Halo Models of Large Scale Structure

Abstract

We review the formalism and applications of the halo-based description of nonlinear gravitational clustering. In this approach, all mass is associated with virialized dark matter halos; models of the number and spatial distribution of the halos, and the distribution of dark matter within each halo, are used to provide estimates of how the statistical properties of large scale density and velocity fields evolve as a result of nonlinear gravitational clustering. We first describe the model, and demonstrate its accuracy by comparing its predictions with exact results from numerical simulations of nonlinear gravitational clustering. We then present several astrophysical applications of the halo model: these include models of the spatial distribution of galaxies, the nonlinear velocity, momentum and pressure fields, descriptions of weak gravitational lensing, and estimates of secondary contributions to temperature fluctuations in the cosmic microwave background.

166 pages, 60 figures (low resolution in most color figures); Invited review article for Physics Reports (final version in press). Compact versions with two pages on one and full resolution figures are available from http://www.its.caltech.edu/~asante

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• The Sunyaev-Zeldovich effect in CMB-calibrated theories applied to the Cosmic Background Imager anisotropy power at l > 2000
• Recovering the nonlinear density field from the galaxy distribution with a Poisson-Lognormal filter
• Did JWST observe imprints of axion miniclusters or primordial black holes?
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• General Requirements on Matter Power Spectrum Predictions for Cosmology with Weak Lensing Tomography
• The Local Bias Model in the Large Scale Halo Distribution
• Nonlinear structure formation in Nonlocal Gravity
• Looking at cosmic near-infrared background radiation anisotropies
• A General Study of the Influence of Catastrophic Photometric Redshift Errors on Cosmology with Cosmic Shear Tomography
• Towards a self-consistent halo model for the nonlinear large-scale structure
• Galaxy-halo alignments in the Horizon-AGN cosmological hydrodynamical simulation
• Is the Cosmic Microwave Background Circularly Polarized?
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Accurate cosmic shear errors: do we need ensembles of simulations?
• Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release
• Halo model and halo properties in Galileon gravity cosmologies
• The Far-Infrared Background Correlation with CMB Lensing
• The clustering of radio galaxies at z~0.55 from the 2SLAQ LRG survey
• Distribution function approach to redshift space distortions. Part IV: perturbation theory applied to dark matter
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• Back in the saddle: Large-deviation statistics of the cosmic log-density field
• Spectral Line De-confusion in an Intensity Mapping Survey
• Galaxy clustering from COMBO-17: The halo occupation distribution at <z>=0.6
• The Near-IR Background Intensity and Anisotropies During The Epoch of Reionization
• Higher Order Contributions to the 21 cm Power Spectrum
• Shapes of clusters and groups of galaxies: Comparison of model predictions with observations
• Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space
• HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements
• From Weak Lensing to non-Gaussianity via Minkowski Functionals
• Cross-correlation of Planck CMB Lensing and CFHTLenS Galaxy Weak Lensing Maps
• The velocity function of gas-rich galaxies
• Tidal alignments as a contaminant of redshift space distortions
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• The halo model for cosmology: a pedagogical review
• Scale Dependent Galaxy Bias in the SDSS as a function of Luminosity and Colour
• Clustering properties of $g$-selected galaxies at $z\sim 0.8$
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• Weighing neutrinos with cosmic neutral hydrogen
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• The environmental dependence of galaxy clustering in the Sloan Digital Sky Survey
• CHIME/FRB Catalog 1 results: statistical cross-correlations with large-scale structure
• Cross-Correlation of Cosmic Shear and Extragalactic Gamma-ray Background: Constraints on the Dark Matter Annihilation Cross-Section
• Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
• The 21cm bispectrum as a probe of non-Gaussianities due to X-ray heating
• Very small-scale clustering of quasars from a complete quasar lens survey
• Impact of Secondary non-Gaussianities on the Search for Primordial Non-Gaussianity with CMB Maps
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion
• How unusual are the Shapley Supercluster and the Sloan Great Wall?
• The Swift/BAT AGN Spectroscopic Survey -- IX. The Clustering Environments of an Unbiased Sample of Local AGN
• The clustering of SDSS galaxy groups: mass and color dependence
• Tomography of the Fermi-LAT gamma-ray diffuse extragalactic signal via cross-correlations with galaxy catalogs
• The halo model in a massive neutrino cosmology
• A flexible modelling of galaxy assembly bias
• The cross-correlation between galaxies of different luminosities and Colors
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• An estimate of the local ISW signal, and its impact on CMB anomalies
• Implications of the Fermi-LAT diffuse gamma-ray measurements on annihilating or decaying Dark Matter
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Halo modelling in chameleon theories
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• Unveiling Galaxy Bias via the Halo Model, KiDS and GAMA
• On Combining Galaxy Clustering and Weak Lensing to Unveil Galaxy Biasing via the Halo Model
• Constraining evolution in the Halo Model using galaxy redshift surveys
• Perturbative approach to covariance matrix of the matter power spectrum
• Simulating Structure Formation of the Local Universe
• Dark matter searches in the gamma-ray extragalactic background via cross-correlations with galaxy catalogues
• 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
• Information content in the halo-model dark-matter power spectrum
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• Large scale structure in non-standard cosmologies
• Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise
• Modelling Void Abundance in Modified Gravity
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• Particle dark matter searches in the anisotropic sky
• Galaxies flowing in the oriented saddle frame of the cosmic web
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Galaxy-Galaxy Lensing in the DES Science Verification Data
• Distribution function approach to redshift space distortions, Part III: halos and galaxies
• Breaking degeneracies in the first galaxies with clustering
• Dark matter annihilation and its effect on CMB and Hydrogen 21 cm observations
• Testing the Cosmological Principle with CatWISE Quasars: A Bayesian Analysis of the Number-Count Dipole
• Prospects for Detecting Dark Matter Halo Substructure with Pulsar Timing
• The Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?
• Fuzzy Dark Matter and the Dark Energy Survey Year 1 Data
• Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
• On the contribution of fluorescence to Ly$\alpha$ halos (LAHs) around star forming galaxies
• ISW measurements with photometric redshift surveys: 2MASS results and future prospects
• The clustering of Ly-alpha emitters in a LambdaCDM Universe
• The Benefits of CMB Delensing
• The DEEP2 Galaxy Redshift Survey: Clustering of Groups and Group Galaxies at z~1
• The correlation structure of dark matter halo properties
• The Impact of Intrinsic Alignments: Cosmological Constraints from a Joint Analysis of Cosmic Shear and Galaxy Survey Data
• Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
• Modelling galaxy clustering: Is new physics needed in galaxy formation models?
