Large scale bias and the peak background split

Abstract

Dark matter haloes are biased tracers of the underlying dark matter distribution. We use a simple model to provide a relation between the abundance of dark matter haloes and their spatial distribution on large scales. Our model shows that knowledge of the unconditional mass function alone is sufficient to provide an accurate estimate of the large scale bias factor. Then we use the mass function measured in numerical simulations of SCDM, OCDM and LCDM to compute this bias. Comparison with these simulations shows that this simple way of estimating the bias relation and its evolution is accurate for less massive haloes as well as massive ones. In particular, we show that haloes which are less/more massive than typical M* haloes at the time they form are more/less strongly clustered than formulae based on the standard Press-Schechter mass function predict.

8 pages, 6 figures, submitted to MNRAS corrected y-label for fig.4 (newlabel = 1 + oldlabel)

References in corpus (6)

• Accurate fitting formula for the two-point correlation function of the dark matter halos
• Biasing and the distribution of dark matter haloes
• Modelling the evolution of galaxy clustering
• Accurate determination of the Lagrangian bias for the dark matter halos
• How the dark matter halos cluster in Lagrangian space
• Empirical Constraints on the First Stars and Quasars

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• The 21 centimeter emission from the reionization epoch: extended and point source foregrounds
• The XMM Large Scale Structure survey: The X-ray pipeline and survey selection function
• Probing Anisotropies of the Stochastic Gravitational Wave Background with LISA
• Halo Clustering with Non-Local Non-Gaussianity
• Internal properties and environments of dark matter halos
• The Formation of the First Stars in the Universe
• Cluster Density Profiles as a Test of Modified Gravity
• Massive black holes lurking in Milky Way satellites
• The effects of baryons on the halo mass function
• On the Level of Cluster Assembly Bias in SDSS
• ORIGAMI: Delineating Halos using Phase-Space Folds
• Global Probes of the Impact of Baryons on Dark Matter Halos
• Populating Dark Matter Haloes with Galaxies: Comparing the 2dFGRS with Mock Galaxy Redshift Surveys
• Cluster abundance normalization from observed mass-temperature relation
• Unbiased constraints on ultralight axion mass from dwarf spheroidal galaxies
• Redshift space correlations and scale-dependent stochastic biasing of density peaks
• Direct collapse black hole formation from synchronized pairs of atomic cooling halos
• Position-dependent power spectrum of the large-scale structure: a novel method to measure the squeezed-limit bispectrum
• Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: cosmological implications
• The Clustering of Massive Halos
• The REACH radiometer for detecting the 21-cm hydrogen signal from redshift 7.5 to 28
• Tests for primordial non-Gaussianity
• Scale-dependent galaxy bias, CMB lensing-galaxy cross-correlation, and neutrino masses
• Predicting the cosmological constant with the scale-factor cutoff measure
• Black Hole and Galaxy Coevolution from Continuity Equation and Abundance Matching
• Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
• Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
• Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
• How does radiative feedback from a UV background impact reionization?
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• Ly-alpha Emitting Galaxies at z = 2.1: Stellar Masses, Dust and Star Formation Histories from Spectral Energy Distribution Fitting
• Dark matter annihilation or unresolved astrophysical sources? Anisotropy probe of the origin of cosmic gamma-ray background
• HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies
• Spitzer bright, UltraVISTA faint sources in COSMOS: the contribution to the overall population of massive galaxies at z=3-7
• On the radiative efficiencies, Eddington ratios, and duty cycles of luminous high-redshift quasars
• Infrared background signatures of the first black holes
• The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution
• Dissecting the properties of optically-thick hydrogen at the peak of cosmic star formation history
• The Keck+Magellan Survey for Lyman Limit Absorption I: The Frequency Distribution of Super Lyman Limit Systems
• Future Galaxy Cluster Surveys: The Effect of Theory Uncertainty on Constraining Cosmological Parameters
• The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
• Interpreting the Observed Clustering of Red Galaxies at z~3
• The real-space clustering of luminous red galaxies around z<0.6 quasars in the Sloan Digital Sky Survey
• The effect of foreground subtraction on cosmological measurements from Intensity Mapping
• Testing the Warm Dark Matter paradigm with large-scale structures
• Cosmological Constraints From Weak Lensing Peak Statistics With CFHT Stripe 82 Survey
• Collapse Barriers and Halo Abundance: Testing the Excursion Set Ansatz
• The Halo Distribution of 2dF Galaxies
• The Gaussian streaming model and Lagrangian effective field theory
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: II. The clustering of quasars and their dark environment
• Redshift space bias and beta from the halo model
• Neutrino physics from precision cosmology
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• Constraining chameleon models with cosmology
• Scaling Laws in the Distribution of Galaxies
• Reconstructing the Cosmic Velocity and Tidal Fields with Galaxy Groups Selected from the Sloan Digital Sky Survey
• The mass function of high redshift seed black holes
• Linear and nonlinear contributions to pairwise peculiar velocities
• Dark Matter Subhaloes in Numerical Simulations
• A Comparison of Cosmological Codes: Properties of Thermal Gas and Shock Waves in Large Scale Structures
• ICE-COLA: Towards fast and accurate synthetic galaxy catalogues optimizing a quasi $N$-body method
• Halo bias in mixed dark matter cosmologies
• Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
• Constraints on the IMF of the first stars
• Baryon acoustic signature in the clustering of density maxima
• On The Assembly History of Dark Matter Haloes
• The Evidence of Absence: Galaxy Voids in the Excursion Set Formalism
• Spherical Collapse and the Halo Model in Braneworld Gravity
• The Beginning and Evolution of the Universe
• The redshift space power spectrum in the halo model
• An excursion set model of the cosmic web: The abundance of sheets, filaments and halos
• Constraining sterile neutrino cosmologies with strong gravitational lensing observations at redshift z~0.2
• The assembly bias of dark matter haloes to higher orders
• The Fossil Phase in the Life of a Galaxy Group
• The Impact of Cooling and Feedback on Disc Galaxies
• Dark energy and the evolution of spherical overdensities
• Revealing the galaxy-halo connection in IllustrisTNG
• On the origin of the fundamental metallicity relation and the scatter in galaxy scaling relations
• Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties
• Intensity Mapping of Lyman-alpha Emission During the Epoch of Reionization
• A survey of high-$z$ galaxies: SERRA simulations
• The universal nature of subhalo accretion
• Peak-Background Split, Renormalization, and Galaxy Clustering
• Metal Absorption Lines as Probes of the Intergalactic Medium Prior to the Reionization Epoch
• Abundance of damped Lyman-alpha absorbers in cosmological SPH simulations
• The Number of Supernovae from Primordial Stars in the Universe
• JKCS041: a colour-detected galaxy cluster at z_phot=1.9 with deep potential well as confirmed by X-ray data
• Clustering of K-selected Galaxies at 2<z<3.5: Evidence for a Color-Density Relation
• The Abundance and Radial Distribution of Satellite Galaxies
• Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias
• Studying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2
• Supermassive Black Holes in the Hierarchical Universe: A General Framework and Observational Tests
• Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time
• The Horizon Run N-body Simulation: Baryon Acoustic Oscillations and Topology of Large Scale Structure of the Universe
• Dark energy in light of the early JWST observations: case for a negative cosmological constant?
• Predicting the number, spatial distribution and merging history of dark matter haloes
• Measuring neutrino masses and dark energy with weak lensing tomography
• 21CMMC with a 3D light-cone: the impact of the co-evolution approximation on the astrophysics of reionisation and cosmic dawn
• Using Galaxy Two-point Correlation Functions to Determine the Redshift Distributions of Galaxies Binned by Photometric Redshift
• What is L*?: Anatomy of the Galaxy Luminosity Function
• Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
• Evolution in the structural properties of early-type Brightest Cluster Galaxies at small lookback time and dependence on the environment
• Peaks theory and the excursion set approach
• Cubic Halo Bias in Eulerian and Lagrangian Space
• Dependence of Halo Properties on Interaction History, Environment and Cosmology
• The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey
• The Role of the Dust in Primeval Galaxies: A Simple Physical Model for Lyman Break Galaxies and Lyman Alpha Emitters
• Galaxy Assembly Bias on the Red Sequence
• Cosmological Origin of the Stellar Velocity Dispersions in Massive Early-Type Galaxies
• The impact of massive neutrinos on the abundance of massive clusters
• Constraints on dark matter annihilation from CMB observations before Planck
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• The First Stars in The Universe
• The History and Morphology of Helium Reionization
• Size bias and differential lensing of strongly lensed, dusty galaxies identified in wide-field surveys
• Non-linear Structure Formation in Cosmologies with Early Dark Energy
• The Large-scale Distribution of Cool Gas around Luminous Red Galaxies
• The Galaxy Power Spectrum and Bispectrum in Redshift Space
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• Effects and Detectability of Quasi-Single Field Inflation in the Large-Scale Structure and Cosmic Microwave Background
• Substructure of fuzzy dark matter haloes
• Three-Dimensional Identification and Reconstruction of Galaxy Systems within Deep Redshift Surveys
• Measurement of Galaxy Clustering at z~7.2 and the Evolution of Galaxy Bias from 3.8<z<8 in the XDF, GOODS-S AND GOODS-N
• Early Formation and Late Merging of the Giant Galaxies
• Halo properties in models with dynamical Dark Energy
• Halo-model signatures from 380,000 SDSS Luminous Red Galaxies with photometric redshifts
• GOTPM: A Parallel Hybrid Particle-Mesh Treecode
• Cross-correlation Weak Lensing of SDSS Galaxy Clusters III: Mass-to-light Ratios
• Intensity mapping of [CII] from early galaxies
• Modeling halo mass functions in chameleon f(R) gravity
• Forecasts on the Dark Energy and Primordial Non-Gaussianity Observations with the Tianlai Cylinder Array
• Radio Galaxy populations and the multi-tracer technique: pushing the limits on primordial non-Gaussianity
• Constraints on leptonically annihilating Dark Matter from reionization and extragalactic gamma background
• Evaluating Semi-Analytic Halo Merging Histories
• The Three-Point Correlation Function of Luminous Red Galaxies in the Sloan Digital Sky Survey
• An improved model for the formation times of dark matter haloes
• Secondary anisotropies of the CMB
• Dark matter and structure formation a review
• Non-Gaussian Halo Bias Re-examined: Mass-dependent Amplitude from the Peak-Background Split and Thresholding
• The Halo Mass Function from Excursion Set Theory. III. Non-Gaussian Fluctuations
• \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities
• Galaxy bispectrum, primordial non-Gaussianity and redshift space distortions
• The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos
• Cross-correlation between the CMB lensing potential measured by Planck and high-z sub-mm galaxies detected by the Herschel-ATLAS survey
• Bispectrum and Nonlinear Biasing of Galaxies: Perturbation Analysis, Numerical Simulation and SDSS Galaxy Clustering
• The NGC 5846 Group: Dynamics and the Luminosity Function to M_R=-12
• The most luminous quasars do not live in the most massive dark matter haloes at any redshift
• PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
• keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: The Most General Case
• A Comparison of Semi-Analytic and Smoothed Particle Hydrodynamics Galaxy Formation
• The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5
• Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids
• De-contamination of cosmological 21-cm maps
• Weighing Neutrinos with Galaxy Cluster Surveys
• On the Distribution of Haloes, Galaxies and Mass
• Preheating by Previrialization and its Impact on Galaxy Formation
• Imaging of SDSS z>6 quasar fields: gravitational lensing, companion galaxies and the host dark matter halos
• The Weak Lensing Signal and the Clustering of BOSS Galaxies I: Measurements
• Clustering of Star-forming Galaxies Near a Radio Galaxy at z=5.2
• The image separation distribution of strong lenses: Halo versus subhalo populations
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• Cosmological performance of SKA HI galaxy surveys
• A hydrodynamical halo model for weak-lensing cross correlations
• Probing Reionization with Intensity Mapping of Molecular and Fine Structure Lines
• Clustering of Lyman alpha emitters at z ~ 4.5
• A model for the cosmological evolution of low frequency radio sources
• Properties of host haloes of Lyman-break galaxies and Lyman-alpha Emitters from their number densities and angular clustering
• On Squeezed Limits in Single-Field Inflation - Part I
• Constraining the primordial black hole abundance with 21cm cosmology
• The Void Size Function in Dynamical Dark Energy Cosmologies
• Searching for dark matter halos in the Suprime-Cam 2 sq deg field
• Cross-Correlation Lensing: Determining Galaxy and Cluster Mass Profiles from Statistical Weak Lensing Measurements
• Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types
• Clustering of Radio Galaxies and Quasars
• Dark Photon Stars: Formation and Role as Dark Matter Substructure
• Binary Aggregations in Hierarchical Galaxy Formation: The Evolution of the Galaxy Luminosity Function
• Dissecting and Modelling Galaxy Assembly Bias
• Probing Dark Low-mass Halos and Primordial Black Holes with Frequency-dependent Gravitational Lensing Dispersions of Gravitational Waves
• Formation of galactic nuclei with multiple supermassive black holes at high redshifts
• Simulations and symmetries
• High-redshift radio galaxies: a potential new source of 21-cm fluctuations
• The Masses, Ancestors and Descendents of Extremely Red Objects: Constraints from Spatial Clustering
• Large scale bias and the inaccuracy of the peak-background split
• Environmental dependence in the ellipsoidal collapse model
• cosmoabc: Likelihood-free inference via Population Monte Carlo Approximate Bayesian Computation
• Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
• Excursion set peaks: a self-consistent model of dark halo abundances and clustering
• Interpreting LOFAR 21-cm signal upper limits at z~9.1 in the context of high-z galaxy and reionisation observations
• Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering
• Damped Lyman-alpha systems in high-resolution hydrodynamical simulations
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Evolution of Massive Haloes in non-Gaussian Scenarios
• The Effect of Gas Physics on the Halo Mass Function
• Constraints on the missing baryons from the kinetic Sunyaev-Zeldovich effect in Planck data
• Bias Loop Corrections to the Galaxy Bispectrum
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• On the reach of perturbative descriptions for dark matter displacement fields
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from counts and stacked weak-lensing
• The subtlety of Ly-a photons: changing the expected range of the 21-cm signal
• An analytic model for the bispectrum of galaxies in redshift space
• High-Redshift Galaxies from Early JWST Observations: Constraints on Dark Energy Models
• A New Constraint on Reionization from Evolution of the Ly$\alpha$ Luminosity Function at $z\sim 6-7$ Probed by a Deep Census of $z=7.0$ Ly$\alpha$ Emitter Candidates to 0.3 $L^{\ast }$
• The physics of gas phase metallicity gradients in galaxies
• Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• High-Redshift Star Formation in a Time-Dependent Lyman-Werner Background
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• CosmoBolognaLib: C++ libraries for cosmological calculations
• The Spatial Clustering of ROSAT All-Sky Survey AGNs II. Halo Occupation Distribution Modeling of the Cross Correlation Function
• The Three Causes of Low-Mass Assembly Bias
• Structure formation in inhomogeneous Early Dark Energy models
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey III: The Power Spectrum
• Noisy weak-lensing convergence peak statistics near clusters of galaxies and beyond
• Cosmological Reconstruction From Galaxy Light: Neural Network Based Light-Matter Connection
• Self-Consistent Theory of Halo Mergers
• Blazars in the early Universe
• The distribution of red and blue galaxies in groups: an empirical test of the halo model
• Modeling Intra-Cluster Gas in Triaxial Dark Halos : An Analytical Approach
• The Epoch of Reionization in Models with Reduced Small Scale Power
• Spherical collapse model in dark energy cosmologies
• The stellar-subhalo mass relation of satellite galaxies
• The brief era of direct collapse black hole formation
• A dark matter interpretation for the ARCADE excess?
