Analytic model for galaxy and dark matter clustering

Abstract

We investigate an analytic model to compute nonlinear power spectrum of dark matter, galaxies and their cross-correlation. The model is based on Press-Schechter halos, which cluster and have realistic dark matter profiles. The total power spectrum is a sum of two contributions, one from correlations betwen the halos and one from correlations within the same halo. We show that such a model can give dark matter power spectra which match well with the results of N-body simulations, provided that concentration parameter decreases with the halo mass. Galaxy power spectrum differs from dark matter power spectrum because pair weighted number of galaxies increases less rapidly than the halo mass, as predicted by theoretical models and observed in clusters. In this case the resulting power spectrum becomes a power law with the slope closed to the observed. Such a model also predicts a later onset of nonlinear clustering compared to the dark matter, which is needed to reconcile the CDM models with the data. Generic prediction of this model is that bias is scale dependent and nonmonotonic. For red or elliptical galaxies bias in power spectrum may be scale dependent even on very large scales. Our predictions for galaxy-dark matter correlations, which can be observed through the galaxy-galaxy lensing, show that these cannot be interpreted simply as an average halo profile of a typical galaxy, because different halo masses dominate at different scales and because larger halos host more than one galaxy. We discuss the prospects of using cross-correlations in combination with galaxy clustering to determine the dark matter power spectrum (ABRIDGED).

16 pages, 7 figures, submitted to Phys. Rev. D

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• Constraints on Hyperluminous QSO Lifetimes via Fluorescent Lya Emitters at Z~2.7
• The Scale-Dependence of Halo Assembly Bias
• An Analytical Approach to Inhomogeneous Structure Formation
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• Combining Probes of Large-Scale Structure with CosmoLike
• Dark Energy Constraints from Baryon Acoustic Oscillations
• Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• Isolating Geometry in Weak Lensing Measurements
• Kinetic Sunyaev-Zel'dovich effect from halo rotation
• Precision cluster mass determination from weak lensing
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Accurate Modeling of Weak Lensing with the sGL Method
• Reconstructing the distribution of haloes and mock galaxies below the resolution limit in cosmological simulations
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• An analytical model for the non-linear redshift-space power spectrum
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• The Angular Power Spectrum of EDSGC Galaxies
• Weak Lensing Mass Measurements of Substructures in COMA Cluster with Subaru/Suprime-Cam
• 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
• TheHaloMod: An online calculator for the halo model
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Line-of-sight effects in strong lensing: Putting theory into practice
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• Systematic effects in the sound horizon scale measurements
• Galaxy Clustering Topology in the Sloan Digital Sky Survey Main Galaxy Sample: a Test for Galaxy Formation Models
• 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
• A Brighter Past: Galaxy Luminosity Function At High Redshifts
• Interpreting the Clustering of Distant Red Galaxies
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• A KiDS weak lensing analysis of assembly bias in GAMA galaxy groups
• Measuring our universe from galaxy redshift surveys
• Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models
• Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe
• 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
• Modeling The Large Scale Bias of Neutral Hydrogen
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• Complete Treatment of Galaxy Two-Point Statistics: Gravitational Lensing Effects and Redshift-Space Distortions
• Substructure and the halo model of large-scale structure
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• 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)
• Quasar-Galaxy and Galaxy-Galaxy Cross-Correlations: Model Predictions with Realistic Galaxies
• Non-Gaussianity and large-scale structure in a two-field inflationary model
• Halo Structures of Gravitational Lens Galaxies
• High Redshift Galaxy Populations and their Descendants
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• Environmental Effects on Real-Space and Redshift-Space Galaxy Clustering
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Halo Zeldovich model and perturbation theory: dark matter power spectrum and correlation function
• Mapping the allowed parameter space for decaying dark matter models
• Breaking Halo Occupation Degeneracies with Marked Statistics
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• The Small-scale Clustering of Luminous Red Galaxies via Cross-Correlation Techniques
• Testing a new analytic model for gravitational lensing probabilities
• Including beyond-linear halo bias in halo models
• A simple model linking galaxy and dark matter evolution
• Joint analysis of the thermal Sunyaev-Zeldovich effect and 2MASS galaxies: Probing gas physics in the local Universe and beyond
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• The DEEP2 Galaxy Redshift Survey: The Voronoi-Delaunay Method catalog of galaxy groups
• Measuring the neutrino mass from future wide galaxy cluster catalogues
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Noise in strong lensing cosmography
• Constraining warm dark matter with cosmic shear power spectra
• Integrated Sachs Wolfe Effect and Rees Sciama Effect
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• The Halo Occupation Distribution of Active Galactic Nuclei
• Local stochastic non-Gaussianity and N-body simulations
• 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
• Relations Between Environments of Quasars and Galaxy Formation
• Squared temperature-temperature power spectrum as a probe of the CMB bispectrum
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters
• The effect of primordial black holes on 21 cm fluctuations
• The role of thermal evaporation in galaxy formation
• Observing dynamical friction in galaxy clusters
• Angular power spectrum of gamma-ray sources for GLAST: blazars and clusters of galaxies
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Don't cross the streams: caustics from Fuzzy Dark Matter
• Precision modelling of the matter power spectrum in a Planck-like Universe
• Angular power spectrum of galaxies in the 2MASS Redshift Survey
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Joint likelihood function of cluster counts and $n$-point correlation functions: Improving their power through including halo sample variance
• Higher-order moments of the lensing shear and other spin two fields
• Correlation between galaxies and QSO in the SDSS:na signal from gravitational lensing magnification?
