Stable clustering, the halo model and nonlinear cosmological power spectra

Abstract

We present the results of a large library of cosmological N-body simulations, using power-law initial spectra. The nonlinear evolution of the matter power spectra is compared with the predictions of existing analytic scaling formulae based on the work of Hamilton et al. The scaling approach has assumed that highly nonlinear structures obey `stable clustering' and are frozen in proper coordinates. Our results show that, when transformed under the self-similarity scaling, the scale-free spectra define a nonlinear locus that is clearly shallower than would be required under stable clustering. Furthermore, the small-scale nonlinear power increases as both the power-spectrum index n and the density parameter Omega decrease, and this evolution is not well accounted for by the previous scaling formulae. This breakdown of stable clustering can be understood as resulting from the modification of dark-matter haloes by continuing mergers. These effects are naturally included in the analytic `halo model' for nonlinear structure; using this approach we are able to fit both our scale-free results and also our previous CDM data. This approach is more accurate than the commonly-used Peacock--Dodds formula and should be applicable to more general power spectra. Code to evaluate nonlinear power spectra using this method is available from http://as1.chem.nottingham.ac.uk/~res/software.html Following publication, we will make the power-law simulation data available through the Virgo website http://www.mpa-garching.mpg.de/Virgo

V2: 23 Latex Pages. Replaced with a version consistent with refereed journal article. Section 3.4 reduced, Fig added to section 6, references added

References in corpus (46)

• A Universal Density Profile from Hierarchical Clustering
• The Structure of Cold Dark Matter Halos
• Dark Matter Substructure in Galactic Halos
• Large scale bias and the peak background split
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• Mass function of dark matter halos
• An analytic model for the spatial clustering of dark matter haloes
• Analytic model for galaxy and dark matter clustering
• Halo Formation in Warm Dark Matter Models
• Halo occupation numbers and galaxy bias
• Nonlinear evolution of cosmological power spectra
• Reconstructing the linear power spectrum of cosmological mass fluctuations
• How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
• Evolution of structure in cold dark matter universes
• The Nature of Galaxy Bias and Clustering
• Spatial correlation function and pairwise velocity dispersion of galaxies: CDM models versus the Las Campanas Survey
• Deriving the Nonlinear Cosmological Power Spectrum and Bispectrum from Analytic Dark Matter Halo Profiles and Mass Functions
• Hydra: An Adaptive--Mesh Implementation of PPPM--SPH
• Baryonic Signatures in Large-Scale Structure
• High-Order Correlations of Peaks and Halos: a Step toward Understanding Galaxy Biasing
• Cosmic Shear Statistics and Cosmology
• PTHalos: A fast method for generating mock galaxy distributions
• Biasing and the distribution of dark matter haloes
• Loop Corrections in Non-Linear Cosmological Perturbation Theory II. Two-point Statistics and Self-Similarity
• Hydra: A Parallel Adaptive Grid Code
• A comparison of the evolution of the density field in perturbation theory and numerical simulations - II Counts in cells analysis
• Can Baryonic Features Produce the Observed 100 Mpc Clustering?
• Self-similarity and scaling behavior of scale-free gravitational clustering
• Phase Information and the Evolution of Cosmological Density Perturbations
• Analytical Approximations to the Low-Order Statistics of Dark Matter Distribution
• Self-Similar Evolution of Gravitational Clustering: N-Body Simulations of the n=-2 Spectrum
• Modelling the Nonlinear Gravitational Clustering in the Expanding Universe
• The non-linear correlation function and the shapes of virialized halos
• Pattern in Nonlinear Gravatational Clustering: A Numerical Investigation
• A New Parallel P3M Code for Very Large-Scale Cosmological Simulations
• Does Gravitational Clustering Stabilize On Small Scales?
• What Does It Take to Stabilize Gravitational Clustering?
• Previrialization: Perturbative and N-Body Results
• The Evolution of Correlation Functions and Power Spectra in Gravitational Clustering
• Linearizing the Observed Power Spectrum
• Scaling Relations for Gravitational Collapse in Two Dimensions
• A Universal Profile of the Dark Matter Halo and the Two-point Correlation Function
• A Simple Method for Computing the Non-Linear Mass Correlation Function with Implications for Stable Clustering
• The effects of anti-correlation on gravitational clustering
• Mean-pairwise peculiar velocity in cosmological N-body simulations: time-variation, scale-dependence and stable condition

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• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• Constraints on cosmic hemispherical power anomalies from quasars
• The Atacama Cosmology Telescope: Cross-Correlation of CMB Lensing and Quasars
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• Interpreting the Observed Clustering of Red Galaxies at z~3
• The Halo Distribution of 2dF Galaxies
• Testing the Warm Dark Matter paradigm with large-scale structures
• The real-space clustering of luminous red galaxies around z<0.6 quasars in the Sloan Digital Sky Survey
• Weak lensing of the CMB
• Scaling Laws in the Distribution of Galaxies
• Shear Selected Cluster Cosmology I: Tomography and Optimal Filtering
• Constraining chameleon models with cosmology
• Cosmological Information in Weak Lensing Peaks
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Cosmological Constraints on Dark Matter Interactions with Ordinary Matter
• A preference for a non-zero neutrino mass from cosmological data
• Spherical Collapse and the Halo Model in Braneworld Gravity
• Analytic model for the matter power spectrum, its covariance matrix, and baryonic effects
• Weak lensing from space: first cosmological constraints from three-point shear statistics
• Do stochastic inhomogeneities affect dark-energy precision measurements?
• Accurate estimators of power spectra in N-body simulations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• An improved fitting formula for the dark matter bispectrum
• The clustering of H-alpha emitters at z=2.23 from HiZELS
• Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit
• Weak-Lensing Mass Calibration of ACTPol Sunyaev-Zel'dovich Clusters with the Hyper Suprime-Cam Survey
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• The Abundance and Radial Distribution of Satellite Galaxies
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• Density split statistics: joint model of counts and lensing in cells
• Cosmic Shear Results from the Deep Lens Survey - II: Full Cosmological Parameter Constraints from Tomography
• The zCOSMOS Survey. The dependence of clustering on luminosity and stellar mass at z=0.2-1
• The Cosmological Impact of Intrinsic Alignment Model Choice for Cosmic Shear
• Studying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2
• Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
• Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
• Survey geometry and the internal consistency of recent cosmic shear measurements
• Clustering of Lyman Break Galaxies at z=4 and 5 in The Subaru Deep Field: Luminosity Dependence of The Correlation Function Slope
• Observational bounds on the cosmic radiation density
• The 6dF Galaxy Survey: Bulk Flows on $50-70h^{-1}$ Mpc scales
• The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with 3-point correlation functions
• Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
• Bayesian non-linear large scale structure inference of the Sloan Digital Sky Survey data release 7
• Constraints on the Alignment of Galaxies in Galaxy Clusters from $\sim$14,000 Spectroscopic Members
• Beyond Limber: Efficient computation of angular power spectra for galaxy clustering and weak lensing
• The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field
• The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey
• Measuring neutrino masses and dark energy with weak lensing tomography
• A direct measurement of the linear bias of mid-infrared-selected quasars at z~1 using cosmic microwave background lensing
• Fourier analysis of luminosity-dependent galaxy clustering
• Finding Evidence for Massive Neutrinos using 3D Weak Lensing
• Cosmological parameter constraints for Horndeski scalar-tensor gravity
• The 2dF Galaxy Redshift Survey: Wiener Reconstruction of the Cosmic Web
• Multiple inflation and the WMAP 'glitches' II. Data analysis and cosmological parameter extraction
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment
• A CMB lensing mass map and its correlation with the cosmic infrared background
• Matching current observational constraints with nonminimally coupled dark energy
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Luminosity and Color Dependence and Redshift Evolution
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• Halo-model signatures from 380,000 SDSS Luminous Red Galaxies with photometric redshifts
• Galaxy-galaxy lensing constraints on the relation between baryons and dark matter in galaxies in the Red Sequence Cluster Survey 2
• 2D-FFTLog: Efficient computation of real space covariance matrices for galaxy clustering and weak lensing
• Analysis of two-point statistics of cosmic shear: III. Covariances of shear measures made easy
• Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
• Rapid modelling of the redshift-space power spectrum multipoles for a masked density field
• Cosmological parameters from combined second- and third-order aperture mass statistics of cosmic shear
• Estimating Cosmological Parameter Covariance
• Intrinsic galaxy shapes and alignments II: Modelling the intrinsic alignment contamination of weak lensing surveys
• Cosmology in the era of Euclid and the Square Kilometre Array
• Measuring neutrino masses with a future galaxy survey
• Extending cosmological tests of General Relativity with the Square Kilometre Array
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: I. Real Space
• New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• Detection of warm and diffuse baryons in large scale structure from the cross-correlation of gravitational lensing and the thermal Sunyaev-Zeldovich effect