• Early Structure Formation and Reionization in a Cosmological Model with a Running Primordial Power Spectrum
• Primordial Non-Gaussianity from Biased Tracers: Likelihood Analysis of Real-Space Power Spectrum and Bispectrum
• Cosmological Simulations for Combined-Probe Analyses: Covariance and Neighbour-Exclusion Bias
• The integrated Sachs-Wolfe Effect -- Large Scale Structure Correlation
• unWISE tomography of Planck CMB lensing
• Galaxy Formation at z~3: Constraints from Spatial Clustering
• Large-Scale Structure in Brane-Induced Gravity II. Numerical Simulations
• Large-Scale Structure Shocks at Low and High Redshifts
• Cosmology from the Thermal Sunyaev-Zel'dovich Power Spectrum: Primordial non-Gaussianity and Massive Neutrinos
• Cosmic voids in modified gravity models with massive neutrinos
• Weak Gravitational Lensing Bispectrum
• The Nature of Extremely Red H-[4.5]>4 Galaxies revealed with SEDS and CANDELS
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• Simulations of Axion Minihalos
• Pair-Instability Supernovae at the Epoch of Reionization
• The Dependence of the Galaxy Luminosity Function on Large-Scale Environment
• The statistical properties of LCDM halo formation
• Revealing dark matter substructure with anisotropies in the diffuse gamma-ray background
• 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
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• Constraints on the correlation between QSO luminosity and host halo mass from high-redshift quasar clustering
• Probing the galaxy-halo connection in UltraVISTA to $z\sim 2$
• On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond $\Lambda$CDM
• The angle-averaged squeezed limit of nonlinear matter N-point functions
• Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
• Assessing the redshift evolution of massive black holes and their hosts
• Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
• Faint Submillimeter Galaxies Revealed by Multifield Deep ALMA Observations: Number Counts, Spatial Clustering, and A Dark Submillimeter Line Emitter
• LoCuSS: Hydrostatic Mass Measurements of the High-$L_X$ Cluster Sample -- Cross-calibration of Chandra and XMM-Newton
• The Anisotropic Distribution of Satellite Galaxies
• Primordial power spectrum in light of JWST observations of high redshift galaxies
• Towards a self-consistent halo model for the nonlinear large-scale structure
• The impact of Early Dark Energy on non-linear structure formation
• Modeling Dynamical Dark Energy
• Nonlinear structure formation in Nonlocal Gravity
• The Multiwavelength Survey by Yale-Chile (MUSYC): Wide K-band Imaging, Photometric Catalogs, Clustering and Physical Properties of Galaxies at z~2
• The distribution of ejected subhalos and its implication for halo assembly bias
• The Local Bias Model in the Large Scale Halo Distribution
• Chemical evolution in a model for the joint formation of quasars and spheroids
• The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
• Constraints on the annihilation cross section of dark matter particles from anisotropies in the diffuse gamma-ray background measured with Fermi-LAT
• Did JWST observe imprints of axion miniclusters or primordial black holes?
• On the linearity of tracer bias around voids
• Spherical collapse model with shear and angular momentum in dark energy cosmologies
• Sunyaev-Zeldovich effect from hydrodynamical simulations: maps and low order statistics
• Bayesian inference of galaxy formation from the K-band luminosity function of galaxies: tensions between theory and observation
• The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys
• Effective Models for Statistical Studies of Galaxy-Scale Gravitational Lensing
• Distribution function approach to redshift space distortions. Part IV: perturbation theory applied to dark matter
• The clustering of radio galaxies at z~0.55 from the 2SLAQ LRG survey
• Halo model and halo properties in Galileon gravity cosmologies
• The Persistence of Population III Star Formation
• SXDF-ALMA 2 arcmin${}^2$ Deep Survey: 1.1-mm Number Counts
• Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
• The SDSS-DR12 large-scale cross-correlation of Damped Lyman Alpha Systems with the Lyman Alpha Forest
• Spectral Line De-confusion in an Intensity Mapping Survey
• The cosmology dependence of weak lensing cluster counts
• The Near-IR Background Intensity and Anisotropies During The Epoch of Reionization
• The 21cm Signature of the First Stars
• Galaxy clustering from COMBO-17: The halo occupation distribution at <z>=0.6
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey I: Probing galaxy cluster magnetic fields with line of sight rotation measures
• Projection effects in the strong lensing study of subhaloes
• The nature of dark matter from the global high redshift HI 21 cm signal
• Cosmology with intensity mapping techniques using atomic and molecular lines
• UV Radiative Feedback on High-Redshift Proto-Galaxies
• Simulating the assembly of galaxies at redshifts z = 6 - 12
• Mass functions in coupled Dark Energy models
• Clustering, Bias and the Accretion Mode of X-ray selected AGN
• Distribution of Damped Lyman-alpha Absorbers in a Lambda Cold Dark Matter Universe
• The Impact of Box Size on the Properties of Dark Matter Haloes in Cosmological Simulations
• Chameleon Halo Modeling in f(R) Gravity
• Reionization and Galaxy Formation in Warm Dark Matter Cosmologies
• Dark matter halo abundances, clustering and assembly histories at high redshift
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Do Distinct Cosmological Models Predict Degenerate Halo Populations?
• Verifying the consistency relation for the scale-dependent bias from local primordial non-Gaussianity
• PRIMUS + DEEP2: Clustering of X-ray, Radio and IR-AGN at z~0.7
• The First Generation of Star-Forming Haloes
• The halo model for cosmology: a pedagogical review
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• The abundance of dark galaxies
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Lyman Alpha Emitters and Lyman Break Galaxies: dichotomous twins?
• Primordial Non-Gaussianity and the NRAO VLA Sky Survey
• The environmental dependence of galaxy clustering in the Sloan Digital Sky Survey
• Can Dark Matter Annihilation Dominate the Extragalactic Gamma-Ray Background?
• Weighing neutrinos with cosmic neutral hydrogen
• A novel approach in the WIMP quest: Cross-Correlation of Gamma-Ray Anisotropies and Cosmic Shear
• Early galaxy formation in warm dark matter cosmologies
• Interpreting the Global 21-cm Signal from High Redshifts. II. Parameter Estimation for Models of Galaxy Formation
• Exploring reionisation and high-z galaxy observables with recent multi-redshift MWA upper limits on the 21-cm signal
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• Accurate Predictions for the Scale-Dependent Galaxy Bias from Primordial Non-Gaussianity
• Lensing Optical Depth for Substructure and Isolated Dark Matter Halos
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• The impact of baryon physics on the structure of high-redshift galaxies
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• A physical model for the evolving UV luminosity function of high redshift galaxies and their contribution to the cosmic reionization
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• Cross-Correlation of Cosmic Shear and Extragalactic Gamma-ray Background: Constraints on the Dark Matter Annihilation Cross-Section
• Weak lensing measurement of galaxy clusters in the CFHTLS-Wide survey
• How Dark Matter Reionized The Universe
• The Extended Starformation History of the First Generation of Stars, and the Reionization of Cosmic Hydrogen
• Where Do Galaxies End?
• The Implications of a Pre-reionization 21 cm Absorption Signal for Fuzzy Dark Matter
• Comparison of Analytical Mass Functions with Numerical Simulations
• How unusual are the Shapley Supercluster and the Sloan Great Wall?
• The 2dF Galaxy Redshift Survey: Clustering properties of radio galaxies
• Very small-scale clustering of quasars from a complete quasar lens survey
• Clustering of sub-millimeter galaxies in a self-regulated baryon collapse model
• Probing Dark Matter Substructure with Pulsar Timing
• On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion
• Signatures of reionization on Lyman alpha emitters
• CMB photons shedding light on dark matter
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• The clustering of SDSS galaxy groups: mass and color dependence
• Focusing on Warm Dark Matter with Lensed High-redshift Galaxies
• Halo bias in Lagrangian Space: Estimators and theoretical predictions
• Correlation properties of the kinematic Sunyaev-Zel'dovich effect and implications for Dark Energy
• Hierarchical Formation of Galaxies with Dynamical Response to Supernova-Induced Gas removal
• Spherical collapse in $\nu \Lambda CDM$
• The halo model in a massive neutrino cosmology
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Baryonic Conversion Tree: The global assembly of stars and dark matter in galaxies from the SDSS
• A new stochastic approach to cumulative weak lensing
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Foreground contamination in Ly-alpha intensity mapping during the epoch of reionization
• Production of Sterile Neutrino Dark Matter and the 3.5 keV line
• The 21 cm signal and the interplay between dark matter annihilations and astrophysical processes
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• Machine learning cosmological structure formation
• Universal at last? The splashback mass function of dark matter halos
• Constraints on Warm Dark Matter models from high-redshift long gamma-ray bursts
• Primordial non-Gaussianity from the covariance of galaxy cluster counts
• Halo modelling in chameleon theories
• GLAMER Part II: Multiple Plane Gravitational Lensing
• The VIMOS-VLT Deep Survey: Luminosity dependence of clustering at z~1
• Modelling the correlation between the thermal Sunyaev Zel'dovich effect and the cosmic infrared background
• Non-Gaussian Aspects of Thermal and Kinetic Sunyaev-Zel'dovich Effects
• Probing the Epoch of Reionization with Milky Way Satellites
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• The atomic Hydrogen content of the post-reionization Universe
• CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales
• Constraining halo occupation properties of X-ray AGNs using clustering of Chandra sources in the Bootes survey region
• A Lightcone Catalogue from the Millennium-XXL Simulation
• Constraining evolution in the Halo Model using galaxy redshift surveys
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Dark matter searches in the gamma-ray extragalactic background via cross-correlations with galaxy catalogues
• Clustering properties of moderate luminosity X-ray selected Type 1 and Type 2 AGN at z~3
• Particle dark matter searches in the anisotropic sky
• Cosmic Neutron Star Merger Rate and Gravitational Waves constrained by the R Process Nucleosynthesis
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• Numerical resolution limits on subhalo abundance matching
• Limits on Population III star formation in minihaloes implied by Planck
• The Brightest Ly$\alpha$ Emitter: Pop III or Black Hole?
