Large-Scale Galaxy Bias

Abstract

This review presents a comprehensive overview of galaxy bias, that is, the statistical relation between the distribution of galaxies and matter. We focus on large scales where cosmic density fields are quasi-linear. On these scales, the clustering of galaxies can be described by a perturbative bias expansion, and the complicated physics of galaxy formation is absorbed by a finite set of coefficients of the expansion, called bias parameters. The review begins with a detailed derivation of this very important result, which forms the basis of the rigorous perturbative description of galaxy clustering, under the assumptions of General Relativity and Gaussian, adiabatic initial conditions. Key components of the bias expansion are all leading local gravitational observables, which include the matter density but also tidal fields and their time derivatives. We hence expand the definition of local bias to encompass all these contributions. This derivation is followed by a presentation of the peak-background split in its general form, which elucidates the physical meaning of the bias parameters, and a detailed description of the connection between bias parameters and galaxy statistics. We then review the excursion-set formalism and peak theory which provide predictions for the values of the bias parameters. In the remainder of the review, we consider the generalizations of galaxy bias required in the presence of various types of cosmological physics that go beyond pressureless matter with adiabatic, Gaussian initial conditions: primordial non-Gaussianity, massive neutrinos, baryon-CDM isocurvature perturbations, dark energy, and modified gravity. Finally, we discuss how the description of galaxy bias in the galaxies' rest frame is related to clustering statistics measured from the observed angular positions and redshifts in actual galaxy catalogs.

259 pages, 39 figures, 15 tables; published in Physics Reports; v2: minor corrections and clarifications, references added; v3: substantially revised and improved version; v4: minor edits and clarifications reflecting published version, corrected mistakes in Eqs. (7.57)-(7.58); v5: minor corrections [Eq. (5.5)] and updated references

References in corpus (657)

• Planck 2015 results. XIII. Cosmological parameters
• A Universal Density Profile from Hierarchical Clustering
• Dynamics of dark energy
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Modified Gravity and Cosmology
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• Non-Gaussian features of primordial fluctuations in single field inflationary models
• Large scale bias and the peak background split
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
• Is Cosmic Speed-Up Due to New Gravitational Physics?
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
• Halo Models of Large Scale Structure
• Dark Energy and the Accelerating Universe
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• Toward a halo mass function for precision cosmology: the limits of universality
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• The 3D power spectrum of galaxies from the SDSS
• Mass function of dark matter halos
• An analytic model for the spatial clustering of dark matter haloes
• Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
• Disappearing cosmological constant in f(R) gravity
• 4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results
• Beyond the Cosmological Standard Model
• Non-Gaussianity from Inflation: Theory and Observations
• Analytic model for galaxy and dark matter clustering
• Using the Evolution of Clusters to Constrain Omega
• The Effective Field Theory of Inflation
• Acoustic Signatures in the Primary Microwave Background Bispectrum
• Massive neutrinos and cosmology
• The Dark Energy Survey: more than dark energy - an overview
• Halo occupation numbers and galaxy bias
• The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
• Observational Signatures and Non-Gaussianities of General Single Field Inflation
• An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
• The Dark Side of the Halo Occupation Distribution
• Power Spectrum Analysis of Three-Dimensional Redshift Surveys
• The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
• Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
• Cosmology and fundamental physics with the Euclid satellite
• Dancing in the dark: galactic properties trace spin swings along the cosmic web
• Triaxial Modeling of Halo Density Profiles with High-resolution N-body Simulations
• The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
• The large-scale structure of the Universe
• Cosmic Growth History and Expansion History
• Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations
• An Effective Field Theory of Gravity for Extended Objects
• Merger rates in hierarchical models of galaxy formation. II: Comparison with N-body simulations
• Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)
• The age dependence of halo clustering
• 1/R gravity and Scalar-Tensor Gravity
• A test of the nature of cosmic acceleration using galaxy redshift distortions
• How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
• Transients from Initial Conditions in Cosmological Simulations
• Cosmological Non-Linearities as an Effective Fluid
• The Effective Field Theory of Cosmological Large Scale Structures
• The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
• Primordial Non-Gaussianities from Inflation Models
• Linking halo mass to galaxy luminosity
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• Formation and evolution of galaxy dark matter halos and their substructure
• Quasi-Single Field Inflation and Non-Gaussianities
• The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
• Redshift-Space Distortions, Pairwise Velocities and Nonlinearities
• Renormalized Cosmological Perturbation Theory
• New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy-galaxy lensing, clustering, and stellar mass functions from z=0.2 to z=1
• The 2dF Galaxy Redshift Survey: The dependence of galaxy clustering on luminosity and spectral type
• The linear power spectrum of observed source number counts
• Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
• The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
• A hierarchy of voids: Much ado about nothing
• The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
• Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
• The Nature of Galaxy Bias and Clustering
• The shape of non-Gaussianities
• Constraints on local primordial non-Gaussianity from large scale structure
• What galaxy surveys really measure
• Nonlinear Evolution of Baryon Acoustic Oscillations
• Fingers of God
