reionization epoch
• Warm dark matter and the ionization history of the Universe
• Strong lensing statistics and the power spectrum normalisation
• Can Early Dark Energy be Detected in Non-Linear Structure?
• Radio source feedback in galaxy evolution
• Cluster mass functions in the quintessential Universe
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Weak Lensing as a Calibrator of the Cluster Mass-Temperature Relation
• Accurate Weak Lensing of Standard Candles. II. Measuring sigma8 with Supernovae
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• Primordial non-Gaussianity and Dark Energy constraints from Cluster Surveys
• 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
• A low-scatter survey-based mass proxy for clusters of galaxies
• Microwave-Sky Simulations and Projections for Galaxy Cluster Detection with the Atacama Cosmology Telescope
• Statistical and systematic errors in redshift-space distortion measurements from large surveys
• Minimum size of 21-cm simulations
• Powellsnakes II: a fast Bayesian approach to discrete object detection in multi-frequency astronomical data sets
• Halo abundances within the cosmic web
• 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
• The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
• Nonlinear Bias of Cosmological Halo Formation in the Early Universe
• Galaxy groups in the 2dF galaxy redshift survey: Luminosity and Mass Statistics
• The Sunyaev-Zeldovich Background
• Effects of the initial conditions on cosmological $N$-body simulations
• Decaying Cold Dark Matter and the Evolution of the Cluster Abundance
• Relativistic numerical cosmology with Silent Universes
• Substructure in dark matter halos: Towards a model of the abundance and spatial distribution of subclumps
• The halo mass function in interacting Dark Energy models
• Supermassive Black Hole Formation at High Redshifts Through a Primordial Magnetic Field
• Cross-Calibration of Cluster Mass-Observables
• Reliability of the dark matter clustering in cosmological N-body simulation on scales below the mean separation length of particles
• 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
• A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
• The REFLEX II galaxy cluster survey: power spectrum analysis
• Are Clusters Standard Candles? Galaxy Cluster Scaling Relations With the Sunyaev-Zeldovich Effect
• Most massive halos with Gumbel Statistics
• The Effects of Massive Substructures on Image Multiplicities in Gravitati onal Lenses
• Constraining Cosmology with High Convergence Regions in Weak Lensing Surveys
• 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
• Testing cold dark matter with the low mass Tully-Fisher relation
• Weak Lensing Observables in the Halo Model
• The Selection Function of SZ Cluster Surveys
• The impact of halo shapes on the bispectrum in cosmology
• GMOS Spectroscopy of SCUBA Galaxies Behind A851
• Statistics of Sunyaev-Zel'dovich Cluster Surveys
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Cosmography using strongly lensed gravitational waves from binary black holes
• Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps
• Halo Mass Functions in Early Dark Energy Cosmologies
• The Cluster Galaxy Circular Velocity Function
• How Unusual is the Milky Way's Assembly History?
• A measurement of galaxy halo mass from the surrounding HI Lyα absorption
• Strong gravitational lensing and galactic bulges
• CMB-Cluster Lensing
• The intergalactic medium temperature and Compton y parameter
• 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
• On the Spatial Correlations of Lyman Break Galaxies
• A Short Introduction to Reionization Physics
• Constraining Quasar and IGM Properties Through Bubble Detection in Redshifted 21-cm Maps
• A Simple Empirically Motivated Template for the Unresolved Thermal Sunyaev-Zeldovich Effect
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• Hydrodynamical simulations of coupled and uncoupled quintessence models I: Halo properties and the cosmic web
• Weak lensing in the second post-Newtonian approximation: Gravitomagnetic potentials and the integrated Sachs-Wolfe effect
• Reionisation in sterile neutrino cosmologies
• A general framework to test gravity using galaxy clusters I: Modelling the dynamical mass of haloes in $f(R)$ gravity
• Influence of Population III stars on cosmic chemical evolution
• Cluster scaling relations from cosmological hydrodynamic simulations in dark energy dominated universe
• A new model to predict weak-lensing peak counts III. Filtering technique comparisons
• The Mass Function of Unprocessed Dark Matter Halos and Merger Tree Branching Rates
• Cosmology with clusters of galaxies
• Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
• A closer look at CMB constraints on WIMP dark matter
• Probing the existence of a rich galaxy overdensity at z=5.2
• 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
• Toward Understanding Environmental Effects in SDSS Clusters
• Small-scale galaxy clustering in the EAGLE simulation
• First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Comparing halo bias from abundance and clustering
• Cluster Ellipticities as a Cosmological Probe
• Probability of the most massive cluster under non-Gaussian initial conditions
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs
• Do dark matter halos explain lensing peaks?