• Cross-correlation between the CMB lensing potential measured by Planck and high-z sub-mm galaxies detected by the Herschel-ATLAS survey
• Towards optimal parallel PM N-body codes: PMFAST
• PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS
• Large-N expansions applied to gravitational clustering
• Future CMB tests of dark matter: ultra-light axions and massive neutrinos
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
• Estimation of cosmological parameters using adaptive importance sampling
• New Early Dark Energy is compatible with current LSS data
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• Cosmological performance of SKA HI galaxy surveys
• A hydrodynamical halo model for weak-lensing cross correlations
• Measuring dark energy properties with 3D cosmic shear
• Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model
• Simulations of Baryon Oscillations
• The Atacama Cosmology Telescope: Lensing of CMB Temperature and Polarization Derived from Cosmic Infrared Background Cross-Correlation
• Reconstructing the Near-IR Background Fluctuations from known Galaxy Populations using Multiband Measurements of Luminosity Functions
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• Probing Dark Low-mass Halos and Primordial Black Holes with Frequency-dependent Gravitational Lensing Dispersions of Gravitational Waves
• Dark Sky Simulations: Early Data Release
• N-Body Simulations of Alternate Gravity Models
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• Average and dispersion of the luminosity-redshift relation in the concordance model
• Simulations and symmetries
• Cosmic shear analysis of archival HST/ACS data: I. Comparison of early ACS pure parallel data to the HST/GEMS Survey
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
• Galaxy Bispectrum from Massive Spinning Particles
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Interpreting the unresolved intensity of cosmologically redshifted line radiation
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
• First Measurement of the Cross-Correlation of CMB Lensing and Galaxy Lensing
• RCSLenS: Testing gravitational physics through the cross-correlation of weak lensing and large-scale structure
• The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
• Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample
• Information content of the non-linear power spectrum: the effect of beat-coupling to large scales
• An analytic model for the bispectrum of galaxies in redshift space
• The Sigma-8 Tension is a Drag
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• Tests of Gravity from Imaging and Spectroscopic Surveys
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• GaBoDS: The Garching-Bonn Deep Survey: VI. Cosmic shear analysis
• The stellar-subhalo mass relation of satellite galaxies
• Weak lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data
• Cosmological constraints from COMBO-17 using 3D weak lensing
• Mapping Growth and Gravity with Robust Redshift Space Distortions
• Dark matter statistics for large galaxy catalogs: power spectra and covariance matrices
• A parametrization of the growth index of matter perturbations in various Dark Energy models and observational prospects using a Euclid-like survey
• Large-Scale Structure in Brane-Induced Gravity II. Numerical Simulations
• Cosmological Simulations for Combined-Probe Analyses: Covariance and Neighbour-Exclusion Bias
• Cosmic Cartography of the Large-Scale Structure with Sloan Digital Sky Survey Data Release 6
• DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos
• Dark Energy Survey Year 3 Results: Optimizing the Lens Sample in Combined Galaxy Clustering and Galaxy-Galaxy Lensing Analysis
• Bias due to neutrinos must not uncorrect'd go
• Constraints on the correlation between QSO luminosity and host halo mass from high-redshift quasar clustering
• The DEEP2 Galaxy Redshift Survey: Clustering Dependence on Galaxy Stellar Mass and Star Formation Rate at z~1
• Fast simulations for intensity mapping experiments
• The angle-averaged squeezed limit of nonlinear matter N-point functions
• Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• High-redshift post-reionization cosmology with 21cm intensity mapping
• Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
• Simulations of Weak Gravitational Lensing - II : Including Finite Support Effects in Cosmic Shear Covariance Matrices
• Measuring the lensing potential with tomographic galaxy number counts
• The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10${}^3$ submillimeter galaxies in the UKIDSS-UDS field
• Nonlinear growth in modified gravity theories of dark energy
• Cosmology with the Square Kilometre Array
• Using neural networks to estimate redshift distributions. An application to CFHTLenS
• The VLT LBG Redshift Survey - III. The clustering and dynamics of Lyman-break galaxies at z ~ 3
• Is there concordance within the concordance $\Lambda$CDM model?
• Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
• Nonlinear structure formation in Nonlocal Gravity
• Discreteness Effects in Lambda Cold Dark Matter Simulations: A Wavelet-Statistical View
• The impact of Early Dark Energy on non-linear structure formation
• Two- and three-dimensional wide-field weak lensing mass maps from the Hyper Suprime-Cam Subaru Strategic Program S16A data
• A General Study of the Influence of Catastrophic Photometric Redshift Errors on Cosmology with Cosmic Shear Tomography
• Recovering the nonlinear density field from the galaxy distribution with a Poisson-Lognormal filter
• Delensing Gravitational Wave Standard Sirens with Shear and Flexion Maps
• Cosmological Constraints from a Combination of Galaxy Clustering & Lensing -- II. Fisher Matrix Analysis
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• General Requirements on Matter Power Spectrum Predictions for Cosmology with Weak Lensing Tomography
• Constraints on Neutrino Masses from Weak Lensing
• The Angular Clustering of Infrared-Selected Obscured and Unobscured Quasars
• MPTbreeze: A fast renormalized perturbative scheme
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• Lensing Reconstruction using redshifted 21cm Fluctuations
• Accurate cosmic shear errors: do we need ensembles of simulations?
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• Cosmic variance of weak lensing surveys in the non-Gaussian regime
• Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release
• A 14 $h^{-3}$ Gpc${}^3$ study of cosmic homogeneity using BOSS DR12 quasar sample
• Halo model and halo properties in Galileon gravity cosmologies
• On the complementarity of galaxy clustering with cosmic shear and flux magnification
• Shrinkage Estimation of the Power Spectrum Covariance Matrix
• SKA Weak Lensing I: Cosmological Forecasts and the Power of Radio-Optical Cross-Correlations
• Intrinsic alignments of BOSS LOWZ galaxies II: Impact of shape measurement methods
• The SDSS Coadd: Cosmic Shear Measurement
• Reduced Shear Power Spectrum
• Precision era of the kinetic Sunyaev-Zeldovich effect: simulations, analytical models and observations and the power to constrain reionization
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Cross-correlation of Planck CMB Lensing and CFHTLenS Galaxy Weak Lensing Maps
• Tidal alignments as a contaminant of redshift space distortions
• Performance of internal Covariance Estimators for Cosmic Shear Correlation Functions
• PRIMUS + DEEP2: Clustering of X-ray, Radio and IR-AGN at z~0.7
• The halo model for cosmology: a pedagogical review
• Chameleon Halo Modeling in f(R) Gravity
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• The effect of modified gravity on weak lensing
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Cosmic Web and Environmental Dependence of Screening: Vainshtein vs. Chameleon
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• Tests of redshift-space distortions models in configuration space for the analysis of the BOSS final data release
• An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• On the Probability Distributions of Ellipticity
• Baryonic Acoustic Oscillations via the Renormalization Group
• Dependence of the non-linear mass power spectrum on the equation of state of dark energy
• Predictions for Herschel from LambdaCDM: unveiling the cosmic star formation history
• Clustering of Dust-Obscured Galaxies at z ~ 2
• A bias to CMB lensing measurements from the bispectrum of large-scale structure
• Testing coupled dark energy with next-generation large-scale observations
• Tomography of the Fermi-LAT gamma-ray diffuse extragalactic signal via cross-correlations with galaxy catalogs
• Cosmological constraints from the CFHTLenS shear measurements using a new, accurate and flexible way of predicting nonlinear mass clustering
• Emulators for the non-linear matter power spectrum beyond $\Lambda$CDM
• HI and cosmological constraints from intensity mapping, optical, and CMB surveys
• The halo model in a massive neutrino cosmology
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• Lensing Bias in Cosmic Shear
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Constraining evolution in the Halo Model using galaxy redshift surveys
• Dark Neutrino interactions phase out the Hubble tension
• Constraining neutrino mass with tomographic weak lensing peak counts
• Cosmology with Doppler Lensing
• Full-sky lensing reconstruction of gradient and curl modes from CMB maps
• Constraining Modified Gravity and Growth with Weak Lensing
• Perturbative approach to covariance matrix of the matter power spectrum
• The Vainshtein Mechanism in the Cosmic Web
• Halo modelling in chameleon theories
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• Weak Lensing by Large-Scale Structure with the FIRST Radio Survey
• SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
• Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• Backreaction on the luminosity-redshift relation from gauge invariant light-cone averaging
• The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• An Enlarged Cosmic Shear Survey with the William Herschel Telescope
• Determining the Neutrino Mass Hierarchy with Cosmology
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• The Bispectrum of f(R) Cosmologies
• A Running Spectral Index in Supersymmetric Dark-Matter Models with Quasi-Stable Charged Particles