• Dwarf Dark Matter Halos
• Primordial non-Gaussianity in the large scale structure of the Universe
• Binary Quasars at High Redshift II: Sub-Mpc Clustering at z ~ 3-4
• Information content in the halo-model dark-matter power spectrum
• A Confirmation of the Strong Clustering of Distant Red Galaxies at 2 < z <3
• The Virial Mass Function of Nearby SDSS Galaxy Clusters
• Effects of Strong Gravitational Lensing on Millimeter-Wave Galaxy Number Counts
• Numerical Galaxy Catalog -I. A Semi-analytic Model of Galaxy Formation with N-body simulations
• The Canada-France deep fields survey-II: Lyman-break galaxies and galaxy clustering at z~3
• Precision cosmology with a wide area XMM cluster survey
• The Kurtosis of the Cosmic Shear Field
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Tracing mass and light in the Universe: where is the dark matter?
• Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization
• DEMNUni: Massive neutrinos and the bispectrum of large scale structures
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• Testing the Cosmological Principle with CatWISE Quasars: A Bayesian Analysis of the Number-Count Dipole
• Modeling the nonlinear clustering in modified gravity models I: A fitting formula for matter power spectrum of f(R) gravity
• Challenges for Kinetic Unified Dark Matter
• Fuzzy Dark Matter and the Dark Energy Survey Year 1 Data
• Imprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scales
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample
• CHORUS II. Subaru/HSC Determination of the Ly$\alpha$ Luminosity Function at $z=7.0$: Constraints on Cosmic Reionization Model Parameter
• The potential of X-ray cluster surveys to constrain primordial non-Gaussianity
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space
• Accurate and Efficient Halo-based Galaxy Clustering Modelling with Simulations
• The Impact of Intrinsic Alignments: Cosmological Constraints from a Joint Analysis of Cosmic Shear and Galaxy Survey Data
• Weak lensing mass map and peak statistics in Canada-France-Hawaii Telescope Stripe 82 survey
• A double take on early and interacting dark energy from JWST
• Cosmological Measurements with Forthcoming Radio Continuum Surveys
• Arc Statistics in Cosmological Models with Dark Energy
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• Hierarchical Growth and Cosmic Star Formation: Enrichment, Outflows and Supernova Rates
• The DEEP2 Galaxy Redshift Survey: Clustering of Groups and Group Galaxies at z~1
• Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity
• Toward an accurate mass function for precision cosmology
• Constraining primordial non-Gaussianity via a multitracer technique with surveys by Euclid and Square Kilometre Array
• Future Evolution of Bound Superclusters in an Accelerating Universe
• Impact of Baryonic Processes on Weak Lensing Cosmology: Power Spectrum, Non-Local Statistics, and Parameter Bias
• MOKA: a new tool for Strong Lensing Studies
• Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2
• Simulating the X-ray Forest
• Cosmic variance of the galaxy cluster weak lensing signal
• Particle dark matter searches outside the Local Group
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• The Clustering of High-Redshift (2.9 $\le$ z $\le$ 5.1) Quasars in SDSS Stripe 82
• Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
• Resolving Small-Scale Dark Matter Structures Using Multi-Source Indirect Detection
• Numerical and Analytical Predictions for the Large-Scale Sunyaev-Zel'dovich Effect
• H-ATLAS: The cosmic abundance of dust from the far-infrared background power spectrum
• Strong clustering of underdense regions and the environmental dependence of clustering from Gaussian initial conditions
• Joint analysis of cluster number counts and weak lensing power spectrum to correct for the super-sample covariance
• How to Grow a Healthy Merger Tree
• Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy Studies
• The Shape-Alignment relation in $\Lambda$CDM Cosmic Structures
• Separate Universe Consistency Relation and Calibration of Halo Bias
• Linear response to long wavelength fluctuations using curvature simulations
• Structure formation in cosmologies with oscillating dark energy
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
• A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
• Distinguishing models of reionization using future radio observations of 21-cm 1-point statistics
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Impact of H_2-based star formation model on the z>=6 luminosity function and the ionizing photon budget for reionization
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• Large Scale Environment of a $z=6.61$ Luminous Quasar Probed by Ly$\alpha$ Emitters and Lyman Break Galaxies
• Modeling dark matter subhalos in a constrained galaxy: Global mass and boosted annihilation profiles
• Probing Small-Scale Power Spectra with Pulsar Timing Arrays
• The luminosity and stellar mass functions of GRB host galaxies: Insight into the metallicity bias
• The Scale-Dependence of Halo Assembly Bias
• The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect
• Deriving an Accurate Formula of Scale-dependent Bias with Primordial Non-Gaussianity: An Application of the Integrated Perturbation Theory
• The LBT Bootes Field Survey: I. The Rest-frame UV and Luminosity Functions and Clustering of Bright Lyman Break Galaxies at z~3
• The Radio Scream from Black Holes at Cosmic Dawn: A Semi-Analytic Model for the Impact of Radio Loud Black-Holes on the 21 cm Global Signal
• A fresh look into the interacting dark matter scenario
• Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation
• Mass and Concentration estimates from Weak and Strong Gravitational Lensing: a Systematic Study
• A New Halo Finding Method for N-Body Simulations
• The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• Combining Probes of Large-Scale Structure with CosmoLike
• The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• Impact of Scale Dependent Bias and Nonlinear Structure Growth on the ISW Effect: Angular Power Spectra
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• High redshift formation and evolution of central massive objects I: model description
• Accurate mass and velocity functions of dark matter halos
• Systematic effects in large-scale angular power spectra of photometric quasars and implications for constraining primordial nongaussianity
• Scale Dependence of Halo Bispectrum from Non-Gaussian Initial Conditions in Cosmological N-body Simulations
• Cosmology in 2D: the concentration-mass relation for galaxy clusters
• How well do cosmological simulations reproduce individual-halo properties?
• Distribution function approach to redshift space distortions. Part V: perturbation theory applied to dark matter halos
• An analytical model for the non-linear redshift-space power spectrum
• The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• Pairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matter Model using the Bullet Cluster
• The halo-model description of marked statistics
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Cosmic Mass Functions from Gaussian Stochastic Diffusion Processes
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Accurate Modeling of Weak Lensing with the sGL Method
• The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology
• Optimized detection of shear peaks in weak lensing maps
• Fluctuations in the High-Redshift Lyman-Werner and Lyman-alpha Radiation Backgrounds
• The contribution of high redshift galaxies to the Near-Infrared Background
• LoCuSS: The infall of X-ray groups onto massive clusters
• TheHaloMod: An online calculator for the halo model
• High redshift quasars and the supermassive black hole mass budget: constraints on quasar formation models
• The role of HD cooling in primordial star formation
• Clustering of quasars in a wide luminosity range at redshift 4 with Subaru Hyper Suprime-Cam wide field imaging
• Constraining primordial magnetic fields through large scale structure
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Intensity mapping of H-alpha, H-beta, [OII] and [OIII] lines at z<5
• Implications for Primordial Non-Gaussianity (f_NL) from weak lensing masses of high-z galaxy clusters
• Scale dependent halo bias in the excursion set approach
• COSMOS: Stochastic bias from measurements of weak lensing and galaxy clustering
• Quasars and galaxy formation
• Capturing Halos at High Redshifts
• Objective Classification of Galaxy Spectra using the Information Bottleneck Method
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• The clustering and abundance of star-forming and passive galaxies at $z\sim 2$
• The Evolution of Bias - Generalized
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization
• Probing small-scale cosmological fluctuations with the 21 cm forest: effects of neutrino mass, running spectral index and warm dark matter
• Mock Catalogs for the DEEP2 redshift survey
• A suppressed contribution of low mass galaxies to reionization due to supernova feedback
• Correlations of Cosmic Tidal Fields
• Hemispherical Asymmetry and Local non-Gaussianity: a Consistency Condition
• On CMB B-Mode Non-Gaussianity
• A fast method for computing strong-lensing cross sections: Application to merging clusters
• Gravitational Lensing Statistics in Universes Dominated by Dark Energy
• CosmicGrowth Simulations---Cosmological simulations for structure growth studies
• Supersonic Relative Velocity between Dark Matter and Baryons: A Review
• Separating Accretion and Mergers in the Cosmic Growth of Black Holes with X-ray and Gravitational Wave Observations
• Cosmic web dependence of galaxy clustering and quenching in SDSS
• Measuring the topology of reionization with Betti numbers
• Heating of the Intergalactic Medium by Primordial Miniquasars
• The First Billion Years of a Warm Dark Matter Universe
• FlowPM: Distributed TensorFlow Implementation of the FastPM Cosmological N-body Solver
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Direct collapse black hole formation via high-velocity collisions of protogalaxies
• Tomographic-spectral approach for dark matter detection in the cross-correlation between cosmic shear and diffuse gamma-ray emission
• Cosmology without cosmic variance
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• Accuracy of slow-roll formulae for inflationary perturbations: implications for primordial black hole formation
• Testing models of supermassive black hole seed formation through gravity waves
• Power spectrum and correlation function errors: Poisson vs. Gaussian shot noise
• The Strömgren sphere, the environment and the reionization in the local universe of the highest redshift QSOs
• Mass Function of Low Mass Dark Halos
• The Asiago-ESO/RASS QSO Survey. III. Clustering analysis and its theoretical interpretation
• Gravitational Lensing Magnification and Time Delay Statistics for Distant Supernovae
• Substructure and the halo model of large-scale structure
• Quasar-Galaxy and Galaxy-Galaxy Cross-Correlations: Model Predictions with Realistic Galaxies
• Dwarf Galaxies in the NGC 1023 Group
• Dark energy constraints from lensing-detected galaxy clusters
• Scale-dependent halo bias from scale-dependent growth
• Evidence of cross-correlation between the CMB lensing and the gamma-ray sky
• The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
• Probing the Core Structure of Dark Halos with Tangential and Radial Arc Statistics
• Near-Field Limits on the Role of Faint Galaxies in Cosmic Reionization
• Halo Concentrations and Weak-Lensing Number Counts in Dark Energy Cosmologies
• Non-Gaussianity and large-scale structure in a two-field inflationary model
• Voids in Modified Gravity Reloaded: Eulerian Void Assignment
• Halo abundances and counts-in-cells: The excursion set approach with correlated steps
• Light-cone anisotropy in 21cm fluctuations during the epoch of reionization
• First detection of scale-dependent linear halo bias in $N$-body simulations with massive neutrinos
• Halo clustering and g_{NL}-type primordial non-Gaussianity
• Probing Dark Matter with Future CMB Measurements
• A Fast Radio Burst Occurs Every Second throughout the Observable Universe
• Coupled Quintessence and the Halo Mass Function
• Impact of Primordial Ultracompact Minihaloes on the Intergalactic Medium and First Structure Formation
• Mass Function of Rich Galaxy Clusters and Its Constraint on sigma_8
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• Cross-correlating the gamma-ray sky with catalogs of galaxy clusters
• A halo model approach for the 21-cm power spectrum at cosmic dawn
• Magnification-Temperature Correlation: the Dark Side of ISW Measurements
• Improved optical mass tracer for galaxy clusters calibrated using weak lensing measurements
• The nonlinear matter power spectrum
• The Cosmic Timeline Implied by the JWST High-redshift Galaxies
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Using Large Scale Structure to test Multifield Inflation
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters
• Optimal linear reconstruction of dark matter from halo catalogs
• Measuring primordial non-Gaussianity through weak lensing peak counts
• Including beyond-linear halo bias in halo models
• Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping
• The clustering properties of radio-selected AGN and star-forming galaxies up to redshifts z~3
• A simple model linking galaxy and dark matter evolution
• Non-Gaussianity from Large-Scale Structure Surveys
• Lensing Magnification: Implications for Counts of Submillimeter Galaxies and SZ Clusters
• Clustering of i-dropout galaxies at z=6 in GOODS and the UDF
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• New constraints on ${\sigma }_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• Leptonic dark matter annihilation in the evolving universe: constraints and implications
• Monolithic or hierarchical star formation? A new statistical analysis
• Comments on the size of the simulation box in cosmological N-Body simulations
• Sensitivity of galaxy cluster dark energy constraints to halo modeling uncertainties
• The Role of Heating and Enrichment in Galaxy Formation
• Integrated Sachs Wolfe Effect and Rees Sciama Effect
• Excursion Set Halo Mass Function and Bias in a Stochastic Barrier Model of Ellipsoidal Collapse
• Squared temperature-temperature power spectrum as a probe of the CMB bispectrum
• Self-consistent semi-analytic models of the first stars
• Constraining warm dark matter with cosmic shear power spectra
• On the faint-end of the high-$z$ galaxy luminosity function
• Cosmic String Loops as the Seeds of Super-Massive Black Holes
• Impact of the Primordial Stellar Initial Mass Function on the 21-cm Signal
• Formation times and masses of dark matter haloes
• Local stochastic non-Gaussianity and N-body simulations
• The Bias and Mass Function of Dark Matter Halos in Non-Markovian Extension of the Excursion Set Theory
• Perturbation theory and excursion set estimates of the probability distribution function of dark matter, and a method for reconstructing the initial distribution function
• Cosmological and Astrophysical Implications of the Sunyaev-Zel'dovich Effect
• On the Nonspherical Nature of Halo Formation
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope
• An interpretable machine learning framework for dark matter halo formation
• The visibility of Lyman Alpha Emitters: constraining reionization, ionizing photons and dust
• Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys
• Exploring the liminality: properties of haloes and subhaloes in borderline $f(R)$ gravity
• The Contribution Of Inverse Compton Scattering To The Diffuse Extragalactic Gamma-Ray Background From Annihilating Dark Matter
• Detecting shocked intergalactic gas with X-ray and radio observations
• Modelling large-scale halo bias using the bispectrum
• Glimmering in the dark: modeling the low-mass end of the $M_{\bullet }-\sigma$ relation and of the quasar luminosity function
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• Measuring the Nonlinear Biasing Function from a Galaxy Redshift Survey
• Spherical Collapse and Cluster Counts in Modified Gravity Models
• Likelihood Methods for Cluster Dark Energy Surveys
• Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function
• A high precision semi-analytic mass function
• On the road to percent accuracy V: the non-linear power spectrum beyond $\Lambda$CDM with massive neutrinos and baryonic feedback
• X-Ray Evolution of Active Galactic Nuclei and Hierarchical Galaxy Formation
• The Imprint of f(R) Gravity on Non-Linear Structure Formation
• On Ellipsoidal Collapse and Primordial Black-Hole Formation
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Imprints of Oscillatory Bispectra on Galaxy Clustering
• Relativistic wide-angle galaxy bispectrum on the light-cone
• Higher-order moments of the lensing shear and other spin two fields
• The Host Halos of OI Absorbers in the Reionization Epoch
• Joint likelihood function of cluster counts and $n$-point correlation functions: Improving their power through including halo sample variance
• Testing anthropic predictions for Lambda and the CMB temperature
• Redshifted 21 Centimeter Emission from Minihalos Before Reionization
• Non-universality of the mass function: dependence on the growth rate and power spectrum shape
• The Impact of Energy Feedback on Quasar Evolution and Black Hole Demographics
• Weak-Lensing Halo Numbers and Dark-Matter Profiles
• Satellite Luminosities in Galaxy Groups
• Constraining the Quasar Contribution to the Reionisation of Cosmic Hydrogen
• Shot noise and biased tracers: a new look at the halo model
• Excursion Set Theory for generic moving barriers and non-Gaussian initial conditions
• High-energy neutrinos from sources in clusters of galaxies
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Can Early Dark Energy be Detected in Non-Linear Structure?