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• Effects of the complex mass distribution of dark matter halos on weak lensing cluster surveys
• Supermassive Black Hole Merger Rates: Uncertainties from Halo Merger Theory
• 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
• Why Newton's gravity is practically reliable in the large-scale cosmological simulations
• Constraining the inner density slope of massive galaxy clusters
• Re-ionizing the Universe without Stars
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• On the Average Comoving Number Density of Halos
• Mass functions and bias of dark matter halos
• Exact Extreme Value Statistics and the Halo Mass Function
• 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
• Halo Concentration and the Dark Matter Power Spectrum
• Cluster correlations in redshift space
• Excursion set theory for modified gravity: Eulerian versus Lagrangian environments
• Constraints on the Inner Cluster Mass Profile and the Power Spectrum Normalization from Strong Lensing Statistics
• Constraining cosmology with shear peak statistics: tomographic analysis
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• The effects of massive neutrinos on the linear point of the correlation function
• Groups in the Millennium Simulation and in SDSS DR7
• The mass function dependence on the dynamical state of dark matter haloes
• Can Non-Gaussian Cosmological Models Explain the WMAP's High Optical Depth for Reionization?
• The Most Massive Black Holes in the Universe: Effects of Mergers in Massive Galaxy Clusters
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Clustering of dark matter halos on the light-cone: scale-, time- and mass-dependence of the halo biasing in the Hubble volume simulations
• The effects of primordial non-Gaussianity on the cosmological reionization
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• Constraining the halo mass function with observations
• The Goldilocks problem of the quasar contribution to reionization
• On Physical Scales of Dark Matter Halos
• Composition of Low Redshift Halo Gas
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• Galaxy Zoo: Multi-Mergers and the Millennium Simulation
• Southern Cosmology Survey I: Optical Cluster Detections and Predictions for the Southern Common-Area Millimeter-Wave Experiments
• A Snapshot Survey for Gravitational Lenses Among z>=4.0 Quasars: II. Constraints on the 4.0<z<4.5 Quasar Population
• Tests of Gravity with Galaxy Clusters
• Radio Point Sources and the Thermal SZ Power Spectrum
• WMAP5 and the Cluster Mass Function
• Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey
• Keck spectroscopy of z=1-3 ULIRGs from the Spitzer SWIRE survey
• Constraining cosmological parameters with the clustering properties of galaxy clusters in optical and X-ray bands
• Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters
• A Comparison of Simulated and Analytic Major Merger Counts
• On the abundance of collapsed objects
• Some improvements to the spherical collapse model
• Sunyaev-Zel'dovich Predictions for the Planck Surveyor Satellite using the Hubble Volume Simulations
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VII The Mass Function of Galaxy Clusters
• Gravitational Redshifts in Simulated Galaxy Clusters
• Conditional Probabilities in the Excursion Set Theory. Generic Barriers and non-Gaussian Initial Conditions
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Schechter vs. Schechter: Sub-Arcsecond Gravitational Lensing and Inner Halo Profiles
• Searching for Intergalactic Shocks with the SKA
• The clustering of the first galaxy halos
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Lensing Sunyaev-Zel'dovich Clusters
• Fast Identification of Bound Structures in Large N-body Simulations
• Dark energy parameterizations and their effect on dark halos
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: III. Properties of the expected SZ-cluster sample
• On the starting redshift for cosmological simulations: Focusing on halo properties
• Mass Variance from Archival X-ray Properties of Dark Energy Survey Year-1 Galaxy Clusters
• Flux-limited strong gravitational lensing and dark energy
• Photon Number Conserving Models of H II Bubbles during Reionization
• Galaxy Evolution and Cosmology with the Square Kilometre Array
• Testing the Modified Press-Schechter Model against N-Body Simulations
• Richness-based masses of rich and famous galaxy clusters
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Gamma-ray probe of cosmic-ray pressure in galaxy clusters and cosmological implications
• Baryons: What, When and Where?