• Modeling the nonlinear clustering in modified gravity models I: A fitting formula for matter power spectrum of f(R) gravity
• Mapping the Real Space Distributions of Galaxies in SDSS DR7: II. Measuring the growth rate, clustering amplitude of matter and biases of galaxies at redshift $0.1$
• A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
• The Redshift-Space Cluster-Galaxy Cross-Correlation Function: I. Modeling Galaxy Infall onto Millennium Simulation Clusters and SDSS Groups
• Difficulties Distinguishing Dark Energy from Modified Gravity via Redshift Distortions
• Cosmic Shear Covariance Matrix in $w$CDM: Cosmology Matters
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• An Empirically-Calibrated Model For Interpreting the Evolution of Galaxies During the Reionization Era
• Accurate and Efficient Halo-based Galaxy Clustering Modelling with Simulations
• Banana Split: Testing the Dark Energy Consistency with Geometry and Growth
• On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
• Primordial non-Gaussianity without tails -- how to measure fNL with the bulk of the density PDF
• Fuzzy Dark Matter and the Dark Energy Survey Year 1 Data
• Planck Sunyaev-Zel'dovich Cluster Mass Calibration using Hyper Suprime-Cam Weak Lensing
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Prospects for Detecting Dark Matter Halo Substructure with Pulsar Timing
• Joint Measurement of Lensing-Galaxy Correlations Using SPT and DES SV Data
• On the contribution of fluorescence to Ly$\alpha$ halos (LAHs) around star forming galaxies
• The Impact of Intrinsic Alignments: Cosmological Constraints from a Joint Analysis of Cosmic Shear and Galaxy Survey Data
• On the insufficiency of arbitrarily precise covariance matrices: non-Gaussian weak lensing likelihoods
• The Benefits of CMB Delensing
• The nature of the unresolved extragalactic soft CXB
• Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
• How clustering dark energy affects matter perturbations
• Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
• The Correlation Between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe
• Cosmic variance of the galaxy cluster weak lensing signal
• The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies
• Biased Dark Energy Constraints from Neglecting Reduced Shear in Weak Lensing Surveys
• The Cosmic Thermal History Probed by Sunyaev-Zeldovich Effect Tomography
• On the connection between the intergalactic medium and galaxies: The HI-galaxy cross-correlation at z < 1
• Toward an accurate mass function for precision cosmology
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• Baryon impact on weak lensing peaks and power spectrum: low-bias statistics and self-calibration in future surveys
• Anisotropies of gravitational-wave standard sirens as a new cosmological probe without redshift information
• Beyond the Damping Tail: Cross-Correlating the Kinetic Sunyaev-Zel'dovich Effect with Cosmic Shear
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• The Clustering of High-Redshift (2.9 $\le$ z $\le$ 5.1) Quasars in SDSS Stripe 82
• Resolving Small-Scale Dark Matter Structures Using Multi-Source Indirect Detection
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
• Cosmological constraints on neutrino plus axion hot dark matter
• Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies
• An ideal mass assignment scheme for measuring the Power Spectrum with FFTs
• Linear perturbative theory of the discrete cosmological N-body problem
• Learning from the Scatter in Type Ia Supernovae
• The three dimensional power spectrum of dark and luminous matter from the VIRMOS-DESCART cosmic shear survey
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• Non-Gaussianity and the CMB Bispectrum: confusion between Primordial and Lensing-Rees Sciama contribution?
• Structure formation in cosmologies with oscillating dark energy
• Testing dark energy paradigms with weak gravitational lensing
• Cosmological Backreaction from Perturbations
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
• Fitting the nonlinear matter bispectrum by the Halofit approach
• A Unified Analysis of Four Cosmic Shear Surveys
• Non-detection of a statistically anisotropic power spectrum in large-scale structure
• The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions
• Halo-model Analysis of the Clustering of Photometrically Selected Galaxies from SDSS
• A Step in Understanding the $S_8$ Tension
• Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• On the road to percent accuracy II: calibration of the non-linear matter power spectrum for arbitrary cosmologies
• Precision reconstruction of the dark matter-neutrino relative velocity from N-body simulations
• Measurement of Cosmic Shear with the Space Telescope Imaging Spectrograph
• Bias to CMB Lensing Reconstruction from Temperature Anisotropies due to Large-Scale Galaxy Motions
• The ring statistics - how to separate E- and B-modes of cosmic shear correlation functions on a finite interval
• Angular Signatures of Annihilating Dark Matter in the Cosmic Gamma-Ray Background
• The non-Gaussianity of the cosmic shear likelihood - or: How odd is the Chandra Deep Field South?
• A Cosmic Coincidence: The Power-Law Galaxy Correlation Function
• Streaming velocities and the baryon-acoustic oscillation scale
• Unfolding the matter distribution using 3-D weak gravitational lensing
• Constraints on early dark energy from CMB lensing and weak lensing tomography
• Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• Combining Probes of Large-Scale Structure with CosmoLike
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• 3D Photometric Cosmic Shear
• Reducing Noise in Cosmological N-body Simulations with Neutrinos
• 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
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• Cosmic shear full nulling: sorting out dynamics, geometry and systematics
• Simulations of Wide-Field Weak Lensing Surveys II: Covariance Matrix of Real Space Correlation Functions
• A cross-correlation study of the Fermi-LAT $\gamma$-ray diffuse extragalactic signal
• Simulations of weak gravitational lensing
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• Unveiling the Dynamics of the Universe
• Clustering of quasars in a wide luminosity range at redshift 4 with Subaru Hyper Suprime-Cam wide field imaging
• Analytic Methods for Cosmological Likelihoods
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• PkANN - II. A non-linear matter power spectrum interpolator developed using artificial neural networks
• TheHaloMod: An online calculator for the halo model
• Probing cosmology with weak lensing selected clusters I: Halo approach and all-sky simulations
• A Large Sky Simulation of the Gravitational Lensing of the Cosmic Microwave Background
• Full-sky maps for gravitational lensing of the CMB
• The Born and Lens-Lens Corrections to Weak Gravitational Lensing Angular Power Spectra
• Calibration of the Mass-Temperature Relation for Clusters of Galaxies Using Weak Gravitational Lensing
• Baryonic effects on the matter bispectrum
• The nature of assembly bias - I. Clues from a LCDM cosmology
• Insights from probability distribution functions of intensity maps
• Impact of the non-Gaussian covariance of the weak lensing power spectrum and bispectrum on cosmological parameter estimation
• COSMOS: Stochastic bias from measurements of weak lensing and galaxy clustering
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Multitracer CMB delensing maps from Planck and WISE data
• CMB-lensing beyond the Born approximation
• The full squeezed CMB bispectrum from inflation
• Systematic effects in the sound horizon scale measurements
• Clustering of luminous red galaxies II: small scale redshift space distortions
• Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• CMB Lensing Beyond the Power Spectrum: Cosmological Constraints from the One-Point PDF and Peak Counts
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• The Mira-Titan Universe IV. High Precision Power Spectrum Emulation
• Dynamical Dark Energy simulations: high accuracy Power Spectra at high redshift
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: II. Fourier and Redshift Space
• Testing (modified) gravity with 3D and tomographic cosmic shear
• Intrinsic alignments in the cross-correlation of cosmic shear and CMB weak lensing
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Matter trispectrum: theoretical modelling and comparison to N-body simulations
• Cosmological constraints with weak lensing peak counts and second-order statistics in a large-field survey
• The Dark Energy Survey Year 3 and eBOSS: constraining galaxy intrinsic alignments across luminosity and colour space
• Towards quantitative control on discreteness error in the non-linear regime of cosmological N body simulations
• Complete Treatment of Galaxy Two-Point Statistics: Gravitational Lensing Effects and Redshift-Space Distortions
• Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias
• The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• The VLT LBG Redshift Survey I: Clustering and Dynamics of ~1000 Galaxies at z~3
• Weak Lensing and CMB: Parameter forecasts including a running spectral index
• Clipping the Cosmos: The Bias and Bispectrum of Large Scale Structure
• Substructure and the halo model of large-scale structure
• CFHTLS weak-lensing constraints on the neutrino masses
• Cosmological nonlinear hydrodynamics with post-Newtonian corrections
• The Asiago-ESO/RASS QSO Survey. III. Clustering analysis and its theoretical interpretation
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Cross-correlation between cosmic microwave background lensing and galaxy intrinsic alignment as a contaminant to gravitational lensing cross-correlated probes of the universe
• Spatial Correlation Function of X-ray Selected AGN
• 2dFLenS and KiDS: Determining source redshift distributions with cross-correlations
• QSO-LRG 2-Point Cross-Correlation Function and Redshift-Space Distorions
• Dark energy constraints from lensing-detected galaxy clusters
• Testing a new analytic model for gravitational lensing probabilities
• Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
• The nonlinear matter power spectrum
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• What is the best way to measure baryonic acoustic oscillations?