• Signatures of primordial black holes as seeds of supermassive black holes
• Lyman Break Galaxies and the Lyman-alpha Forest
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Joint analysis of cluster number counts and weak lensing power spectrum to correct for the super-sample covariance
• Dissipationless Merging and the Assembly of Central Galaxies
• Strong clustering of underdense regions and the environmental dependence of clustering from Gaussian initial conditions
• Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
• Intensity Mapping as a Probe of Axion Dark Matter
• Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
• Beyond the Damping Tail: Cross-Correlating the Kinetic Sunyaev-Zel'dovich Effect with Cosmic Shear
• Finite Source Effects in Strong Lensing: Implications for the Substructure Mass Scale
• Shot noise in the astrophysical gravitational-wave background
• Fitting the nonlinear matter bispectrum by the Halofit approach
• The Cosmic Near Infrared Background II: Fluctuations
• Structure formation in cosmologies with oscillating dark energy
• A multiscale approach to environment and its influence on the colour distribution of galaxies
• Non-Gaussian halo assembly bias
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• Responses in Large-Scale Structure
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• Modeling dark matter subhalos in a constrained galaxy: Global mass and boosted annihilation profiles
• The VIMOS-VLT Deep Survey. The dependence of clustering on galaxy stellar mass at z~1
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Ultraviolet Luminosity Density of the Universe During the Epoch of Reionization
• Prospects for constraining the shape of non-Gaussianity with the scale-dependent bias
• Imprint of galaxy clustering in the cosmic gamma-ray background
• Halo-model Analysis of the Clustering of Photometrically Selected Galaxies from SDSS
• Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• Combining Probes of Large-Scale Structure with CosmoLike
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• The clustering and bias of radio-selected AGN and star-forming galaxies in the COSMOS field
• Detecting Gamma-Ray Anisotropies from Decaying Dark Matter: Prospects for Fermi LAT
• Constraining the Baryon Abundance with the Kinematic Sunyaev-Zel'dovich Effect: Projected-Field Detection Using Planck, WMAP, and unWISE
• Reconstructing the distribution of haloes and mock galaxies below the resolution limit in cosmological simulations
• Systematic effects in large-scale angular power spectra of photometric quasars and implications for constraining primordial nongaussianity
• The halo-model description of marked statistics
• Distribution function approach to redshift space distortions. Part V: perturbation theory applied to dark matter halos
• Accurate mass and velocity functions of dark matter halos
• Vorticity of IGM Velocity Field on Large Scales
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• Rejuvenating Power Spectra II: the Gaussianized galaxy density field
• Accurate Modeling of Weak Lensing with the sGL Method
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Lagrangian or Eulerian; Real or Fourier? Not All Approaches to Large-Scale Structure Are Created Equal
• A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments
• The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring H(z) and D_A(z) at z = 0.57 with Clustering Wedges
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• TheHaloMod: An online calculator for the halo model
• Intensity mapping of H-alpha, H-beta, [OII] and [OIII] lines at z<5
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Fluctuations in the High-Redshift Lyman-Werner and Lyman-alpha Radiation Backgrounds
• The contribution of high redshift galaxies to the Near-Infrared Background
• Probing the diffuse baryon distribution with the lensing-tSZ cross-correlation
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Baryonic effects on the matter bispectrum
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• Systematic effects in the sound horizon scale measurements
• Interpreting the Clustering of Distant Red Galaxies
• A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups
• On CMB B-Mode Non-Gaussianity
• Probing Cosmic Reionization and Molecular Gas Growth with TIME
• Measuring our universe from galaxy redshift surveys
• The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
• A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample
• Towards understanding the structure of voids in the cosmic web
• Cosmic web dependence of galaxy clustering and quenching in SDSS
• Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models
• Modeling The Large Scale Bias of Neutral Hydrogen
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Substructure and the halo model of large-scale structure
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Tomographic-spectral approach for dark matter detection in the cross-correlation between cosmic shear and diffuse gamma-ray emission
• Complete Treatment of Galaxy Two-Point Statistics: Gravitational Lensing Effects and Redshift-Space Distortions
• Group connectivity in COSMOS: a tracer of mass assembly history
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• Cosmological Acceleration and Gravitational Collapse
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zeldovich effect cross-correlations
• Quasar-Galaxy and Galaxy-Galaxy Cross-Correlations: Model Predictions with Realistic Galaxies
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• Evidence of cross-correlation between the CMB lensing and the gamma-ray sky
• Halo Structures of Gravitational Lens Galaxies
• High Redshift Galaxy Populations and their Descendants
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Elucidating Galaxy Assembly Bias in SDSS
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• Gravitational redshifts from large-scale structure
• A halo model approach for the 21-cm power spectrum at cosmic dawn
• Fourier analysis of multi-tracer cosmological surveys
• Breaking Halo Occupation Degeneracies with Marked Statistics
• Halo Zeldovich model and perturbation theory: dark matter power spectrum and correlation function
• Lagrangian perturbation theory for modified gravity
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• Cross-correlating the gamma-ray sky with catalogs of galaxy clusters
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios
• On the Power Spectrum of Dark Matter Substructure in Strong Gravitational Lenses
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• Including beyond-linear halo bias in halo models
• The Inhomogeneous Ionizing Background Following Reionization
• Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Lensing Magnification: Implications for Counts of Submillimeter Galaxies and SZ Clusters
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Update on decaying and annihilating heavy dark matter with the 6-year IceCube HESE data
• Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
• Cosmology from supernova magnification maps
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Halo Occupation Number, Mass-to-Light Ratios and Omega_m
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• Perturbation theory approach for the power spectrum: from dark matter in real space to massive haloes in redshift space
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• Scale-dependent bias and the halo model
• Integrated Sachs Wolfe Effect and Rees Sciama Effect
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• Faint Submillimeter Galaxies identified through their optical/near-infrared colours I: spatial clustering and halo masses
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): An unbiased estimate of the growth rate of structure at $⟨\mathbf{z}⟩=0.85$ using the clustering of luminous blue galaxies
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• A tale of two populations: the stellar mass of central and satellite galaxies
• Why does the Jeans Swindle work?
• Structure Formation in Modified Gravity Scenarios
• Effects of Unstable Dark Matter on Large-Scale Structure and Constraints from Future Surveys
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Weak lensing constraints on splashback around massive clusters
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• Energy ejection in the collapse of a cold spherical self-gravitating cloud
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• SDSS-IV MaNGA: Galaxy Pair Fraction and Correlated Active Galactic Nuclei
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Angular averaged consistency relations of large-scale structures
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles
• On the road to percent accuracy V: the non-linear power spectrum beyond $\Lambda$CDM with massive neutrinos and baryonic feedback
• Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Spherical Collapse and Cluster Counts in Modified Gravity Models
• On Ellipsoidal Collapse and Primordial Black-Hole Formation
• The effect of early dark matter halos on reionization
• Matter power spectrum from a Lagrangian-space regularization of perturbation theory
• The Imprint of f(R) Gravity on Non-Linear Structure Formation
• Modeling color-dependent galaxy clustering in cosmological simulations
• Satellite Luminosities in Galaxy Groups
• Correlation between galaxies and QSO in the SDSS:na signal from gravitational lensing magnification?