• The halo light cone catalogues of \Abacus{AbacusSummit}
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Gravitational lensing magnification without multiple imaging
• Imprints of quasar duty cycle on the 21cm signal from the Epoch of Reionization
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• Cosmology and Astrophysics from Relaxed Galaxy Clusters V: Consistency with Cold Dark Matter Structure Formation
• Changes in the halo formation rates due to features in the primordial spectrum
• Electromagnetic signatures of supermassive black hole binaries resolved by PTAs
• Neutrino Signatures from the First Stars
• Turning noise into signal: learning from the scatter in the Hubble diagram
• The Total Mass of Dark Matter Haloes
• Cluster counts: calibration issue or new physics?
• Detecting Reionization in the Star Formation Histories of High-Redshift Galaxies
• Physical component analysis of galaxy cluster weak gravitational lensing data
• A new model for the full shape of the large-scale power spectrum
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• Influence of Projection in Cluster Cosmology Studies
• The hybrid SZ power spectrum: Combining cluster counts and SZ fluctuations to probe gas physics
• Galaxy Luminosity Functions in WINGS clusters
• CMB constraints on a physical model of reionization
• Cosmological parameter constraints from CMB lensing with cosmic voids
• On an Analytical Framework for Voids: Their abundances, density profiles and local mass functions
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• Will Multiple Probes of Dark Energy find Modified Gravity?
• Pairwise velocities in the Halo Model: Luminosity and Scale Dependence
• Constraints on shear and rotation with massive galaxy clusters
• Into the Lyα jungle: exploring the circumgalactic medium of galaxies at z ~ 4-5 with MUSE
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• X-ray Cluster Constraints on Non-Gaussianity
• A Solution to the Missing Link in the Press-Schechter Formalism
• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
• Dark Matter-baryon segregation in the non-linear evolution of coupled Dark Energy model
• Euclid: Effect of sample covariance on the number counts of galaxy clusters
• The mass function and distribution of velocity dispersions for UZC groups of galaxies
• Are Simulations of CDM Consistent with Galactic-Scale Observations at High Redshift?
• The Epoch of Reionization 21-cm Bispectrum: The impact of light-cone effects and detectability
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• Non-Gaussian Scatter in Cluster Scaling Relations
• The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
• The peculiar velocities of satellites of external disk galaxies
• Figure rotation of dark halos in CDM simulations
• Galaxy Clusters as a probe of early dark energy
• Probing Population III Initial Mass Functions with He II/H$\alpha$ Intensity Mapping
• The build-up of halos within Press-Schechter theory
• Vector dark energy and high-z massive clusters
• The Formation and Evolution of the First Massive Black Holes
• How many arcminute-separation lenses are expected in the 2dF QSO survey?
• Universal Merger Histories of Dark-Matter Haloes
• Taming assembly bias for primordial non-Gaussianity
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• Measuring Bulk Flow of Galaxy Clusters using Kinematic Sunyaev-Zel'dovich effect: Prediction for Planck
• Detecting the gravitational wave background from primordial black hole dark matter
• Measurements of the Cosmological Evolution of Magnetic Fields with the Square Kilometre Array
• Stochastic background of gravitational waves generated by pre-galactic black holes
• Passive Evolution of Galaxy Clustering
• A determination of dark matter bispectrum with a large set of N-body simulations
• Can We Detect the Anisotropic Shapes of Quasar HII Regions During Reionization Through The Small-Scale Redshifted 21cm Power Spectrum?