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• The mass density field in simulated non-Gaussian scenarios
• Clustering on very small scales from a large sample of confirmed quasar pairs: Does quasar clustering track from Mpc to kpc scales?
• Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey
• Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters
• Constraining interacting dark energy with CMB and BAO future surveys
• Including beyond-linear halo bias in halo models
• The Impact of Magnification and Size Bias on Weak Lensing Power Spectrum and Peak Statistics
• Wide-area tomography of CMB lensing and the growth of cosmological density fluctuations
• How robust are inflation model and dark matter constraints from cosmological data?
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• A Multi-Parameter Investigation of Gravitational Slip
• The matter power spectrum in redshift space using effective field theory
• Quantification of discreteness effects in cosmological N-body simulations: I. Initial Conditions
• PkANN - I. Non-linear matter power spectrum interpolation through artificial neural networks
• Measuring Galaxy Clustering and the Evolution of [CII] Mean Intensity with far-IR Line Intensity Mapping During 0.5 < z < 1.5
• Comments on the size of the simulation box in cosmological N-Body simulations
• Perturbation theory approach for the power spectrum: from dark matter in real space to massive haloes in redshift space
• Constraining Modified Gravity with Euclid
• Testing one-loop galaxy bias: Power spectrum
• Unscreening Modified Gravity in the Matter Power Spectrum
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• Probing decisive answers to dark energy questions from cosmic complementarity and lensing tomography
• Faint Submillimeter Galaxies identified through their optical/near-infrared colours I: spatial clustering and halo masses
• Cosmological constraints from the convergence 1-point probability distribution
• Growth of Cosmic Structure
• Constraining warm dark matter with cosmic shear power spectra
• Structure Formation in Modified Gravity Scenarios
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Cosmology with Equivalence Principle Breaking in the Dark Sector
• Effects of Unstable Dark Matter on Large-Scale Structure and Constraints from Future Surveys
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• What can be learned from the lensed cosmic microwave background B-mode polarization power spectrum?
• The Accuracy of Weak Lensing Simulations
• Search for features in the spectrum of primordial perturbations using Planck and other datasets
• Perturbation theory and excursion set estimates of the probability distribution function of dark matter, and a method for reconstructing the initial distribution function
• Weak lensing predictions for modified gravities at non-linear scales
• Beware of commonly used approximations I: errors in forecasts
• Discrepancies between CFHTLenS cosmic shear & Planck: new physics or systematic effects?
• Fast generation of ensembles of cosmological N-body simulations via mode-resampling
• Precision modelling of the matter power spectrum in a Planck-like Universe
• Probing dark energy and neutrino mass from upcoming lensing experiments of CMB and galaxies
• Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function
• Using dark energy to suppress power at small scales
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• Lensing Corrections to Features in the Angular Two-Point Correlation Function and Power Spectrum
• The one-loop matter bispectrum as a probe of gravity and dark energy
• A new method for the Alcock-Paczynski test
• Large-Scale Structure in Brane-Induced Gravity I. Perturbation Theory
• Shot noise and biased tracers: a new look at the halo model
• Consistent cosmic shear in the face of systematics: a B-mode analysis of KiDS-450, DES-SV and CFHTLenS
• Impact of shell crossing and scope of perturbative approaches in real and redshift space
• GaBoDS: The Garching-Bonn Deep Survey: VII. Probing galaxy bias using weak gravitational lensing
• Fast Estimation of Gravitational and Primordial Bispectra in Large Scale Structures
• SKA Weak Lensing II: Simulated Performance and Survey Design Considerations
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• The integrated 3-point correlation function of cosmic shear
• Going deep with Minkowski functionals of convergence maps
• Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing -- validation on cosmological simulations
• Can Early Dark Energy be Detected in Non-Linear Structure?
• Future weak lensing constraints in a dark coupled universe
• The Signature of Large Scale Structures on the Very High Energy Gamma-Ray Sky
• Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS and 2dFLenS
• A fast particle-mesh simulation of non-linear cosmological structure formation with massive neutrinos
• Large-scale inhomogeneities may improve the cosmic concordance of supernovae
• HerMES: detection of cosmic magnification of sub-mm galaxies using angular cross-correlation
• Accurate Analytic Model for the Weak Lensing Convergence One-Point Probability Distribution Function and its Auto-Covariance
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• Self calibration of photometric redshift scatter in weak lensing surveys
• A bias in cosmic shear from galaxy selection: results from ray-tracing simulations
• SUNGLASS: A new weak lensing simulation pipeline
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Testing standard perturbation theory and the Eulerian local biasing scheme against N-body simulations
• Evolution of the Dark Matter Distribution with 3-D Weak Lensing
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Unbiased clustering estimate with VIPERS slit assignment
• Dark Matter Gravitational Clustering With a Long-Range Scalar Interaction
• The 2dF QSO Redshift Survey - XV. Correlation analysis of redshift-Space distortions
• WFIRST Science Investigation Team "Cosmology with the High Latitude Survey" Annual Report 2017
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• Power spectrum tomography of dark matter annihilation with local galaxy distribution
• Imaging Systematics and Clustering of DESI Main Targets
• The Non-Linear Matter Power Spectrum in Warm Dark Matter Cosmologies
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• Power spectrum multipoles on the curved sky: an application to the 6-degree Field Galaxy Survey
• CMB-lensing beyond the leading order: temperature and polarization anisotropies
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• Effect of clustering on extragalactic source counts with low-resolution instruments
• Transverse Velocities with the Moving Lens Effect
• Constraining the Mass-Richness Relationship of redMaPPer Clusters with Angular Clustering
• How Late can the Dark Matter form in our universe?
• Projected Constraints on Modified Gravity Cosmologies from 21 cm Intensity Mapping
• Power Spectrum Estimation from Peculiar Velocity Catalogues
• Prospects for clustering and lensing measurements with forthcoming intensity mapping and optical surveys
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Revisiting CFHTLenS cosmic shear: Optimal E/B mode decomposition using COSEBIs and compressed COSEBIs
• CMB Lensing Bispectrum from Nonlinear Growth of the Large Scale Structure
• Cosmology with 6 parameters in the Stage-IV era: efficient marginalisation over nuisance parameters
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Accelerating Large-Scale-Structure data analyses by emulating Boltzmann solvers and Lagrangian Perturbation Theory
• Simultaneous constraints on the number and mass of relativistic species
• Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies
• Fingerprinting Dark Energy II: weak lensing and galaxy clustering tests
• Constraining Dark Energy Evolution with Gravitational Lensing by Large Scale Structures
• Constraining the initial conditions of the Universe using large scale structure
• Effects of the initial conditions on cosmological $N$-body simulations
• KiDS-450: Tomographic Cross-Correlation of Galaxy Shear with {\it Planck} Lensing
• DES Y1 Results: Validating cosmological parameter estimation using simulated Dark Energy Surveys
• Cosmological information in Gaussianised weak lensing signals
• The clustering of X-ray selected AGN at z=0.1
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• The HI content of dark matter halos at $z\approx 0$ from ALFALFA
• Free-Free Emission at Low Radio Frequencies
• COSMOS weak-lensing constraints on modified gravity
• Probing dark energy with tomographic weak-lensing aperture mass statistics
• Effects of baryons on weak lensing peak statistics
• Polarization as an indicator of intrinsic alignment in radio weak lensing
• Intrinsic alignment of redMaPPer clusters: cluster shape - matter density correlation
• Systematic corrections to the measured cosmological constant as a result of local inhomogeneity
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• Observational constraints on early dark energy
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• The REFLEX II galaxy cluster survey: power spectrum analysis
• Clustering of X-Ray-Selected AGN
• Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data
• Combining perturbation theories with halo models for the matter bispectrum
• Using the Zeldovich dynamics to test expansion schemes
• CLUMP-3D. Three dimensional lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster
• Probing the primordial Universe with MeerKAT and DES
• Integrated approach to cosmology: Combining CMB, large-scale structure and weak lensing
• Statistical modelling of the cosmological dispersion measure
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Tomographic analyses of the CMB lensing and galaxy clustering to probe the linear structure growth
• Equation of State of Dark Matter after Planck Data
• Magnification effect on the detection of primordial non-Gaussianity from photometric surveys
• Evolution of the Clustering of Photometrically Selected SDSS Galaxies
• Weak Lensing Observables in the Halo Model
• Extragalactic gamma-ray signal from Dark Matter annihilation: a power spectrum based computation
• Constraining Cosmology with High Convergence Regions in Weak Lensing Surveys
• Observational constraints on cosmic neutrinos and dark energy revisited
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Beyond the traditional Line-of-Sight approach of cosmological angular statistics
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Constraints on warm dark matter from weak lensing in anomalous quadruple lenses
• Propagators in Lagrangian space
• Characterizing the linear growth rate of cosmological density perturbations in an f(R) model
• What is half a neutrino? Reviewing cosmological constraints on neutrinos and dark radiation
• Precise Estimation of Cosmological Parameters Using a More Accurate Likelihood Function
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Are Light Sterile Neutrinos Preferred or Disfavored by Cosmology?