• Formation time distribution of dark matter haloes: theories versus N-body simulations
• Efficient cold outflows driven by cosmic rays in high redshift galaxies and their global effects on the IGM
• Weak Lensing as a Calibrator of the Cluster Mass-Temperature Relation
• On the evolution of clustering of 24um-selected galaxies
• Joint Analysis of Gravitational Lensing, Clustering and Abundance: Toward the Unification of Large-Scale Structure Analysis
• Warm dark matter and the ionization history of the Universe
• Small-scale shear: Peeling off diffuse subhalos with gravitational waves
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• Dark Matter Microhalos From Simplified Models
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Were progenitors of local L* galaxies Lyman-alpha emitters at high redshift?
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• Large Scale Structure of the Universe
• Bispectrum Supersample Covariance
• Dark Matter microphysics and 21 cm observations
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• Optimal dataset combining in f_nl constraints from large scale structure in an idealised case
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• Is there enough star formation in simulated protoclusters?
• Effect of clustering on extragalactic source counts with low-resolution instruments
• Bias deconstructed: Unravelling the scale dependence of halo bias using real space measurements
• AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization
• The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys
• The Difference PDF of 21-cm Fluctuations: A Powerful Statistical Tool for Probing Cosmic Reionization
• Redshift space 21 cm power spectra from reionization
• Power spectrum tomography of dark matter annihilation with local galaxy distribution
• Halo stochasticity in global clustering analysis
• Galaxy groups in the 2dF galaxy redshift survey: Luminosity and Mass Statistics
• Nonlinear Bias of Cosmological Halo Formation in the Early Universe
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Observation of small scale structure using sextupole lensing
• Minimum size of 21-cm simulations
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• Looking for Population III stars with He II line intensity mapping
• ASOHF: a new adaptive spherical overdensity halo finder
• The 21 Centimeter Forest
• What Does It Take to Stabilize Gravitational Clustering?
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• Galaxy cluster number count data constraints on cosmological parameters
• Formation of Massive Population III Galaxies through Photoionization Feedback: A Possible Explanation for CR7
• Halo abundances within the cosmic web
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• The halo mass function in interacting Dark Energy models
• Galaxy-CMB Cross-Correlation as a Probe of Alternative Models of Gravity
• 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
• Substructure in dark matter halos: Towards a model of the abundance and spatial distribution of subclumps
• Ultraviolet Background Radiation from Cosmic Structure Formation
• Light to Mass Variations with Environment
• The Oxford-Dartmouth Thirty Degree Survey II: Clustering of Bright Lyman Break Galaxies - Strong Luminosity Dependent Bias at z=4
• The environmental dependence of clustering in hierarchical models
• The Habitable Epoch of the Early Universe
• Radial profile and log-normal fluctuations of intra-cluster medium as an origin of systematic bias of spectroscopic temperature
• Constraining the initial conditions of the Universe using large scale structure
• Angular correlations in the cosmic gamma-ray background from dark matter annihilation around intermediate-mass black holes
• Gamma Ray Burst and star formation rates: The physical origin for the redshift evolution of their ratio
• Population III Star Formation In Large Cosmological Simulations I. Halo Temporal and Physical Environment
• Dark Matter Annihilation around Intermediate Mass Black Holes: an update
• Clustering of X-Ray-Selected AGN
• A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
• Reducing sample variance: halo biasing, non-linearity and stochasticity
• Multitracer technique for galaxy bispectrum - An application to constraints on non-local primordial non-Gaussianities -
• The impact of correlated projections on weak lensing cluster counts
• Biases on the cosmological parameters and thermal SZ residuals
• Constraint of Void Bias on Primordial non-Gaussianity
• Information Content of Higher-Order Galaxy Correlation Functions
• Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
• Modeling Galaxy Clustering by Color
• AMICO galaxy clusters in KiDS-DR3: Constraints on cosmological parameters and on the normalisation of the mass-richness relation from clustering
• Most massive halos with Gumbel Statistics
• Intensity mapping with neutral hydrogen and the Hidden Valley simulations
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: I. Construction of all-sky thermal and kinetic SZ-maps
• Dark Matter Signatures in the Anisotropic Radio Sky
• Predictions for Ultra-Deep Radio Counts of Star-Forming Galaxies
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Constraining Cosmology with High Convergence Regions in Weak Lensing Surveys
• Exploring the cosmic 21-cm signal from the Epoch of Reionisation using the Wavelet Scattering Transform
• Statistics of Sunyaev-Zel'dovich Cluster Surveys
• The Las Campanas Distant Cluster Survey -- The Correlation Function
• The impact of halo shapes on the bispectrum in cosmology
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Small-scale structure and 21cm fluctuations by primordial black holes
• Weak Lensing Observables in the Halo Model
• Precision Cosmology
• Low-mass suppression of the satellite luminosity function due to the supersonic baryon--cold-dark-matter relative velocity
• Constraining global properties of the Draco dwarf spheroidal galaxy
• Cross-correlation of weak lensing and gamma rays: implications for the nature of dark matter
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• A local bias approach to the clustering of discrete density peaks
• Mixed dark matter: matter power spectrum and halo mass function
• The Cluster Galaxy Circular Velocity Function
• Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps
• Up to 100,000 reliable strong gravitational lenses in future dark energy experiments
• Anisotropic cosmic optical background bound for decaying dark matter in light of the LORRI anomaly
• A Prescription for Galaxy Biasing Evolution as a Nuisance Parameter
• Theoretical predictions on the clustering of SCUBA galaxies and implications for small-scale fluctuations at sub-mm wavelengths
• Numerical simulations of dwarf galaxy merger trees
• Halo Mass Functions in Early Dark Energy Cosmologies
• The Environmental Dependence of the Incidence of Galactic Tidal Features
• Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
• Studying the Sources of Cosmic Reionization with 21-cm Fluctuations
• Galaxy groups in the 2dF galaxy redshift survey: Large Scale Structure with Groups
• The cross-correlation between 21cm intensity mapping maps and the Lyman-alpha forest in the post-reionization era
• Constraints on the temperature of the intergalactic medium at z=8.4 with 21-cm observations
• CFHTLenS: A Weak Lensing Shear Analysis of the 3D-Matched-Filter Galaxy Clusters
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• The baryonic mass-velocity relation; clues to feedback processes during structure formation and the cosmic baryon inventory
• Fuzzy Dark Matter as a Solution to Reconcile the Stellar Mass Density of High-z Massive Galaxies and Reionization History
• Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• Confronting Galactic and Extragalactic $\gamma$-ray observed by Fermi-LAT with Annihilating Dark Matter in Inert Higgs Doublet Model
• Constraining modified theory of gravity with galaxy bispectrum
• The rise and fall of a challenger: the Bullet Cluster in $\Lambda$ Cold Dark Matter simulations
• On the reliability of merger-trees and the mass growth histories of dark matter haloes
• Adaptive Mesh Refinement Simulations of the Ionization Structure and Kinematics of Damped Ly$\alpha$ Systems with Self-consistent Radiative Transfer
• The importance of magnification effects in galaxy-galaxy lensing
• On the statistics of proto-cluster candidates detected in the Planck all-sky survey
• Cosmological N-Body Simulations with a Large-Scale Tidal Field
• The Maximum B-mode Polarization of the Cosmic Microwave Background from Inhomogeneous Reionization
• Formation of Globular Cluster Systems II: Impact of the Cutoff of the Cluster Initial Mass Function
• MOIRCS Deep Survey. II. Clustering Properties of K-band Selected Galaxies in GOODS-North Region
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Detecting the relativistic bispectrum in 21cm intensity maps
• Influence of Population III stars on cosmic chemical evolution
• Predicting the Clustering of X-Ray Selected Galaxy Clusters in Flux-Limited Surveys
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• Circular Polarization of the CMB: A probe of the First stars
• A general framework to test gravity using galaxy clusters I: Modelling the dynamical mass of haloes in $f(R)$ gravity
• Excursion set theory for modified gravity: correlated steps, mass functions and halo bias
• Zipf's Law from Scale-free Geometry
• Modeling peculiar velocities of dark matter halos
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Cosmological Radio Emission induced by WIMP Dark Matter
• Reionisation in sterile neutrino cosmologies
• Measuring redshift through X-ray spectroscopy of galaxy clusters: results from Chandra data and future prospects
• Clustering and Bias Measurements of SDSS Voids
• Cosmology with clusters of galaxies
• LISA detection of massive black hole binaries: imprint of seed populations and of exterme recoils
• On estimating cosmology-dependent covariance matrices
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• Probability of the most massive cluster under non-Gaussian initial conditions
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• Impact of systematics on cosmological parameters from future Galaxy Clusters surveys
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• A closer look at CMB constraints on WIMP dark matter
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Rapid simulation rescaling from standard to modified gravity models
• Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
• A new model to predict weak-lensing peak counts III. Filtering technique comparisons
• Galactic winds and the Lya forest
• Confusion noise at far-IR to millimeter wavelengths
• The origin of dispersion in DLA metallicities
• Comparing halo bias from abundance and clustering
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Triaxial collapse and virialisation of dark-matter haloes
• Calibrating the Galaxy Halo - Black Hole Relation Based on the Clustering of Quasars
• The Halo Mass-Bias Redshift Evolution in the $\Lambda$CDM Cosmology
• Constraining the X-ray heating and reionization using 21-cm power spectra with Marginal Neural Ratio Estimation
• Non-Gaussianity of the Cosmic Infrared Background anisotropies I : Diagrammatic formalism and application to the angular bispectrum
• Propagating sample variance uncertainties in redshift calibration: simulations, theory and application to the COSMOS2015 data
• The initial shear field in models with primordial local non-Gaussianity and implications for halo and void abundances
• Supermassive Black Hole Merger Rates: Uncertainties from Halo Merger Theory
• Angular momentum and clustering properties of early dark matter halos
• Was the Universe Reionized at Redshift 10?