• Redshifted 21 Centimeter Emission from Minihalos Before Reionization
• Joint likelihood function of cluster counts and $n$-point correlation functions: Improving their power through including halo sample variance
• Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background
• Simulations of the cosmic infrared and submillimeter background for future large surveys: I. Presentation and first application to Herschel/SPIRE and Planck/HFI
• Impact of shell crossing and scope of perturbative approaches in real and redshift space
• Shot noise and biased tracers: a new look at the halo model
• Higher-order moments of the lensing shear and other spin two fields
• The Next Generation Fornax Survey (NGFS): III. Revealing the Spatial Substructure of the Dwarf Galaxy Population inside half of Fornax's Virial Radius
• Power spectra in the eikonal approximation with adiabatic and non-adiabatic modes
• Cross-correlating galaxy catalogs and gravitational waves: a tomographic approach
• Exploring galaxy colour in different environments of the cosmic web with SDSS
• Fast Estimation of Gravitational and Primordial Bispectra in Large Scale Structures
• Post-collapse perturbation theory in 1D cosmology -- beyond shell-crossing
• HerMES: detection of cosmic magnification of sub-mm galaxies using angular cross-correlation
• Dark Matter Microhalos From Simplified Models
• Large Scale Structure Formation in Eddington-inspired Born-Infeld Gravity
• Scale-dependent Galaxy Bias
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• Accurate Weak Lensing of Standard Candles. II. Measuring sigma8 with Supernovae
• Axion decay and anisotropy of near-IR extragalactic background light
• The galaxy-halo connection in the VIDEO Survey at 0.5<z<1.7
• On the reach of perturbative methods for dark matter density fields
• The Signature of Large Scale Structures on the Very High Energy Gamma-Ray Sky
• Joint Analysis of Gravitational Lensing, Clustering and Abundance: Toward the Unification of Large-Scale Structure Analysis
• Halo abundances in the f_{nl} model
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• The Non-Linear Matter Power Spectrum in Warm Dark Matter Cosmologies
• Constraining the Mass-Richness Relationship of redMaPPer Clusters with Angular Clustering
• Bispectrum Supersample Covariance
• The observable 21cm signal from reionization may be perturbative
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• Redshift space 21 cm power spectra from reionization
• Power spectrum tomography of dark matter annihilation with local galaxy distribution
• Probability of primordial black hole formation and its dependence on the radial profile of initial configurations
• On the implementation of the spherical collapse model for dark energy models
• The dependence of the pairwise velocity dispersion on galaxy properties
• Constraining Dark Energy Evolution with Gravitational Lensing by Large Scale Structures
• The massive end of the luminosity and stellar mass functions and clustering from CMASS to SDSS: Evidence for and against passive evolution
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• The clustering of typical Ly$\alpha$ emitters from $z\sim 2.5-6$: host halo masses depend on Ly$\alpha$ and UV luminosities
• Edgeworth streaming model for redshift space distortions
• The Power Spectra of Polarized, Dusty Filaments
• Modeling the Very Small-Scale Clustering of Luminous Red Galaxies
• Constraints on Light WIMP candidates from the Isotropic Diffuse Gamma-Ray Emission
• Luminous Red Galaxies in hierarchical cosmologies
• Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Disantangling the effects of Doppler velocity and primordial non-Gaussianity in galaxy power spectra
• Testing phenomenological and theoretical models of dark matter density profiles with galaxy clusters
• A Higher Probability of Detecting Lensed Supermassive Black Hole Binaries by LISA
• Updated Constraints on Primordial Black Hole Evaporation
• The HI content of dark matter halos at $z\approx 0$ from ALFALFA
• Free-Free Emission at Low Radio Frequencies
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• The environmental dependence of clustering in hierarchical models
• Substructure in dark matter halos: Towards a model of the abundance and spatial distribution of subclumps
• The Secondary Spin Bias of Dark Matter Haloes
• Priors on red galaxy stochasticity from hybrid effective field theory
• LOFAR observations of the XMM-LSS field
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Statistical modelling of the cosmological dispersion measure
• Clustering of X-Ray-Selected AGN
• The impact of correlated projections on weak lensing cluster counts
• Kinematic Modelling of Disc Galaxies using Graphics Processing Units
• How much a galaxy knows about its large-scale environment?: An information theoretic perspective
• Combining perturbation theories with halo models for the matter bispectrum
• Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters I: Analysis with the Three Hundred Simulations
• Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Weak Lensing Observables in the Halo Model
• Extragalactic gamma-ray signal from Dark Matter annihilation: a power spectrum based computation
• Evolution of the Clustering of Photometrically Selected SDSS Galaxies
• Combining cluster number counts and galaxy clustering
• Small-scale structure and 21cm fluctuations by primordial black holes
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• The impact of halo shapes on the bispectrum in cosmology
• Propagators in Lagrangian space
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
• Constraining Cosmology with High Convergence Regions in Weak Lensing Surveys
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Dark Matter Signatures in the Anisotropic Radio Sky
• Super-sample covariance approximations and partial sky coverage
• Kinematic consistency relations of large-scale structures
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• Anisotropic cosmic optical background bound for decaying dark matter in light of the LORRI anomaly
• On the Physical Requirements for a Pre-Reionization Origin of the Unresolved Near-Infrared Background
• A Redefinition of the Halo Boundary Leads to a Simple yet Accurate Halo Model of Large Scale Structure
• Cosmological Constraints from the Large Scale Weak Lensing of SDSS MaxBCG Clusters
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• Halo Mass Functions in Early Dark Energy Cosmologies
• Intensity mapping cross-correlations II: HI halo models including shot noise
• Cross-correlation of weak lensing and gamma rays: implications for the nature of dark matter
• The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z $\sim$ 1
• Contributions to the Dark Matter 3-Pt Function from the Radiation Era
• CFHTLenS: A Weak Lensing Shear Analysis of the 3D-Matched-Filter Galaxy Clusters
• Dependence of halo bias on mass and environment
• Euclid: Forecasts from the void-lensing cross-correlation
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• The Correlated Formation Histories of Massive Galaxies and Their Dark Matter Halos
• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• Machine Learning for Observational Cosmology
• Cosmological N-Body Simulations with a Large-Scale Tidal Field
• Problems with Pencils: Lensing Covariance of Supernova Distance Measurements
• On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos
• Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
• Did WMAP see Moving Local Structures?
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• The importance of magnification effects in galaxy-galaxy lensing
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Interloper bias in future large-scale structure surveys
• IR Background Anisotropies in Spitzer GOODS images and constraints on first galaxies
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Cosmological Radio Emission induced by WIMP Dark Matter
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• The Maximum B-mode Polarization of the Cosmic Microwave Background from Inhomogeneous Reionization
• Gravitational Lensing of Schwarzschild and Charged Black Holes Immersed in Perfect Fluid Dark Matter Halo
• Cosmological Lower Bound on Dark Matter Masses from the Soft Gamma-ray Background
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Dark Matter via Many Copies of the Standard Model
• CMB Polarization towards Clusters as a Probe of the Integrated Sachs-Wolfe Effect
• Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
• Compact groups in theory and practice -- IV. The connection to large-scale structure
• Stability of Cool Cores During Galaxy Cluster Growth: A Joint $Chandra$/SPT Analysis of 67 Galaxy Clusters Along a Common Evolutionary Track Spanning 9 Gyr
• Cosmological searches for a non-cold dark matter component
• Robust PCA and MIC statistics of baryons in early mini-haloes
• Rapid simulation rescaling from standard to modified gravity models
• Expansion schemes for gravitational clustering: computing two-point and three-point functions
• Modeling the evolution of infrared galaxies : clustering of galaxies in the Cosmic Infrared Background
• Comparing PyMorph and SDSS photometry. II. The differences are more than semantics and are not dominated by intracluster light
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Comparing halo bias from abundance and clustering
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• On estimating cosmology-dependent covariance matrices
• Next-to-leading resummations in cosmological perturbation theory
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• Why Newton's gravity is practically reliable in the large-scale cosmological simulations
• Propagating sample variance uncertainties in redshift calibration: simulations, theory and application to the COSMOS2015 data
• The distribution of Lyman-limit absorption systems during and after reionization
• The Second Radio Synchrotron Background Workshop: Conference Summary and Report
• The earliest galaxies seen in 21 cm line absorption
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Cosmic Structure Formation with Kinetic Field Theory
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• Cross-Correlation Studies between CMB Temperature Anisotropies and 21 cm Fluctuations
• Non-Gaussianity of the Cosmic Infrared Background anisotropies I : Diagrammatic formalism and application to the angular bispectrum
• Stellar-to-halo mass relation of cluster galaxies
• The squeezed matter bispectrum covariance with responses
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• Impact of Redshift Information on Cosmological Applications with Next-Generation Radio Surveys
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• Constraining Primordial Magnetic Fields with Future Cosmic Shear Surveys
• Galaxy Clustering and Dark Energy
• Deciphering the Archaeological Record: Cosmological Imprints of Non-Minimal Dark Sectors
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• What determines large scale galaxy clustering: halo mass or local density?