• Shot noise and biased tracers: a new look at the halo model
• The splashback radius of optically selected clusters with Subaru HSC Second Public Data Release
• Modeling color-dependent galaxy clustering in cosmological simulations
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• 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
• Galaxy cluster mass estimation with deep learning and hydrodynamical simulations
• Subhalo statistics of galactic halos: beyond the resolution limit
• Accurate Weak Lensing of Standard Candles. II. Measuring sigma8 with Supernovae
• Scale-dependent Galaxy Bias
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• Large Scale Structure of the Universe
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Tomographic Magnification of Lyman Break Galaxies in The Deep Lens Survey
• Evolution of the Dark Matter Distribution with 3-D Weak Lensing
• On the implementation of the spherical collapse model for dark energy models
• Bispectrum Supersample Covariance
• Optimal Weighting in Galaxy Surveys: Application to Redshift-Space Distortions
• The Non-Linear Matter Power Spectrum in Warm Dark Matter Cosmologies
• Power spectrum tomography of dark matter annihilation with local galaxy distribution
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• The Power Spectra of Polarized, Dusty Filaments
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Luminous Red Galaxies in hierarchical cosmologies
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• The dependence of the pairwise velocity dispersion on galaxy properties
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• Cosmic Voids and Galaxy Bias in the Halo Occupation Framework
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Reliability of the dark matter clustering in cosmological N-body simulation on scales below the mean separation length of particles
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Using the Zeldovich dynamics to test expansion schemes
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• How much a galaxy knows about its large-scale environment?: An information theoretic perspective
• Modeling Galaxy Clustering by Color
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Dark Matter Signatures in the Anisotropic Radio Sky
• Combining cluster number counts and galaxy clustering
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• The impact of halo shapes on the bispectrum in cosmology
• Weak Lensing Observables in the Halo Model
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Completeness in Photometric and Spectroscopic Searches for Clusters
• Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations
• On the Physical Requirements for a Pre-Reionization Origin of the Unresolved Near-Infrared Background
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• The relation between stellar mass and weak lensing signal around galaxies: Implications for MOND
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• Using Weak Lensing to find Halo Masses
• A Multiband Study of the Galaxy Populations of the First Four Sunyaev--Zeldovich Effect selected Galaxy Clusters
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Circular Polarization of the CMB: A probe of the First stars
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• The effect of (strong) discrete absorption systems on the lyman alpha forest flux power spectrum
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Rapid simulation rescaling from standard to modified gravity models
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Cosmological searches for a non-cold dark matter component
• Galaxy clustering and projected density profiles as traced by satellites in photometric surveys: Methodology and luminosity dependence
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• Testing spherical evolution for modelling void abundances
• On estimating cosmology-dependent covariance matrices
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• The Halo Mass-Bias Redshift Evolution in the $\Lambda$CDM Cosmology
• Modelling the cosmic neutral hydrogen from DLAs and 21 cm observations
• Extending the Coyote emulator to dark energy models with standard $w_0$-$w_a$ parametrization of the equation of state
• Intrinsic/Extrinsic Density-Ellipticity Correlations and Galaxy-Galaxy Lensing
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• Weak lensing shear and aperture-mass from linear to non-linear scales
• Linear bias forecasts for emission line cosmological surveys
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Shear-Selected Clusters From the Deep Lens Survey III: Masses from Weak Lensing
• Power spectrum for the small-scale Universe
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• Spatial and Dynamical Biases in Velocity Statistics of Galaxies
• What determines large scale galaxy clustering: halo mass or local density?