• Cosmological Constraints from the Large Scale Weak Lensing of SDSS MaxBCG Clusters
• Intensity mapping cross-correlations II: HI halo models including shot noise
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Magnification Bias Corrections to Galaxy-Lensing Cross-Correlations
• Dark energy imprints on the kinematic Sunyaev-Zel'dovich signal
• Measurement of the Cold Dark Matter-Neutrino Dipole in the TianNu Simulation
• Simulations of Galileon modified gravity: Clustering statistics in real and redshift space
• The Angular Power Spectra of Photometric SDSS LRGs
• Constraints on inflation with LSS surveys: features in the primordial power spectrum
• Machine Learning for Observational Cosmology
• The intergalactic medium temperature and Compton y parameter
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• MultiDarkLens Simulations: weak lensing light-cones and data base presentation
• Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys
• Forecasts of non-Gaussian parameter spaces using Box-Cox transformations
• The Correlated Formation Histories of Massive Galaxies and Their Dark Matter Halos
• Cosmic Shear Tomography and Efficient Data Compression using COSEBIs
• Detecting the relativistic galaxy bispectrum
• The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Interloper bias in future large-scale structure surveys
• Effect of lensing non-Gaussianity on the CMB power spectra
• The Copernican principle in light of the latest cosmological data
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
• Bispectrum covariance in the flat-sky limit
• Moving around the cosmological parameter space: a nonlinear power spectrum reconstruction based on high-resolution cosmic responses
• Fast Edge Corrected Measurement of the Two-Point Correlation Function and the Power Spectrum
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• A local measurement of the growth rate from peculiar velocities and galaxy clustering correlations in the 6dF Galaxy Survey
• Cosmology with Superluminous Supernovae
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Synergies between intensity maps of hydrogen lines
• Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments
• Is there evidence for anomalous dipole anisotropy in the large-scale structure?
• Cosmological Three-Point Function: Testing The Halo Model Against Simulations
• Confusion noise at far-IR to millimeter wavelengths
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• Information Gains from Cosmological Probes
• Impact of next-to-leading order contributions to CMB lensing
• Backreaction of Cosmological Perturbations in Covariant Macroscopic Gravity
• Intrinsic alignment contamination to CMB lensing-galaxy weak lensing correlations from tidal torquing
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• Expansion schemes for gravitational clustering: computing two-point and three-point functions
• From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Cosmic Structure Formation with Kinetic Field Theory
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
• PSF Anisotropy and Systematic Errors in Weak Lensing Surveys
• Model-independent curvature determination with 21cm intensity mapping experiments
• The squeezed matter bispectrum covariance with responses
• Extending the Coyote emulator to dark energy models with standard $w_0$-$w_a$ parametrization of the equation of state
• Testing gravity with $E_G$: mapping theory onto observations
• Analyzing the cosmic variance limit of remote dipole measurements of the cosmic microwave background using the large-scale kinetic Sunyaev Zel'dovich effect
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Reconstruction of the redshift-space galaxy density field
• What is the distance to the CMB?
• Comparison of weak lensing by NFW and Einasto halos and systematic errors
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Weak lensing shear and aperture-mass from linear to non-linear scales
• Galaxy Clustering and Dark Energy
• Deciphering the Archaeological Record: Cosmological Imprints of Non-Minimal Dark Sectors
• Towards accurate modelling of the ISW effect, the non-linear contribution
• Precision cosmology in muddy waters: Cosmological constraints and N-body codes
• Full-sky ray-tracing simulation of weak lensing using ELUCID simulations: exploring galaxy intrinsic alignment and cosmic shear correlations
• Power Spectra to 1% Accuracy between Dynamical Dark Energy Cosmologies
• Non-linear matter power spectrum from Time Renormalisation Group: efficient computation and comparison with one-loop
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• Disentangling Dark Physics with Cosmic Microwave Background Experiments
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• Power spectrum for the small-scale Universe
• Probing Early Modification of Gravity with Planck, ACT and SPT
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Modeling Extragalactic Foregrounds and Secondaries for Unbiased Estimation of Cosmological Parameters From Primary CMB Anisotropy
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• Disentangling dark sector models using weak lensing statistics
• On the current status of Modified Gravity
• Weak lensing statistics from the Coyote Universe
• Luminous Red Galaxy Clustering at z~0.7 - First Results using AAOmega
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Weak lensing by galaxy troughs with modified gravity
• Improving PSF modelling for weak gravitational lensing using new methods in model selection
• Modeling the Phase-Space Distribution around Massive Halos
• Remapping dark matter halo catalogues between cosmological simulations
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• The OH line contamination of 21 cm intensity fluctuation measurements for z=1~4
• Tomographic weak lensing shear spectra from large N-body and hydrodynamical simulations
• Multi-Fidelity Emulation for the Matter Power Spectrum using Gaussian Processes
• Three-Point Correlations in f(R) Models of Gravity
• Testing gravity with galaxy-galaxy lensing and redshift-space distortions using CFHT-Stripe 82, CFHTLenS and BOSS CMASS datasets
• Flat-Sky Pseudo-Cls Analysis for Weak Gravitational Lensing
• Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared
• On the information content of the matter power spectrum
• Constraint on $f(R)$ Gravity through the Redshift Space Distortion
• Fast Weak Lensing Simulations with Halo Model
• Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
• Kinetic Sunyaev-Zeldovich effect in modified gravity
• The dark flow induced small scale kinetic Sunyaev Zel'dovich effect
• Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey
• Probing dark energy models with extreme pairwise velocities of galaxy clusters from the DEUS-FUR simulations
• The COS Absorption Survey of Baryon Harbors: The Galaxy Database and Cross-Correlation Analysis of OVI Systems
• Inhomogeneous systematic signals in cosmic shear observations
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Lensed CMB temperature and polarization maps from the Millennium Simulation
• Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
• Weak Lensing by Line-of-sight Halos as the Origin of Flux-ratio Anomalies in Quadruply Lensed QSOs
• Stacked Weak Lensing Mass Calibration: Estimators, Systematics, and Impact on Cosmological Parameter Constraints
• Power spectrum modelling of galaxy and radio intensity maps including observational effects
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• Testing gravity on cosmological scales with cosmic shear, cosmic microwave background anisotropies, and redshift-space distortions
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Contamination of early-type galaxy alignments to galaxy lensing-CMB lensing cross-correlation
• Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors
• Behavioural Movement Strategies in Cyclic Models
• Hunting down systematics in baryon acoustic oscillations after cosmic high noon
• KiDS-450: Enhancing cosmic shear with clipping transformations
• Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• The integrated Sachs-Wolfe effect in cosmologies with coupled dark matter and dark energy
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field
• Cross-correlation cosmic shear with the SDSS and VLA FIRST surveys
• Fast Generation of Covariance Matrices for Weak Lensing
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Enhancement of gravitational waves at Q-ball decay including non-linear density perturbations
• Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82
• Measuring the geometry of the Universe in the presence of isocurvature modes
• Multiple Lensing of the Cosmic Microwave Background anisotropies
• Non-linear weak lensing forecasts
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• A new cosmic shear function: Optimised E-/B-mode decomposition on a finite interval
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• Halo model prediction of the cosmic magnification statistics: the full non-linear contribution
• Going Nonlinear with Dark Energy Cosmologies
• The Effect of Large-Scale Structure on the Magnification of High-Redshift Sources by Cluster-Lenses
• Intelligent Design: On the Emulation of Cosmological Simulations
• On the validity of the Born approximation for weak cosmic flexions
• Monte Carlo Control Loops for cosmic shear cosmology with DES Year 1
• Signatures of First Stars in Galaxy Surveys: Multi-Tracer Analysis of the Supersonic Relative Velocity Effect and the Constraints from the BOSS Power Spectrum Measurements
• Non-Gaussian errors of baryonic acoustic oscillations
• Covariance matrices for halo number counts and correlation functions
• Disentangling dark energy and cosmic tests of gravity from weak lensing systematics
• Tomographic imaging of the Fermi-LAT gamma-ray sky through cross-correlations: A wider and deeper look
• Higher Order Statistics for Three-dimensional Shear and Flexion
• An optimal survey geometry of weak lensing survey: minimizing super-sample covariance
• Measurement of a Cosmographic Distance Ratio with Galaxy and CMB Lensing
• Cosmic Shear as a Probe of Galaxy Formation Physics
• 3D galaxy clustering with future wide-field surveys: Advantages of a spherical Fourier-Bessel analysis
• Subhaloes in Scale-Free Cosmologies
• DM haloes in the fifth-force cosmology
• Improved Mixed Dark Matter Halo Model for Ultralight Axions
• Three-point phase correlations: A new measure of non-linear large-scale structure
• Precision growth index using the clustering of cosmic structures and growth data
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Weak Lensing Peak Finding: Estimators, Filters, and Biases
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• Quantifying resolution in cosmological N-body simulations using self-similarity
• The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Measuring Coherent Motions in the Universe
• Baryon Pasting Algorithm: Halo-based and Particle-based Pasting Methods
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Measuring Unified Dark Matter with 3D Cosmic Shear
• Measuring the transition to homogeneity with photometric redshift surveys
• The Subaru FMOS galaxy redshift survey (FastSound). V. Intrinsic alignments of emission line galaxies at $z\sim 1.4$
• Constraining the dark energy dynamics with the cosmic microwave background bispectrum
• Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Non-linear relativistic contributions to the cosmological weak-lensing convergence
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
• A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear Surveys
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Probing Dark Energy with Baryonic Acoustic Oscillations at High Redshifts
• Constraining neutrino masses with the ISW-galaxy correlation function
• Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
• Measurement of the integrated Sachs-Wolfe effect using the AllWISE data release
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• Modified Gravity: the CMB, Weak Lensing and General Parameterisations
• Debiasing inference with approximate covariance matrices and other unidentified biases
• Cosmology with Standard Sirens: the Importance of the Shape of the Lensing Magnification Distribution
• Changes in the halo formation rates due to features in the primordial spectrum
• Gravitational Dynamics of an Infinite Shuffled Lattice of Particles
• Effects of halo substructure on the power spectrum and bispectrum
• Peculiar Velocities into the Next Generation: Cosmological Parameters From Large Surveys without Bias from Nonlinear Structure
• Angular ellipticity correlations in a composite alignment model for elliptical and spiral galaxies and inference from weak lensing
• From linear to non-linear scales: analytical and numerical predictions for the weak lensing convergence
• Galaxy-galaxy weak gravitational lensing in $f(R)$ gravity
• The Impact of Nonlinear Structure Formation on the Power Spectrum of Transverse Momentum Fluctuations and the Kinetic Sunyaev-Zel'dovich Effect
• Fourier Band-Power E/B-mode Estimators for Cosmic Shear
• Consistency of cosmic shear analyses in harmonic and real space
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• Impact of Dark Matter Substructure on the Matter and Weak Lensing Power Spectra
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• The FLAMINGO project: Baryon effects on the matter power spectrum
• Will Multiple Probes of Dark Energy find Modified Gravity?