• The Cosmological History of Accretion onto Dark Halos and Supermassive Black Holes
• The clustering of baryonic matter. I: a halo-model approach
• The Effect of Radiative Cooling on the Sunyaev-Zel'dovich Cluster Counts and Angular Power Spectrum: Analytic Treatment
• Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Statistical Properties of Radio Halos in Galaxy Clusters and Origin of Seed Electrons for Reacceleration
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• A high-resolution cosmological simulation of a strong gravitational lens
• On the equivalence between the effective cosmology and excursion set treatments of environment
• Cold dark energy constraints from the abundance of galaxy clusters
• Precision cosmology with a combination of wide and deep Sunyaev-Zeldovich cluster surveys
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• A Baryonic Effect on the Merger Timescale of Galaxy Clusters
• Extending Recovery of the Primordial Matter Power Spectrum
• Cluster Lensing of QSOs as a Probe of LCDM and Dark Energy Cosmologies
• Extreme value statistics of weak lensing shear peak counts
• Constraining quasar host halo masses with the strength of nearby Lyman-alpha forest absorption
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• On the cosmological mass function theory
• Weak lensing by triaxial galaxy clusters
• Detection and Fundamental Applications of Individual First Galaxies
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• The Size Distribution of Void Filaments in a LCDM Cosmology
• Counts of galaxy clusters as cosmological probes: the impact of baryonic physics
• A Phenomenological Model for the Intracluster Medium that matches X-ray and Sunyaev-Zel'dovich observations
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• 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 Diffuse Gamma-Ray Flux from Clusters of Galaxies
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• The Mass Function of Void Groups as a Probe of the Primordial non-Gaussianity
• The evolution of star formation activity in galaxy groups
• Tracing the Nature of Dark Energy with Galaxy Distribution
• Statistics of Quasars Multiply Imaged by Galaxy Clusters
• Halo Occupation Distribution of Massive Galaxies since z = 1
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• Are the 2dFGRS superstructures a problem for hierarchical models?
• Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
• Optical Galaxy Clusters in the Deep Lens Survey
• The most massive Population III stars
• Optimizing measurements of cluster velocities and temperatures for CCAT-prime and future surveys
• Competitive Accretion in Sheet Geometry and the Stellar IMF
• A Better Way to Define Dark Matter Haloes
• Probing dark energy with the next generation X-ray surveys of galaxy clusters
• The Race Between Stars and Quasars in Reionizing Cosmic Hydrogen
• The abundance of dark matter haloes down to Earth mass
• Virial halo mass function in the $Planck$ cosmology
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect
• The distribution of two-dimensional eccentricity of Sunyaev-Zeldovich Effect and X-ray surface brightness profiles
• Large Scale Structure Forecast Constraints on Particle Production During Inflation
• Validation of Selection Function, Sample Contamination and Mass Calibration in Galaxy Cluster Samples
• Sunyaev-Zel'dovich Cluster Survey Simulations for Planck
• Properties of High Redshift Quasars-I: Evolution of the super-massive black-hole to halo mass ratio
• Probing a cosmological model with a $\Lambda ={\Lambda }_0+3\beta H^2$ decaying-vacuum
• 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
• The Effect of Formation Redshifts on the Cluster Mass-Temperature Relation
• Dynamics and constraints of the dissipative Liouville cosmology
• Neutrino Mass Inference from SZ Surveys
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• Pure Density Evolution of the Ultraviolet Quasar Luminosity Function at $2\lesssim z\lesssim 6$
• Pregalactic LiBeB Production by Supernova Cosmic Rays
• Cosmological Perturbations and the Running Cosmological Constant Model
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• 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
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Testing model independent modified gravity with future large scale surveys
• The Halo Occupation Distribution of HI from 21cm Intensity Mapping at Moderate Redshifts
• Discriminating power of milli-lensing observations for dark matter models
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• Halo Mass Definition and Multiplicity Function
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• Constraining CMB-consistent primordial voids with cluster evolution
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
• Statistics of gravitational potential perturbations: A novel approach to deriving the X-ray temperature function
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• Detailed theoretical predictions of the outskirts of dark matter halos
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Expected properties of the Two-Point Autocorrelation Function of the IGM
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Evidence for new physics from clusters ?