• Precision cosmology in muddy waters: Cosmological constraints and N-body codes
• Halo Concentration and the Dark Matter Power Spectrum
• Constraining Primordial Magnetic Fields with Future Cosmic Shear Surveys
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• An observational proxy of halo assembly time and its correlation with galaxy properties
• The evolution of the galaxy content of dark matter haloes
• An Optical Catalog of Galaxy Clusters Obtained from an Adaptive Matched Filter Finder Applied to SDSS DR9 Data
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• A Divided Universe: Red and Blue Galaxies and their Preferred Environments
• Cosmological Structure Formation in Decaying Dark Matter Models
• Multi-Fidelity Emulation for the Matter Power Spectrum using Gaussian Processes
• Halo assembly bias from Separate Universe simulations
• Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
• Where are the z=4 Lyman Break Galaxies? Results from Conditional Luminosity Function Models of Luminosity-dependent Correlation Functions
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Remapping dark matter halo catalogues between cosmological simulations
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above $\sim 1$ arcmin
• Gravitational Flexion by Elliptical Dark Matter Haloes
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Galaxy surveys, inhomogeneous reionization, and dark energy
• Masses of high-z galaxy hosting haloes from angular clustering and their evolution in the CDM model
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
• Equal-time Consistency Relations in the Large-Scale Structure of the Universe
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Impacts of satellite galaxies on the redshift-space distortions
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• Testing the Halo Model Against the SDSS Photometric Survey
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• The Effect of Large-Scale Structure on the Magnification of High-Redshift Sources by Cluster-Lenses
• Halo model prediction of the cosmic magnification statistics: the full non-linear contribution
• Power Spectrum Normalisation and the Non-Gaussian Halo Model
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Understanding the PSCz Galaxy Power Spectrum with N-body Simulations
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Understanding the non-linear clustering of high redshift galaxies
• HInet: Generating neutral hydrogen from dark matter with neural networks
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• The detection of the imprint of filaments on cosmic microwave background lensing
• The impact of baryons on the sensitivity of dark energy measurements
• Determining neutrino properties using future galaxy redshift surveys
• The halo light cone catalogues of \Abacus{AbacusSummit}
• Tidal alignments as a contaminant of the galaxy bispectrum
• Constraining the properties of gaseous halos via cross-correlations of upcoming galaxy surveys and thermal Sunyaev-Zel'dovich maps
• The Atacama Cosmology Telescope: Weighing distant clusters with the most ancient light
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Effects of halo substructure on the power spectrum and bispectrum
• Spatial Clustering of High Redshift Lyman Break Galaxies
• Measuring the Distribution of Galaxies Between Halos
• Taking advantage of photometric galaxy catalogues to determine the halo occupation distribution
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Probing the Cosmic X-ray and MeV Gamma-ray Background Radiation through the Anisotropy
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• Observational Measures of Halo Properties Beyond Mass
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• The FLAMINGO project: Baryon effects on the matter power spectrum
• Impact of Dark Matter Substructure on the Matter and Weak Lensing Power Spectra
• From linear to non-linear scales: analytical and numerical predictions for the weak lensing convergence
• The galaxy-galaxy lensing contribution to the cosmic shear two point function
• How well can (renormalized) perturbation theory predict dark matter clustering properties?
• Is it possible to tell the difference between fermionic and bosonic hot dark matter?
• Cosmic Infrared Background anisotropies as a window into primordial non-Gaussianity
• Cosmological Vlasov-Poisson Simulations of Structure Formation with Relic Neutrinos: Nonlinear Clustering and the Neutrino Mass
• Smallest Remnants of Early Matter Domination
• Impact of astrophysics on cosmology forecasts for 21 cm surveys
• The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
• A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
• Higher-order Convergence Statistics for Three-dimensional Weak Gravitational Lensing
• Weak lensing mass modeling bias and the impact of miscentring
• A Bayesian method for combining theoretical and simulated covariance matrices for large-scale structure surveys
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• The peculiar velocities of satellites of external disk galaxies
• Testing redMaPPer centring probabilities using galaxy clustering and galaxy-galaxy lensing
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Divergence of Perturbation Theory in Large Scale Structures
• A determination of dark matter bispectrum with a large set of N-body simulations
• The clustering of baryonic matter. I: a halo-model approach
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Amending the halo model to satisfy cosmological conservation laws
• The galaxy correlation function as a constraint on galaxy formation physics
• Universal clustering of dark matter in phase space
• Effects of Baryonic Feedback on the Cosmic Web
• Quantifying substructures in {\it Hubble Frontier Field} clusters: comparison with $\Lambda CDM$ simulations
• Passive Evolution of Galaxy Clustering
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• Subhaloes gone Notts: the clustering properties of subhaloes
• Absorber Model: the Halo-like model for the Lyman-alpha forest
• Imprints of gravitational lensing in the Planck CMB data at the location of WISExSCOS galaxies
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Weak Lensing of the CMB: Power Spectrum Covariance
• Higher-order Statistics of Weak Lensing Shear and Flexion
• Effects of biasing on the galaxy power spectrum at large scales
• Double Distribution of Dark Matter Halos with respect to Mass and Local Overdensity
• Cosmology from weak lensing alone and implications for the Hubble tension
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Second Moment of Halo Occupation Number
• Gravity's smoking gun?