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• Detecting Dark Matter Substructures on Small Scales with Fast Radio Bursts
• An alternative to grids and glasses: Quaquaversal pre-initial conditions for N-body simulations
• The galaxy-galaxy lensing contribution to the cosmic shear two point function
• Cross-correlation of WMAP7 and the WISE Full Data Release
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• How well can (renormalized) perturbation theory predict dark matter clustering properties?
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• Peculiar velocities into the next generation: cosmological parameters from the SFI++ survey
• Precision Prediction for the Cosmological Density Distribution
• The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
• A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond
• A hierarchical field-level inference approach to reconstruction from sparse Lyman-$\alpha$ forest data
• RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• Barry and the BAO Model Comparison
• Precision Prediction of the Log Power Spectrum
• Dark Energy from the log-transformed convergence field
• A Semi-analytic Ray-tracing Algorithm for Weak Lensing
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• Crawling the Cosmic Network: Exploring the Morphology of Structure in the Galaxy Distribution
• Efficient calculation of cosmological neutrino clustering with both linear and non-linear gravity
• Weak lensing of large scale structure in the presence of screening
• The Clustering of X-ray Luminous Quasars
• Hierarchy in the Phase Space and Dark Matter Astronomy
• Cosmological gravity on all scales: simple equations, required conditions, and a framework for modified gravity
• Weak lensing tomography with orthogonal polynomials
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
• Fitting and forecasting non-linear coupled dark energy
• On the degeneracy between baryon feedback and massive neutrinos as probed by matter clustering and weak lensing
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• Galaxy Peculiar Velocities From Large-Scale Supernova Surveys as a Dark Energy Probe
• Understanding the faint red galaxy population using large-scale clustering measurements from SDSS DR7
• Improved constraints on reionisation from CMB observations: A parameterisation of the kSZ effect
• Perturbation theory with dispersion and higher cumulants: non-linear regime
• CFHTLenS: A Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics
• What do cluster counts really tell us about the Universe?
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• General Modified Gravity With 21cm Intensity Mapping: Simulations and Forecast
• Universal Merger Histories of Dark-Matter Haloes
• Constraining primordial non-Gaussianity by combining next-generation galaxy and 21 cm intensity mapping surveys
• Effect of Measurement Errors on Predicted Cosmological Constraints from Shear Peak Statistics with LSST
• Cosmic variance of $H_0$ in light of forthcoming high-redshift surveys
• Controlling intrinsic-shear alignment in three-point weak lensing statistics
• The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• Precision of diffuse 21-cm lensing
• Nonlinear modulation of the HI power spectrum on ultra-large scales. I
• Weak Gravitational Lensing as a Method to Constrain Unstable Dark Matter
• The nonlinear power spectrum in clustering quintessence cosmologies
• Weak gravitational lensing of intrinsically aligned galaxies
• Halo collapse: virialization by shear and rotation in dynamical dark-energy models. Effects on weak-lensing peaks
• Constraints on the growth rate using the observed galaxy power spectrum
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• Modelling the matter bispectrum at small scales in modified gravity
• Constraining gravity at large scales with the 2MASS Photometric Redshift catalogue and Planck lensing
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• A new model framework for circumgalactic Ly$\alpha$ radiative transfer constrained by galaxy-Ly$\alpha$ forest clustering
• Enhancing cosmic shear with the multi-scale lensing PDF
• The clustering of baryonic matter. I: a halo-model approach
• Cross-correlating 2D and 3D galaxy surveys
• Out-of-Core Hydrodynamic Simulations for Cosmological Applications
• Estimating the weak-lensing rotation signal in radio cosmic shear surveys
• Photometric Selection of Emission Line Galaxies, Clustering Analysis and a Search for the ISW effect
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• A hybrid approach to CMB lensing reconstruction on all-sky intensity maps
• The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2\le z<1$ by PDF analysis
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• Smooth Particle Lensing
• A precise symbolic emulator of the linear matter power spectrum
• Growth index of matter perturbations in the light of Dark Energy Survey
• Integrated Cosmological Probes: Extended Analysis
• SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) IV: Spatial clustering and halo masses of 450-$\mu$m-selected sub-millimeter galaxies
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Testing PSF Interpolation In Weak Lensing With Real Data
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• Measurement of Redshift Space Power Spectrum for BOSS galaxies and the Growth Rate at redshift 0.57
• Weak Lensing of Baryon Acoustic Oscillations
• Testing dark energy using pairs of galaxies in redshift space
• Cosmic Microwave Background--Weak Lensing Correlation: Analytical and Numerical Study of Non-linearity and Implications for Dark Energy
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• Characterizing unknown systematics in large scale structure surveys
• Nonlinearities in modified gravity cosmology I: signatures of modified gravity in the nonlinear matter power spectrum
• Tracing the cosmological evolution of stars and cold gas with CMB spectral surveys
• Color Tomography
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• Markov-chain reconstruction of the 2dF Galaxy Redshift Survey real-space power spectrum
• Born-corrections to weak lensing of the cosmic microwave background temperature and polarisation anisotropies
• Extending Recovery of the Primordial Matter Power Spectrum
• Halo Occupation Distribution of Massive Galaxies since z = 1
• Measuring weak lensing correlations of Type Ia Supernovae
• Searching for anisotropic stochastic gravitational-wave backgrounds with constellations of space-based interferometers
• Modeling of weak lensing statistics. I. Power spectrum and bispectrum
• Theoretical and numerical perspectives on cosmic distance averages
• Toward understanding the anisotropic point spread function of Suprime-Cam and its impact on cosmic shear measurement
• Evolution of the Cosmological Density Distribution Function: A New Analytical Model
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• Weak Lensing by Intergalactic Mini-Structures in Quadruple Lens Systems: Simulation and Detection
• Raytracing simulations of coupled dark energy models
• Evolution of isolated overdensities as a control on cosmological N body simulations
• Optimising cosmic shear surveys to measure modifications to gravity on cosmic scales
• Halo-Galaxy Lensing: A Full Sky Approach
• Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys
• Non-linear gravitational clustering of cold matter in an expanding universe: indications from 1D toy models
• Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy
• Constraining the primordial power spectrum from SNIa lensing dispersion
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Utilizing Type Ia Supernovae in a Large, Fast, Imaging Survey to Constrain Dark Energy
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Scale Transformations, Tree-level Perturbation Theory, and the Cosmological Matter Bispectrum
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Estimating Cosmological Parameters from the Dark Matter Distribution
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Fast estimation of aperture mass statistics II: Detectability of higher order statistics in current and future surveys
• Detecting Cosmic Strings with Lensed Fast Radio Bursts
• Analytical marginalisation over photometric redshift uncertainties in cosmic shear analyses
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• 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
• Evolution of skewness and kurtosis of cosmic density fields
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• The clustering of X-ray AGN at 0.5 < z < 4.5: host galaxies dictate dark matter halo mass
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• The dipole anisotropy of WISE x SuperCOSMOS number counts
• Analytical halo model of galactic conformity
• Time of flight of ultra-relativistic particles in a realistic Universe: a viable tool for fundamental physics?