• Relative velocity of dark matter and baryonic fluids and the formation of the first structures
• Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity
• Biasing and Hierarchical Statistics in Large-scale Structure
• Dark Energy vs. Modified Gravity
• Weak Lensing of the CMB: A Harmonic Approach
• Weighing Neutrinos with Galaxy Surveys
• The Effective Field Theorist's Approach to Gravitational Dynamics
• Intrinsic and Extrinsic Galaxy Alignment
• Relativistic second-order perturbations of the Einstein-de Sitter Universe
• MEASURING GALAXY MASSES USING GALAXY-GALAXY GRAVITATIONAL LENSING
• Measuring cosmological parameters with galaxy surveys
• The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering
• Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
• The Kilo-Degree Survey
• Recovery of the Power Spectrum of Mass Fluctuations from Observations of the Lyman-alpha Forest
• Non-Gaussianities in Single Field Inflation and their Optimal Limits from the WMAP 5-year Data
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• A discriminating probe of gravity at cosmological scales
• The effect of primordial non-Gaussianity on halo bias
• Assembly bias in the clustering of dark matter haloes
• Stochastic Nonlinear Galaxy Biasing
• Limits on non-Gaussianities from WMAP data
• Large-scale structure, the cosmic microwave background, and primordial non-gaussianity
• Measuring primordial non-gaussianity without cosmic variance
• Deriving the Nonlinear Cosmological Power Spectrum and Bispectrum from Analytic Dark Matter Halo Profiles and Mass Functions
• The Physics of the Intergalactic Medium
• Transients from Initial Conditions: A Perturbative Analysis
• New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
• Halo assembly bias and its effects on galaxy clustering
• Quasar Clustering and the Lifetime of Quasars
• Model-independent insights into the nature of the Lyman-alpha forest and the distribution of matter in the universe
• Massive Neutrinos and the Non-linear Matter Power Spectrum
• Confirmation of general relativity on large scales from weak lensing and galaxy velocities
• Signatures of Supersymmetry from the Early Universe
• The splashback radius as a physical halo boundary and the growth of halo mass
• Adiabatic Modes in Cosmology
• The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z=0.8 in the first data release
• Non-Linear Evolution of the Bispectrum of Cosmological Perturbations
• Cosmology with Weak Lensing Surveys
• Gravity and Large-Scale Non-local Bias
• Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation
• Improved forecasts for the baryon acoustic oscillations and cosmological distance scale
• Galaxy Formation and Large-Scale Bias
• The Bispectrum as a Signature of Gravitational Instability in Redshift-Space
• Generation and Characterization of Large Non-Gaussianities in Single Field Inflation
• Inferring the dark matter power spectrum from the Lyman-alpha forest in high-resolution QSO absorption spectra
• Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7
• The abundance of high-redshift objects as a probe of non-Gaussian initial conditions
• Testing cosmological structure formation using redshift-space distortions
• Intrinsic galaxy alignments from the 2SLAQ and SDSS surveys: luminosity and redshift scalings and implications for weak lensing surveys
• Large-scale clustering of galaxies in general relativity
• Chromo-Natural Inflation: Natural inflation on a steep potential with classical non-Abelian gauge fields
• Violation of non-Gaussianity consistency relation in a single field inflationary model
• The Mass-Concentration-Redshift Relation of Cold Dark Matter Halos
• The shape of the SDSS DR5 galaxy power spectrum
• Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures
• The Non-Parametric Model for Linking Galaxy Luminosity with Halo/Subhalo Mass
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS): measuring growth rate and geometry with anisotropic clustering
• Cosmology and the Bispectrum
• Halo Assembly Bias in Hierarchical Structure Formation
• The universality of the virial halo mass function and models for non-universality of other halo definitions
• Evidence for Quadratic Tidal Tensor Bias from the Halo Bispectrum
• Solid Inflation
• General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?
• The Cosmological Impact of Luminous TeV Blazars I: Implications of Plasma Instabilities for the Intergalactic Magnetic Field and Extragalactic Gamma-Ray Background
• How to measure redshift-space distortions without sample variance
• Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
• The Angular Trispectrum of the CMB
• Non-linear Evolution of f(R) Cosmologies III: Halo Statistics
• The IR-resummed Effective Field Theory of Large Scale Structures
• The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth
• The Scale Dependence of Halo and Galaxy Bias: Effects in Real Space
• Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure
• The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity and non-linear galaxy bias
• The Power Spectrum of Mass Fluctuations Measured from the Lyman-alpha Forest at Redshift z=2.5
• Effective field theory approach to quasi-single field inflation and effects of heavy fields
• Toward a Measurement of the Cosmological Geometry at z~2: Predicting Lyman-alpha Forest Correlation in Three Dimensions, and the Potential of Future Data Sets
• A marked correlation function analysis of halo formation times in the Millennium Simulation
• Non-Gaussianity as a Particle Detector
• Evolution of the angular momentum of protogalaxies from tidal torques: Zel'dovich approximation
• Convolution Lagrangian perturbation theory for biased tracers
• The effect of neutrinos on the matter distribution as probed by the Intergalactic Medium
• Gravitational clustering of relic neutrinos and implications for their detection
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies I: bias and gravity
• High-Order Correlations of Peaks and Halos: a Step toward Understanding Galaxy Biasing
• The one-dimensional Ly-alpha forest power spectrum from BOSS
• Resonant Non-Gaussianity
• Signatures of Initial State Modifications on Bispectrum Statistics
• Equivalence Principle and the Baryon Acoustic Peak
• The time-evolution of bias
• The Observed Squeezed Limit of Cosmological Three-Point Functions
• A 2.5% measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies
• The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Modeling the clustering and halo occupation distribution of BOSS-CMASS galaxies in the Final Data Release
• The Intermediate-Scale Clustering of Luminous Red Galaxies
• Bias in the Effective Field Theory of Large Scale Structures
• Scale-dependent bias induced by local non-Gaussianity: A comparison to N-body simulations