• Perturbation theory for nonlinear halo power spectrum: the renormalized bias and halo bias
• Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
• Extending Recovery of the Primordial Matter Power Spectrum
• Magnification bias as a novel probe for primordial magnetic fields
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• On the Clustering of Faint Red Galaxies
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Probing reionization with the cross power spectrum of 21 cm and near-infrared radiation backgrounds
• The Imperial IRAS-FSC Redshift Catalogue: luminosity functions, evolution and galaxy bias
• The cosmic web connection to the dark matter halo distribution through gravity
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• The Halo Occupation Distribution of Obscured Quasars: Revisiting the Unification Model
• Some observational tests of a minimal galaxy formation model
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• Quasi-equilibrium models of high-redshift disc galaxy evolution
• Tracing the Nature of Dark Energy with Galaxy Distribution
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Analytical halo model of galactic conformity
• 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
• Modeling Redshift-Space Clustering with Abundance Matching
• Parametrizations for tests of gravity
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• How do galaxies populate halos in extreme density environments? An analysis of the Halo Occupation Distribution in SDSS
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• The 21-cm signals from ultracompact minihalos as a probe of primordial small-scale fluctuations
• The redshift and scale dependence of the cosmic shear signal from numerical simulations
• Observational constraints of an anisotropic boost due to the projection effects using redMaPPer clusters
• On the Redshift Evolution of MgII Absorption Systems
• Lyman-$\alpha$ Polarization Intensity Mapping
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Matter power spectra in dynamical-Dark Energy cosmologies
• Robustness of the covariance matrix for galaxy clustering measurements
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Matter bispectrum of large-scale structure with Gaussian and non-Gaussian initial conditions: Halo models, perturbation theory, and a three-shape model
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• The Halo Occupation Distribution of HI from 21cm Intensity Mapping at Moderate Redshifts
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• Linear and non-linear perturbations in dark energy models
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• A Halo Model with Environment Dependence: Theoretical Considerations
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Clustering of gamma-ray selected 2LAC Fermi Blazars
• A physical and concise halo model based on the depletion radius
• The Global Environment of Small Galaxy Systems
• The clustering and halo occupation distribution of Lyman-break galaxies at $z\sim 4$
• Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Galaxy Clusters in the Line of Sight to Background Quasars: II. Environmental effects on the sizes of baryonic halo sizes
• Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
• Time evolution of the stochastic linear bias of interacting galaxies on linear scales
• The structure of the merging RCS 231953+00 Supercluster at z ~ 0.9
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• The Clustering of Extremely Red Objects
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• A group-galaxy cross-correlation function analysis in zCOSMOS
• Internal Cluster Structure
• Shear and magnification angular power spectra and higher-order moments from weak gravitational lensing
• Correlation function: biasing and fractal properties of the cosmic web
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• The Morphology of the Thermal Sunyaev-Zel'dovich Sky
• Cluster-Cluster Lensing and the Case of Abell 383
• The star formation history in the last 10 billion years from CIB cross-correlations
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• Toward an Improved Analytical Description of Lagrangian Bias
• Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment
• The bias of weighted dark matter halos from peak theory
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• A galaxy-halo model of large-scale structure
• Detectability of Weak Lensing Modifications under Galileon Theories
• Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
• Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
• Improving three-dimensional mass mapping with weak gravitational lensing using galaxy clustering
• Statistical Properties of Thermal Sunyaev-Zel'dovich Maps
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Neglecting Primordial non-Gaussianity Threatens Future Cosmological Experiment Accuracy
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• KiDS-1000: Weak lensing and intrinsic alignment around luminous red galaxies
• Distribution of Dust around Galaxies: An Analytic Model
• Galaxy power spectrum and biasing results from the LOFAR Two-metre Sky Survey (first data release)
• Structure and evolution of magnetized clusters: entropy profiles, S-T and L_X-T relations
• Cosmological constraints from the masses and abundances of L* galaxies
• The ALHAMBRA survey: evolution of galaxy spectral segregation
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Simulating the formation of cosmic structure
• 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
• The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• The effect of cluster magnetic field on the Sunyaev Zeldovich power spectrum
• Precision cosmology with baryons: non-radiative hydrodynamics of galaxy groups
• Is the misalignment of the Local Group velocity and the 2MASS Redshift Survey dipole typical in a LambdaCDM model?