• Non-Gaussianity Constraints using Future Radio Continuum Surveys and the Multi-Tracer Technique
• Effects of the complex mass distribution of dark matter halos on weak lensing cluster surveys
• Gravitational lensing of the CMB by galaxy clusters
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• Delensing Cosmic Microwave Background B-modes with the Square Kilometre Array Radio Continuum Survey
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• A new smooth-$k$ space filter approach to calculate halo abundances
• Non-local bias in the halo bispectrum with primordial non-Gaussianity
• The earliest galaxies seen in 21 cm line absorption
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Spectroscopic follow-up of a cluster candidate at z = 1.45
• Constraining warm dark matter with 21 cm line fluctuations due to minihalos
• Revealing the cosmic web dependent halo bias
• The PEP survey: clustering of infrared-selected galaxies and structure formation at z~2 in the GOODS South
• Galaxy Clustering and Dark Energy
• Feedback from Clustered Sources During Reionization
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• Distinguishing standard reionization from dark matter models
• Halo Concentration and the Dark Matter Power Spectrum
• Power spectrum for the small-scale Universe
• Evidence for inhomogeneous reionization in the local Universe from metal-poor globular cluster systems
• The 400d Galaxy Cluster Survey Weak Lensing Programme: I: MMT/Megacam Analysis of CL0030+2618 at z=0.50
• Small-scale structure and the Lyman-$\alpha$ forest baryon acoustic oscillation feature
• The Sources of Extreme Ultraviolet and Soft X-ray Backgrounds
• Exact Extreme Value Statistics and the Halo Mass Function
• Distribution of the very first PopIII stars and their relation to bright z~6 quasars
• The observed galaxy bispectrum from single-field inflation in the squeezed limit
• Statistical properties of the Burgers equation with Brownian initial velocity
• Cosmological constraints from abundance, weak-lensing and clustering of galaxy clusters: application to the SDSS
• Mass functions and bias of dark matter halos
• Cosmological constraints from line intensity mapping with interlopers
• Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum
• On the Average Comoving Number Density of Halos
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• Self-Calibrated Cluster Counts as a Probe of Primordial Non-Gaussianity
• The effects of primordial non-Gaussianity on the cosmological reionization
• Groups in the Millennium Simulation and in SDSS DR7
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• How covariant is the galaxy luminosity function?
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• The importance of stepping up in the excursion set approach
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• Cosmological Structure Formation in Decaying Dark Matter Models
• The Most Massive Black Holes in the Universe: Effects of Mergers in Massive Galaxy Clusters
• The cosmological dependence of halo and galaxy assembly bias
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• Fast Weak Lensing Simulations with Halo Model
• An improved model of HII bubbles during the epoch of reionization
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• Statistics of Merging Peaks of Random Gaussian Fluctuations: Skeleton Tree Formalism
• Excursion set theory for modified gravity: Eulerian versus Lagrangian environments
• Clustering of dark matter halos on the light-cone: scale-, time- and mass-dependence of the halo biasing in the Hubble volume simulations
• The OH line contamination of 21 cm intensity fluctuation measurements for z=1~4
• The mass function dependence on the dynamical state of dark matter haloes
• An application of extreme value statistics to the most massive galaxy clusters at low and high redshifts
• Halo assembly bias from Separate Universe simulations
• Remapping dark matter halo catalogues between cosmological simulations
• Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey
• Gravitational lensing effects on the gamma-ray burst Hubble diagram
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• Evolution of spherical overdensities in holographic dark energy models
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• Probing high-redshift galaxies with Ly$\alpha$ intensity mapping
• Strong gravitational lensing: why no central black holes?
• Highly-Ionized Oxygen Absorbers in the Intergalactic Medium
• Scale Radii and Aggregation Histories of Dark Haloes
• H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above $\sim 1$ arcmin
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• On Physical Scales of Dark Matter Halos
• Using the cluster mass function from weak lensing to constrain neutrino masses
• Gravitational Flexion by Elliptical Dark Matter Haloes
• Composition of Low Redshift Halo Gas
• Mask Effects on Cosmological Studies with Weak Lensing Peak Statistics
• CMB spectral distortions from black holes formed by vacuum bubbles
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• Constraints on black hole duty cycles and the black hole-halo relation from SDSS quasar clustering
• Constraining cosmological parameters with the clustering properties of galaxy clusters in optical and X-ray bands
• Nonlinear evolution of initially biased tracers in modified gravity
• Self-consistency of the Excursion Set Approach
• Cosmological shock waves: clues to the formation history of haloes
• One- and Two-point Source Statistics from the LOFAR Two-metre Sky Survey First Data Release
• Counts of high-redshift GRBs as probe of primordial non-Gaussianities
• Constraining the halo mass function with observations
• Some improvements to the spherical collapse model
• Large Scale Anisotropic Bias from Primordial non-Gaussianity
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Searching for Sterile Neutrino with X-ray Intensity Mapping
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• An analytic model for the epoch of halo creation
• Testing the Halo Model Against the SDSS Photometric Survey
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Impacts of satellite galaxies on the redshift-space distortions
• The halo bias inside cosmic voids
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• Conditional Mass Functions and Merger Rates of Dark Matter Halos in the Ellipsoidal Collapse Model
• A model for the metallicity evolution of damped Lyman-alpha systems
• A Comparison of Simulated and Analytic Major Merger Counts
• Detection of cross-correlation between gravitational lensing and gamma rays
• Point Source Contamination in CMB Non-Gaussianity Analyses
• Equal-time Consistency Relations in the Large-Scale Structure of the Universe
• ALMA reveals large overdensity and strong clustering of galaxies in quasar environments at $z\sim 4$
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• Clustering dark energy and halo abundances
• Conditional Probabilities in the Excursion Set Theory. Generic Barriers and non-Gaussian Initial Conditions
• Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field
• The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Masses of high-z galaxy hosting haloes from angular clustering and their evolution in the CDM model
• Probing ultra-light axions with the 21-cm Signal during Cosmic Dawn
• Large-scale clustering as a probe of the origin and the host environment of fast radio bursts
• Modeling star formation in dwarf spheroidal galaxies: a case for extended dark matter halos
• The correlation function of X-ray galaxy clusters in the RASS1 Bright Sample
• VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2<z<2.1 selected from Spitzer IRAC 3.6 micron and 4.5 micron photometry
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
• The formation of CDM haloes II: collapse time and tides
• Halos and voids in a multifractal model of cosmic structure
• Halo model prediction of the cosmic magnification statistics: the full non-linear contribution
• Understanding the non-linear clustering of high redshift galaxies
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• ASKI: full-sky lensing map making algorithms
• Optimizing weak lensing mass estimates for cluster profile uncertainty
• History of Hydrogen Reionization in the Cold Dark Matter Model
• The clustering of the first galaxy halos
• A Conditional Luminosity Function Model of the Cosmic Far-Infrared Background Anisotropy Power Spectrum
• Lensing Sunyaev-Zel'dovich Clusters
• No Tension: JWST Galaxies at $z>10$ Consistent with Cosmological Simulations
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Probing Cosmic Origins with CO and [CII] Emission Lines
• The Halo Void (Dust) Model of Large Scale Structure
• Soliton Merger Rates and Enhanced Axion Dark Matter Decay
• Characterizing dark interactions with the halo mass accretion history and structural properties
• The probability distribution function of the SZ power spectrum: an analytical approach
• Non-local bias contribution to third-order galaxy correlations
• The luminosities of the brightest cluster galaxies and brightest satellites in SDSS groups
• Subhaloes in Scale-Free Cosmologies
• Testing the Modified Press-Schechter Model against N-Body Simulations
• Magnification of Photometric LRGs by Foreground LRGs and Clusters in SDSS
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• Halo Abundance and Assembly History with Extreme-Axion Wave Dark Matter at $z\ge 4$
• Long Gamma-Ray Bursts and Their Host Galaxies at High Redshift
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Population III Star Clusters in the Reionized Universe
• Lyman-Break Galaxies at $z\sim 3$ in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission
• Pair Correlations and Merger Bias
• Radiative feedback and cosmic molecular gas: the role of different radiative sources
• An Analytic Model for the Axis-Ratio Distribution of Dark Matter Halos from the Primordial Gaussian Density Field
• Cosmological signatures of tilted isocurvature perturbations: reionization and 21cm fluctuations
• Tidal alignments as a contaminant of the galaxy bispectrum
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Predictions of the causal entropic principle for environmental conditions of the universe
• COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
• Cluster Mergers and the Origin of the ARCADE-2 Excess
• Re-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores
• CosmoReionMC: A package for estimating cosmological and astrophysical parameters using CMB, Lyman-α absorption and global 21 cm data
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• Photon Number Conserving Models of H II Bubbles during Reionization
• Spherical collapse and halo mass function in the symmetron model
• The halo light cone catalogues of \Abacus{AbacusSummit}
• On Correlated Random Walks and 21-cm Fluctuations During Cosmic Reionization
• Effects of halo substructure on the power spectrum and bispectrum
• The halo mass function and inner structure of ETHOS haloes at high redshift
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• A fast radio burst in the direction of the Virgo cluster
• Turning noise into signal: learning from the scatter in the Hubble diagram
• Modeling the QSO luminosity and spatial clustering at low redshifts
• SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Confronting Cold Dark Matter Predictions with Observed Galaxy Rotations
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• A Predicted New Population of UV-faint Galaxies at z>4
• A short review on clustering dark energy
• Cluster counts: calibration issue or new physics?
• Growth of spherical overdensities in scalar-tensor cosmologies
• Constraints on nature of ultra light dark matter particles with 21cm forest
• Measuring the Cosmic Equation of State with Galaxy Clusters in the DEEP2 Redshift Survey
• The Total Mass of Dark Matter Haloes
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos
• The large scale clustering of radio sources
• Gravitational lensing magnification without multiple imaging
• Clustering of Intermediate Luminosity X-ray selected AGN at z~3
• Cosmic Reionization May Still Have Started Early and Ended Late: Confronting Early Onset with CMB Anisotropy and 21 cm Global Signals
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• Enhanced Rates of Fast Radio Bursts from Galaxy Clusters
• Detectability of the gravitational redshift effect from the asymmetric galaxy clustering
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Progenitor delay-time distribution of short gamma-ray bursts: Constraints from observations
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• A Lower Limit on the Halo Mass to form Supermassive Black Holes
• Influence of Projection in Cluster Cosmology Studies
• Synergising semi-analytical models and hydrodynamical simulations to interpret JWST data from the first billion years
• Detecting Reionization in the Star Formation Histories of High-Redshift Galaxies
• Impact of Dark Matter Substructure on the Matter and Weak Lensing Power Spectra
• On an Analytical Framework for Voids: Their abundances, density profiles and local mass functions
• The hybrid SZ power spectrum: Combining cluster counts and SZ fluctuations to probe gas physics
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• The galaxy-galaxy lensing contribution to the cosmic shear two point function
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• The halo mass of optically-luminous quasars at z=1-2 measured via gravitational deflection of the cosmic microwave background
• Shot noise and scatter in the star formation efficiency as a source of 21-cm fluctuations
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• A Solution to the Missing Link in the Press-Schechter Formalism
• On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
• CMB lensing reconstruction biases from masking extragalactic sources
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• 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
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• Weak lensing peak count as a probe of f(R) theories
• Are Simulations of CDM Consistent with Galactic-Scale Observations at High Redshift?
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Evidence for Merger-Driven Activity in the Clustering of High Redshift Quasars
• The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
• Warm dark matter constraints from high-$z$ Direct Collapse Black Holes using the JWST
• Cosmological gamma ray and neutrino backgrounds due to neutralino dark matter annihilation
• Is it possible to tell the difference between fermionic and bosonic hot dark matter?
• 21 cm Forest Constraints on Primordial Black Holes
• The universal multiplicity function: counting halos and voids
• Can decaying particle explain cosmic infrared background excess?
• Known Unknowns of Dark Matter Annihilation over Cosmic Time
• Understanding the redshift evolution of the luminosity functions of Lyman-alpha emitters
• Constraints on shear and rotation with massive galaxy clusters
• Pairwise velocities in the Halo Model: Luminosity and Scale Dependence
• How to Build a Catalogue of Linearly-Evolving Cosmic Voids
• The inner structure of very massive elliptical galaxies: implications for the inside-out formation mechanism of z~2 galaxies
• Effects of Photoionization and Photoheating on Lyman-alpha Forest Properties from Cholla Cosmological Simulations
• Understanding large-scale structure in the SSA22 protocluster region using cosmological simulations
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• Vector dark energy and high-z massive clusters
• Perturbation theory with dispersion and higher cumulants: non-linear regime
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• On a novel approach using massive clusters at high redshifts as cosmological probe
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• What do cluster counts really tell us about the Universe?
• ALP dark matter with non-periodic potentials: parametric resonance, halo formation and gravitational signatures
• Where can we really find the First Stars' Remnants today?
• Practical Cosmology with Lenses
• The build-up of halos within Press-Schechter theory
• Long gamma-ray burst rate at very high redshift
• Probing Population III Initial Mass Functions with He II/H$\alpha$ Intensity Mapping
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• On the peculiar momentum of baryons after Reionization
• How many arcminute-separation lenses are expected in the 2dF QSO survey?