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• Clustering properties of high redshift red galaxies in SA22 from the UKIDSS DXS
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• The ISW-tSZ cross correlation: ISW extraction out of pure CMB data
• Exploring KSZ velocity reconstruction with $N$-body simulations and the halo model
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Large-Scale Non-Gaussianities in the 21 cm Background Anisotropies From the Era of Reionization
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• Radio signatures from encounters between Neutron Stars and QCD-Axion Minihalos around Primordial Black Holes
• The evolution of the galaxy content of dark matter haloes
• Background cosmological dynamics in $f(R)$ gravity and observational constraints
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• Revealing the cosmic web dependent halo bias
• Self-Calibration Technique for 3-point Intrinsic Alignment Correlations in Weak Lensing Surveys
• AGN environments at z<1.5 in the UKIDSS Ultra-Deep Survey
• Linear and non-linear bias: predictions vs. measurements
• A dynamics-based density profile for dark haloes -- II. Fitting function
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• An improved model of HII bubbles during the epoch of reionization
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• Modeling the Phase-Space Distribution around Massive Halos
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• The influence of halo assembly on galaxies and galaxy groups
• SDSS-IV MaNGA: The Radial Profile of Enhanced Star Formation in Close Galaxy Pairs
• Cosmological Structure Formation in Decaying Dark Matter Models
• Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: Statistical and systematic error budgets for future experiments
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• Fast Weak Lensing Simulations with Halo Model
• Modeling the clustering of dark-matter haloes in resummed perturbation theories
• Environmental Quenching and Galactic Conformity in the Galaxy Cross-Correlation Signal
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Halo Exclusion Criteria Impacts Halo Statistics
• Effects of superstructure environment on galaxy groups
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Galaxy surveys, inhomogeneous reionization, and dark energy
• Cosmological constraints on dark matter annihilation and decay: Cross-correlation analysis of the extragalactic $\gamma$-ray background and cosmic shear
• H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above $\sim 1$ arcmin
• Detection of cross-correlation between gravitational lensing and gamma rays
• Probing galaxy assembly bias with LRG weak lensing observations
• Masses of high-z galaxy hosting haloes from angular clustering and their evolution in the CDM model
• Future Constraints on the Reionization History and the Ionizing Sources from Gamma-ray Burst Afterglows
• Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Searching for Sterile Neutrino with X-ray Intensity Mapping
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Anisotropy Studies of the Unresolved Far-infrared Background
• Impacts of satellite galaxies on the redshift-space distortions
• Sensitivity of dark matter haloes to their accretion histories
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• The role of the eROSITA all-sky survey in searches for sterile neutrino dark matter
• Search for sharp and smooth spectral signatures of $\mu \nu$SSM gravitino dark matter with Fermi-LAT
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
• Towards a non-Gaussian model of redshift space distortions
• Equal-time Consistency Relations in the Large-Scale Structure of the Universe
• Covariance of the galaxy angular power spectrum with the halo model
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• First detection of galaxy-galaxy-galaxy lensing in RCS. A new tool for studying the matter environment of galaxy pairs
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
• Understanding the non-linear clustering of high redshift galaxies
• Characterizing dark interactions with the halo mass accretion history and structural properties
• On the validity of the Born approximation for weak cosmic flexions
• Splashback radius of nonspherical dark matter halos from cosmic density and velocity fields
• Clustering of the IR Background Light with Spitzer: Contribution from Resolved Sources
• Halos and voids in a multifractal model of cosmic structure
• Optimizing weak lensing mass estimates for cluster profile uncertainty
• The SZ effect contribution to WMAP. A Cross-Correlation between WMAP and ROSAT
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• Intrinsic Alignments and Splashback Radius of Dark Matter Halos from Cosmic Density and Velocity Fields
• The Halo Void (Dust) Model of Large Scale Structure
• The clustering amplitude of X-ray selected AGN at z=0.8: Evidence for a negative dependence on accretion luminosity
• The Effect of Large-Scale Structure on the Magnification of High-Redshift Sources by Cluster-Lenses
• Secondary non-Gaussianity and Cross-Correlation Analysis
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• How to Search for Islands of Neutral Hydrogen in the $z\sim 5.5$ IGM
• The luminosities of the brightest cluster galaxies and brightest satellites in SDSS groups
• A Conditional Luminosity Function Model of the Cosmic Far-Infrared Background Anisotropy Power Spectrum
• Deviations from tidal torque theory: environment dependences on halo angular momentum growth
• Understanding the PSCz Galaxy Power Spectrum with N-body Simulations
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• A Measurement of Primordial Non-Gaussianity Using WMAP 5-Year Temperature Skewness Power Spectrum
• Halo model prediction of the cosmic magnification statistics: the full non-linear contribution
• First measurement of the characteristic depletion radius of dark matter haloes from weak lensing
• A direct detection of neutral hydrogen intensity mapping on Mpc scales at $z\approx 0.32$ and $z\approx 0.44$
• The probability distribution function of the SZ power spectrum: an analytical approach
• Steepened inner density profiles of group galaxies via interactions: An N-body analysis
• Improved Mixed Dark Matter Halo Model for Ultralight Axions
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• The effects of halo alignment and shape on the clustering of galaxies
• The clustering of submillimeter galaxies detected with ALMA
• Higher Order Statistics for Three-dimensional Shear and Flexion
• Tidal alignments as a contaminant of the galaxy bispectrum
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• The Fractal Geometry of the Cosmic Web and its Formation
• Covariance matrices for halo number counts and correlation functions
• The impact of baryons on the sensitivity of dark energy measurements
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• The detection of the imprint of filaments on cosmic microwave background lensing
• Pair Correlations and Merger Bias
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• Tomographic imaging of the Fermi-LAT gamma-ray sky through cross-correlations: A wider and deeper look
• The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Effects of halo substructure on the power spectrum and bispectrum
• Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Spatial Clustering from GALEX-SDSS samples: Star Formation History and large-scale clustering
• A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol
• Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
• Debiasing inference with approximate covariance matrices and other unidentified biases
• A short review on clustering dark energy
• Polarization of 21cm Radiation from the Epoch of Reionization
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• Effects of Velocity-Dependent Dark Matter Annihilation on the Energy Spectrum of the Extragalactic Gamma-ray Background
• The age dependence of galaxy clustering
• The Sunyaev-Zeldovich Effect from Quasar Feedback
• Kinematic Sunyaev-Zeldovich Cosmic Microwave Background Temperature Anisotropies Generated by Gas in Cosmic Structures
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• Taking advantage of photometric galaxy catalogues to determine the halo occupation distribution
• The Clustering Evolution of Dusty Star-Forming Galaxies
• The two and three-loop matter bispectrum in perturbation theories
• The hybrid SZ power spectrum: Combining cluster counts and SZ fluctuations to probe gas physics
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Contribution to Unresolved Infrared Fluctuations from Dwarf Galaxies at Redshifts of 2-3
• A new model for the full shape of the large-scale power spectrum
• Clustering at high redshift: The connection between Lyman Alpha emitters and Lyman break galaxies
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Describing galaxy weak lensing measurements from tenths to tens of Mpc and up to z~0.6 with a single model
• The Excursion set approach: Stratonovich approximation and Cholesky decomposition
• Detectability of the gravitational redshift effect from the asymmetric galaxy clustering
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• How well can (renormalized) perturbation theory predict dark matter clustering properties?