• Number Counts and Dynamical Vacuum Cosmologies
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• 21-cm signatures of residual HI inside cosmic HII regions during reionization
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• On the Angular Correlation Function of SZ Clusters : Extracting cosmological information from a 2D catalog
• Cluster Probes of Dark Energy Clustering
• Stacking Clusters in the ROSAT All-Sky Survey
• High-redshift voids in the excursion set formalism
• The mass function of the Las Campanas loose groups of galaxies
• Cusp-core problem and strong gravitational lensing
• How far are the sources of IceCube neutrinos? Constraints from the diffuse TeV gamma-ray background
• Bumpy Power Spectra and Galaxy Clusters
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• A prescription for the conditional mass function of dark matter haloes
• Biases on cosmological parameter estimators from galaxy cluster number counts
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• Constraining thawing and freezing models with cluster number counts
• Comparing cosmic shear measures - Optimizing the Information content of cosmic shear data vectors
• Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• Cluster-Cluster Lensing and the Case of Abell 383
• Toward an Improved Analytical Description of Lagrangian Bias
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Nonlinear stochastic biasing of halos: Analysis of cosmological N-body simulations and perturbation theories
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Modelling the stochasticity of high-redshift halo bias
• Nonsingular density profiles of dark matter halos and Strong gravitational lensing
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Constraining Cosmological Models by the Cluster Mass Function
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• The Properties of X-ray Cold Fronts in a Statistical Sample of Simulated Galaxy Clusters
• Semi-numeric simulations of helium reionization and the fluctuating radiation background
• Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ΛCDM
• Multiply-imaged time-varying sources behind galaxy clusters - Comparing FRBs to QSOs, SNe, and GRBs
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Dynamical quintessence fields Press-Schechter mass function: detectability and effect on dark haloes
• Unveiling cosmological information on small scales with line intensity mapping
• Probing dark energy via galaxy cluster outskirts
• Testing the accuracy of likelihoods for cluster abundance cosmology
• The ALFALFA HI velocity width function
• Implications of the Lyman alpha Emission Line from a Candidate z=10 Galaxy
• A novel approach to cosmological non-linearities as an effective fluid
• Variation in the escape fraction of ionising photons from galaxies and the redshifted 21-cm power spectrum during reionization
• Spherical collapse of dark matter haloes in tidal gravitational fields
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• The galaxy luminosity function around groups
• Gravitational Collapse of Baryonic and Dark matter
• Cosmological constraints from the masses and abundances of L* galaxies
• Evolution of the cosmological mass function in a moving barrier model
• Using clusters in SZE + x-ray surveys as an ensemble of rulers to constrain cosmology
• Predicting the clustering properties of galaxy clusters detectable for the Planck satellite
• The mass and temperature functions in a moving barrier model
• The amplitude of mass fluctuations and mass density of the Universe constrained by strong gravitational lensing
• Strong-lensing cosmography using third-generation gravitational-wave detectors
• CMB-Normalized Predictions for Sunyaev-Zel'dovich effect fluctuations
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• Deep learning insights into cosmological structure formation
• The U-band Galaxy Luminosity Function of Nearby Clusters
• Simulating the formation of cosmic structure
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Halo abundances and shear in void models
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Constraining stellar assembly and AGN feedback at the peak epoch of star formation
• Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations
• Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy
• On the primordial information available to galaxy redshift surveys
• An Introduction into the Theory of Cosmological Structure Formation
• The virialization density of peaks with general density profiles under spherical collapse
• Systematic errors in the determination of Hubble constant due to the asphericity and non-isothermality of clusters of galaxies
• Setting the Stage: Structures from Gaussian Random Fields
• 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
• Gravitational wave constraints on extended dark matter structures
• Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
• X-ray Clusters of Galaxies as Cosmological Tools
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Halo Model Analysis of Cluster Statistics
• Sunyaev-Zel'dovich power spectrum with decaying cold dark matter
• The spherical collapse model with shell crossing
• Recovering the Tidal Field in the Projected Galaxy Distribution
• X-ray galaxy clusters abundance and mass temperature scaling
• Do all QSOs have the same black hole mass?