• The strongest gravitational lenses: II. Is the large Einstein radius of MACS J0717.5+3745 in conflict with LCDM?
• A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing
• Universal Merger Histories of Dark-Matter Haloes
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Spectral Distortion of the CMB by the Cumulative CO Emission from Galaxies throughout Cosmic History
• It takes two to know one: Computing accurate one-point PDF covariances from effective two-point PDF models
• Weak Gravitational Lensing as a Method to Constrain Unstable Dark Matter
• Taming assembly bias for primordial non-Gaussianity
• Virialization of high redshift dark matter haloes
• Figure rotation of dark halos in CDM simulations
• Nonlinear modulation of the HI power spectrum on ultra-large scales. I
• The clustering properties of the first galaxies
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• The Cosmological History of Accretion onto Dark Halos and Supermassive Black Holes
• The Density Contrast of the Shapley Supercluster
• Modelling the asymmetry of the halo cross-correlation function with relativistic effects at quasi-linear scales
• Stochastic background of gravitational waves generated by pre-galactic black holes
• Fossil Ionized Bubbles Around Dead Quasars During Reionization
• 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
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Globular Cluster Formation in the Virgo Cluster
• Modelling the matter bispectrum at small scales in modified gravity
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Can We Detect the Anisotropic Shapes of Quasar HII Regions During Reionization Through The Small-Scale Redshifted 21cm Power Spectrum?
• The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization
• Growth index of matter perturbations in the light of Dark Energy Survey
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• Subhaloes gone Notts: the clustering properties of subhaloes
• Determine the galaxy bias factors on large scales using bispectrum method
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Searching for axion-like particle decay in the near-infrared background: an updated analysis
• Stochastic bias in multi-dimensional excursion set approaches
• A scale dependent bias on linear scales: the case for HI intensity mapping at z=1
• Effective Window Function for Lagrangian Halos
• Statistical Properties of Radio Halos in Galaxy Clusters and Origin of Seed Electrons for Reacceleration
• The clustering of baryonic matter. I: a halo-model approach
• Constraints on the Baryonic Compression and Implications for the Fraction of Dark Halo Lenses
• Dense Regions in Supersonic Isothermal Turbulence
• Late time sky as a probe of steps and oscillations in primordial Universe
• Optimal Transport Reconstruction of Baryon Acoustic Oscillations
• Constraining the growth rate by combining multiple future surveys
• Probing the Pre-Reionization Epoch with Molecular Hydrogen Intensity Mapping
• On the cosmological mass function theory
• Renormalization of Lagrangian bias via spectral parameters
• Distortion of the luminosity function of high-redshift galaxies by gravitational lensing
• Extreme value statistics of weak lensing shear peak counts
• The Wouthuysen Field Absorption Trough in Cosmic Strings Wakes
• Searching for gamma-ray emission from galaxy clusters at low redshift
• Impacts of biasing schemes in the one-loop integrated perturbation theory
• Predicting the number of giant arcs expected in the next generation wide-field surveys from space
• Matter Distribution around Galaxies
• On the equivalence between the effective cosmology and excursion set treatments of environment
• Halo bias in the excursion set approach with correlated steps
• Detection and Fundamental Applications of Individual First Galaxies
• Weak Lensing of the CMB: Power Spectrum Covariance
• Cluster Lensing of QSOs as a Probe of LCDM and Dark Energy Cosmologies
• How do Primordial Black Holes change the Halo Mass Function and Structure?
• Cold dark energy constraints from the abundance of galaxy clusters
• Oscillating Bispectra and Galaxy Clustering: A Novel Probe of Inflationary Physics with Large-Scale Structure
• Bayesian Model Selection with Future 21cm Observations of The Epoch of Reionisation
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Perturbation theory for nonlinear halo power spectrum: the renormalized bias and halo bias
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• The Size Distribution of Void Filaments in a LCDM Cosmology
• Double Distribution of Dark Matter Halos with respect to Mass and Local Overdensity
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Probing dark matter signals in neutrino telescopes through angular power spectrum
• The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems
• Imaging dark matter at the smallest scales with $z\approx 1$ lensed stars
• Constraints on Modified Gravity from Sunyaev-Zeldovich Cluster Surveys
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• The cosmological free-free signal from galaxy groups and clusters
• The 21cm radiation from minihalos as a probe of small primordial non-Gaussianity
• Non-Gaussian Halo Mass Function and Non-Spherical Halo Collapse: Theory vs. Simulations
• Spherical collapse model in agegraphic dark energy cosmologies
• Cosmology from weak lensing alone and implications for the Hubble tension
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Tracing the Nature of Dark Energy with Galaxy Distribution
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• The correlation of extragalactic $\gamma$-rays with cosmic matter density distributions from weak-gravitational lensing
• Probing reionization with the cross power spectrum of 21 cm and near-infrared radiation backgrounds
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• Planck Lensing and Cosmic Infrared Background Cross-Correlation with Fermi-LAT: Tracing Dark Matter Signals in the Gamma-Ray Background
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• Small scale clustering of late forming dark matter
• Non-Gaussian bias: insights from discrete density peaks
• Halo Occupation Distribution of Massive Galaxies since z = 1
• Theoretical and numerical perspectives on cosmic distance averages
• Remnants of Galactic subhalos and their impact on indirect dark matter searches
• The halo mass function conditioned on density from the Millennium Simulation: insights into missing baryons and galaxy mass functions
• The cosmic web connection to the dark matter halo distribution through gravity
• Photometric Properties of the Most Massive High-Redshift Galaxies
• Stochastic gravitational wave background from cold dark matter halos
• Constraining isocurvature perturbations with the 21cm emission from minihaloes
• 21cmFirstCLASS I. Cosmological tool for $\Lambda$CDM and beyond
• Anthropic predictions for vacuum energy and neutrino masses in the light of WMAP-3
• The Infrared Glow of First Stars
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• The Mass Function of Void Groups as a Probe of the Primordial non-Gaussianity
• Calculation of the critical overdensity in the spherical-collapse approximation
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• The abundance of dark matter haloes down to Earth mass
• Large Scale Structure Forecast Constraints on Particle Production During Inflation
• Marked correlation functions in perturbation theory
• Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• The most massive Population III stars
• Euclid: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes
• Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
• On the Markovian assumption in the excursion set approach: the approximation of Markov Velocities
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• Can ultralight dark matter explain the age-velocity dispersion relation of the Milky Way disc: A revised and improved treatment
• Measuring Linear and Non-linear Galaxy Bias Using Counts-in-Cells in the Dark Energy Survey Science Verification Data
• Diffuse Gamma Ray Background from Annihilating Dark Matter in Density Spikes around Supermassive Black Holes
• Bounds on WIMP dark matter from galaxy clusters at low redshift
• Cosmic Variance In the Transparency of the Intergalactic Medium After Reionization
• Brightest Cluster Galaxies Trace Weak Lensing Mass Bias and Halo Triaxiality in The Three Hundred Project
• Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription
• Virial halo mass function in the $Planck$ cosmology
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Probing dark energy with the next generation X-ray surveys of galaxy clusters
• Stacking weak lensing signals of SZ clusters to constrain cluster physics
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• Testing Multi-Field Inflation with Galaxy Bias
• Statistical properties of the linear tidal shear
• Strong Evolution in the Luminosity-Velocity Relation at z>1?
• Large-scale bias of dark matter halos
• Sunyaev-Zel'dovich Cluster Survey Simulations for Planck
• Halo/Galaxy Bispectrum with Primordial non-Gaussianity from integrated Perturbation Theory (iPT)
• The imprint of cosmological non-Gaussianities on primordial structure formation
• EDGES result versus CMB and low-redshift constraints on ionization histories
• The Ratio of CO to Total Gas Mass in High Redshift Galaxies
• Mass of clusters in simulations
• Superclusters with thermal SZ effect surveys
• A Merger Tree with Microsolar Mass Resolution: Application to $\gamma$-ray Emission from Subhalo Population
• Probing the cosmic microwave background temperature using the Sunyaev-Zeldovich effect
• The Environment on few Mpc scales of Infrared Luminous Galaxies at Redshifts z~1
• Structure formation in dark energy cosmologies described by PADE parameterization
• Validity of strong lensing statistics for constraints on the galaxy evolution model
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Can radiative cooling and nongravitational heating explain simultaneously the global X-ray properties of clusters and the unresolved cosmic X-ray background ?
• Spin and structural halo properties at high redshift in a LCDM Universe
• Galaxy clustering at cosmic dawn from JWST/NIRCam observations to redshift z$\sim$11
• Evolution of perturbations in distinct classes of canonical scalar field models of dark energy
• The fractal distribution of haloes
• Detecting the non-Gaussianity of the 21-cm signal during reionisation with the Wavelet Scattering Transform
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Probing a cosmological model with a $\Lambda ={\Lambda }_0+3\beta H^2$ decaying-vacuum
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Cosmology through arc statistics I: sensitivity to ${\Omega }_m$ and ${\sigma }_8$
• Non-Gaussianity of the Cosmic Infrared Background anisotropies II : Predictions of the bispectrum and constraints forecast
• Spherical collapse in Generalized Dark Matter models
• Close Pairs as Proxies for Galaxy Cluster Mergers
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• The UV luminosity function at 0.6 < z < 1 from UVCANDELS
• Cosmology before noon with multiple galaxy populations
• Statistical properties of dark matter mini-haloes at z >= 15
• Measurement of Void Bias Using Separate Universe Simulations
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• Testing model independent modified gravity with future large scale surveys
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• A Consistent Comparison of Bias Models using Observational Data
• Probing primordial non-Gaussianity with 21 cm fluctuations from minihalos
• The Flatness and Sudden Evolution of the Intergalactic Ionizing Background
• Merger history trees of dark matter haloes in moving barrier models
• Probing the Evolution of Gas Mass Fraction with Sunyaev-Zel'dovich Effect
• A Halo Model with Environment Dependence: Theoretical Considerations
• Finding bright $z\ge 6.6$ Lyman-$\alpha$ emitters with lensing: prospects for Euclid
• Future Cosmology: New Physics and Opportunity from the China Space Station Telescope (CSST)
• Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Extraction of cluster parameters with future Sunyaev-Zel'dovich observations
• Distribution of primordial black holes and 21cm signature
• Cluster counts III. $\Lambda$CDM extensions and the cluster tension
• Halo assembly bias from a deep learning model of halo formation
• Implementation of a Fourier Matched Filter in CMB Analyses. Application to ISW Studies
• Cosmological Perturbations and the Running Cosmological Constant Model
• Cosmic dichotomy in the hosts of rapidly star-forming systems at low and high redshifts
• Pregalactic LiBeB Production by Supernova Cosmic Rays
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• Not-so-little Red Dots: Two massive and dusty starbursts at z~5-7 pushing the limits of star formation discovered by JWST in the COSMOS-Web survey
• Probing Compensated Isocurvature with the 21-cm Signal during Cosmic Dawn
• The escape fraction of ionizing photons from high redshift galaxies
• Statistics of gravitational potential perturbations: A novel approach to deriving the X-ray temperature function
• Excursion set peaks in energy as a model for haloes
• Early Science Result from the Japanese Virtual Observatory: AGN and Galaxy Clustering at z = 0.3 to 3.0
• Interpolating Masked Weak Lensing Signal with Karhunen-Loeve Analysis
• Dark matter halo creation in moving barrier models
• On the Angular Correlation Function of SZ Clusters : Extracting cosmological information from a 2D catalog
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• High-redshift voids in the excursion set formalism
• Cross-Correlation of Near and Far-Infrared Background Anisotropies as Traced by Spitzer and Herschel
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• The Rise of Dwarfs and the Fall of Giants: Galaxy Formation Feedback Signatures in the Halo Satellite Luminosity Function
• Evidence for new physics from clusters ?
• The Extreme Tail of the Non-Gaussian Mass Function
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• Generating extremely large-volume reionisation simulations
• Signatures of dark and baryonic structures on weakly lensed gravitational waves
• A physical and concise halo model based on the depletion radius
• Probing higher-order primordial non-Gaussianity with galaxy surveys
• Cluster Probes of Dark Energy Clustering
• The Clustering of Extremely Red Objects
• Biased tracer reconstruction with halo mass information
• 200 Mpc Sized Structure in the 2dF QSO Redshift Survey
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) cluster survey IV: Superclusters in the local Universe at z <= 0.03
• Galaxy clustering measurements out to redshift z$\sim$8 from Hubble Legacy Fields
• Number Counts and Dynamical Vacuum Cosmologies
• Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
• Cross-correlation between thermal Sunyaev-Zeldovich effect and the integrated Sachs-Wolfe effect
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Separate Universe calibration of the dependence of halo bias on cosmic web anisotropy
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Modeling active galactic nuclei: ongoing problems for the faint-end of the luminosity function
• Imprint of non-linear effects on HI intensity mapping on large scales
• Observing relativistic features in large-scale structure surveys -- I: Multipoles of the power spectrum
• Synergies across the spectrum for particle dark matter indirect detection: how HI intensity mapping meets gamma rays
• Boosting small-scale structure via primordial black holes and implications for sub-GeV dark matter annihilation
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• Cluster-Cluster Lensing and the Case of Abell 383
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• The Irrelevance of Primordial Black Hole Clustering in the LVK mass range
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• Pushing JWST to the extremes: search and scrutiny of bright galaxy candidates at z$\simeq$15-30
• A prescription for the conditional mass function of dark matter haloes
• Clusters of galaxies: setting the stage
• Distance-Redshift Relation in a Realistic Inhomogeneous Universe
• Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function
• Quasars at intermediate redshift are not special; but they are often satellites
• Searching for Signal of Primordial Black Hole from CMB Lensing and $\gamma$-ray Emissions
• Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• 21cm forest probes on the axion dark matter in the post-inflationary Peccei-Quinn symmetry breaking scenarios
• Biases on cosmological parameter estimators from galaxy cluster number counts
• Relativistic bias in neutrino cosmologies
• Constraining thawing and freezing models with cluster number counts
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• Evolution of the gas mass fraction in galaxy clusters
• Small scale contributions to CMB: A coherent analysis
• The First Billion Years project: gamma-ray bursts at z>5
• Non-Gaussian CMB and LSS statistics beyond polyspectra
• A galaxy-halo model of large-scale structure
• The HI Bias during the Epoch of Reionization
• Unveiling cosmological information on small scales with line intensity mapping
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Nonlinear stochastic biasing of halos: Analysis of cosmological N-body simulations and perturbation theories
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• The generalized evolution of linear bias: a tool to test gravity
• A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Higher multipoles of the galaxy bispectrum in redshift space
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Gravitational waves from merging intermediate-mass black holes : II Event rates at ground-based detectors
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Formation of the large-scale structure of the Universe
• Possible arcminute-separation gravitational lensed QSOs in the 2dF QSO survey
• Triggering the formation of direct collapse black holes by their congeners
• Constraining Cosmological Models by the Cluster Mass Function
• Constraining the growth of perturbations with lensing of supernovae
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey II: Unveiling a pancake structure with a 100 Mpc radius in the local Universe
• Spherical collapse of dark matter haloes in tidal gravitational fields
• Probing Oscillons of Ultra-Light Axion-like Particle by 21cm Forest
• Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
• The bias of weighted dark matter halos from peak theory
• Clustering of CODEX clusters
• Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey III: The Perseus-Pisces supercluster and the Southern Great Wall as traced by X-ray luminous galaxy clusters
• The high-redshift tail of stellar reionization in LCDM is beyond the reach of the low-$\ell$ CMB
• Modelling the stochasticity of high-redshift halo bias
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• Testing the accuracy of likelihoods for cluster abundance cosmology
• Measuring neutrino masses with joint JWST and DESI DR2 data
• Constraining structure formation using EDGES
• Semi-numeric simulations of helium reionization and the fluctuating radiation background
• Simulations for a next-generation UHECR observatory
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• High-z dusty star-forming galaxies: a top-heavy initial mass function?
• Measuring dark matter ellipticity of Abell 901/902 using Particle Based Lensing
• Star formation in high redshift galaxies including Supernova feedback: effect on stellar mass and luminosity functions
• Constraints on small-scale primordial density fluctuation from cosmic microwave background through dark matter annihilation
• Evolution of the cosmological mass function in a moving barrier model
• Jetted Tidal Disruptions of Stars as a Flag of Intermediate Mass Black Holes at High Redshifts
• Searching for the first stars with the Gaia mission
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate
• 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
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy
• Deep learning insights into cosmological structure formation
• Order statistics applied to the most massive and most distant galaxy clusters
• Linking X-ray AGN with dark matter halos: a model compatible with AGN luminosity function and large-scale clustering properties
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• The mass and temperature functions in a moving barrier model
• Light-Cone Distortion of the Clustering and Abundance of Massive Galaxies at High-Redshifts
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• The Highest-Energy Cosmic Rays Cannot be Dominantly Protons from Steady Sources
• Testing General Relativity Using the Evolution of Linear Bias
• Probing the cluster pressure profile with thermal Sunyaev-Zeldovich effect and weak lensing cross-correlation
• Cosmological constraints from the masses and abundances of L* galaxies
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Cluster abundance and large scale structure
• Bias and Conditional Mass Function of Dark Halos Based on the Nonspherical Collapse Model
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Predicting the clustering properties of galaxy clusters detectable for the Planck satellite
• Distribution of Dust around Galaxies: An Analytic Model
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
• Oxygen pumping II: Probing the Inhomogeneous Metal Enrichment at the Epoch of Reionization with High Frequency CMB Observations
• Probing the growth of supermassive black holes at z>6 with LOFAR
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• An Introduction into the Theory of Cosmological Structure Formation
• Missing baryons, bulk flows and the E-mode polarization of the Cosmic Microwave Background
• The virialization density of peaks with general density profiles under spherical collapse
• Non-Gaussian Halo Bias Beyond the Squeezed Limit
• Finding Core Collapse Supernova from the Epoch of Reionization Behind Cluster Lenses
• Mapping discrete galaxies at cosmic dawn with 21-centimeter observations
• Recovering the Tidal Field in the Projected Galaxy Distribution
• On the expected purity of photometric galaxy surveys targeting the Cosmic Dawn
• Maximum amplitude of the high-redshift 21-cm absorption feature
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Shot noise in multi-tracer constraints on $f_{\text{NL}}$ and relativistic projections: Power Spectrum
• The influence of primordial magnetic fields on the spherical collapse model in cosmology
• A Global Semi-Analytic Model of the First Stars and Galaxies Including Dark Matter Halo Merger Histories
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• Is the misalignment of the Local Group velocity and the 2MASS Redshift Survey dipole typical in a LambdaCDM model?
• On the Evolution of High-Redshift Active Galactic Nuclei
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• X-ray Clusters of Galaxies as Cosmological Tools
• The full-sky Spherical Fourier-Bessel power spectrum in general relativity
• Astrophysical information from the Rayleigh-Jeans Tail of the CMB
• Probing the fluctuating Ultra-violet background using the Hubble Frontier Fields
• Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
• Can Early Dark Energy be Probed by the High-Redshift Galaxy Abundance?
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Matrix Formalism of Excursion Set Theory: A new approach to statistics of dark matter halo counting
• Uncertainties in the S-Z selected cluster angular power spectrum
• Statistics of Dark Matter Halos in the Excursion Set Peak Framework
• Weighing neutrinos using high redshift galaxy luminosity functions
• Remapping simulated halo catalogues in redshift space
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Halo Model Analysis of Cluster Statistics
• Constraint on dark matter annihilation with dark star formation using Fermi extragalactic diffuse gamma-ray background data
• Clustering of the AKARI NEP Deep Field 24 $\mu$m selected galaxies
• CMB Comptonization in Clusters: Spectral and Angular Power from Evolving Polytropic Gas
• Extended Press-Schechter theory and the density profiles of dark matter haloes
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• Probing the circumgalactic baryons through cross-correlations
• The galaxy bias at second order in general relativity with Non-Gaussian initial conditions
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• Antisymmetric Cross-correlation between H I and CO Line Intensity Maps as a New Probe of Cosmic Reionization
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions
• The very wide-field $gzK$ galaxy survey -- II. The relationship between star-forming galaxies at $z\sim 2$ and their host haloes based upon HOD modelling
• Dark matter halo mass functions and density profiles from mass and energy cascade
• Non-Gaussian Tails of Cosmological Density Distribution Function from Dark Halo Approach
• Galaxy flows within 8,000 km/s from Numerical Action methods
• Constraints on Running of Non-Gaussianity from Large Scale Structure Probes
• A roadmap to cosmological parameter analysis with third-order shear statistics II: Analytic covariance estimate
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• An Extended Zel'dovich Model for the Halo Mass Function
• Starlight from JWST: Implications for star formation and dark matter models
• Cosmological constraints from multiple tracers in spectroscopic surveys
• Numerical action reconstruction of the dynamical history of dark matter haloes in N-body simulations
• Constraining Thawing Dark Energy using Galaxy Cluster Number Counts
• A study on the Clustering Properties of Radio-Selected sources in the Lockman Hole Region at 325 MHz
• Cell Count Moments in the Halo Model
• Non-perturbative halo clustering from cosmological density peaks
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• CHAM: a fast algorithm of modelling non-linear matter power spectrum in the sCreened HAlo Model
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• CMB Anisotropies from Outflows in Lyman Break Galaxies
• Cosmological constraints from a 2D SZ catalog
• The influence of mergers on the cluster temperature function and cosmological parameters derived from it
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Understanding the Impact of Semi-numeric Reionization Models when using CNNs
• Relativistic distortions in galaxy density-ellipticity correlations: gravitational redshift and peculiar velocity effects
• Calibration of Nonthermal Pressure in Global Dark Matter Simulations of Clusters of Galaxies
• A new test for the stable clustering hypothesis
• Unveiling Neutrino Halos with CMB Lensing
• Pushing the Limits of Detectability: Mixed Dark Matter from Strong Gravitational Lenses
• Self-Consistent Theory of Halo Mergers - II: CDM Power Spectra
• Gravitational lensing effects on sub-millimetre galaxy counts
• Cosmological test of local position invariance from the asymmetric galaxy clustering
• Constraining Dark Energy From Splitting Angle Statistic of Strong Gravitational Lenses
• Anisotropies in Cosmological 21 cm Background by Oscillons/I-balls of Ultra-light Axion-like Particle
• Spherical Collapse Approach for Non-standard Dark Matter Models and Enhanced Early Galaxy Formation in JWST
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Is There a Universal Mass Function?
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• An Evolving Entropy Floor in the Intracluster Gas?
• Galaxy Statistics in Pencil-beam Surveys at High Redshifts
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Foreground Removal of CO Intensity Mapping Using Deep Learning
• Searching for the earliest galaxies in the 21 cm forest
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• Cross-Correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys
• Choose to smooth: Gaussian streaming with the truncated Zel'dovich approximation
• Is GN-z11 powered by a super-Eddington massive black hole?
• Can we distinguish early dark energy from a cosmological constant?
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• Cosmological Filaments in the light of Excursion Set of Saddle Points
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• Interlopers speak out: studying the dark universe using small-scale lensing anisotropies
• Merging History Trees for Dark Matter Halos: Tests of the Merging Cell Model in a CDM Cosmology
• Probing axion dark matter with 21cm fluctuations from minihalos
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• Spherical collapse and cluster number counts in dark energy models disformally coupled to dark matter
• Implications of multi-axion dark matter on structure formation
• Exploring the relationship between black hole accretion and star formation with blind mid-/far-infrared spectroscopic surveys
• Spherical collapse in coupled quintessence with a $\Lambda$CDM background
• Modified initial power spectrum and too big to fail problem
• Simulated vs. observed UV emission at high redshift: a hint for a clumpy ISM?