• Weak Lensing of the Primary CMB Bispectrum
• Cosmological parameter constraints from CMB lensing with cosmic voids
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• Cosmological Vlasov-Poisson Simulations of Structure Formation with Relic Neutrinos: Nonlinear Clustering and the Neutrino Mass
• A Bayesian method for combining theoretical and simulated covariance matrices for large-scale structure surveys
• Characterizing the local gamma-ray Universe via angular cross-correlations
• The 21-cm forest as a simultaneous probe of dark matter and cosmic heating history
• Relation between the Turnaround radius and virial mass in $f(R)$ model
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Measuring nonlinear galaxy bias at z~0.8
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• CMB lensing reconstruction biases from masking extragalactic sources
• Is it possible to tell the difference between fermionic and bosonic hot dark matter?
• The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
• Optimal filters for the moving lens effect
• Evolution of hierarchical clustering in the CFHTLS-Wide since z~1
• Higher-order Convergence Statistics for Three-dimensional Weak Gravitational Lensing
• Pairwise velocities in the Halo Model: Luminosity and Scale Dependence
• Characterizing fast radio bursts through statistical cross-correlations
• The Clustering of X-ray Luminous Quasars
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• Extending the halo mass resolution of $N$-body simulations
• Violent and mild relaxation of an isolated self-gravitating uniform and spherical cloud of particles
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• Smallest Remnants of Early Matter Domination
• The Integrated Bispectrum and Beyond
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• Can decaying particle explain cosmic infrared background excess?
• Halo based reconstruction of the cosmic mass density field
• Kinetic Sunyaev-Zel'dovich tomography with line-intensity mapping
• The sizes of disc galaxies in intermediate-redshift clusters
• Impact of astrophysics on cosmology forecasts for 21 cm surveys
• Primordial trispectrum from kSZ tomography
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• Weak Gravitational Lensing as a Method to Constrain Unstable Dark Matter
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• Dark matter halo occupation: environment and clustering
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• Clustering of star-forming galaxies detected in mid-infrared with the Spitzer wide-area survey
• Amending the halo model to satisfy cosmological conservation laws
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• The Schrödinger-Poisson method for Large-Scale Structure
• Modelling the matter bispectrum at small scales in modified gravity
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• A determination of dark matter bispectrum with a large set of N-body simulations
• Weak gravitational lensing of intrinsically aligned galaxies
• The galaxy correlation function as a constraint on galaxy formation physics
• Passive Evolution of Galaxy Clustering
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
• Subhaloes gone Notts: the clustering properties of subhaloes
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• The clustering of baryonic matter. I: a halo-model approach
• A scale dependent bias on linear scales: the case for HI intensity mapping at z=1
• Absorber Model: the Halo-like model for the Lyman-alpha forest
• Reconstructing large scales at cosmic dawn
• Patchy blazar heating: diversifying the thermal history of the intergalactic medium
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Modelling Baryonic Effects on Galaxy Cluster Mass Profiles
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Imprints of gravitational lensing in the Planck CMB data at the location of WISExSCOS galaxies
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Non-Gaussianity in WMAP Data Due to the Correlation of CMB Lensing Potential with Secondary Anisotropies
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Divergence of Perturbation Theory in Large Scale Structures
• Calibrating photometric redshift distributions with cross-correlations
• Modelling the asymmetry of the halo cross-correlation function with relativistic effects at quasi-linear scales
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• Cosmic Microwave Background--Weak Lensing Correlation: Analytical and Numerical Study of Non-linearity and Implications for Dark Energy
• Measuring gravitational lensing of the cosmic microwave background using cross correlation with large scale structure
• Late time sky as a probe of steps and oscillations in primordial Universe
• Perturbation theory with dispersion and higher cumulants: framework and linear theory
• Optimal Transport Reconstruction of Baryon Acoustic Oscillations
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Cosmology from weak lensing alone and implications for the Hubble tension
• Probing Intra-Halo Light with Galaxy Stacking in CIBER Images
• Improving models of the cosmic infrared background using CMB lensing mass maps
• Probing the large scale structure using gravitational-wave observations of binary black holes
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Halo models of HI selected galaxies
• Tracing the cosmological evolution of stars and cold gas with CMB spectral surveys
• The scale-dependent signature of primordial non-Gaussianity in the large-scale structure of cosmic reionization
• Perturbation theory for nonlinear halo power spectrum: the renormalized bias and halo bias
• Higher-order Statistics of Weak Lensing Shear and Flexion
• Nonlinearities in modified gravity cosmology I: signatures of modified gravity in the nonlinear matter power spectrum
• Double Distribution of Dark Matter Halos with respect to Mass and Local Overdensity
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Magnification bias as a novel probe for primordial magnetic fields
• Astrophysical interpretation of the anisotropies in the unresolved gamma-ray background
• The cosmic web connection to the dark matter halo distribution through gravity
• Cosmological constraints with the sub-millimetre galaxies Magnification Bias after large scale bias corrections
• Halo Occupation Distribution of Massive Galaxies since z = 1
• Modeling of weak lensing statistics. I. Power spectrum and bispectrum
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• The Imperial IRAS-FSC Redshift Catalogue: luminosity functions, evolution and galaxy bias
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• Clustering Properties of restframe UV selected galaxies I: the correlation length derived from GALEX data in the local Universe
• Dark Matter Halos from the Inside Out
• Non-linear gravitational clustering of cold matter in an expanding universe: indications from 1D toy models
• Cosmological Angular Trispectra and Non-Gaussian Covariance
• The dark matter dispersion tensor in perturbation theory
• The HI-halo mass relation at redshift $z\sim 1$ from the Minkowski functionals of 21 cm intensity maps
• Beyond Kaiser bias: mildly non-linear two-point statistics of densities in distant spheres
• Some observational tests of a minimal galaxy formation model
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• Testing dark matter halo properties using self-similarity
• 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
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Dichotomy in host environments and signs of recycled AGN
• Parametrizations for tests of gravity
• Analytical halo model of galactic conformity
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Implications for Dark Matter Direct Detection in the Presence of LIGO-Motivated Primordial Black Holes
• Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• How do galaxies populate halos in extreme density environments? An analysis of the Halo Occupation Distribution in SDSS
• Clustering of Local Extrema in Planck CMB maps
• On the estimation of gravity-induced non-Gaussianities from weak lensing surveys
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at $z\sim 0.7$
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• A Better Way to Define Dark Matter Haloes
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Accuracy of analytical models of the large-scale matter distribution
• Impact of Point Source Clustering on Cosmological Parameters with CMB Anisotropies
• Scale Transformations, Tree-level Perturbation Theory, and the Cosmological Matter Bispectrum
• Polarization Signals of the 21 cm Background from the Era of Reionization
• Lyman-$\alpha$ Polarization Intensity Mapping
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• The fractal distribution of haloes
• The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function
• Non-Gaussianity of the Cosmic Infrared Background anisotropies II : Predictions of the bispectrum and constraints forecast
• Towards an understanding of third-order galaxy-galaxy lensing
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Towards optimal estimation of the galaxy power spectrum
• Patchy Screening of the CMB from Dark Photons
• Volume Statistics as a Probe of Large-Scale Structure
• Cosmological Probes of Structure Growth and Tests of Gravity
• Eulerian and Lagrangian propagators for the adhesion model (Burgers dynamics)
• On the accuracy of common moment-based radiative transfer methods for simulating reionization
• Matter power spectra in dynamical-Dark Energy cosmologies
• Large-scale bias of dark matter halos
• Testing the consistency of three-point halo clustering in Fourier and configuration space
• Hierarchical Phase Space Structure of Dark Matter Haloes: Tidal debris, Caustics, and Dark Matter annihilation
• Reconstruction of Cluster Masses using Particle Based Lensing I: Application to Weak Lensing
• Protohalo Constraints to the Resonant Annihilation of Dark Matter
• Modelling the shapes of the largest gravitationally bound objects
• Self-calibrating the gravitational shear-intrinsic ellipticity-intrinsic ellipticity (GII) cross-correlation
• On the Redshift Evolution of MgII Absorption Systems
• Constraining primordial black holes as a fraction of dark matter through accretion disk luminosity
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• The Breakdown Scale of HI Bias Linearity
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Measurement of Void Bias Using Separate Universe Simulations
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• 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
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• A Halo Model with Environment Dependence: Theoretical Considerations
• Variations of cosmic large-scale structure covariance matrices across parameter space
• Matter bispectrum of large-scale structure with Gaussian and non-Gaussian initial conditions: Halo models, perturbation theory, and a three-shape model
• Linear and non-linear perturbations in dark energy models
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• N-body simulations of gravitational redshifts and other relativistic distortions of galaxy clustering
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• Do galaxy mergers prefer under-dense environments?