• 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
• A blind detection of a large, complex, Sunyaev--Zel'dovich structure
• Extended Press-Schechter theory and the density profiles of dark matter haloes
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Efficient simulation of discrete galaxy populations and associated radiation fields during the first billion years
• Dark matter halo mass functions and density profiles from mass and energy cascade
• The rms peculiar velocity of galaxy clusters for different cluster masses and radii
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius
• Dust obscuration studies along quasar sight lines using simulated galaxies
• Numerical action reconstruction of the dynamical history of dark matter haloes in N-body simulations
• Galaxy flows within 8,000 km/s from Numerical Action methods
• Detection of a CMB decrement towards a cluster of mJy radiosources
• The Impact of Secondary non-Gaussianities in the CMB on Cosmological Parameter Estimation
• Third-order cosmological perturbations of zero-pressure multi-component fluids: Pure general relativistic nonlinear effects
• Studying Dark Energy with Galaxy Cluster Surveys
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• A new test for the stable clustering hypothesis
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• An Extended Zel'dovich Model for the Halo Mass Function
• Understanding the Cosmic Mass Function High Mass Behaviour
• Can we distinguish early dark energy from a cosmological constant?
• 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
• Cross-correlation between the soft X-ray background and SZ Sky
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• Compact source detection in multi-channel microwave surveys: from SZ clusters to polarized sources
• Cosmic expansion and structure formation in running vacuum cosmologies
• Gravitational lensing effects on sub-millimetre galaxy counts
• Biasing and Genus Statistics of Dark Matter Halos in the Hubble Volume Simulation
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Constraining the mass-concentration relation through weak lensing peak function
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• An Evolving Entropy Floor in the Intracluster Gas?
• Self-Consistent Theory of Halo Mergers - II: CDM Power Spectra
• Predictions for the Counts of Faint, High-Redshift Galaxies in the Mid-Infrared
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• Imprint of massive neutrinos on Persistent Homology of large-scale structure
• Cosmological Implications and Physical Properties of an X-Ray Flux-Limited Sample of Galaxy Clusters
• 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
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• The fractional Brownian motion and the halo mass function
• Non-Markov Excursion Set Model of Dark Matter Halo Abundances
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• Constraints on the warm dark matter model from gravitational lensing
• The abundance and environment of dark matter haloes
• Probing the Primordial Power Spectrum with Cluster Number Counts
• X-ray cluster cosmology
• Core Mass Estimates in Strong Lensing Galaxy Clusters Using a Single-Halo Lens Model
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Optimizing the yield of Sunyaev-Zel'dovich cluster surveys
• Halo mass function in scale invariant models
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Haloes at the ragged edge: The importance of the splashback radius
• Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
• Tree-less 3d Friends-of-Friends using Spatial Hashing
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• Complementary Cosmological Simulations
• The baryon mass function for galaxy clusters
• Anisotropies in the redshift-space correlations of galaxy groups and clusters I: Simulated catalogues
• Nonlinear structure formation in Bound Dark Energy
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• The Effects of Relativistic Corrections on Cosmological Parameter Estimations from SZE Cluster Surveys
• Improvements in the M-T relation and mass function and the measured Omega_m through clusters evolution
• Deep learning insights into non-universality in the halo mass function
• Complementarity of Future Dark Energy Probes
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Cluster Assembly Times as a Cosmological Test
• Observations of Ly$\alpha$ Emitters at High Redshift
• An expanded merger-tree description of cluster evolution
• Cluster contribution to the X-ray background as a cosmological probe
• 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
• Cosmic reionization constraints on the nature of cosmological perturbations
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• On the reliability of initial conditions for dissipationless cosmological simulations
• DUET - The Dark Universe Exploration Telescope
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
• The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Non-linear matter power spectrum without screening dynamics modelling in $f(R)$ gravity
• Universality of the halo mass function in screened gravity theories
• Dark matter haloes: a multistream view
• An X-ray Galaxy Cluster Survey for Investigations of Dark Energy
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions
• An Empirical Mass Function Distribution
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Strong Lensing Probabilities in a Cosmological Model with a Running Primordial Power Spectrum
• Accurate halo mass functions from the simplest excursion set theory
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• Massive Black Hole Mergers
• Stochastic backgrounds of gravitational waves from cosmological sources - The role of dark energy
• Measuring Omega_m using clusters evolution
• Structural and Photometric Properties of the Andromeda Satellite Dwarf Galaxy Lacerta I from Deep Imaging with WIYN pODI
• Evolution of Power Spectrum in Non-Gaussian Models
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Bayesian analysis of spatially distorted cosmic signals from Poissonian data
• AMICO galaxy clusters in KiDS-1000: cosmological sample
• Machine Learning and Structure Formation in Modified Gravity
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Thermodynamic evolution of the cosmological baryonic gas : II. Galaxy formation
• Systematic bias in the estimate of cluster mass and the fluctuation amplitude from cluster abundance statistics
• A Parameter-free Statistical Measurement of Halos with Power Spectra
• Stochastic Gravitational Wave Background originating from Halo Mergers
• Convergence of halo statistics: code comparison between Rockstar and CompaSO using scale-free simulations
• Global 21 cm signal: a promising probe of primordial features
• Characterising the optical properties of galaxy clusters with GMPhoRCC
• 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
• The Splashback Mass Function in the Presence of Massive Neutrinos
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• Simulating Binary Primordial Black Hole Mergers in Dark Matter Halos
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Simulations and Observations of the Microwave Universe
• Cosmological parameters from Galaxy Clusters: an Introduction
• Statistical Properties of Supercluster-Like Filaments from Cosmological Simulations
• The Halo Mass Function Redshift Dependence
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Cosmological constraints from the thermal Sunyaev Zeldovich power spectrum?