• Cosmic Shear from Galaxy Spins
• Generation of Vorticity and Velocity Dispersion by Orbit Crossing
• Galaxy Assembly Bias: A Significant Source of Systematic Error in the Galaxy-Halo Relationship
• The Three-Point Correlation Function in Cosmology
• Probing Primordial Non-Gaussianity with Large-Scale Structure
• Renormalized Halo Bias
• Halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditions
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• Flowing with Time: a New Approach to Nonlinear Cosmological Perturbations
• Intrinsic alignments of SDSS-III BOSS LOWZ sample galaxies
• Loop Corrections in Non-Linear Cosmological Perturbation Theory
• Primordial non-gaussianity, statistics of collapsed objects, and the Integrated Sachs-Wolfe effect
• The pseudo-evolution of halo mass
• Understanding higher-order nonlocal halo bias at large scales by combining the power spectrum with the bispectrum
• Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
• 4MOST - 4-metre Multi-Object Spectroscopic Telescope
• Virial masses of galactic halos from galaxy-galaxy lensing: theoretical modeling and application to SDSS
• Biased Tracers and Time Evolution
• Super-Sample Covariance in Simulations
• Cosmology with massive neutrinos II: on the universality of the halo mass function and bias
• Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
• Perturbation Theory Reloaded: Analytical Calculation of Non-linearity in Baryonic Oscillations in the Real Space Matter Power Spectrum
• Single-Field Consistency Relations of Large Scale Structure
• Large-scale bias in the Universe: bispectrum method
• DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos
• Redshift evolution of clustering
• Resumming Cosmic Perturbations
• The dependence of dark halo clustering on the formation epoch and the concentration parameter
• Halo Stochasticity from Exclusion and non-linear Clustering
• Symmetries and Consistency Relations in the Large Scale Structure of the Universe
• Large scale bias and stochasticity of halos and dark matter
• The Effective Field Theory of Large Scale Structures at Two Loops
• A Spherical Harmonic Analysis of Redshift Space
• Skewness and Kurtosis in Large-Scale Cosmic Fields
• Detection of the Splashback Radius and Halo Assembly bias of Massive Galaxy Clusters
• Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations
• Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
• Review of local non-Gaussianity from multi-field inflation
• Clustering of dark matter tracers: renormalizing the bias parameters
• Galaxy Bias and non-Linear Structure Formation in General Relativity
• Multi-Point Propagators in Cosmological Gravitational Instability
• The Bispectrum of IRAS Galaxies
• On the Renormalization of the Effective Field Theory of Large Scale Structures
• Influence of global cosmological expansion on local dynamics and kinematics
• The signature of the first stars in atomic hydrogen at redshift 20
• Minimizing the stochasticity of halos in large-scale structure surveys
• Testing Tidal-Torque Theory: II. Alignment of Inertia and Shear and the Characteristics of Proto-haloes
• The bias field of dark matter haloes
• Precision measurement of the local bias of dark matter halos
• A Halo Model of Galaxy Colors and Clustering in the SDSS
• A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
• Constraining primordial non-Gaussianity with future galaxy surveys
• Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxies
• Non-gaussianities and the Stimulated creation of quanta in the inflationary universe
• The overdensity and masses of the friends-of-friends halos and universality of the halo mass function
• An efficient implementation of massive neutrinos in non-linear structure formation simulations
• Correlation Function in Deep Redshift Space as a Cosmological Probe
• Large-scale non-Gaussian mass function and halo bias: tests on N-body simulations
• Primordial non-Gaussianity: large-scale structure signature in the perturbative bias model
• Constraining Peaks in Gaussian Primordial Density Fields: an Application of the Hoffman-Ribak Method
• Galilean invariance and the consistency relation for the nonlinear squeezed bispectrum of large scale structure
• `Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function
• The Clustering of Galaxies in SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: Constraints on Primordial Non-Gaussianity
• Constraints on the Effects of Locally-biased Galaxy Formation
• No-Go Theorems for Generalized Chameleon Field Theories
• Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-Gaussianity
• The Luminosity-Weighted or `Marked' Correlation Function
• A Spherical Harmonic Approach to Redshift Distortion and a Measurement of Omega from the 1.2 Jy IRAS Redshift Survey
• Lagrangian theory of gravitational instability of Friedman-Lemaitre cosmologies - generic third-order model for non-linear clustering
• The Statistics of Density Peaks and the Column Density Distribution of the Lyman-Alpha Forest
• Primordial non-Gaussianity from the large scale structure
• Origin and evolution of halo bias in linear and non-linear regimes
• Structure formation from non-Gaussian initial conditions: multivariate biasing, statistics, and comparison with N-body simulations
• Primordial non-Gaussianity, scale-dependent bias, and the bispectrum of galaxies
• Modeling scale-dependent bias on the baryonic acoustic scale with the statistics of peaks of Gaussian random fields
• Limits on f_NL parameters from WMAP 3yr data
• Southern Sky Redshift Survey: Clustering of Local Galaxies
• Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters
• Testing General Relativity on Horizon Scales and the Primordial non-Gaussianity
• Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces
• Going beyond the Kaiser redshift-space distortion formula: a full general relativistic account of the effects and their detectability in galaxy clustering
• Dynamical Masses in Modified Gravity
• The (not so) squeezed limit of the primordial 3-point function
• Biasing and the distribution of dark matter haloes
• Measuring the 3D Clustering of Undetected Galaxies Through Cross Correlation of their Cumulative Flux Fluctuations from Multiple Spectral Lines
• Skewness Induced by Gravity
• The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture
• Physical effects on the Lyman-alpha forest flux power spectrum: damping wings, ionizing radiation fluctuations, and galactic winds
• The Effective Field Theory of Large Scale Structure at Two Loops: the apparent scale dependence of the speed of sound
• Suppression and Spatial Variation of Early Galaxies and Minihalos
• Constraining ultra large-scale cosmology with multiple tracers in optical and radio surveys
• How to suppress the shot noise in galaxy surveys
• Dark matter clustering: a simple renormalization group approach
• Disentangling non-Gaussianity, bias and GR effects in the galaxy distribution
• Assembly bias and the dynamical structure of dark matter halos
• Detectability of the effect of Inflationary non-Gaussianity on halo bias
• The Cosmological Mass Distribution Function in the Zel'dovich Approximation
• The dependence on environment of Cold Dark Matter Halo properties
• Redshift-Space Clustering of SDSS Galaxies --- Luminosity Dependence, Halo Occupation Distribution, and Velocity Bias
• The Nonlinear Evolution of Rare Events
• Separate Universe Simulations
• Dominance of gauge artifact in the consistency relation for the primordial bispectrum
• Spherical collapse in quintessence models with zero speed of sound
• Redshift Space Distortions of the Correlation Function in Wide Angle Galaxy Surveys
• Probing cosmology and gravity with redshift-space distortions around voids
• Calibrating the Baryon Oscillation Ruler for Matter and Halos
• Asymmetric galaxy correlation functions
• Loop Corrections in Non-Linear Cosmological Perturbation Theory II. Two-point Statistics and Self-Similarity
• Evidence of Halo Assembly Bias in Massive Clusters
• Large-scale BAO signatures of the smallest galaxies
• Clustering Fossils from the Early Universe
• Information content of weak lensing power spectrum and bispectrum: including the non-Gaussian error covariance matrix
• Imprint of inflation on galaxy shape correlations
• Constraints on primordial non-Gaussianity from 800,000 photometric quasars
• Constraining Anisotropic Baryon Oscillations
• Beyond the Linear-Order Relativistic Effect in Galaxy Clustering: Second-Order Gauge-Invariant Formalism
• The Halo Mass Function from Excursion Set Theory. II. The Diffusing Barrier
• Algorithms for bispectra: forecasting, optimal analysis, and simulation
• The Physical Origin of Scale Dependent Bias in Cosmological Simulations
• Environmental Dependence of Cold Dark Matter Halo Formation
• Simulating nonlinear cosmological structure formation with massive neutrinos
• Primordial non-Gaussianity in the Bispectrum of the Halo Density Field
• Wiener Reconstruction of Density, Velocity, and Potential Fields from All-Sky Galaxy Redshift Surveys
• Cosmic Rulers
• Time-Sliced Perturbation Theory for Large Scale Structure I: General Formalism
• Signatures of anisotropic sources in the squeezed-limit bispectrum of the cosmic microwave background
• Ionizing radiation fluctuations and large-scale structure in the Lyman-alpha forest
• Halo Clustering with Non-Local Non-Gaussianity
• Velocity bias in a LCDM model
• The effects of UV background correlations on LyA forest flux statistics
• Cosmic Error and the Statistics of Large Scale Structure
• Position-dependent power spectrum of the large-scale structure: a novel method to measure the squeezed-limit bispectrum
• Redshift space correlations and scale-dependent stochastic biasing of density peaks
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• The Clustering of Massive Halos
• The nonlinear redshift-space power spectrum of galaxies
• Galaxy Bias and Primordial Non-Gaussianity
• ALMA Observation of 158 micron [CII] Line and Dust Continuum of a z=7 Normally Star-forming Galaxy in the Epoch of Reionization
• Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
• Redshift-Space Distortions with the Halo Occupation Distribution II: Analytic Model
• Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
• Redshift-space distortions around voids
• On Detecting Halo Assembly Bias with Galaxy Populations
• Signature of primordial non-Gaussianity of phi^3-type in the mass function and bias of dark matter haloes
• Optimal Constraints on Local Primordial Non-Gaussianity from the Two-Point Statistics of Large-Scale Structure
• The large-scale 3-point correlation function of the SDSS BOSS DR12 CMASS galaxies
• The Gravitational Shear--Intrinsic Ellipticity Correlation Functions of Luminous Red Galaxies in Observation and in the $\Lambda$CDM Model
• Collapse Barriers and Halo Abundance: Testing the Excursion Set Ansatz
• Large-Scale Structure with Gravitational Waves II: Shear
• Non-local Lagrangian bias
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Eulerian bias and the galaxy density field
• ZOMG-I. How the cosmic web inhibits halo growth and generates assembly bias
• Halo bias in mixed dark matter cosmologies
• The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX): Description and Early Pilot Survey Results
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): a cosmological forecast
• Baryon acoustic signature in the clustering of density maxima
• Neutrino Clustering in Cold Dark Matter Halos : Implications for Ultra High Energy Cosmic Rays
• The assembly bias of dark matter haloes to higher orders
• The impact of baryonic processes on the two-point correlation functions of galaxies, subhaloes and matter
• Peak-Background Split, Renormalization, and Galaxy Clustering
• A comparison of the evolution of the density field in perturbation theory and numerical simulations - II Counts in cells analysis
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• The VIMOS Public Extragalactic Redshift Survey: Measuring the growth rate of structure around cosmic voids
• Signature of Primordial Non-Gaussianity on Matter Power Spectrum
• The scale of homogeneity of the galaxy distribution in SDSS DR6
• The Correlation Function in Redshift Space: General Formula with Wide-angle Effects and Cosmological Distortions
• The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with 3-point correlation functions
• The Effective Field Theory of Dark Matter and Structure Formation: Semi-Analytical Results
• Physical Bias of Galaxies From Large-Scale Hydrodynamic Simulations
• Peaks theory and the excursion set approach
• 1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions
• Non-Gaussian statistics of critical sets in 2 and 3D: Peaks, voids, saddles, genus and skeleton
• The impact of massive neutrinos on the abundance of massive clusters
• A generalized local ansatz and its effect on halo bias
• One step beyond: The excursion set approach with correlated steps
• Non-Perturbative Effects of Geometry in Wide-Angle Redshift Distortions
• Stochasticity of Bias and Nonlocality of Galaxy Formation: Linear Scales
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• Wide Angle Redshift Distortions Revisited
• The Structure of Halos: Implications for Group and Cluster Cosmology
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: I. Real Space
• An improved model for the formation times of dark matter haloes
• Redshift-Space Distortions with the Halo Occupation Distribution I: Numerical Simulations
• Bispectrum and Nonlinear Biasing of Galaxies: Perturbation Analysis, Numerical Simulation and SDSS Galaxy Clustering
• Observational Evidence for an Age Dependence of Halo Bias
• Non-Gaussian Halo Bias Re-examined: Mass-dependent Amplitude from the Peak-Background Split and Thresholding
• The Halo Mass Function from Excursion Set Theory. III. Non-Gaussian Fluctuations
• Galaxy bispectrum, primordial non-Gaussianity and redshift space distortions
• Large-scale bias in the Universe II: redshift space bispectrum
• Higher order corrections to the large scale matter power spectrum in the presence of massive neutrinos
• Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
• On the Distribution of Haloes, Galaxies and Mass
• One-particle-irreducible consistency relations for cosmological perturbations
• Radiative Transfer Modeling of Lyman Alpha Emitters. II. New Effects in Galaxy Clustering
• Recursive Solutions of Lagrangian Perturbation Theory
• Large-Scale Structure and Gravitational Waves III: Tidal Effects
• Bias and high-order galaxy correlation functions in the APM Galaxy Survey
• Observational evidence for stochastic biasing
• The 3-point function in large scale structure: redshift distortions and galaxy bias
• The Local Theory of the Cosmic Skeleton
• Large-Scale Clustering of Cosmic Voids
• Intrinsic alignments of galaxies in the EAGLE and cosmo-OWLS simulations
• Large scale bias and the inaccuracy of the peak-background split
• Environmental dependence in the ellipsoidal collapse model
• Small Scale Perturbations in a General MDM Cosmology
• Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering
• On Separate Universes
• Excursion set peaks: a self-consistent model of dark halo abundances and clustering
• Self-similarity and scaling behavior of scale-free gravitational clustering
• Einstein's legacy in galaxy surveys
• RCSLenS: Testing gravitational physics through the cross-correlation of weak lensing and large-scale structure
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Near optimal bispectrum estimators for large-scale structure
• Cosmological Perturbation Theory and the Spherical Collapse Model - I. Gaussian Initial Conditions
• Resolving Cosmic Neutrino Structure: A Hybrid Neutrino N-body Scheme
• Observed galaxy number counts on the lightcone up to second order: I. Main result
• Lagrangian Evolution of the Weyl Tensor
• Detection of galaxy assembly bias
• Biased-estimations of the Variance and Skewness
• Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
• Simulating Voids
• The Mass Function of Cosmic Structures with Non-Spherical Collapse
• Measuring the growth of matter fluctuations with third-order galaxy correlations
• The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
• Inflationary tensor fossils in large-scale structure
• Constraining Gravity at the Largest Scales through CMB Lensing and Galaxy Velocities
• Implementing the DC Mode in Cosmological Simulations with Supercomoving Variables
• Systematic Renormalization of the Effective Theory of Large Scale Structure
• Weak Gravitational Lensing Bispectrum
• Time-analyticity of Lagrangian particle trajectories in ideal fluid flow
• The angle-averaged squeezed limit of nonlinear matter N-point functions
• The Three-point Function as a Probe of Models for Large-scale Structure
• Scale-dependent bias in the BAO-scale intergalactic neutral hydrogen
• The Local Bias Model in the Large Scale Halo Distribution
• On the Statistics of Biased Tracers in the Effective Field Theory of Large Scale Structures
• Linear redshift space distortions for cosmic voids based on galaxies in redshift space
• Parity violation of primordial magnetic fields in the CMB bispectrum
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• Simulating Redshift-Space Distortions for Galaxy Pairs with Wide Angular Separation
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• Equations of Gravitational Instability are Non-Local
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• N-body simulations with generic non-Gaussian initial conditions II: Halo bias
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• Consequences of Symmetries and Consistency Relations in the Large-Scale Structure of the Universe for Non-local bias and Modified Gravity
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density
• Spherical collapse in $\nu \Lambda CDM$
• All-Sky Analysis of the General Relativistic Galaxy Power Spectrum
• Perturbative approach to covariance matrix of the matter power spectrum
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• Optimal limits on primordial magnetic fields from CMB temperature bispectrum of passive modes
• Primordial non-Gaussianity in the large scale structure of the Universe
• Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume
• Action approach to cosmological perturbations: the 2nd order metric in matter dominance
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• Locally Biased Galaxy Formation and Large Scale Structure
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• Two Ways of Biasing Galaxy Formation
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• Supersonic Relative Velocity Effect on the Baryonic Acoustic Oscillation Measurements
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• The two-loop bispectrum of large-scale structure
• A robust measurement of the first higher-derivative bias of dark matter halos
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• The one-loop bispectrum of galaxies in redshift space from the Effective Field Theory of Large-Scale Structure
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• The quasi-linear nearby Universe
• Linear bias forecasts for emission line cosmological surveys
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• The squeezed matter bispectrum covariance with responses
• Redshift-space streaming velocity effects on the Lyman-$\alpha$ forest baryon acoustic oscillation scale
• The physical origins of low-mass spin bias
• Lagrangian cosmological perturbation theory at shell-crossing
• Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks
• Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra
• Cosmological Information in Skew Spectra of Biased Tracers in Redshift Space
• Galaxy shape statistics in the effective field theory
• Galaxy Bias and ${\sigma }_8$ from Counts in Cells from the SDSS Main Sample
• Cosmological perturbations for two cold fluids in $\Lambda$CDM
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• Wide-angle and relativistic effects in Fourier-space clustering statistics
• Halo assembly bias from Separate Universe simulations
• What Can We Learn by Combining the Skew Spectrum and the Power Spectrum?
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Cosmology inference at the field level from biased tracers in redshift-space
• Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space
• Interacting dark energy from the joint analysis of the power spectrum and bispectrum multipoles with the EFTofLSS
• Nonlinear evolution of initially biased tracers in modified gravity
• Correcting correlation functions for redshift-dependent interloper contamination
• Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Generalized covariant prescriptions for averaging cosmological observables
• Euclid: The search for primordial features
• Spectral distortion anisotropies from single-field inflation
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Anisotropic halo assembly bias and redshift-space distortions
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• SuperFaB: a fabulous code for Spherical Fourier-Bessel decomposition
• Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
• Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses
• EFTofLSS meets simulation-based inference: ${\sigma }_8$ from biased tracers
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• Modeling HI at the field level
• Unveiling dark forces with measurements of the Large Scale Structure of the Universe
• Weighing neutrinos with the halo environment
• The Weak Lensing Bispectrum Induced By Gravity
• The Likelihood for LSS: Stochasticity of Bias Coefficients at All Orders
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• Some assembly required: assembly bias in massive dark matter halos
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Local primordial non-Gaussianity in the relativistic galaxy bispectrum
• Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos
• Coupling parsec and gigaparsec scales: primordial non-Gaussianity with multi-tracer intensity mapping
• The Ly$\alpha$ forest flux correlation function: a perturbation theory perspective
• Taking measurements of the kinematic Sunyaev-Zel'dovich effect forward: including uncertainties from velocity reconstruction with forward modeling
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck I: Construction of CMB Lensing Maps and Modeling Choices
• Reconstructing the baryon acoustic oscillations using biased tracers
• Light Fields during Inflation from BOSS and Future Galaxy Surveys
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• The bias of dark matter tracers: assessing the accuracy of mapping techniques
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• Primordial non-Gaussianity and non-Gaussian Covariance
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• The universal multiplicity function: counting halos and voids
• A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond
• Impact of bias and redshift-space modelling for the halo power spectrum: Testing the effective field theory of large-scale structure
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• Bayesian cosmic density field inference from redshift space dark matter maps
• New Shapes of Primordial Non-Gaussianity from Quasi-Single Field Inflation with Multiple Isocurvatons
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• Multi-tracer power spectra and bispectra: Formalism
• Gravitational wave fossils in nonlinear regime: halo tidal bias and intrinsic alignments from gravitational wave separate universe simulations
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• Localizing Transformations of the Galaxy-Galaxy Lensing Observable
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Probing primordial non-Gaussianity with Fast Radio Bursts
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• Density reconstruction from biased tracers and its application to primordial non-Gaussianity
• Probing massive neutrinos with the Minkowski functionals of the galaxy distribution
• Integrated Sachs-Wolfe-galaxy cross-correlation bounds on the two branches of the minimal theory of massive gravity
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Quadratic shape biases in three-dimensional halo intrinsic alignments
• Tracer-Field Cross-Correlations with $k$-Nearest Neighbor Distributions
• Renormalization of Lagrangian bias via spectral parameters
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• Full-sky bispectrum in redshift space for 21cm intensity maps
• Cosmology from weak lensing alone and implications for the Hubble tension
• The cosmic web connection to the dark matter halo distribution through gravity
• The HI-halo mass relation at redshift $z\sim 1$ from the Minkowski functionals of 21 cm intensity maps
• Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe
• Cosmological Angular Trispectra and Non-Gaussian Covariance
• Renormalisation of linear halo bias in N-body simulations
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• The clustering of critical points in the evolving cosmic web
• Statistics of biased tracers in variance-suppressed simulations
• Squeezing $f_{\mathrm{NL}}$ out of the matter bispectrum with consistency relations
• General relativistic effects in the galaxy bias at second order
• Star-Galaxy Image Separation with Computationally Efficient Gaussian Process Classification
• Local Primordial Non-Gaussianities and Super-Sample Variance
• BAO scale inference from biased tracers using the EFT likelihood
• Marked correlation functions in perturbation theory
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• A Better Way to Define Dark Matter Haloes
• Two-loop power spectrum with full time- and scale-dependence and EFT corrections: impact of massive neutrinos and going beyond EdS
• Impact of survey geometry and super-sample covariance on future photometric galaxy surveys
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• Lagrangian approach to super-sample effects on biased tracers at field level: galaxy density fields and intrinsic alignments
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• Optimal computation of anisotropic galaxy three point correlation function multipoles using 2DFFTLOG formalism
• Clustering of Local Extrema in Planck CMB maps
• Efficient parallel algorithm for estimating higher-order polyspectra
• Effects of primordial black holes quantum gravity decay on galaxy clustering
• Cosmological Probes of Structure Growth and Tests of Gravity
• fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
• Testing the consistency of three-point halo clustering in Fourier and configuration space
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• The Breakdown Scale of HI Bias Linearity
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• The Stellar Kinematics of Void Dwarf Galaxies Using KCWI
• Measurement of Void Bias Using Separate Universe Simulations
• The Lyman-$\alpha$ power spectrum - CMB lensing convergence cross-correlation
• Halo assembly bias from a deep learning model of halo formation
• Perturbation theory of LSS in the $\Lambda$CDM Universe: exact time evolution and the two-loop power spectrum
• Small-scale clustering of Primordial Black Holes: cloud-in-cloud and exclusion effects
• Cosmology before noon with multiple galaxy populations
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• The Odd-Parity Galaxy Bispectrum
• Optical depth to reionization from perturbative 21cm clustering
• Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
• Understanding the Reconstruction of the Biased Tracer
• Grid-based calculations of redshift-space matter fluctuations from perturbation theory: UV sensitivity and convergence at the field level
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
• A new scale in the bias expansion
• Cosmological homogeneity scale estimates are dressed
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• Observing relativistic features in large-scale structure surveys -- I: Multipoles of the power spectrum
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• Testing the equivalence principle on cosmological scales using the odd multipoles of galaxy cross-power spectrum and bispectrum
• Robust Neural Network-Enhanced Estimation of Local Primordial Non-Gaussianity
• Cosmology using numerical relativity
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• Testing General Relativity with the Doppler magnification effect
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• Euclid preparation. Modelling spectroscopic clustering on mildly nonlinear scales in beyond-$\Lambda$CDM models
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
• Structure formation in an anisotropic universe: Eulerian perturbation theory
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
• DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Super-sample tidal modes on the celestial sphere
• Non-Gaussian CMB and LSS statistics beyond polyspectra
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• Impact of stellar population synthesis choices on forward modelling-based redshift distribution estimates
• Opening Reionization: Quantitative Morphology of the Epoch of Reionization and Its Connection to the Cosmic Density Field
• Large Scale Structure Reconstruction with Short-Wavelength Modes
• Bayesian Control Variates for optimal covariance estimation with pairs of simulations and surrogates
• Estimating the Integrated Bispectrum from Weak Lensing Maps
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• The statistics of peaks of weakly non-Gaussian random fields: Effects of bispectrum in two- and three-dimensions
• Integrated perturbation theory for cosmological tensor fields. III. Projection effects
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Neutrino winds on the sky
• Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear halo density field
• The biasing phenomenon
• Revisiting GeV-scale annihilating dark matter with the AMS-02 positron fraction
• Skewing the CMB$\times$LSS: a Fast Method for Bispectrum Analysis
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• The galaxy bias at second order in general relativity with Non-Gaussian initial conditions
• First test of the consistency relation for the large-scale structure using the anisotropic three-point correlation function of BOSS DR12 galaxies (An explanatory video is available at https://youtu.be/Zi36ooLPhss.)
• Integrated perturbation theory for cosmological tensor fields. II. Loop corrections
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Direct signatures of the formation time of galaxies
• fNL - gNL mixing in the matter density field at higher orders
• A study on the Clustering Properties of Radio-Selected sources in the Lockman Hole Region at 325 MHz
• Large scale distribution of mass versus light from Baryon Acoustic Oscillations: Measurement in the final SDSS-III BOSS Data Release 12
• Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
• Power spectrum in the presence of large-scale overdensity and tidal fields: breaking azimuthal symmetry
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• Non-perturbative halo clustering from cosmological density peaks
• The Renormalization Group for Large-Scale Structure: Primordial non-Gaussianities
• The phenomenology of the external field effect in cold dark matter models
• The halo bias for number counts on the light cone from relativistic N-body simulations
• 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
• Imprint of massive neutrinos on Persistent Homology of large-scale structure
• The halo 3-point correlation function: a methodological analysis
• Study on the mapping of halo clustering from real space to redshift space
• Validating galaxy clustering models with Fixed & Paired and Matched-ICs simulations: application to Primordial Non-Gaussianities
• BullFrog: Multi-step perturbation theory as a time integrator for cosmological simulations
• Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
• Color dependence of clustering of massive galaxies at 0.5$\le z\le$2.5: similar spatial distributions between green valley galaxies and AGNs
• Weak Lensing Trispectrum and Kurt-Spectra
• The flat-sky approximation to galaxy number counts -- redshift space correlation function
• On the galaxy 3-point correlation function in Modified Gravity
• A model-independent tripartite test of cosmic distance relations
• Apparent parity violation in the observed galaxy trispectrum
• The Effective Field Theory and Perturbative Analysis for Log-Density Fields
• KiDS-Legacy: Angular galaxy clustering from deep surveys with complex selection effects
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• Covariant Decomposition of The Non-Linear Galaxy Number Counts and Their Monopole
• Second-order peculiar velocity field as a novel probe of scalar-tensor theories
• On general-relativistic Lagrangian perturbation theory and its non-perturbative generalization
• Consistency relations for the Lagrangian halo bias and their implications
• Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure
• Fast Calculation of Nonlinear Redshift-space Galaxy Power Spectrum Including Selection Bias
• Can the sound horizon-free measurement of $H_0$ constrain early new physics?
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Unveiling the Universe with Emerging Cosmological Probes
• Anatomy of Parity-violating Trispectra in Galaxy Surveys
• Multi-wavelength consensus of large-scale linear bias
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• The effect of finite halo size on the clustering of neutral hydrogen
• Decoupling Local Primordial non-Gaussianity from Relativistic Effects in the Galaxy Bispectrum
• Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
• An Ising model for galaxy bias
• A rising tide: Intrinsic alignments since the turn of the millennium
• The environment-dependence of the growth of the most massive objects in the Universe
• The large-separation expansion of peak clustering in Gaussian random fields
• CSST Cosmological Emulator III: Hybrid Lagrangian Bias Expansion Emulation of Galaxy Clustering
• Which is a better cosmological probe: Number counts or cosmic magnification?