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• Quijote-PNG: The Information Content of the Halo Mass Function
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• The Integrated Bispectrum in Modified Gravity Theories
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
• Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
• 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
• A physical and concise halo model based on the depletion radius
• How accurate is our knowledge of galaxy bias?
• Probing scalar tensor theories for gravity in redshift space
• A group-galaxy cross-correlation function analysis in zCOSMOS
• Halo asphericity and the shear 3-pt function
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Reionization and feedback in overdense regions at high redshift
• Downsizing of Star Formation Measured from the Clustered Infrared Background Correlated with Quasars
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Can AGN and galaxy clusters explain the surface brightness fluctuations of the cosmic X-ray background?
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• The Global Environment of Small Galaxy Systems
• Excursion set peaks in energy as a model for haloes
• Impact of early dark energy on the Planck SZ cluster sample
• Synergies across the spectrum for particle dark matter indirect detection: how HI intensity mapping meets gamma rays
• The Rise of Dwarfs and the Fall of Giants: Galaxy Formation Feedback Signatures in the Halo Satellite Luminosity Function
• Cross-correlation between the cosmic microwave and infrared backgrounds for integrated Sachs-Wolfe detection
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Cosmic Microwave Background Bispectrum from the Lensing--Rees-Sciama Correlation Reexamined: Effects of Non-linear Matter Clustering
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• Signatures of the Baryon Acoustic Oscillations on 21cm Emission Background
• Non-Gaussianity of the Cosmic Baryon Fluid: Log-Poisson Hierarchy Model
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• New metrics to probe the dynamical state of galaxy clusters
• Conditional Cumulants in Weakly Non-linear Regime
• The star formation history in the last 10 billion years from CIB cross-correlations
• Constraints on halo formation from cross-correlations with correlated variables
• Analytical halo models of cosmic tidal fields
• Searching for patchy reionization from cosmic microwave background with hybrid quadratic estimators
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• A galaxy-free phenomenological model for the 21-cm power spectrum during reionization
• Dynamics of finite and infinite self-gravitating systems with cold quasi-uniform initial conditions
• A theoretical estimate of intrinsic ellipticity bispectra induced by angular momenta alignments
• Inference of gravitational lensing and patchy reionization with future CMB data
• Group galaxy number density profiles far out: is the 'one-halo' term NFW out to $>10$ virial radii?
• SHALOS: Statistical Herschel-ATLAS Lensed Objects Selection
• Prospects for Determining the Mass Distributions of Galaxy Clusters on Large Scales Using Weak Gravitational Lensing
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• The Morphology of the Thermal Sunyaev-Zel'dovich Sky
• The Multi-Tracer Optimal Estimator applied to VIPERS
• Cosmology with the thermal-kinetic Sunyaev-Zel'dovich effect
• Boosting small-scale structure via primordial black holes and implications for sub-GeV dark matter annihilation
• The Clustering of Undetected High-redshift Black Holes and Their Signatures in Cosmic Backgrounds
• Dynamics of minimally coupled dark energy in spherical halos of dark matter
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment
• Probing Oscillons of Ultra-Light Axion-like Particle by 21cm Forest
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
• Galaxy growth by merging in the nearby universe
• Cosmology with the Planck cluster sample
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• A galaxy-halo model of large-scale structure
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• A Cross-correlation Study between IceCube Neutrino Events and the Fermi Unresolved Gamma-ray Sky
• The bias of weighted dark matter halos from peak theory
• Euclid: Covariance of weak lensing pseudo-$C_{\ell }$ estimates. Calculation, comparison to simulations, and dependence on survey geometry
• The HI Bias during the Epoch of Reionization
• The XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties
• Consistency Relations in Effective Field Theory
• Detecting ultra-high energy cosmic ray anisotropies through cross-correlations
• Flat spectrum radio quasars and BL Lacs dominate the anisotropy of the unresolved gamma-ray background
• Weak lensing of gravitational waves in wave optics: Beyond the Born approximation
• Impact of radio sources and cosmic infrared background on thermal Sunyaev-Zel'dovich - gravitational lensing cross correlation
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Semi-numeric simulations of helium reionization and the fluctuating radiation background
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Mixed three-point correlation functions of the nonlinear integrated Sachs-Wolfe effect and their detectability
• Statistical Properties of Thermal Sunyaev-Zel'dovich Maps
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Likelihood-free Forward Modeling for Cluster Weak Lensing and Cosmology
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Testing the accuracy of likelihoods for cluster abundance cosmology
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Higher multipoles of the galaxy bispectrum in redshift space
• Neglecting Primordial non-Gaussianity Threatens Future Cosmological Experiment Accuracy
• 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
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey
• Universal scaling laws and density slope for dark matter haloes
• Dark-ages reionization and galaxy formation simulation XI: Clustering and halo masses of high redshift galaxies
• Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
• Projection effects of large-scale structures on weak-lensing peak abundances
• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
• Estimating the Integrated Bispectrum from Weak Lensing Maps
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Gravitational Collapse of Baryonic and Dark matter
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Intensity Mapping without Cosmic Variance
• A framework to measure the properties of intergalactic metal systems with two-point flux statistics
• Asymptotic expansions for the Large Scale Structure
• Single parameter galaxy classification: The Principal Curve through the multi-dimensional space of galaxy properties
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Weak Lensing Skew-Spectrum
• On the primordial information available to galaxy redshift surveys
• Distribution of Dust around Galaxies: An Analytic Model
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Galaxy power spectrum and biasing results from the LOFAR Two-metre Sky Survey (first data release)
• Impact of tidal environment on galaxy clustering in GAMA
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Cross-correlating Sunyaev-Zel'dovich and Weak Lensing Maps
• Rapid Simulations of Halo and Subhalo Clustering
• CMB and 21cm bounds on early structure formation boosted by primordial black hole entropy fluctuations
• The thermal SZ tomography
• The EDGES measurement disfavors an excess radio background during the cosmic dawn
• Gravitational lensing of the cosmic microwave background by nonlinear structures
• Cosmological feedback from a halo assembly perspective
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Neutrino winds on the sky
• The cosmic shear three-point functions
• The pairwise velocity probability density function in models with local primordial non-Gaussianity
• Is the misalignment of the Local Group velocity and the 2MASS Redshift Survey dipole typical in a LambdaCDM model?