• Spatial clustering in the ESO-Sculptor Survey: two-point correlation functions by galaxy type at redshifts 0.1 - 0.5
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Sunyaev-Zel'dovich contribution in CMB analysis
• Determination of the Linear Mass Power Spectrum From the Mass Function of Galaxy Clusters
• AMI-CL J0300+2613: a Galactic anomalous-microwave-emission ring masquerading as a galaxy cluster
• Effect of the Cosmological Constant on Halo Size
• Directional miscentering dependence in weak lensing mass bias
• The MeerKAT Fornax Survey VI. The collapse of the galaxy HI Mass Function in Fornax
• Probability distribution and statistical properties of spherically compensated cosmic regions in $\Lambda$CDM cosmology
• Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
• Galaxies and Cluster of Galaxies as Peak Patches of the Density Field
• Formation of Dark Matter Haloes in a Homogeneous Dark Energy Universe
• On Local Approximations to the Nonlinear Evolution of Large-Scale Structure
• The Contribution of Galaxies to the $3.4\mu \mathrm{m}$ Cosmic Infrared Background as Measured Using WISE
• Quinstant Dark Energy Predictions for Structure Formation
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid
• The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to $z=1$
• Excursion Sets with a "Perfect" Collapse Model
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• A flat faint end of the Fornax cluster galaxy luminosity function
• Tracking through equality
• Measuring the baryon fraction in cluster of galaxies with Kinematic Sunyaev Zeldovich and a Standard Candle
• The haloes that reionized the Universe
• Modeling Dark Matter Halos with Nonlinear Field Theories
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Extended Hernquist-Springel formalism for cosmic star formation
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• 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
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• Effects of dynamical friction on perturbations for evolving dark energy
• Searching for Clusters with SUMSS
• Dark Energy Simulations
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• Transition between order and chaos in a composite disk galaxy model with a massive nucleus and a dark matter halo
• Particle Reacceleration by Turbulence and Radio Constraints on Multi-Messenger High-Energy Emission from the Coma Cluster
• The Mass Function of Dark Matter Haloes in a Cosmological Model with a Running Primordial Power Spectrum
• Slicing cluster mass functions with a Bayesian razor
• Ginnungagap -- a massively parallel cosmological initial conditions generator
• Cosmological constraints from clustering properties of galaxy clusters
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• The History of Galaxy Formation in Groups: An Observational Perspective
• A redshift distortion free correlation function at third order in the nonlinear regime
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• Using Dark Matter Haloes to Learn about Cosmic Acceleration: A New Proposal for a Universal Mass Function
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos
• Probing power spectrum enhancement at small scales with the SKA
• BRIGHT lights, BIG city: Massive galaxies, giant Ly-a nebulae, and proto--clusters
• Universality of the halo mass function in modified gravity cosmologies
• Mass functions from the excursion set model
• The Relic Neutrino Backround from the First Stars
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Clustering properties of TGSS radio sources
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• 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
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity