Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes

Abstract

The Press--Schechter, excursion set approach allows one to make predictions about the shape and evolution of the mass function of bound objects. It combines the assumption that objects collapse spherically with the assumption that the initial density fluctuations were Gaussian and small. While the predicted mass function is reasonably accurate at the high mass end, it has more low mass objects than are seen in simulations of hierarchical clustering. This discrepancy can be reduced substantially if bound structures are assumed to form from an ellipsoidal, rather than a spherical collapse. In the spherical model, a region collapses if the initial density within it exceeds a threshold value, delta_sc. This value is independent of the initial size of the region, and since the mass of the collapsed object is related to its initial size, delta_sc is independent of final mass. In the ellipsoidal model, the collapse of a region depends on the surrounding shear field, as well as on its initial overdensity. Therefore, there is a relation between the density threshold value required for collapse, and the mass of the final object. We provide a fitting function to this delta_ec(m) relation for initially Gaussian fields which simplifies the inclusion of ellipsoidal dynamics in the excursion set approach. We discuss the relation between the excursion set predictions and the halo distribution in high resolution N-body simulations, and show that our simple parametrization of the ellipsoidal collapse model represents a significant improvement on the spherical model on an object-by-object basis. Finally, we show that the associated statistical predictions, the mass function and the large scale halo-to-mass bias relation, are also more accurate than the standard predictions.

12 pages, 6 figures, submitted to MNRAS

References in corpus (1)

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• The halo model for cosmology: a pedagogical review
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Robust Velocity-induced Acoustic Oscillations at Cosmic Dawn
• A Model For Infall Around Virialized Halos
• On Random Walks with a General Moving Barrier
• The velocity function of gas-rich galaxies
• Dark matter halo abundances, clustering and assembly histories at high redshift
• PRIMUS + DEEP2: Clustering of X-ray, Radio and IR-AGN at z~0.7
• Effects of Critical Collapse on Primordial Black-Hole Mass Spectra
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• Do Distinct Cosmological Models Predict Degenerate Halo Populations?
• Weighing neutrinos with cosmic neutral hydrogen
• N-body simulations with generic non-Gaussian initial conditions II: Halo bias
• AGN clustering in the local Universe: an unbiased picture from Swift-BAT
• Constraining the physical properties of the first lensed $z\sim 10-16$ galaxy candidates with JWST
• Large-scale assembly bias of dark matter halos
• Predictions for Herschel from LambdaCDM: unveiling the cosmic star formation history
• Cross-Correlation of Cosmic Shear and Extragalactic Gamma-ray Background: Constraints on the Dark Matter Annihilation Cross-Section
• The clustering of SDSS galaxy groups: mass and color dependence
• Halo bias in Lagrangian Space: Estimators and theoretical predictions
• On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion
• Exploring the high-redshift PBH-$\Lambda$CDM Universe: early black hole seeding, the first stars and cosmic radiation backgrounds
• The 2dF Galaxy Redshift Survey: The clustering of galaxy groups
• The 21 cm signal and the interplay between dark matter annihilations and astrophysical processes
• Machine learning cosmological structure formation
• The suppression of direct collapse black hole formation by soft X-ray irradiation
• Seeding the Second Star: enrichment from population III, dust evolution, and cloud collapse
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• Unique Signatures of Population III Stars in the Global 21-cm Signal
• Universal at last? The splashback mass function of dark matter halos
• Modelling the correlation between the thermal Sunyaev Zel'dovich effect and the cosmic infrared background
• Physical Characterization of Early Galaxies in the Webb's First Deep Field SMACS J0723.3-7323
• Halo modelling in chameleon theories
• The 21cm Power Spectrum After Reionization
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• The Birth and Growth of Neutralino Haloes
• A Confirmation of the Strong Clustering of Distant Red Galaxies at 2 < z <3
• Modelling Void Abundance in Modified Gravity
• Bayesian inference of cosmic density fields from non-linear, scale-dependent, and stochastic biased tracers
• Binary Quasars at High Redshift II: Sub-Mpc Clustering at z ~ 3-4
• Clustering properties of moderate luminosity X-ray selected Type 1 and Type 2 AGN at z~3
• Primordial non-Gaussianity in the large scale structure of the Universe
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• Cosmic Shear Covariance Matrix in $w$CDM: Cosmology Matters
• Modeling the nonlinear clustering in modified gravity models I: A fitting formula for matter power spectrum of f(R) gravity
• The Little Engines That Could? Globular Clusters Contribute Significantly to Reionization-era Star Formation
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Constraints on the mass-concentration relation of cold dark matter halos with 11 strong gravitational lenses
• Characterization of Dark-Matter-induced anisotropies in the diffuse gamma-ray background
• Shear and rotation in Chaplygin cosmology
• The Millennium Run Observatory: First Light
• Toward a Universal Formulation of the Halo Mass Function
• An Empirically-Calibrated Model For Interpreting the Evolution of Galaxies During the Reionization Era
• Fuzzy Dark Matter and the Dark Energy Survey Year 1 Data
• The potential of X-ray cluster surveys to constrain primordial non-Gaussianity
• The nature of the unresolved extragalactic soft CXB
• Annual Modulation in Direct Dark Matter Searches
• Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity
• Constraining First Star Formation with 21cm-Cosmology
• Galaxy Formation in Preheated Intergalactic Media
• The clustering of Ly-alpha emitters in a LambdaCDM Universe
• A double take on early and interacting dark energy from JWST
• Lyman Break Galaxies and the Lyman-alpha Forest
• Implications of multiple high-redshift galaxy clusters
• Modelling the observed luminosity function and clustering evolution of Lyman-$\alpha$ emitters: growing evidence for late reionization
• 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
• PINOCCHIO and the hierarchical build-up of dark matter haloes
• How to Grow a Healthy Merger Tree
• On Primordial Black Holes and secondary gravitational waves generated from inflation with solo/multi-bumpy potential
• Extended Spherical Collapse and the Accelerating Universe
• The enrichment history of cosmic metals
• Ellipsoidal halo finders and implications for models of triaxial halo formation
• Separate Universe Consistency Relation and Calibration of Halo Bias
• An analytical model for the accretion of dark matter subhalos
• Measurement of the halo bias from stacked shear profiles of galaxy clusters
• Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy Studies
• Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
• Structure formation in cosmologies with oscillating dark energy
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Extragalactic gamma-ray background radiation from dark matter annihilation
• Evaluating machine learning techniques for predicting power spectra from reionization simulations
• Non-Gaussian halo assembly bias
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Modeling dark matter subhalos in a constrained galaxy: Global mass and boosted annihilation profiles
• A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
• Orientation Bias of Optically Selected Galaxy Clusters and Its Impact on Stacked Weak Lensing Analyses
• The VIMOS-VLT Deep Survey. The dependence of clustering on galaxy stellar mass at z~1
• The effect of cosmic web filaments on the properties of groups and their central galaxies
• A fresh look into the interacting dark matter scenario
• The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions
• Constraints on black hole fuelling modes from the clustering of X-ray AGN
• Halo-model Analysis of the Clustering of Photometrically Selected Galaxies from SDSS
• Massive and old quiescent galaxies at high redshift
• Measuring the circum- and inter-galactic baryon contents with fast radio bursts
• Quantum fluctuations masquerade as halos: Bounds on ultra-light dark matter from quadruply-imaged quasars
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• Mass and Concentration estimates from Weak and Strong Gravitational Lensing: a Systematic Study
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• An Analytical Approach to Inhomogeneous Structure Formation
• Spatial Correlation Function of the Chandra Selected Active Galactic Nuclei
• Accurate mass and velocity functions of dark matter halos
• How well do cosmological simulations reproduce individual-halo properties?
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• A hierarchy of voids: More ado about nothing
• Cosmology in 2D: the concentration-mass relation for galaxy clusters
• Inner cusps of the first dark matter haloes: Formation and survival in a cosmological context
• An analytical model for the non-linear redshift-space power spectrum
• Galactic ionising photon budget during the Epoch of Reionisation in the Cosmic Dawn II simulation
• Imprints of the Early Universe on Axion Dark Matter Substructure
• Scale dependent halo bias in the excursion set approach
• The contribution of high redshift galaxies to the Near-Infrared Background
• Bayesian joint analysis of cluster weak lensing and Sunyaev-Zel'dovich effect data
• The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• The XMM-Newton wide-field survey in the COSMOS field: V. Angular Clustering of the X-ray Point Sources
• The splashback boundary of haloes in hydrodynamic simulations
• Luminosity dependent clustering of star-forming BzK galaxies at redshift 2
• Constraints on the small-scale power spectrum of density fluctuations from high-redshift gamma-ray bursts
• Clustering of quasars in a wide luminosity range at redshift 4 with Subaru Hyper Suprime-Cam wide field imaging
• Capturing Halos at High Redshifts
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• COSMOS: Stochastic bias from measurements of weak lensing and galaxy clustering
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Interpreting the Clustering of Distant Red Galaxies
• The nature of assembly bias - I. Clues from a LCDM cosmology
• EMMA: an AMR cosmological simulation code with radiative transfer
• An Effective Model for the Cosmic-Dawn 21-cm Signal
• Dwarf Galaxy Formation Was Suppressed By Cosmic Reionization
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• Cosmological constraints from 21cm surveys after reionization
• The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: the divergence of passive and star-forming galaxies
• The Mass Function of Void Galaxies in the SDSS Data Release 2
• A New Statistical Model for Population III Supernova Rates: Discriminating Between $\Lambda$CDM and WDM Cosmologies
• CosmicGrowth Simulations---Cosmological simulations for structure growth studies
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Effect of radiative transfer on damped Lyman-alpha and Lyman limit systems in cosmological SPH simulations
• Mass Function of Low Mass Dark Halos
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• Constraining resonant dark matter self-interactions with strong gravitational lenses
• Substructure and the halo model of large-scale structure
• How well do we know the Halo Mass Function?
• Modeling The Large Scale Bias of Neutral Hydrogen
• UVUDF: UV Luminosity Functions at the cosmic high-noon
• The VLT LBG Redshift Survey I: Clustering and Dynamics of ~1000 Galaxies at z~3
• The Strömgren sphere, the environment and the reionization in the local universe of the highest redshift QSOs
• Accuracy of slow-roll formulae for inflationary perturbations: implications for primordial black hole formation
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• Testing the Running of non-Gaussianity through the CMB mu-distortion and the Halo Bias
• Maximum redshift of gravitational wave merger events
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• The XMM--NEWTON Omega Project: II.Cosmological implications from the high redshift L-T relation of X-ray clusters
• Halo abundances and counts-in-cells: The excursion set approach with correlated steps
• QSO-LRG 2-Point Cross-Correlation Function and Redshift-Space Distorions
• Scale-dependent halo bias from scale-dependent growth
• The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
• Elucidating Galaxy Assembly Bias in SDSS
• The correlation between the distribution of galaxies and 21cm emission at high redshifts
• The Persistent Percolation of Single-Stream Voids
• Cosmic Ballet III: halo spin evolution in the cosmic web
• The clustering and evolution of H-alpha emitters at z~1 from HiZELS
• Sizes and ages of SDSS ellipticals: Comparison with hierarchical galaxy formation models
• What is the best way to measure baryonic acoustic oscillations?
• The Small-scale Clustering of Luminous Red Galaxies via Cross-Correlation Techniques
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• Weighing obscured and unobscured quasar hosts with the CMB
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• Bayesian modelling of clusters of galaxies from multi-frequency pointed Sunyaev--Zel'dovich observations
• Measuring the Dark Matter Halo Mass of X-ray AGN at z~1 using photometric redshifts
• Primordial black holes as dark matter: Interferometric tests of phase transition origin
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping
• Richness-mass relation self-calibration for galaxy clusters
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• Predicting the density profiles of the first halos
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• Local stochastic non-Gaussianity and N-body simulations
• Excursion Set Halo Mass Function and Bias in a Stochastic Barrier Model of Ellipsoidal Collapse
• Faint Submillimeter Galaxies identified through their optical/near-infrared colours I: spatial clustering and halo masses
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• The Bias and Mass Function of Dark Matter Halos in Non-Markovian Extension of the Excursion Set Theory
• On the faint-end of the high-$z$ galaxy luminosity function
• Perturbation theory and excursion set estimates of the probability distribution function of dark matter, and a method for reconstructing the initial distribution function
• The primordial matter power spectrum on sub-galactic scales
• The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population
• On the Nonspherical Nature of Halo Formation
• An interpretable machine learning framework for dark matter halo formation
• A Study of Massive and Evolved Galaxies at High Redshift
• Very Massive Stars in High-Redshift Galaxies
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function
• The Search for the Farthest Quasar: Consequences for Black Hole Growth and Seed Models
• The Imprint of f(R) Gravity on Non-Linear Structure Formation
• On Ellipsoidal Collapse and Primordial Black-Hole Formation
• Spherical Collapse and Cluster Counts in Modified Gravity Models
• A high precision semi-analytic mass function
• TDCOSMO III: Dark matter substructure meets dark energy -- the effects of (sub)halos on strong-lensing measurements of $H_0$
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Clusters of galaxies in the microwave band: influence of the motion of the Solar System
• Excursion Set Theory for generic moving barriers and non-Gaussian initial conditions
• Cosmology with the cluster mass function: mass estimators and shape systematics in large weak lensing surveys
• Weak-Lensing Halo Numbers and Dark-Matter Profiles
• $\text{Mangrove}$: Learning Galaxy Properties from Merger Trees
• Feedback from galactic stellar bulges and hot gaseous haloes of galaxies
• Breaking a dark degeneracy: The gamma-ray signature of early matter domination
• On Modeling and Measuring the Temperature of the z~5 IGM
• Large Scale Structure of the Universe
• The Impact of Theoretical Uncertainties in the Halo Mass Function and Halo Bias on Precision Cosmology
• Warm dark matter and the ionization history of the Universe
• Finding the Missing Baryons with Fast Radio Bursts and Sunyaev-Zeldovich Maps
• Joint Analysis of Gravitational Lensing, Clustering and Abundance: Toward the Unification of Large-Scale Structure Analysis
• Signatures of metal-free star formation in Planck 2015 Polarization Data
• Formation time distribution of dark matter haloes: theories versus N-body simulations
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• Excursion Sets and Non-Gaussian Void Statistics
• From Images to Dark Matter: End-To-End Inference of Substructure From Hundreds of Strong Gravitational Lenses
• Updated measurements of the dark matter halo masses of obscured quasars with improved WISE and Planck data
• An Improved Calculation of the Non-Gaussian Halo Mass Function
• Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Radio source feedback in galaxy evolution
• Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• Halo abundances in the f_{nl} model
• The observable 21cm signal from reionization may be perturbative
• Optimal dataset combining in f_nl constraints from large scale structure in an idealised case
• Is there enough star formation in simulated protoclusters?
• AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization
• Phase-Space Spectral Line De-confusion in Intensity Mapping
• Dark Matter microphysics and 21 cm observations
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Statistical and systematic errors in redshift-space distortion measurements from large surveys
• The formation of CDM haloes I: Collapse thresholds and the ellipsoidal collapse model
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys
• Halo stochasticity in global clustering analysis
• Cross correlation of Lyman-alpha absorbers with gas-rich galaxies
• Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Luminous Red Galaxies in hierarchical cosmologies
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• Origin of Cosmic Chemical Abundances
• Probing the Radio Loud/Quiet AGN dichotomy with quasar clustering
• The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
• The Contribution of z<6 Sources to the Spatial Coherence in the Unresolved Cosmic near-Infrared and X-ray Backgrounds
• Constraining the initial conditions of the Universe using large scale structure
• The clustering of X-ray selected AGN at z=0.1
• Preheating of the Universe by cosmic rays from primordial supernovae at the beginning of cosmic reionization
• Relating the structure of dark matter halos to their assembly and environment
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Clustering of infrared-bright dust-obscured galaxies revealed by the Hyper Suprime-Cam and WISE
• JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78
• Substructure in dark matter halos: Towards a model of the abundance and spatial distribution of subclumps
• The environmental dependence of clustering in hierarchical models
• The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements
• Bayesian inferences of galaxy formation from the K-band luminosity and HI mass functions of galaxies: constraining star formation and feedback
• Clustering of X-Ray-Selected AGN
• Spatial clustering and halo occupation distribution modeling of local AGN via cross-correlation measurements with 2MASS galaxies
• AMICO galaxy clusters in KiDS-DR3: Constraints on cosmological parameters and on the normalisation of the mass-richness relation from clustering
• Saraswati: An Extremely Massive ~ 200 Megaparsec Scale Supercluster
• Towards a general parametrization of the warm dark matter halo mass function
• Do Cosmic Rays Heat the Early Intergalactic Medium?
• Why does the clustering of haloes depend on their formation history
• Properties of fossil groups in cosmological simulations and galaxy formation models
• The Las Campanas Distant Cluster Survey -- The Correlation Function
• Forecasting [C II] line-intensity mapping measurements between the end of reionization and the epoch of galaxy assembly
• Evolution of the Clustering of Photometrically Selected SDSS Galaxies
• Testing cold dark matter with the low mass Tully-Fisher relation
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Axion Miniclusters Made Easy
• The Cluster Galaxy Circular Velocity Function
• On the Physical Requirements for a Pre-Reionization Origin of the Unresolved Near-Infrared Background
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model
• Nonspherical similarity solutions for dark halo formation
• Detection of Quasar Feedback from the Thermal Sunyaev-Zel'dovich Effect in Planck
• Mixed dark matter: matter power spectrum and halo mass function
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Predicting dark matter halo formation in N-body simulations with deep regression networks
• Galaxy groups in the 2dF galaxy redshift survey: Large Scale Structure with Groups
• Quantifying the Line-of-Sight Halo Contribution to the Dark Matter Convergence Power Spectrum from Strong Gravitational Lenses
• Studying high-z galaxies with [CII] intensity mapping
• Prospects of constraining reionization model parameters using Minkowski tensors and Betti numbers
• The cross-correlation between 21cm intensity mapping maps and the Lyman-alpha forest in the post-reionization era
• Dark matter annihilation from intermediate-mass black holes: Contribution to the extragalactic gamma-ray background
• Angular correlation functions of X-ray point-like sources in the full exposure XMM-LSS field
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• High-precision multi-band measurements of the angular clustering of X-ray sources
• A Short Introduction to Reionization Physics
• A general framework to test gravity using galaxy clusters I: Modelling the dynamical mass of haloes in $f(R)$ gravity
• Detecting the relativistic bispectrum in 21cm intensity maps
• An effective description of Laniakea: impact on cosmology and the local determination of the Hubble constant
• Rapid simulation rescaling from standard to modified gravity models
• Comparing halo bias from abundance and clustering
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• A closer look at CMB constraints on WIMP dark matter
• Satellite quenching was not important for z$\sim$1 clusters: most quenching occurred during infall
• Formation and Evolution of Early-Type Galaxies. III Star formation history as a function of mass and over-density
• The Halo Mass-Bias Redshift Evolution in the $\Lambda$CDM Cosmology
• The initial shear field in models with primordial local non-Gaussianity and implications for halo and void abundances
• Annealing a Follow-up Program: Improvement of the Dark Energy Figure of Merit for Optical Galaxy Cluster Surveys
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Triaxial collapse and virialisation of dark-matter haloes
• Evaporation of planetary atmospheres due to XUV illumination by quasars
• Large scale clustering measurements with photometric redshifts: comparing the dark matter halos of X-ray AGN, star-forming and passive galaxies at z~1
• The earliest galaxies seen in 21 cm line absorption
• The power spectrum amplitude from clusters revisited: σ_8 using simulations with preheating and cooling
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• Calibrating the Galaxy Halo - Black Hole Relation Based on the Clustering of Quasars
• Non-local bias in the halo bispectrum with primordial non-Gaussianity
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• Luminosity Dependent X-ray AGN Clustering ?
• Non-Gravitational Contributions to the Clustering of Ly-alpha Selected Galaxies: Implications for Cosmological Surveys
• Distinguishing standard reionization from dark matter models
• Mass functions and bias of dark matter halos
• Constraining Primordial Magnetic Fields with Future Cosmic Shear Surveys
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• On the Average Comoving Number Density of Halos
• The ISW-tSZ cross correlation: ISW extraction out of pure CMB data
• Revealing the cosmic web dependent halo bias
• Galaxy Clustering and Dark Energy
• The Dearth of Chemically Enriched Warm-Hot Circumgalactic Gas
• Reionization Bias in High Redshift Quasar Near-Zones
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Cluster correlations in redshift space
• The AGN-galaxy-halo connection: The distribution of AGN host halo masses to z=2.5
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• AGN environments at z<1.5 in the UKIDSS Ultra-Deep Survey
• The Local Group: The Ultimate Deep Field
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering
• Impact of astrophysical processes on the gamma-ray background from dark matter annihilations
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• The influence of halo assembly on galaxies and galaxy groups
• ALP Dark Matter Mini-Clusters from Kinetic Fragmentation
• An improved model of HII bubbles during the epoch of reionization
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• The importance of stepping up in the excursion set approach
• Constraining cosmological parameters with the clustering properties of galaxy clusters in optical and X-ray bands
• ELUCID V. Lighting dark matter halos with galaxies
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• The importance of galaxy formation histories in models of reionization
• Ultra-faint high-redshift galaxies in the Frontier Fields
• Probing high-redshift galaxies with Ly$\alpha$ intensity mapping
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• DEMNUni: disentangling dark energy from massive neutrinos with the void size function
• Effects of superstructure environment on galaxy groups
• Local and global environmental effects on galaxies and active galactic nuclei
• Self-consistency of the Excursion Set Approach
• Constraints on black hole duty cycles and the black hole-halo relation from SDSS quasar clustering
• How accurate is it to update the cosmology of your halo catalogues?
• An MCMC Fitting Method for Triaxial Dark Matter Haloes
• Conditional Mass Functions and Merger Rates of Dark Matter Halos in the Ellipsoidal Collapse Model
• Future Constraints on the Reionization History and the Ionizing Sources from Gamma-ray Burst Afterglows
• Some improvements to the spherical collapse model
• Lensing constraints on ultradense dark matter halos
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• Clustering dark energy and halo abundances
• The halo bias inside cosmic voids
• Prompt cusps and the dark matter annihilation signal
• On the abundance of collapsed objects
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• A Comparison of Simulated and Analytic Major Merger Counts
• Measuring nonlocal Lagrangian peak bias
• Conditional Probabilities in the Excursion Set Theory. Generic Barriers and non-Gaussian Initial Conditions
• Scale-Dependent Bias of Galaxies from Baryonic Acoustic Oscillations
• 21cm signal sensitivity to dark matter decay
• The clustering amplitude of X-ray selected AGN at z=0.8: Evidence for a negative dependence on accretion luminosity
• Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82
• Diffuse gamma-ray constraints on dark matter revisited. I: the impact of subhalos
• Searching for Intergalactic Shocks with the SKA
• The Halo Void (Dust) Model of Large Scale Structure
• Characterizing dark interactions with the halo mass accretion history and structural properties
• The formation of CDM haloes II: collapse time and tides
• An Observational Limit on the Earliest GRBs
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• Soliton Merger Rates and Enhanced Axion Dark Matter Decay
• Testing Lambda CDM cosmology at turnaround: where to look for violations of the bound?
• Statistics of Dark Matter Halos from the Excursion Set Approach
• Shell-crossing in a $\Lambda$CDM Universe
• The clustering of the first galaxy halos
• The locations of halo formation and the peaks formalism
• Computation of the Halo Mass Function Using Physical Collapse Parameters: Application to Non-Standard Cosmologies
• Press-Schechter primordial black hole mass functions and their observational constraints
• The Accretion and Cooling of Preheated Gas in Dark Matter Halos
• The HI mass function of group galaxies in the ALFALFA survey
• DM haloes in the fifth-force cosmology
• Properties of Wide-separation Lensed Quasars by Clusters of Galaxies in the SDSS
• Evolution of high-redshift quasar hosts and promotion of massive black hole seed formation
• CosmoReionMC: A package for estimating cosmological and astrophysical parameters using CMB, Lyman-α absorption and global 21 cm data
• On Correlated Random Walks and 21-cm Fluctuations During Cosmic Reionization
• Testing the Modified Press-Schechter Model against N-Body Simulations
• Structure Formation and the Global 21-cm Signal in the Presence of Coulomb-like Dark Matter-Baryon Interactions
• The dependence of the X-ray AGN clustering on the properties of the host galaxy
• The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution Functions
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• When do cosmic peaks, filaments or walls merge? A theory of critical events in a multi-scale landscape
• The giant arc statistics in the three year WMAP cosmological model
• K-mouflage effects on clusters of galaxies
• The Clustering Evolution of Dusty Star-Forming Galaxies
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• The Origin of Dark Matter Halo Profiles
• Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal
• Clustering of Intermediate Luminosity X-ray selected AGN at z~3
• Effects of Velocity-Dependent Dark Matter Annihilation on the Energy Spectrum of the Extragalactic Gamma-ray Background
• Changes in the halo formation rates due to features in the primordial spectrum
• The halo mass function and inner structure of ETHOS haloes at high redshift
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• The Excursion set approach: Stratonovich approximation and Cholesky decomposition
• AGN and QSOs in the eROSITA All-Sky Survey -- Part II: The large-scale structure
• Observational Measures of Halo Properties Beyond Mass
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Globular Clusters in High-Redshift Dwarf Galaxies: A Case Study from the Local Group
• Implication of the Shape of the EDGES Signal for the 21 cm Power Spectrum
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• The Subaru/XMM-Newton Deep Survey (SXDS) -VII. Clustering Segregation with Ultraviolet and Optical Luminosities of Lyman-Break Galaxies at z~3
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• The median density of the Universe
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• Galaxy And Mass Assembly: Estimating galaxy group masses via caustic analysis
• A new model for the full shape of the large-scale power spectrum
• Optimal filters for the moving lens effect
• The bias of dark matter tracers: assessing the accuracy of mapping techniques
• The universal multiplicity function: counting halos and voids
• Constraints on Primordial Power Spectrum from Galaxy Luminosity Functions
• 21 cm Forest Constraints on Primordial Black Holes
• 21cmfish: Fisher-matrix framework for fast parameter forecasts from the cosmic 21-cm signal
• The Supersonic Project: rotational effects of supersonic motions on the first structures in the Universe
• Evidence for Merger-Driven Activity in the Clustering of High Redshift Quasars
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
• BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn
• CMB lensing reconstruction biases from masking extragalactic sources
• The WIRCam Deep Survey II: Mass Selected Clustering
• The Normalization and Slope of the Dark Matter (Sub-)Halo Mass Function on Sub-Galactic Scales
• Observing the First Stars and Black Holes
• X-ray Cluster Constraints on Non-Gaussianity
• Velocity and mass bias in the distribution of dark matter halos
• Extending the halo mass resolution of $N$-body simulations
• Evolution of the Cluster Mass and Correlation Functions in LCDM Cosmology
• The Formation and Evolution of the First Massive Black Holes
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• Constraints on Primordial non-Gaussianity from Future HI Intensity Mapping Experiments
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• Are Faint Supernovae Responsible for Carbon-Enhanced Metal-Poor Stars?
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• The excursion set approach in non-Gaussian random fields
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance
• Synergies between radio, optical and microwave observations at high redshift
• The build-up of halos within Press-Schechter theory
• Taming assembly bias for primordial non-Gaussianity
• The clustering of baryonic matter. I: a halo-model approach
• Diffuse gamma-ray background and cosmic-ray positrons from annihilating dark matter
• Stochastic bias in multi-dimensional excursion set approaches
• Imprint of Inhomogeneous Reionization on the Power Spectrum of Galaxy Surveys at High Redshifts
• Non-Gaussianity and Excursion Set Theory: Halo Bias
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• Dark Matter Microhalos in the Solar Neighborhood: Pulsar Timing Signatures of Early Matter Domination
• Connecting the Extremes: A Story of Supermassive Black Holes and Ultralight Dark Matter
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Effective Window Function for Lagrangian Halos
• The Effect of Radiative Cooling on the Sunyaev-Zel'dovich Cluster Counts and Angular Power Spectrum: Analytic Treatment
• The Cosmological History of Accretion onto Dark Halos and Supermassive Black Holes
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• The Density Contrast of the Shapley Supercluster
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• Non-Gaussian Halo Mass Function and Non-Spherical Halo Collapse: Theory vs. Simulations
• Clustering of Ly-alpha emitters around luminous quasars at z = 2-3: an alternative probe of reionization on galaxy formation
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• On the cosmological mass function theory
• The very wide-field $gzK$ galaxy survey -- I. Details of the clustering properties of star-forming galaxies at $z\sim 2$
• Orbital distribution of infalling satellite halos across cosmic time
• Extending Recovery of the Primordial Matter Power Spectrum
• Spherical collapse model in agegraphic dark energy cosmologies
• Halo bias in the excursion set approach with correlated steps
• Probing dark matter signals in neutrino telescopes through angular power spectrum
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• Double Distribution of Dark Matter Halos with respect to Mass and Local Overdensity
• Weak lensing by triaxial galaxy clusters
• Systematic uncertainties in models of the cosmic dawn
• Cluster Lensing of QSOs as a Probe of LCDM and Dark Energy Cosmologies
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• The Size Distribution of Void Filaments in a LCDM Cosmology
• Magnification bias as a novel probe for primordial magnetic fields
• Strong lensing constraints on primordial black holes as a dark matter candidate
• Lensing effects of misaligned disks in dark matter halos
• Stochastic gravitational wave background from cold dark matter halos
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Dark Matter Halos from the Inside Out
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• Constraining isocurvature perturbations with the 21cm emission from minihaloes
• A Method to Measure the Mass of Damped Ly-alpha Absorber Host Galaxies Using Fluctuations in 21cm Emission
• Halo Occupation Distribution of Massive Galaxies since z = 1
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Small scale clustering of late forming dark matter
• Groups and protocluster candidates in the CLAUDS and HSC-SSP joint deep surveys
• Quasar clustering in a galaxy and quasar formation model based on ultra high-resolution N-body simulations
• Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
• Machine-learning recovery of foreground wedge-removed 21-cm light cones for high-$z$ galaxy mapping
• Push it to the limit: Local Group constraints on high-redshift stellar mass functions for Mstar > 10^5 Msun
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• Are the 2dFGRS superstructures a problem for hierarchical models?
• Modification of the 21-cm power spectrum by X-rays during the epoch of reionisation
• Small scale structures in coupled scalar field dark matter
• Normalization of the Matter Power Spectrum via Higher-Order Angular Correlations of Luminous Red Galaxies
• The Effect of Formation Redshifts on the Cluster Mass-Temperature Relation
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• Matter power spectra in dynamical-Dark Energy cosmologies
• The Universal Specific Merger Rate of Dark Matter Halos
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Structure formation in dark energy cosmologies described by PADE parameterization
• Probing the cosmic microwave background temperature using the Sunyaev-Zeldovich effect
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Clustering dependence on Lyman-$\alpha$ luminosity from MUSE surveys at $3<z<6$
• Evolution of perturbations in distinct classes of canonical scalar field models of dark energy
• Mass of clusters in simulations
• Large-scale bias of dark matter halos
• A simplified model of the formation of structures in the dark matter, and a background of very long gravitational waves
• Modelling the shapes of the largest gravitationally bound objects
• Constraints on the $z\sim 6-13$ intergalactic medium from JWST spectroscopy of Lyman-alpha damping wings in galaxies
• A random-walk model for dark matter halo spins
• A Merger Tree with Microsolar Mass Resolution: Application to $\gamma$-ray Emission from Subhalo Population
• EDGES result versus CMB and low-redshift constraints on ionization histories
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Primordial magnetic fields: consistent initial conditions and impact on high-z structures
• A Consistent Comparison of Bias Models using Observational Data
• Discriminating power of milli-lensing observations for dark matter models
• Halo assembly bias from a deep learning model of halo formation
• Galaxy Tagging: photometric redshift refinement and group richness enhancement
• Primordial Black Hole Formation from Power Spectrum with Finite-width
• The Quasar-LBG Two-point Angular Cross-correlation Function at z ~ 4 in the COSMOS Field
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Testing model independent modified gravity with future large scale surveys
• Modification of the 21-cm power spectrum by quasars during the epoch of reionisation
• Spherical collapse in Generalized Dark Matter models
• Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright sub-millimetre galaxies
• The Flatness and Sudden Evolution of the Intergalactic Ionizing Background
• The effect of stellar encounters on the dark matter annihilation signal from prompt cusps
• Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8
• Uncertainties in primordial black-hole constraints on the primordial power spectrum
• Merger history trees of dark matter haloes in moving barrier models
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• Clustering of gamma-ray selected 2LAC Fermi Blazars
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• The Halo Occupation Distribution of HI from 21cm Intensity Mapping at Moderate Redshifts
• Indra: a Public Computationally Accessible Suite of Cosmological $N$-body Simulations
• Synergies across the spectrum for particle dark matter indirect detection: how HI intensity mapping meets gamma rays
• Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
• Growth of non-linear structures and spherical collapse in the Galileon Ghost Condensate model
• Towards 1% accurate galaxy cluster masses: Including baryons in weak-lensing mass inference
• Implications of a Temperature Dependent IMF III: Mass Growth and Quiescence
• Phase Space dynamics of triaxial collapse: Joint density-velocity evolution
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• A physical and concise halo model based on the depletion radius
• The spatial clustering of ROSAT all-sky survey Active Galactic Nuclei: V. The evolution of broad-line AGN clustering properties in the last 6 Gyr
• Primordial Black Hole Merger Rate in $f(R)$ Gravity
• Primordial Bispectrum and Trispectrum Contributions to the Non-Gaussian Excursion Set Halo Mass Function with Diffusive Drifting Barrier
• Quantifying the tension between cosmological models and JWST red candidate massive galaxies
• The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars
• Galaxy Clusters in the Line of Sight to Background Quasars: II. Environmental effects on the sizes of baryonic halo sizes
• Statistics of gravitational potential perturbations: A novel approach to deriving the X-ray temperature function
• The Imprint of Cosmic Reionization on Galaxy Clustering
• Testing galaxy formation models with galaxy stellar mass functions
• Can AGN and galaxy clusters explain the surface brightness fluctuations of the cosmic X-ray background?
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Evolution of the Cluster Correlation Function
• On the Angular Correlation Function of SZ Clusters : Extracting cosmological information from a 2D catalog
• Stacking Clusters in the ROSAT All-Sky Survey
• High-redshift voids in the excursion set formalism
• Modeling active galactic nuclei: ongoing problems for the faint-end of the luminosity function
• Dark matter halo creation in moving barrier models
• Excursion set peaks in energy as a model for haloes
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• A prescription for the conditional mass function of dark matter haloes
• Toward an Improved Analytical Description of Lagrangian Bias
• An Accurate Comprehensive Approach to Substructure: I. Accreted Subhaloes
• The Clustering of Undetected High-redshift Black Holes and Their Signatures in Cosmic Backgrounds
• Culminating the peak CUSP to descry the dark side of halos
• Which halos host Herschel-ATLAS galaxies in the local Universe?
• Performance study of Lagrangian methods: reconstruction of large scale peculiar velocities and baryonic acoustic oscillations
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-$\alpha$ emitters at $3.3<z<6$
• Analytical halo models of cosmic tidal fields
• Application of cross correlations between CMB and large scale structure to constraints on the primordial non-Gaussianity
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Multiply-imaged time-varying sources behind galaxy clusters - Comparing FRBs to QSOs, SNe, and GRBs
• Quasi-spherical collapse of matter in $\Lambda$CDM
• Nonlinear stochastic biasing of halos: Analysis of cosmological N-body simulations and perturbation theories
• Angular momentum evolution of stellar disks at high redshifts
• Clustering of CODEX clusters
• Impact of a non-Gaussian density field on Sunyaev-Zeldovich observables
• The generalized evolution of linear bias: a tool to test gravity
• Triggering the formation of direct collapse black holes by their congeners
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• The XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties
• Lagrangian bias in the local bias model
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• The bias of weighted dark matter halos from peak theory
• Neglecting Primordial non-Gaussianity Threatens Future Cosmological Experiment Accuracy
• Spherical collapse of dark matter haloes in tidal gravitational fields
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Ellipsoidal collapse and the redshift space probability distribution function of dark matter
• Effects of P-wave Annihilation on the Angular Power Spectrum of Extragalactic Gamma-rays from Dark Matter Annihilation
• CMB distortion from circumgalactic gas
• A novel approach to cosmological non-linearities as an effective fluid
• Non-spherical effects on the mass function of Primordial Black Holes
• Growing the First Galaxies' Merger Trees
• The Anisotropic Two-Point Correlation Functions of the Nonlinear Traceless Tidal Field in the Principal-Axis Frame
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• A Cosmological Solution to the Impossibly Early Galaxy Problem
• Subhalo effective density slope measurements from HST strong lensing data with neural likelihood-ratio estimation
• Massive prompt cusps: A new signature of warm dark matter
• Dark Matter annihilation energy output and its effects on the high-z IGM
• Explanation of high redshift luminous galaxies from JWST by early dark energy model
• Analytic Approach to the Cloud-in-cloud Problem for Non-Gaussian Density Fluctuations
• Evolution of the cosmological mass function in a moving barrier model
• Predicting the clustering properties of galaxy clusters detectable for the Planck satellite
• Bias and Conditional Mass Function of Dark Halos Based on the Nonspherical Collapse Model
• Mapping reionization bubbles in the JWST era I: empirical edge detection with Lyman alpha emission from galaxies
• Light-Cone Distortion of the Clustering and Abundance of Massive Galaxies at High-Redshifts
• The mass and temperature functions in a moving barrier model
• Deep learning insights into cosmological structure formation
• Testing General Relativity Using the Evolution of Linear Bias
• An empirical model to form and evolve galaxies in dark matter halos
• Extragalactic and galactic gamma-rays and neutrinos from annihilating dark matter
• Strong-lensing cosmography using third-generation gravitational-wave detectors
• Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect
• Bianchi IX gravitational collapse of matter inhomogeneities
• Intrinsic alignments of bulges and discs
• Linking X-ray AGN with dark matter halos: a model compatible with AGN luminosity function and large-scale clustering properties
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Alternative High-z Cosmic Tracers and the Dark Energy Equation of State
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• X-ray galaxy clusters abundance and mass temperature scaling
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Constraining higher-order parameters for primordial non-Gaussianities from power spectra and bispectra of imaging survey
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Limits on dark matter annihilation in prompt cusps from the isotropic gamma-ray background
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• An Introduction into the Theory of Cosmological Structure Formation
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
• Extended Press-Schechter theory and the density profiles of dark matter haloes
• The virialization density of peaks with general density profiles under spherical collapse
• Maximum amplitude of the high-redshift 21-cm absorption feature
• Probing Saraswati's heart: evaluating the dynamical state of the massive galaxy cluster A2631 through a comprehensive weak-lensing and dynamical analysis
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Probing the fluctuating Ultra-violet background using the Hubble Frontier Fields
• Lagrangian Statistics of Dark Halos in a LCDM Cosmology
• The effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• Statistics of Dark Matter Halos in the Excursion Set Peak Framework
• Uncertainties in the S-Z selected cluster angular power spectrum
• The causal effect of environment on halo mass and concentration
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• Remapping simulated halo catalogues in redshift space
• The full-sky Spherical Fourier-Bessel power spectrum in general relativity
• An Extended Zel'dovich Model for the Halo Mass Function
• Probing Dark Relativistic Species and Their Interactions with Dark Matter through CMB and 21cm surveys
• Starlight from JWST: Implications for star formation and dark matter models
• Efficient simulation of discrete galaxy populations and associated radiation fields during the first billion years
• Clustering and descendants of MUSYC galaxies at z<1.5
• Probing bursty star formation by cross-correlating extragalactic background light and galaxy surveys
• On merger bias and the clustering of quasars
• The nonlinear redshift space probability distribution function in models with local primordial non-Gaussianity
• Biased cosmological parameter estimation with galaxy cluster counts in the presence of primordial non-Gaussianities
• Anisotropic Halo Model
• Galaxy and Mass Assembly (GAMA): the clustering of galaxy groups
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Dark matter halo mass functions and density profiles from mass and energy cascade
• Understanding the Cosmic Mass Function High Mass Behaviour
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• Simple lessons from complex learning: what a neural network model learns about cosmic structure formation
• Probing the circumgalactic baryons through cross-correlations
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• Cosmological constraints from a 2D SZ catalog
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• CHAM: a fast algorithm of modelling non-linear matter power spectrum in the sCreened HAlo Model
• Power spectrum of density fluctuations, halo abundances and clustering with primordial black holes
• Galaxy Statistics in Pencil-beam Surveys at High Redshifts
• Choose to smooth: Gaussian streaming with the truncated Zel'dovich approximation
• Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations
• Anisotropies in the redshift-space correlations of galaxy groups and clusters II: Analysis of observational cluster samples
• The abundance of Bullet-groups in LCDM
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• Color dependence of clustering of massive galaxies at 0.5$\le z\le$2.5: similar spatial distributions between green valley galaxies and AGNs
• Predictions for the Counts of Faint, High-Redshift Galaxies in the Mid-Infrared
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• Cosmological Implications and Physical Properties of an X-Ray Flux-Limited Sample of Galaxy Clusters
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• Analysing the Epoch of Reionization with three-point correlation functions and machine learning techniques
• The Impact of HI in Galaxies on 21-cm Intensity Fluctuations During the Reionisation Epoch
• Constraining the mass-concentration relation through weak lensing peak function
• Interlopers speak out: studying the dark universe using small-scale lensing anisotropies
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Tetrahedral collapse: a rotational toy model of simultaneous dark-matter halo, filament and wall formation
• Stochastic Model of the Spin Distribution of Dark Matter Halos
• Resolution of the small scale structure issues with dissipative dark matter from multiple Standard Model sectors
• Probing the Primordial Power Spectrum with Cluster Number Counts
• Cosmology at high redshift -- a probe of fundamental physics
• Gravitational Lensing in More Realistic Dark Matter Halo Models
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• Effects of correlation between merging steps on the global halo formation
• Consistency relations for the Lagrangian halo bias and their implications
• Spherical collapse of non-top-hat profiles in the presence of dark energy with arbitrary sound speed
• Getting in shape with minimal energy. A variational principle for protohaloes
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• Effects of tidal gravitational fields in clustering dark energy models
• Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
• Dark matter halo assembly bias: environmental dependence in the non-Markovian excursion set theory
• A comparison of ${\text{H}}_2$ formation models at high redshift
• Halo mass function in scale invariant models
• Enhanced spectrum of primordial perturbations, galaxy formation and small scale structure
• A Random Walk Model for Dark Matter Halo Concentrations
• Anisotropic strong lensing as a probe of dark matter self-interactions
• Non-Markov Excursion Set Model of Dark Matter Halo Abundances
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Screened fifth forces in parity-breaking correlation functions
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
• Multi-wavelength consensus of large-scale linear bias
• On the anisotropic density distribution on large scales
• On the statistical theory of self-gravitating collisionless dark matter flow
• Cluster contribution to the X-ray background as a cosmological probe
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• Constrained simulations and excursion sets: understanding the risks and benefits of `genetically modified' haloes
• Halo Profile Evolution and Velocity Bias
• Nonlinear structure formation in Bound Dark Energy
• Bayesian Multi-line Intensity Mapping
• Exploring the physical origins of halo assembly bias from early times
• New insight into the variability of the Be star $\pi$ Aquarii: Determination of stellar and disk parameters
• Tidal shear and the consistency of microscopic Lagrangian halo approaches
• Clustering of galaxies around AGN in the HSC Wide survey
• Anisotropies in the redshift-space correlations of galaxy groups and clusters I: Simulated catalogues
• Toward More Realistic Mass Functions For Ultradense Dark Matter Halos
• Probing Quintessence Potential with Future Cosmological Surveys
• Massive black holes in high-redshift Lyman Break Galaxies
• Improvements in the M-T relation and mass function and the measured Omega_m through clusters evolution
• Understanding Galaxy Formation and Evolution
• Imprints of the super-Eddington accretion on the quasar clustering
• The baryon mass function for galaxy clusters
• Scale-dependent bias from an inflationary bispectrum: the effect of a stochastic moving barrier
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• Einasto profile as the halo model solution coupled to the depletion radius
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass
• Can prompt cusps of WIMP dark matter be detected as individual gamma-ray sources?
• Mass - concentration relation and weak lensing peak counts
• Integrated Sachs-Wolfe tomography with orthogonal polynomials
• Clustering Measurements of broad-line AGNs: Review and Future
• Matching JWST UV Luminosity Functions with Refined $\Lambda$CDM Halo Models
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Universality of the halo mass function in screened gravity theories
• Large-scale clustering of buried X-ray AGN: Trends in AGN obscuration and redshift evolution
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• The magnitude-redshift relation in a realistic inhomogeneous universe
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• The Impact of ionization Morphology and X-ray Heating on the Cosmological 21cm Skew Spectrum
• Ellipticity and prolaticity of the initial gravitational-shear field at the position of density maxima
• Non-linear density-velocity dynamics in $f(R)$ gravity from spherical collapse
• A new signature of primordial non-Gaussianities from the abundance of galaxy clusters
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Non-linear matter power spectrum without screening dynamics modelling in $f(R)$ gravity
• A Forecast for Large Scale Structure Constraints on Horndeski Gravity with Line Intensity Mapping
• 21-cm Constraints on Dark Matter Annihilation after an Early Matter-Dominated Era
• Constraining equilateral-type primordial non-Gaussianities from imaging surveys
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Mass bias and cosmological constraints from Planck cluster clustering
• Cosmic Variance and the Inhomogeneous UV Luminosity Function of Galaxies During Reionization
• Boosting the 21 cm forest signals by the clumpy substructures
• Constraints on Primordial Magnetic Fields from High Redshift Stellar Mass Density
• Bias-Limited Extraction of Cosmological Parameters
• Tidal virialization of dark matter haloes with clustering dark energy
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions
• High-redshift Galaxies from JWST Observations in More Realistic Dark Matter Halo Models
• Stochasticity in halo formation and the excursion set approach
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Evolution of the Deterministic Collapse Barrier of the Field Clusters as a Probe of Cosmology
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Tantalizing New Physics from the Cosmic Purview
• Scaling of the 1-halo terms with bias
• A spherical hydrodynamical model of cosmic voids in ΛCDM and beyond
• Regular and chaotic dynamics of non-spherical bodies. Zeldovich's pancakes and emission of very long gravitational waves
• The Shocking Truth: The small contribution to hydrogen reionization from gravitational infall
• Evolution of the real-space correlation function from next generation cluster surveys
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• A Hubble constant estimation with dark standard sirens and galaxy cluster catalogues
• Accurate halo mass functions from the simplest excursion set theory
• Angular fluctuations in the CXB: Is Fe 6.4 keV line tomography of the large-scale structure feasible?
• Cosmological constraints on neutrino masses in light of JWST red and massive candidate galaxies
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses
• An Empirical Mass Function Distribution
• An Analytical Approach to the Spin-Distribution of Dark Halos
• Testing Theoretical Models for the Higher-Order Moments of Dark Halo Distribution
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• Statistics for dark matter subhalo searches in gamma rays from a kinematically constrained population model: Fermi-LAT-like telescopes
• Negative feedback effects on star formation history and cosmic reionization
• Cosmology with voids from the Nancy Grace Roman Space Telescope
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• The influence of baryons on low-mass haloes
• Dark matter halo concentrations: a short review
• The Effect of Primordial Anti-Biasing on the Local Measurement of the Key Cosmological Parameters
• Interference in Fuzzy Dark Matter Filaments: Idealised Models and Statistics
• Characterising the optical properties of galaxy clusters with GMPhoRCC
• Statistical Properties of Supercluster-Like Filaments from Cosmological Simulations
• Redshift Horizon for Detecting the First Galaxies in Far-Infared Surveys
• Growth and Feedback from the First Black Holes
• On the statistical theory of self-gravitating collisionless dark matter flow: high order kinematic and dynamic relations
• Zero Metallicity with Zero CPU Hours: Masses of the First Stars on the Laptop
• The influence of superstructures on bright galaxy environments: clustering properties
• The Splashback Mass Function in the Presence of Massive Neutrinos
• The energy shear of protohaloes
• The pair-wise velocity dispersion of galaxies: effects of non radial motions
• The Halo Mass Function from Excursion Set Theory with a Non-Gaussian Trispectrum
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• The cusp-halo relation
• On the statistical theory of self-gravitating collisionless dark matter flow: Scale and redshift variation of velocity and density distributions
• On the Clustering of Compact Galaxy Pairs in Dark Matter Haloes
• Limits on Early Matter Domination from the Isotropic Gamma-Ray Background
• E and B modes of the CMB y-type distortions: polarised kinetic Sunyaev-Zeldovich effect from the reionisation and post-reionisation eras
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• The Supersonic Project: SIGOs, a Proposed Progenitor to Globular Clusters, and their Connections to Gravitational Wave Anisotropies
• The Effects of Dark Matter Annihilation and Dark Matter-Baryon Velocity Offsets at Cosmic Dawn
• The AIDA-TNG project: 3D halo shapes
• On the origin of transient features in cosmological N-Body Simulations
• Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
• Determination of the Linear Mass Power Spectrum From the Mass Function of Galaxy Clusters
• Mass function and assembly of dark halos: an approach to inventory isolated overdense regions in random fields
• Astrophysical uncertainties challenge 21-cm forecasts: A primordial black hole case study
• Toward Gravitational Lensing in Modified Theories of Gravity
• oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization
• Ultradense Dark Matter Halos with Poisson Noise from Stellar-Mass Primordial Black Holes
• Comparison of the linear bias models in the light of the Dark Energy Survey
• VEGA: Voids idEntification using Genetic Algorithm
• On the tomographic cluster clustering as a cosmological probe
• Distinguishing thermal histories of dark matter from structure formation
• Sunyaev-Zel'dovich galaxy clusters number counts : consequences of cluster scaling laws evolution
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Can WIMPs Survive the Legacy of a Magnetised Early Universe?
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Relativistic modeling of cosmological structures with Bianchi IX spacetimes
• On Local Approximations to the Nonlinear Evolution of Large-Scale Structure
• Properties of environment around AGN and luminous galaxy pairs through HSC wide survey
• Linear and nonlinear clusterings of Horndeski-inspired dark energy models with fast transition
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• Individual halo bias in models of $f(R)$ gravity
• The evolution of Balmer jump selected galaxies in the ALHAMBRA survey
• Generalized local ansatz for scale-dependent primordial non-Gaussianities and future galaxy surveys
• Path integral approach for merger rates of dark matter haloes
• Testing the thermal Sunyaev-Zel'dovich power spectrum of a halo model using hydrodynamical simulations
• Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• Excursion Sets with a "Perfect" Collapse Model
• MIDIS: Unveiling the Star Formation History in massive galaxies at $1<z<4.5$ with spectro-photometric analysis
• Cross bispectra and trispectra of the non-linear integrated Sachs-Wolfe effect and the tracer galaxy density field
• Clustering of dark matter in the cosmic web as a probe of massive neutrinos
• Dark Matter Annihilations in the Causal Diamond
• Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
• Impact of the shape of the prestellar density fluctuations on the core mass function
• Effects of dynamical friction on perturbations for evolving dark energy
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• On the virialization threshold for halo mass functions
• Impact of a Rapid Diluted Energy Density on the halo mass function
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• On the first crossing distributions in fractional Brownian motion and the mass function of dark matter haloes
• Sunyaev-Zeldovich Cluster Counts as a Probe of Intra-Supercluster Gas
• The Angular Correlation Function as measured by the GLEAM-X Survey
• Morphology of dark matter haloes beyond triaxiality
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Mass transport in galaxy discs limits black hole growth to sub-Eddington rates
• Cosmological constraints from clustering properties of galaxy clusters
• Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
• Understanding galaxy formation and evolution through an all-sky submillimetre spectroscopic survey
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies
• Determining the Dark Matter distribution in galaxies with Deep Learning
• Probing the warm dark matter mass with [C II] intensity mapping
• Finding High-Redshift Galaxies with JWST
• Axion-Like Particle Dark Matter Intensity Mapping: A New Probe via Cross-Correlation with Galaxy Surveys
• Prompt cusps in hierarchical dark matter halos: Implications for annihilation boost
• Cosmic velocity, density and halo mass function: Insights from deep learning
• Free Cosmic Density Bispectrum on Small Scales
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
• The role of energy shear in the collapse of protohaloes
• Origin & evolution of the Universe
• Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
• Universality of the halo mass function in modified gravity cosmologies
• Skewness as a Probe of Gravity: Real and Redshift Space Counts-In-Cells
• A bubble size distribution model for the Epoch of Reionization
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Investigation of homogeneity and matter distribution on large scales using large quasar groups
• Quijote PNG: The information content of the halo power spectrum and bispectrum
• Exploring the Voids: Luminosity Functions and Magnetic Field
• Numerical approaches to star formation and SuperNovae energy feedback in simulations of galaxy clusters
• LSST Strong Lensing Systems Dark Matter Sensitivity Analysis with Neural Ratio Estimators
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
• Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models
• Compact star forming galaxies as the progenitors of compact quiescent galaxies: clustering result
• Clustering properties of TGSS radio sources
• Mapping the z>=5 SiIV Column Density Distribution onto the Galaxy Stellar Mass Function Using the Cumulative Absorption Cross Section
• Searching for a signature of turnaround in galaxy clusters with convolutional neural networks
• Using Dark Matter Haloes to Learn about Cosmic Acceleration: A New Proposal for a Universal Mass Function
• Quasar clustering at redshift 6
• Islands in Simulated Cosmos: Probing the Hubble Flow around Groups and Clusters
• A general framework for unbiased tests of gravity using galaxy clusters
• Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
• Excess of substructure due to primordial black holes
• Non-Gaussianity in the Squeezed Three-Point Correlation from the Relativistic Effects
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Luminosity Function of Galaxies in Voids: A Modification Inspired by Excursion Set Theory
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Slicing cluster mass functions with a Bayesian razor
• Mass functions from the excursion set model
• Dynamical friction shear and rotation in Chaplygin cosmology
• Segmenting proto-halos with vision transformers