• Probing modified gravity in cosmic filaments
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Remapping simulated halo catalogues in redshift space
• Relaxation of dark matter halos: how to match observational data?
• Galaxy Halo Masses from Weak Gravitational Lensing
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Halo Model Analysis of Cluster Statistics
• Dynamical friction in the primordial neutrino sea
• Quasi-Local Evolution of the Cosmic Gravitational Clustering in Halo Model
• Matrix Formalism of Excursion Set Theory: A new approach to statistics of dark matter halo counting
• An Introduction into the Theory of Cosmological Structure Formation
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• Confronting recent AMS-02 positron fraction and Fermi-LAT Extragalactic Gamma-Ray Background measurements with gravitino dark matter
• A cross-correlation analysis of CMB lensing and radio galaxy maps
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Parameter estimation biases due to contributions from the Rees-Sciama effect to the integrated Sachs-Wolfe spectrum
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Cell Count Moments in the Halo Model
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• 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
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• CHAM: a fast algorithm of modelling non-linear matter power spectrum in the sCreened HAlo Model
• Anisotropic Halo Model
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Remote Dipole Field Reconstruction with Dusty Galaxies
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Inverse-Compton Scattering of the Cosmic Infrared Background
• Simple lessons from complex learning: what a neural network model learns about cosmic structure formation
• Dark matter halo mass functions and density profiles from mass and energy cascade
• The matter distribution in z ~ 0.5 redshift clusters of galaxies. II : The link between dark and visible matter
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Clustering and descendants of MUSYC galaxies at z<1.5
• A roadmap to cosmological parameter analysis with third-order shear statistics II: Analytic covariance estimate
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Autocorrelations of stellar light and mass in the low-redshift Universe
• An Empirical Model For Intrinsic Alignments: Insights From Cosmological Simulations
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
• Cosmology with Weak Lensing Surveys
• Cosmological Constraints on the Very Low Frequency Gravitational-Wave Background
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• On fast Generation of Cosmological Random Fields
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• CMB Anisotropies from Outflows in Lyman Break Galaxies
• Scaling Laws in the Cosmic Structure and Renormalization Group
• Spatial Correlations in the Helium-Ionizing Background
• Topological Defects in Gravitational Lensing Shear Fields
• Cross-correlation between the soft X-ray background and SZ Sky
• Modified initial power spectrum and too big to fail problem
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• Angular Correlation Function Estimators Accounting for Contamination from Probabilistic Distance Measurements
• Cosmological Filaments in the light of Excursion Set of Saddle Points
• Choose to smooth: Gaussian streaming with the truncated Zel'dovich approximation
• Cross-Correlation Studies with CMB Polarization Maps
• Constraining galaxy-halo connection with high-order statistics
• Galaxy populations in haloes in high-density environments
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• Deep learning-driven likelihood-free parameter inference for 21-cm forest observations
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Interlopers speak out: studying the dark universe using small-scale lensing anisotropies
• Cosmological test of local position invariance from the asymmetric galaxy clustering
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Weak Lensing Trispectrum and Kurt-Spectra
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Near-infrared Extragalactic Background Light Fluctuations on Nonlinear Scales
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• Tetrahedral collapse: a rotational toy model of simultaneous dark-matter halo, filament and wall formation
• Probing axion dark matter with 21cm fluctuations from minihalos
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• Modeling the Intergalactic Medium during the Epoch of Reionization
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster
• KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects
• Halo mass function in scale invariant models
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• Baryonic Post-Processing of N-body Simulations, with Application to Fast Radio Bursts
• Probe combination in large galaxy surveys : Application of Fisher information and Shannon entropy to weak lensing
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• Quantification of the multi-streaming effect in Redshift Space Distortion
• Intrinsic size correlations in weak lensing
• Intrinsic alignments of galaxies around cosmic voids
• Gravitational Redshifts in Clusters and Voids
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• The importance of the cosmic web and halo substructure for power spectra
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• The Structure of 2MASS Galaxy Clusters
• Multi-wavelength consensus of large-scale linear bias
• Cosmology in the non-linear regime : the small scale miracle
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• The rotational kinetic Sunyaev-Zeldovich contribution to the temperature asymmetry toward the M31 halo
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• What is the super-sample covariance? A fresh perspective for second-order shear statistics
• Analytic approach to astrometric perturbations of critical curves by substructures
• Nonlinear structure formation in Bound Dark Energy
• Linear theory and velocity correlations of clusters
• The effect of finite halo size on the clustering of neutral hydrogen
• A rising tide: Intrinsic alignments since the turn of the millennium
• An Ising model for galaxy bias
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• The Sunyaev-Zel'dovich effect and Faraday rotation contributions of galaxy groups to the CMB angular power spectrum
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• Power Spectrum and Intermittency of Ly$\alpha$ Transmitted Flux of QSO He2347-4342
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Probing the Neutrino Mass through the Cross Correlation between the Rees-Sciama Effect and Weak Lensing
• Smooth halos in the cosmic web
• Halo Profile Evolution and Velocity Bias
• Methodological refinement of the submillimeter galaxy magnification bias. II. Cosmological analysis with tomography
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• The PAU Survey: Close galaxy pairs identification and analysis
• The Degeneracy of Galaxy Formation Models
• Detecting Electron Density Fluctuations from Cosmic Microwave Background Polarization using a Bispectrum Approach
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Multi-Component Decomposition of Cosmic Infrared Background Fluctuations
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
• Bayesian large-scale structure inference and cosmic web analysis
• Exact Results for Propagators in the Geometrical Adhesion Model
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• Einasto profile as the halo model solution coupled to the depletion radius
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• What is the optimal way to measure the galaxy power spectrum?
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• High-Significance Detection of Correlation Between the Unresolved Gamma-Ray Background and the Large Scale Cosmic Structure
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Galaxy-galaxy lensing in the VOICE deep survey
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• The information content of Cosmic Infrared Background anisotropies
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• 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
• The case for two-dimensional galaxy-galaxy lensing
• A High-Significance Measurement of Correlation Between Unresolved IRAS Sources and Optically-Selected Galaxy Clusters
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Fractals vs. halos: Asymptotic scaling without fractal properties
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Spatial Locality of Galaxy Correlation Function in Phase Space: Samples from the 2MASS Extended Source Catalog
• A comparison of the excess mass around CFHTLenS galaxy-pairs to predictions from a semi-analytic model using galaxy-galaxy-galaxy lensing
• The Spatial Range of Conformity
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• An Empirical Mass Function Distribution
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Lagrangian perturbations theory : Third-order solution for general dark energy models
• Angular fluctuations in the CXB: Is Fe 6.4 keV line tomography of the large-scale structure feasible?