• Revisiting the matter power spectra in $f(R)$ gravity
• Forecasting neutrino masses from galaxy clustering in the Dark Energy Survey combined with the Planck Measurements
• The Adaptive TreePM: An Adaptive Resolution Code for Cosmological N-body Simulations
• The cross-correlation between 3d cosmic shear and the integrated Sachs-Wolfe effect
• The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ~0.7
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Redshift-space correlation functions in large galaxy cluster surveys
• Parameter likelihood of intrinsic ellipticity correlations
• Exponents of non-linear clustering in scale-free one dimensional cosmological simulations
• Matter power spectra in dynamical-Dark Energy cosmologies
• Effect of Mask Regions on Weak Lensing Statistics
• Constraining Light Gravitino Mass from Cosmic Microwave Background
• Detecting Baryon Acoustic Oscillations
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Cosmologically probing ultra-light particle dark matter using 21 cm signals
• Normalization of the Matter Power Spectrum via Higher-Order Angular Correlations of Luminous Red Galaxies
• Large-scale Velocities and Primordial Non-Gaussianity
• Weak Lensing Science, Surveys, and Systematics
• A New Data Compression Method and its Application to Cosmic Shear Analysis
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Galaxy bias from galaxy-galaxy lensing in the DES Science Verification Data
• A Halo Model with Environment Dependence: Theoretical Considerations
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Structure formation in $f(R)$ gravity: A distinguishing probe between the dark energy and modified gravity
• Simulating the Effect of Non-Linear Mode-Coupling in Cosmological Parameter Estimation
• Matter bispectrum of large-scale structure with Gaussian and non-Gaussian initial conditions: Halo models, perturbation theory, and a three-shape model
• Herschel-ATLAS : The spatial clustering of low and high redshift submillimetre galaxies
• Geometry and growth contributions to cosmic shear observables
• The clustering of baryonic matter. II: halo model and hydrodynamic simulations
• Transitioning from Stage-III to Stage-IV: Cosmology from galaxy$\times$CMB lensing and shear$\times$CMB lensing
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Testing the tensor-vector-scalar Theory with the latest cosmological observations
• Linear and non-linear perturbations in dark energy models
• On Mitigation of the Uncertainty in Nonlinear Matter Clustering for Cosmic Shear Tomography
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Measuring the scale dependence of intrinsic alignments using multiple shear estimates
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Spatial matter density mapping of the STAGES Abell A901/2 supercluster field with 3D lensing
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Variations of cosmic large-scale structure covariance matrices across parameter space
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Primordial Non-Gaussianity and the Statistics of Weak Lensing and other Projected Density Fields
• Universal Weak Lensing Distortion of Cosmological Correlation Functions
• The Atacama Cosmology Telescope: limits on dark matter-baryon interactions from DR4 power spectra
• Tomographic local 2D analyses of the WISExSuperCOSMOS all-sky galaxy catalogue
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Using machine learning to compress the matter transfer function $T(k)$
• Describing variations of the Fisher-matrix across parameter space
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Retrieving the three-dimensional matter power spectrum and galaxy biasing parameters from lensing tomography
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Detection of cross-correlation between CMB Lensing and low-density points
• The Dark Matter Haloes and Host Galaxies of MgII Absorbers at z~1
• Interpolating Masked Weak Lensing Signal with Karhunen-Loeve Analysis
• CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• Good and Proper: Self-similarity of N-body Simulations with Proper Force Softening
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• Shear and magnification angular power spectra and higher-order moments from weak gravitational lensing
• Fully relativistic treatment of decaying cold dark matter in $N$-body simulations
• Constraining f(R) gravity with cross-correlation of galaxies and cosmic microwave background lensing
• Linear Systematics Mitigation in Galaxy Clustering in the Dark Energy Survey Year 1 Data
• Parameter constraints from weak lensing tomography of galaxy shapes and cosmic microwave background fluctuations
• Growth of non-linear structures and spherical collapse in the Galileon Ghost Condensate model
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Deep+Wide Lensing Surveys will Provide Exquisite Measurements of the Dark Matter Halos of Dwarf Galaxies
• Weak lensing power spectrum reconstruction by counting galaxies.-- I: the ABS method
• Nonlinear effects of dark energy clustering beyond the acoustic scales
• Imprint of non-linear effects on HI intensity mapping on large scales
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• How accurate is our knowledge of galaxy bias?
• Cosmic Microwave Background Bispectrum from the Lensing--Rees-Sciama Correlation Reexamined: Effects of Non-linear Matter Clustering
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• The Impact of Anisotropic Redshift Distributions on Angular Clustering
• A physical and concise halo model based on the depletion radius
• Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
• Application of cross correlations between CMB and large scale structure to constraints on the primordial non-Gaussianity
• Transient Weak-Lensing by Cosmological Dark Matter Microhaloes
• Comparing cosmic shear measures - Optimizing the Information content of cosmic shear data vectors
• A theoretical estimate of intrinsic ellipticity bispectra induced by angular momenta alignments
• Effects of NII and H$\alpha$ Line Blending on the WFIRST Galaxy Redshift Survey
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• The Multi-Tracer Optimal Estimator applied to VIPERS
• Baryonic feedback measurement from KV450 cosmic shear analysis
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Measuring cosmic shear with the ring statistics
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Accuracy requirements on intrinsic alignments for Stage-IV cosmic shear
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• Mass-varying neutrino in light of cosmic microwave background and weak lensing
• Forecasting the power of Higher Order Weak Lensing Statistics with automatically differentiable simulations
• Ellipsoidal collapse and the redshift space probability distribution function of dark matter
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Mixed three-point correlation functions of the nonlinear integrated Sachs-Wolfe effect and their detectability
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Combining spectroscopic and photometric surveys using angular cross-correlations I: Algorithm and modelling
• Unveiling cosmological information on small scales with line intensity mapping
• Detectability of Weak Lensing Modifications under Galileon Theories
• Euclid: Covariance of weak lensing pseudo-$C_{\ell }$ estimates. Calculation, comparison to simulations, and dependence on survey geometry
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Constraining low redshift [CII] Emission by Cross-Correlating FIRAS and BOSS Data
• Improving three-dimensional mass mapping with weak gravitational lensing using galaxy clustering
• Angular momentum evolution of stellar disks at high redshifts
• The ALHAMBRA survey : Estimation of the clustering signal encoded in the cosmic variance
• Optimising Spectroscopic and Photometric Galaxy Surveys: Same-sky Benefits for Dark Energy and Modified Gravity
• Uneven flows: On cosmic bulk flows, local observers, and gravity
• Lensing smoothing of BAO wiggles
• The adhesion model as a field theory for cosmological clustering
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
• A Clipping Method to Mitigate the Impact of Catastrophic Photometric Redshift Errors on Weak Lensing Tomography
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• Gravitational Collapse of Baryonic and Dark matter
• Redshift space distortions in the presence of non-minimally coupled dark matter
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• The ALHAMBRA survey: evolution of galaxy spectral segregation
• Constraints on neutrino masses from the lensing dispersion of Type Ia supernovae
• Designing Weak Lensing Surveys: A Generalised Eigenmode Analysis
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• RCSLenS: A new estimator for large-scale galaxy-matter correlations
• Evidence of dark energy in different cosmological observations
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Galaxy blending effects in deep imaging cosmic shear probes of cosmology
• The Integrated Sachs-Wolfe Effect in the Bulk Viscous Dark Energy Model
• The statistics of peaks of weakly non-Gaussian random fields: Effects of bispectrum in two- and three-dimensions
• Equilibrium configuration of perfect fluid orbiting around black holes in some classes of alternative gravity theories
• Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy
• Cosmological N-body simulations with generic hot dark matter
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• Correlation function of quasars in real and redshift space from the Sloan Digital Sky Survey Data Release 7
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Non-Gaussian forecasts of weak lensing with and without priors
• Gravitational lensing of the cosmic microwave background by nonlinear structures
• Remapping simulated halo catalogues in redshift space
• The contribution of star-forming galaxies to fluctuations in the cosmic background light
• Locating the Baryon Acoustic Peak
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• Cross-correlating Sunyaev-Zel'dovich and Weak Lensing Maps
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Halo Mass-Concentration Relation at High-Mass End
• Accuracy of power spectra in dissipationless cosmological simulations
• Uncertainties in the S-Z selected cluster angular power spectrum
• Massive Neutrinos in Cosmology
• Weak Lensing of Type Ia Supernovae from the Dark Energy Survey