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Galaxy Halo Masses from Weak Gravitational Lensing
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Rapid Simulations of Halo and Subhalo Clustering
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• A closer look at dark photon explanations of the excess radio background
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Sunyaev-Zel'dovich power spectrum with decaying cold dark matter
• Remapping simulated halo catalogues in redshift space
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Cross-correlating Sunyaev-Zel'dovich and Weak Lensing Maps
• MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
• Cell Count Moments in the Halo Model
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• 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
• Improved Modeling of the Kinematic Sunyaev-Zel'dovich Projected-Fields signal and its Cosmological Dependence
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• Anisotropic Halo Model
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Angular clustering of z~2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Non-Gaussian Tails of Cosmological Density Distribution Function from Dark Halo Approach
• Fast generation of mock galaxy catalogues with COLA
• A new test for the stable clustering hypothesis
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• Cooling flows and the entropy of the intragroup medium
• Galaxy populations in haloes in high-density environments
• Constraining galaxy-halo connection with high-order statistics
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Computing 3 point correlation function randoms counts without the randoms catalogue
• Optical galaxy cluster mock catalogs with realistic projection effects: Validations with the SDSS clusters
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Intrinsic size correlations in weak lensing
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• The importance of the cosmic web and halo substructure for power spectra
• KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects
• The effects of anti-correlation on gravitational clustering
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• Halo mass function in scale invariant models
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• Prospects for disentangling dark matter with weak lensing
• Sunyaev-Zel'dovich anisotropy due to Primordial black holes
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Importance of intracluster scattering and relativistic corrections from tSZ effect with Cosmic Infrared Background
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• The Degeneracy of Galaxy Formation Models
• Halo Profile Evolution and Velocity Bias
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Baryon Pasting the Uchuu Lightcone Simulation
• Galaxy-galaxy lensing in the VOICE deep survey
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• Modeling Pairwise Peculiar Velocity Distribution Function of Dark Matter from Halo Density Profiles
• Weak lensing of the Sunyaev-Zel'dovich sky
• The case for two-dimensional galaxy-galaxy lensing
• A Generalized Method for Measuring Weak Lensing Magnification With Weighted Number Counts
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• A new constant behind the rotational velocity of galaxies
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Joint cluster reconstructions: Combining free-form lensing and X-rays
• Hydrodynamical chemistry simulations of the SZ effect and the impacts from primordial non-Gaussianities
• The SDSS DR7 Galaxy Angular Power Spectrum: Volume-Limits and Galaxy Morphology
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Testing Theoretical Models for the Higher-Order Moments of Dark Halo Distribution
• Evolution of Power Spectrum in Non-Gaussian Models
• Scaling of the 1-halo terms with bias
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks
• Cosmological constraints from galaxy clustering
• The abundance of lensing protoclusters
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Explicit computation of shear three-point correlation functions: the one-halo model case
• Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Dynamics of merging: Post-merger mixing and relaxation of an Illustris galaxy
• The evolution of the halo occupation distribution in cosmic voids
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Mapping luminous and dark matter in the Universe
• An Optimally Weighted Estimator of the Linear Power Spectrum Disentangling the Growth of Density Perturbations Across Galaxy Surveys
• Directional miscentering dependence in weak lensing mass bias
• Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• CMB lensing from early-formed dark matter halos
• Constraining Galaxy-Halo Connection Using Machine Learning
• The Impact of Tomographic Redshift Bin Width Errors on Cosmological Probes
• Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Spectroscopic Confirmation of Two X-ray Diffuse and Massive Galaxy Clusters at Low Redshift
• A hierarchical clustering method for quantifying satellite abundance
• STRAWBERRY: Finding haloes in the gravitational potential
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Cosmic magnification on high-redshift submillimeter galaxies
• Super sample covariance and the volume scaling of galaxy survey covariance matrices
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Validating Planck SZ2 Clusters with Optical Counterparts
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Contribution of Cross-Correlations to the 21cm Angular Power Spectrum in the Epoch of Reionization
• An emulation-based model for the projected correlation function
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Effect of dust in circumgalactic haloes on the cosmic shear power spectrum
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• Revisiting secondary CMB distortions due to kinetic Sunyaev-Zel'dovich effect from quasar bubbles before reionization
• A Non-parametric Method for the Inference of Halo Occupation Distributions