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• Scaling of the 1-halo terms with bias
• Stacked phase-space density of galaxies around massive clusters: Comparison of dynamical and lensing masses
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Modelling the impact of intrinsic size and luminosity correlations on magnification estimation
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• Doppler boosted dust emission and CIB-galaxy cross-correlations: a new probe of cosmology and astrophysics
• Bayesian analysis of cosmic structures
• The impact of AGN X-ray selection on the AGN halo occupation distribution
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Scale Symmetry in the Universe
• Constraints on Primordial Magnetic Fields from High Redshift Stellar Mass Density
• Bound Dark Matter (BDM) towards solving the Small Scale Structure Problem
• In Search of Extraterrestrial Artificial Intelligence Through Dyson Sphere-like structures around Primordial Black Holes
• Secondary B-mode polarization from Faraday rotation in clusters and galaxies
• On the accuracy of the high redshift cluster luminosity function
• Uncertainty in the visibility mask of a survey and its effects on the clustering of biased tracers
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Fingerprint matching of beyond-WIMP dark matter: neural network approach
• Cosmological simulations of structure formation and the Vlasov equation
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping
• Explicit computation of shear three-point correlation functions: the one-halo model case
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Cosmology with Galaxy Correlations
• Dark matter halo concentrations: a short review
• A Physical Bias in Cosmological Simulations
• Neural style transfer of weak lensing mass maps
• Interference in Fuzzy Dark Matter Filaments: Idealised Models and Statistics
• Clustering of K-band selected local galaxies
• Halo Models of Large Scale Structure and Reliability of Cosmological N-Body Simulations
• Lethal radiation from nearby supernovae helps to explain the small cosmological constant
• Influence of baryons on spatial distribution of matter: higher order correlation functions
• The conformity of HI galaxies in ALFALFA-SDSS sample
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Cosmological constraints from galaxy clustering
• The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
• Emergence of smooth distance and apparent magnitude in a lumpy Universe
• Principal Components for Model-Agnostic Modified Gravity with 3x2pt
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Statistical Properties of Supercluster-Like Filaments from Cosmological Simulations
• Weak lensing peak statistics -- steepness versus height
• The impact of halo concentration on the Sunyaev Zel'dovich effect signal from massive galaxy clusters
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Symmetries, Invariants and Generating Functions: Higher-order Statistics of Biased Tracers
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• A Parameter-free Statistical Measurement of Halos with Power Spectra
• Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Clustering and Runaway Merging in a Primordial Black Hole Dominated Universe
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• Maximum likelihood kinetic Sunyaev Zel'dovich velocity reconstruction
• Properties of subhalos in the interacting dark matter scenario
• Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency
• The mass and galaxy distribution around SZ-selected clusters
• Estimating power spectrum of discrete cosmic momentum field with fast Fourier transform
• Statistical Decoupling of Lagrangian Fluid Parcel in Newtonian Cosmology
• Impact of Large-Scale Structure Systematics on Cosmological Parameter Estimation
• One-point Statistics in various cosmic environments in the presence of massive neutrinos
• Angular Diameter Distance Measurement with Galaxy Clustering in the Multipole Space
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
• Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
• Breaking degeneracies with the Sunyaev-Zeldovich full bispectrum
• Mapping luminous and dark matter in the Universe
• Halo Pressure Profile through the Skew Cross-Power Spectrum of Sunyaev-Zel'dovich Effect and CMB Lensing in $\text{Planck}$
• Bayesian Analysis of Wave-Optics Gravitationally Lensed Massive Black Hole Binaries with Space-Based Gravitational Wave Detector
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Introduction to Higher Order Spatial Statistics in Cosmology
• Models for the Clustering of Far-Infrared and Sub-millimetre selected Galaxies
• On the Outskirts of Dark Matter Haloes
• The evolution of the halo occupation distribution in cosmic voids
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• An Order Statistics Approach to the Halo Model for Galaxies
• Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
• Non-screening of the Cosmological Background in K-mouflage modified gravity
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Cosmic Insights from Galaxy Clusters: Exploring Magnification Bias on Sub-millimeter Galaxies
• Cosmic Infrared Background ExpeRiment (CIBER): A Probe of Extragalactic Background Light from Reionization
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• Projection of the gravitational dynamics on a subspace of probability distributions: curl-free Gaussian ansatz
• An Optimally Weighted Estimator of the Linear Power Spectrum Disentangling the Growth of Density Perturbations Across Galaxy Surveys
• Signatures of inhomogeneous dark matter annihilation on 21-cm
• Cosmological Implications of a Neutrino Mass Detection
• Multimessenger Astronomy Beyond the Standard Model: New Window from Quantum Sensors
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Dark Matter and Galaxy Cross-Correlations with the Cherenkov Telescope Array Observatory
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• The invariance of group occupation across the cosmic web
• Challenges in Non-Linear Gravitational Clustering
• Cosmic magnification on high-redshift submillimeter galaxies
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• Constraining Galaxy-Halo Connection Using Machine Learning
• A hierarchical clustering method for quantifying satellite abundance
• Imprints of fermionic and bosonic mixed dark matter on the 21-cm signal at cosmic dawn
• Morpho-statistical characterisation of the spatial galaxy distribution through Gibbs point processes
• A Beginner's Guide to Line Intensity Mapping Power Spectra
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Revealing the formation histories of the first stars with the cosmic near-infrared background
• Predicting halo occupation and galaxy assembly bias with machine learning
• Clustering of dark matter in the cosmic web as a probe of massive neutrinos
• The VIMOS VLT Deep Survey. The different assembly history of passive and star-forming L_B >= L*_B galaxies in the group environment at z < 1
• Extragalactic Background Light: Measurements and Applications
• Covariances of Galaxy Stellar Mass Functions and Correlation Functions
• The pairwise and cross-pairwise y-type polarised kinetic Sunyaev Zeldovich effect from transverse velocity of galaxy clusters
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Generalized local ansatz for scale-dependent primordial non-Gaussianities and future galaxy surveys
• Statistical Imprints of SZ Effects in the Cosmic Microwave Background
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Impact of a Rapid Diluted Energy Density on the halo mass function
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method
• HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• DarkMix: Mixture Models for the Detection and Characterization of Dark Matter Halos
• Addressing Dipole Tension via Clustering in $\Lambda$CDM and beyond
• Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
• On Weak Lensing Response Functions
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• Using a Neural Network Classifier to Select Galaxies with the Most Accurate Photometric Redshifts
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• Fenomenología de modelos supersimétricos: partículas y materia oscura
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• Halo structure and lensing signatures of a polytropic dark matter fluid
• Exploring the Voids: Luminosity Functions and Magnetic Field
• Axion-Like Particle Dark Matter Intensity Mapping: A New Probe via Cross-Correlation with Galaxy Surveys
• On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• Evidence for merging or disruption of red galaxies from the evolution of their clustering
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• A redshift distortion free correlation function at third order in the nonlinear regime
• Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
• Non-Gaussian likelihood of weak lensing power spectra
• Void probability function in the Quijote simulations
• Probing the warm dark matter mass with [C II] intensity mapping
• Testing the growth of cosmic structures during the Dark Ages
• Skew-spectra: a generalization to spin-$s$
• Challenges of standard halo models in constraining galaxy properties from CIB anisotropies
• Secondary CMB anisotropies from magnetized halos --I: Power spectra of the Faraday rotation angle and conversion rate
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Dark Energy Survey Year 3 Results: Three-Point Shear Correlations and Mass Aperture Moments
• Cross-correlations between X-ray clusters and the general galaxy population
• Cosmological free-free emission from dark matter halos in the $\Lambda$CDM model
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• Hybrid $P_{\ell }(k)$: general, unified, non-linear matter power spectrum in redshift space
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Universality of the halo mass function in modified gravity cosmologies
• Stable Clustering Ansatz, Consistency Relations and Gravity Dual of Large-Scale Structure