• A Relativistic Interpretation of Bias in Newtonian Simulations
• Non-linear Cosmological Perturbations for Coupled Dark Energy
• Gravitational Turbulence: the Small-Scale Limit of the Cold-Dark-Matter Power Spectrum
• From matter to galaxies: General relativistic bias for the one-loop bispectrum
• Hawaii Two-0: High-redshift galaxy clustering and bias
• The Spatial Range of Conformity
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps
• Contributions from primordial non-Gaussianity and General Relativity to the galaxy power spectrum
• Non-local contribution from small scales in galaxy-galaxy lensing: Comparison of mitigation schemes
• Optimizing the Evolution of Perturbations in the $\Lambda$CDM Universe
• Anisotropic effective redshift and evolving clustering amplitude
• Constraints on primordial non-Gaussianity using multitracer technique for skew spectrum
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Resonant neutrino self-interactions: Insights from the full shape galaxy power spectrum
• Ray-tracing log-normal simulation for weak gravitational lensing: application to the cross-correlation with galaxies
• Bispectrum constraints on Primordial non-Gaussianities with the eBOSS DR16 quasars
• First Light and Reionisation Epoch Simulations (FLARES) X: Environmental Galaxy Bias and Survey Variance at High Redshift
• Position-Dependent Correlation Function of Weak Lensing Convergence
• Relativistic matter bispectrum of cosmic structures on the light cone
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• Breaking the ${\tau }_{\mathrm{T}}-f$ degeneracy of the kinetic Sunyaev Zel'dovich cosmology in redshift space
• Fast and accurate collapse-time predictions for collisionless matter
• Non-Linearity-Free prediction of the growth-rate $f{\sigma }_8$ using Convolutional Neural Networks
• Cluster-counterpart Voids: Void Identification from Galaxy Density Field
• Nonlinear Redshift-Space Distortions on the Full Sky
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• Reconstructing the Long-wavelength Matter Density Fluctuation Modes from the Scalar-Type Clustering Fossils
• Joint inference of multiplicative and additive systematics in galaxy density fluctuations and clustering measurements
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• Fast simulation mapping: from standard to modified gravity cosmologies using the bias assignment method
• Straightening the Ruler: Field-Level Inference of the BAO Scale with LEFTfield
• Probabilistic Estimators of Lagrangian Shape Biases: Universal Relations and Physical Insights
• The impact of large-scale galaxy clustering on the variance of the Hellings-Downs correlation: numerical results
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Signature of Massive Neutrinos from the Clustering of Critical Points. I. Density-threshold-based Analysis in Configuration Space
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Relativistic second-order initial conditions for simulations of large-scale structure
• Doppler bias: impact of peculiar velocities on color selection and the large scale structure of galaxy surveys
• Probing the independence within the dark sector in the fluid approximation
• Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering
• Linear Relativistic Corrections in the Spherical Fourier-Bessel Power Spectrum
• A model-independent measurement of the expansion and growth rates from BOSS using the FreePower method
• Renormalization group computation of likelihood functions for cosmological data sets
• Zero Metallicity with Zero CPU Hours: Masses of the First Stars on the Laptop
• Scale-dependent halo bias and the squeezed limit bispectrum in the presence of radiation
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Cosmological perturbation theory for large scale structure in phase space
• Extending evolution mapping to massive neutrinos with COMET
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Skewness consistency relation in large-scale structure and test of gravity theory
• Challenges in Cosmic Magnification Reconstruction by Magnification Response
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• The Compressed 3D Lyman-Alpha Forest Bispectrum
• Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs
• The energy shear of protohaloes
• Statistical exploration of halo anisotropic clustering and intrinsic alignments with the mass-Peak Patch algorithm
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• Impact of Redshift Space Distortion on Persistent Homology of cosmic matter density field
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Detecting Relativistic Doppler by Multi-Tracing a Single Galaxy Population
• Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Squeezing information from radio surveys to probe the primordial Universe
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Gaussian Lagrangian Galaxy Bias
• The imprints of massive neutrinos on the three-point correlation function of large-scale structures
• Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• Constraining primordial non-Gaussianity from the large scale structure two-point and three-point correlation functions
• Calculating the EFT likelihood via saddle-point expansion
• Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• Cosmological Implications of a Neutrino Mass Detection
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Speeding up the detectability of the harmonic-space galaxy bispectrum
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Improved renormalization group computation of likelihood functions for cosmological data sets
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity
• Simulation budgeting for hybrid effective field theories
• Cross-correlating the EMU Pilot Survey 1 with CMB lensing: Constraints on cosmology and galaxy bias with harmonic-space power spectra
• Obtaining non-linear galaxy bias constraints from galaxy-lensing phase differences
• A direct detection method of galaxy intrinsic ellipticity-gravitational shear correlation in non-linear regimes using self-calibration
• The Large Scale Structure Bootstrap: perturbation theory and bias expansion from symmetries
• Mitigation of nonlinear galaxy bias with a theoretical-error likelihood
• Lagrangian-space Gaussian ansatz for the matter redshift-space power spectrum and correlation function
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Towards cosmology with Void Lensing: how to find voids sensitive to weak-lensing and numerically interpret them
• Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Delensing CMB B-modes using galaxy surveys: the effect of galaxy bias and matter clustering non-linearities
• Planck isocurvature constraint on primordial black holes lighter than a kiloton
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• Qualitative probe of interacting dark energy with redshift-space distortions
• Perturbation Theory Remixed II: Improved Modeling of Nonlinear Bispectrum
• Super sample covariance and the volume scaling of galaxy survey covariance matrices
• Clustering of the extreme: A theoretical description of weak lensing critical points power spectra in the mildly nonlinear regime
• Non-parametric Lagrangian biasing from the insights of neural nets
• Interacting dark energy from redshift-space galaxy clustering
• Large scale structures: from inflation to today: a brief report
• Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• Differentiable Fuzzy Cosmic-Web for Field Level Inference
• Cosmic voids and BAO with relative baryon-CDM perturbations
• Predicting Halo Formation Time Using Machine Learning
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Searching for Dark Structures: A Comparison of Weak-lensing Convergence Maps and Lensing-weighted Galaxy Density Maps
• Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid
• Realistic systematic biases induced by residual intrinsic alignments in cosmic shear surveys
• Clustering analysis of medium-band selected high-redshift galaxies
• Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field $\mathrm{I}$: 1-Loop Corrections involving Second-Order Densities
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order
• Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field $\mathrm{II}$: 1-Loop Corrections with Third-Order Densities
• On the Connection between Field-Level Inference and $n$-point Correlation Functions
• Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference
• Skew-spectra: a generalization to spin-$s$
• Constraining effective neutrino species with bispectrum of large scale structures
• An effective $\mathbf{\Lambda }$-Szekeres modelling of the local Universe with Cosmicflows-4
• Bridging Simulations and EFT: A Hybrid Model of the Lyman-Alpha Forest Field
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy
• Wasserstein Distance in Cosmological Structure Formation: An Optimal Transport Perspective
• Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Bubble Correlation in First-Order Phase Transitions
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• Non-Gaussianity in the Squeezed Three-Point Correlation from the Relativistic Effects
• Using a Neural Network Classifier to Select Galaxies with the Most Accurate Photometric Redshifts
• Expansion series of the pairwise velocity generating function and its implications on redshift space distortion modeling
• Fisher matrix for multiple tracers: the information in the cross-spectra