• Constraining the mass-concentration relation through weak lensing peak function
• The fractional Brownian motion and the halo mass function
• Gravitational Redshifts in Clusters and Voids
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• Optimizing the yield of Sunyaev-Zel'dovich cluster surveys
• X-ray cluster cosmology
• Consistency relations for the Lagrangian halo bias and their implications
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• The impact of the cosmological constant on past and future star formation
• Structure formation in clustering DBI dark energy model with constant sound speed
• Impact of cosmic rays on the global 21-cm signal during cosmic dawn
• Halo Growth and Merger Rates as a Cosmological Test
• Screened fifth forces in parity-breaking correlation functions
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Constraints on the warm dark matter model from gravitational lensing
• Anisotropic strong lensing as a probe of dark matter self-interactions
• Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
• Halo mass function in scale invariant models
• COMBO-17 measurements of the effect of environment on the type-dependent galaxy luminosity function
• Effects of tidal gravitational fields in clustering dark energy models
• Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
• Intrinsic size correlations in weak lensing
• Lux ex tenebris: The imprint of annihilating dark matter on the intergalactic medium during Cosmic Dawn
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• Modelling the 21 cm Signal From the Epoch of Reionization and Cosmic Dawn
• Probing the Primordial Power Spectrum with Cluster Number Counts
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• Toward optimal cluster power spectrum analysis
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• On the star formation efficiency in high redshift Lyman-α emitters
• Cluster contribution to the X-ray background as a cosmological probe
• Calibrating excursion set reionization models to approximately conserve ionizing photons
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• The baryon mass function for galaxy clusters
• An Analytic Formula for the Supercluster Mass Function
• The Sunyaev-Zel'dovich effect and Faraday rotation contributions of galaxy groups to the CMB angular power spectrum
• Constraining the Neutrino Mass with the Drifting Coefficient of the Field Cluster Mass Function
• Cosmic reionization of hydrogen and helium: contribution from both mini-quasars and stars
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Bayesian Multi-line Intensity Mapping
• Evolution of spherical over-densities in tachyon scalar field model
• Observations of Ly$\alpha$ Emitters at High Redshift
• Halo/Galaxy Bispectrum with Equilateral-type Primordial Trispectrum
• Exploring the physical origins of halo assembly bias from early times
• Testing the Large-Scale Environments of Cool-core and Noncool-core Clusters with Clustering Bias
• What is the super-sample covariance? A fresh perspective for second-order shear statistics
• Cluster Assembly Times as a Cosmological Test
• Reionization in the Light of Dark Stars
• The effect of finite halo size on the clustering of neutral hydrogen
• A physical model for the redshift evolution of high-z Lyman-Break Galaxies
• Deep learning insights into non-universality in the halo mass function
• Smooth halos in the cosmic web
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Dwarf Galaxy Clustering and Missing Satellites
• The growth of DM and DE perturbations in DBI non-canonical scalar field scenario
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• Tidal shear and the consistency of microscopic Lagrangian halo approaches
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Small-scale Effects of Thermal Inflation on Halo Abundance at High-$z$, Galaxy Substructure Abundance and 21-cm Power Spectrum
• LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia Supernova 2022qmx ("SN Zwicky") with HST Template Observations
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Modelling the escape of Lyman Continuum photons from galaxies in the Epoch of Reionization
• Structure formation and quasi-spherical collapse from initial curvature perturbations with numerical relativity simulations
• Impact of dark matter-baryon relative velocity on the 21cm forest
• Einasto profile as the halo model solution coupled to the depletion radius
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Boosting the 21 cm forest signals by the clumpy substructures
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Matching JWST UV Luminosity Functions with Refined $\Lambda$CDM Halo Models
• Mass bias and cosmological constraints from Planck cluster clustering
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Cross-Correlation between Damped Ly-alpha Systems and Ly-break Galaxies in Cosmological SPH Simulations
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Redshifted 21-cm emission signal from the halos in Dark Ages
• Non-linear matter power spectrum without screening dynamics modelling in $f(R)$ gravity
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• What is the optimal way to measure the galaxy power spectrum?
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• The magnitude-redshift relation in a realistic inhomogeneous universe
• The Impact of Non-Equipartition on Cosmological Parameter Estimation from Sunyaev-Zel'dovich Surveys
• A Search for Neutron Star Precession and Interstellar Magnetic Field Variations via Multiepoch Pulsar Polarimetry
• Detecting quasars at very high redshift with next generation X-ray telescopes
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• N-body simulations of structure formation in thermal inflation cosmologies
• Interpreting the statistical properties of high-z extragalactic sources detected by the South Pole Telescope survey
• Properties of Central Regions of the Dark Matter Halos in the Model with a Bump in the Power Spectrum of Density Perturbations
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• Impact of the turnover in the high-z galaxy luminosity function on the 21-cm signal during Cosmic Dawn and Epoch of Reionization
• The Shocking Truth: The small contribution to hydrogen reionization from gravitational infall
• An X-ray Galaxy Cluster Survey for Investigations of Dark Energy
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• High redshift signatures in the 21 cm forest due to cosmic string wakes
• Hydrodynamical chemistry simulations of the SZ effect and the impacts from primordial non-Gaussianities
• Information content in anisotropic cosmological fields: Impact of different multipole expansion scheme for galaxy density and ellipticity correlations
• Machine Learning and Structure Formation in Modified Gravity
• Massive Black Hole Mergers
• Angular fluctuations in the CXB: Is Fe 6.4 keV line tomography of the large-scale structure feasible?
• The strongest gravitational lenses: IV. The order statistics of the largest Einstein radii with cluster mergers
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Origin of Metals around Galaxies I: Catalogs of Metal-line Absorption Doublets from High-Resolution Quasar Spectra
• Bias-Limited Extraction of Cosmological Parameters
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• Evolution of Power Spectrum in Non-Gaussian Models
• The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
• Secondary B-mode polarization from Faraday rotation in clusters and galaxies
• Accurate halo mass functions from the simplest excursion set theory
• Scaling of the 1-halo terms with bias
• Forecasts for Broadband Intensity Mapping of the Ultraviolet-Optical Background with CASTOR and SPHEREx
• Primordial black holes as dark matter candidates: Multi-frequency constraints from cosmic radiation backgrounds
• A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Negative feedback effects on star formation history and cosmic reionization
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• Cosmological constraints on neutrino masses in light of JWST red and massive candidate galaxies
• High-redshift Galaxies from JWST Observations in More Realistic Dark Matter Halo Models
• Modelling the impact of intrinsic size and luminosity correlations on magnification estimation
• Testing Theoretical Models for the Higher-Order Moments of Dark Halo Distribution
• An Analytical Approach to the Spin-Distribution of Dark Halos
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• Constraints on Primordial Magnetic Fields from High Redshift Stellar Mass Density
• Merger rates of dark matter haloes: a comparison between EPS and N-body results
• The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
• The Cosmological Supersymmetron
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• The star formation history inferred from long gamma-ray bursts with high pseudo-redshifts
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Cosmological constraints from galaxy clustering
• Evolution of spherical overdensities in new agegraphic dark energy model
• On the Dark Matter Halos of Optical and IR-selected AGN in the Local Universe
• Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency
• The Halo Mass Function Redshift Dependence
• The Diversity of Environments Around Luminous Quasars at Redshift $z\sim 6$
• The Effect of Primordial Anti-Biasing on the Local Measurement of the Key Cosmological Parameters
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• The Splashback Mass Function in the Presence of Massive Neutrinos
• The Halo Mass Function from Excursion Set Theory with a Non-Gaussian Trispectrum
• The abundance of lensing protoclusters
• Born to be Starless: Revisiting the Missing Satellite Problem
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• Isodensity Statistics on Clustering of High-z Objects in Cosmological Redshift-spaces
• Statistical Properties of Supercluster-Like Filaments from Cosmological Simulations
• A Stochastic Theory of the Hierarchical Clustering III. The Non-universality and Non-stationarity of the Halo Mass Function
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• Stochastic Gravitational Wave Background originating from Halo Mergers
• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• Quinstant Dark Energy Predictions for Structure Formation
• Signatures of inhomogeneous dark matter annihilation on 21-cm
• The imprints of massive neutrinos on the three-point correlation function of large-scale structures
• The Cosmological Mass Function in the Zel'dovich Approximation
• Determination of the Linear Mass Power Spectrum From the Mass Function of Galaxy Clusters
• Models for the Clustering of Far-Infrared and Sub-millimetre selected Galaxies
• Linear and nonlinear clusterings of Horndeski-inspired dark energy models with fast transition
• SZ power spectrum and cluster numbers from an extended merger-tree model
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Primordial Black Hole Mergers as Probes of Dark Matter in Galactic Center
• Distinguishing thermal histories of dark matter from structure formation
• The clustering properties of high-redshift passive galaxies
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Predicting the intensity mapping signal for multi-$J$ CO lines
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• Sunyaev-Zel'dovich contribution in CMB analysis
• Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
• XMM-Newton follow-up of a sample of apparent low surface brightness galaxy groups detected in the ROSAT All-Sky Survey
• Directional miscentering dependence in weak lensing mass bias
• A measurement of the intrahalo light fraction with near-infrared background anisotropies
• Probability distribution and statistical properties of spherically compensated cosmic regions in $\Lambda$CDM cosmology
• Modified cosmology through generalized mass-to-horizon entropy: implications for structure growth and primordial gravitational waves
• Mass function and assembly of dark halos: an approach to inventory isolated overdense regions in random fields
• The Infancy of Cosmic Reionization
• Comparison of the linear bias models in the light of the Dark Energy Survey
• The AIDA-TNG project: 3D halo shapes
• Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST
• ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization
• Self-sustaining star formation fronts in filaments during cosmic dawn
• Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS
• The Effect of Primordial Non-Gaussianities on the Seeds of Super-Massive Black Holes
• The Supersonic Project: SIGOs, a Proposed Progenitor to Globular Clusters, and their Connections to Gravitational Wave Anisotropies
• Formation of Dark Matter Haloes in a Homogeneous Dark Energy Universe
• Direct Collapse Black Hole Candidates from Decaying Dark Matter
• Accelerating HI density predictions during the Epoch of Reionization using a GPR-based emulator on N-body simulations
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• Individual halo bias in models of $f(R)$ gravity
• Excursion Sets with a "Perfect" Collapse Model
• Radiative Transfer Simulations of Ly$\alpha$ Intensity Mapping During Cosmic Reionization Including Sources from Galaxies and the Intergalactic Medium
• On the Habitability of Our Universe
• Testing local position invariance with odd multipoles of galaxy clustering statistics
• 21-cm power spectrum and ionization bias as a probe of long-mode modulated non Gaussian sky
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Elucidating the impact of massive neutrinos on halo assembly bias
• KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
• Impact of baryons on the population of Galactic subhalos and implications for dark matter searches
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• Constraints on the normal branch of DGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
• X-ray luminosity functions of different morphological and X-ray type AGN populations
• Path integral approach for merger rates of dark matter haloes
• The same with less: The cosmic web of warm versus cold dark matter dwarf galaxies
• Dark Energy Simulations
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• On the virialization threshold for halo mass functions
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• Comparison of the spatial and the angular clustering of X-ray AGN
• Clustering of dark matter in the cosmic web as a probe of massive neutrinos
• The Mass Function of Dark Halos in Superclusters and Voids
• Non-parametric Lagrangian biasing from the insights of neural nets
• The haloes that reionized the Universe
• 21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter
• Cosmic magnification on high-redshift submillimeter galaxies
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Population III Star Formation in an X-ray background: I. Critical Halo Mass of Formation and Total Mass in Stars
• Predicting halo occupation and galaxy assembly bias with machine learning
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• Einstein-Cartan cosmology and the high-redshift Universe
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Imprints of fermionic and bosonic mixed dark matter on the 21-cm signal at cosmic dawn
• Extended Hernquist-Springel formalism for cosmic star formation
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Tracking through equality
• WIMP decay as a possible Warm Dark Matter model
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Origin & evolution of the Universe
• Non-Gaussianity in the Squeezed Three-Point Correlation from the Relativistic Effects
• Physics of star formation history and the luminosity function of galaxies therefrom
• Effect of the cosmological transition to metal-enriched star-formation on the hydrogen 21-cm signal
• Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Structure formation in a non-canonical scalar field model of clustering dark energy
• The life and times of dark matter haloes: what will I be when I grow up?
• Probing power spectrum enhancement at small scales with the SKA
• Effect of dust in circumgalactic haloes on the cosmic shear power spectrum
• Quantum geometry from commutators: a Heisenberg-picture framework and a toy application to early structure
• Axion-Like Particle Dark Matter Intensity Mapping: A New Probe via Cross-Correlation with Galaxy Surveys
• Cosmological constraints from clustering properties of galaxy clusters
• The JWST early galaxy crisis resolved by a reionization degeneracy
• Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy
• The Mass of Virialized Dark Matter Haloes
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Probing the warm dark matter mass with [C II] intensity mapping
• Black Hole merger rates in the first billion years in light of JWST data
• Laguerre reconstruction of the correlation function on Baryon Acoustic Oscillation scales
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey
• Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
• Comparison of clustering properties of observed objects and dark matter halos on different mass and spatial scales
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Mass functions from the excursion set model
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• Tracing cosmic voids with fast simulations
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
• Hybrid $P_{\ell }(k)$: general, unified, non-linear matter power spectrum in redshift space
• From Dark Matter Minihalos to Large-Scale Radiative Feedback: A Self-Consistent 3D Simulation of the First Stars and Galaxies using Neural Networks
• Classification of Radio Backgrounds at Cosmic Dawn and 21 cm Signal Confirmation Using Neural Networks
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Spherical Collapse in Modified Gravity Theories
• A model for the emission line galaxy luminosity function and flux ratios at high-redshifts
• A redshift distortion free correlation function at third order in the nonlinear regime
• Kinematic effects of the velocity fluctuations for dark halos population in LCDM model
• Using Dark Matter Haloes to Learn about Cosmic Acceleration: A New Proposal for a Universal Mass Function
• Slicing cluster mass functions with a Bayesian razor
• Power spectrum multipoles and clustering wedges during the Epoch of Reionization
• DLAs and Galaxy Formation
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Cosmic velocity, density and halo mass function: Insights from deep learning
• A general framework for unbiased tests of gravity using galaxy clusters
• Spherical collapse in reconstructed dark energy models
• Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models
• The History of Galaxy Formation in Groups: An Observational Perspective
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• Cosmologia com aglomerados de galáxias
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• Universality of the halo mass function in modified gravity cosmologies
• A bubble size distribution model for the Epoch of Reionization