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• A cross-correlation analysis of CMB lensing and radio galaxy maps
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• A closer look at dark photon explanations of the excess radio background
• Exploring neutrino interactions in light of present and upcoming galaxy surveys
• The cosmic shear three-point functions
• Fast likelihood-free inference in the LSS Stage IV era
• Gravitational collapse in an expanding background and the role of substructure II: Excess power at small scales and its effect of collapse of structures at larger scales
• A Modified TreePM Code
• Parameter estimation biases due to contributions from the Rees-Sciama effect to the integrated Sachs-Wolfe spectrum
• Non-Gaussian error bars in galaxy surveys -- II
• Probing the Cosmological Principle with weak lensing shear
• Skewness as a probe of Baryon Acoustic Oscillations
• Forecast of cross-correlation of CSST cosmic shear tomography with AliCPT-1 CMB lensing
• The bispectrum covariance beyond Gaussianity: A log-normal approach
• Line-of-sight Elongation and Hydrostatic Mass Bias of the Frontier Fields Galaxy Cluster Abell 370
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Skewing the CMB$\times$LSS: a Fast Method for Bispectrum Analysis
• Modeling of weak lensing statistics. II. Configuration-space statistics
• Cosmic Shear E/B-mode Estimation with Binned Correlation Function Data
• Lightcone Averaging and Precision Cosmology
• CUBE -- Towards an Optimal Scaling of Cosmological N-body Simulations
• Photo-z Quality Cuts and their Effect on the Measured Galaxy Clustering
• Gravitationally induced particle production and its impact on structure formation
• Cosmology with Weak Lensing Surveys
• Lensing dispersion of supernova flux: a probe of nonlinear structure growth
• Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data
• Clustering and descendants of MUSYC galaxies at z<1.5
• Forecasts of cosmological constraints from Type Ia supernovae including the weak-lensing convergence
• Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure
• Cell Count Moments in the Halo Model
• Neutrino Masses, Scale-Dependent Growth, and Redshift-Space Distortions
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• Gravitational Lensing Effects on the Baryonic Acoustic Oscillation Signature in the Redshift-Space Correlation Function
• Radio-optical synergies at high redshift to constrain primordial non-Gaussianity
• Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies
• Imprints of dynamical dark energy on weak-lensing measurements
• The non-linear evolution of bispectrum from the scale-free N-body simulation
• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Color dependence of clustering of massive galaxies at 0.5$\le z\le$2.5: similar spatial distributions between green valley galaxies and AGNs
• Evolution of intrinsic ellipticity correlations due to peculiar motion
• Constraining Warm Dark Matter with high-$z$ supernova lensing
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• Constraints on primordial non-Gaussianity from Galaxy-CMB lensing cross-correlation
• Cosmological evolution of the gravitational entropy of the large-scale structure
• Solar System-scale interferometry on fast radio bursts could measure cosmic distances with sub-percent precision
• Weak lensing ellipticities in a strong lensing regime
• Gravitational collapse in an expanding background and the role of substructure I: Planar collapse
• Statistical separation of weak gravitational lensing and intrinsic ellipticities based on galaxy colour information
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• GEO-FPT: a model of the galaxy bispectrum at mildly non-linear scales
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• High-redshift cosmology with oxygen lines from H$\alpha$ surveys
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• A Systematic Study of Projection Biases in Weak Lensing Analysis
• Power Spectrum Precision for Redshift Space Distortions
• Probe combination in large galaxy surveys : Application of Fisher information and Shannon entropy to weak lensing
• Optimising tomography for weak gravitational lensing surveys
• Intrinsic size correlations in weak lensing
• Constraints on non-thermal Dark Matter from Planck lensing extraction
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Cosmological Leverage from the Matter Power Spectrum in the Presence of Baryon and Nonlinear Effects
• Stable clustering and the resolution of dissipationless cosmological N-body simulations
• Numerical convergence of pre-initial conditions on dark matter halo properties
• The Evolution of Early-type Galaxies Selected by Their Spatial Clustering
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Thawing k-essence dark energy in the PAge space
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• Bayesian model selection for dark energy using weak lensing forecasts
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• Redshift distortions in one-dimensional power spectra
• Weighing the Light Gravitino Mass with Weak Lensing Surveys
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• Euclid preparation. Sensitivity to non-standard particle dark matter model
• Estimating small angular scale CMB anisotropy with high resolution N-body simulations: weak lensing
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Probing the Neutrino Mass through the Cross Correlation between the Rees-Sciama Effect and Weak Lensing
• Accurate relativistic observables from post-processing light cone catalogues
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum
• Complementarity of Future Dark Energy Probes
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• Forward modelling of quasar light curves and the cosmological matter power spectrum on milliparsec scales
• Full-Sky Lensing Reconstruction of 21 cm Intensity Maps
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Effects of Redshift Uncertainty on Cross-Correlations of CMB Lensing and Galaxy Surveys
• High accuracy power spectra including baryonic physics in dynamical Dark Energy models
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• Strong lensing time delay: a new way of measuring cosmic shear
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra
• Spectra of dynamical Dark Energy cosmologies from constant-w models
• Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario
• The Cosmic Mach Number: Comparison from Observations, Numerical Simulations and Nonlinear Predictions
• Cross-correlation cosmography with HI intensity mapping
• Kinetic Field Theory: Cosmic Structure Formation and Fluctuation-Dissipation Relations
• A possible explanation of vanishing halo velocity bias
• Fitting functions on the cheap: the relative nonlinear matter power spectrum
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Gravitational Collapse in an Expanding Universe: Scaling Relations for Two-Dimensional Collapse Revisited
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• Self-Similarity of $k$-Nearest Neighbor Distributions in Scale-Free Simulations
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• A Forecast for Large Scale Structure Constraints on Horndeski Gravity with Line Intensity Mapping
• Cosmological inference including massive neutrinos from the matter power spectrum: biases induced by uncertainties in the covariance matrix
• Quasi-2D Weak Lensing Cosmological Constraints Using the PDF-SYM method
• Weak gravitational lensing
• Dynamics of pairwise motions in the fully non-linear regime in LCDM and Modified Gravity cosmologies
• Sloshing and spiral structures breeding a putative radio mini-halo in the environment of a cool-core cluster Abell 795
• Tele-Correlation: Calibrating Shear-Shear Correlation with Real Data
• Einasto profile as the halo model solution coupled to the depletion radius
• The Beylkin-Cramer Summation Rule and A New Fast Algorithm of Cosmic Statistics for Large Data Sets
• Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• The SDSS DR7 Galaxy Angular Power Spectrum: Volume-Limits and Galaxy Morphology
• Weak lensing forecasts for dark energy, neutrinos and initial conditions
• Calibrating baryonic effects in cosmic shear with external data in the LSST era
• The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Intrinsic correlations of galaxy sizes in a hydrodynamical cosmological simulation
• Bayesian analysis of cosmic structures
• Sample variance in N--body simulations and impact on tomographic shear predictions
• Fitting formulae of the reduced-shear power spectrum for weak lensing
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• Improved Halo Model Calibrations for Mixed Dark Matter Models of Ultralight Axions
• Cosmological Perturbation Theory as a Tool for Estimating Box-Scale Effects in N-body Simulations
• Fourier imaging of non-linear structure formation
• Diagnosing multiplicative error by lensing magnification of type Ia supernovae
• Fast simulation mapping: from standard to modified gravity cosmologies using the bias assignment method
• The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
• The impact of super-survey modes on cosmological constraints from cosmic shear fields
• Origin of Metals around Galaxies I: Catalogs of Metal-line Absorption Doublets from High-Resolution Quasar Spectra
• Optimizing the Recovery of Fisher Information in the Dark Matter Power Spectrum
• Bayesian analysis of spatially distorted cosmic signals from Poissonian data
• Prospects for measuring neutrino mass with 21-cm forest
• Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys
• Prospects for cosmic magnification measurements using HI intensity mapping
• Modelling the impact of intrinsic size and luminosity correlations on magnification estimation
• Data Compression and Covariance Matrix Inspection: Cosmic Shear
• KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing
• DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Simulating the epoch of Helium Reionization in photon-conserving semi-numerical code SCRIPT
• Multi-tracing the primordial Universe with future surveys
• Self-calibrating BAO measurements in the presence of Small Displacement Interlopers
• Future constraints on variations of the fine structure constant from combined CMB and weak lensing measurements
• Weak Lensing Reconstruction by Counting DECaLS Galaxies
• A frequentist view on the two-body decaying dark matter model
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Cosmic flexion
• Geometrical constraints on curvature from galaxy-lensing cross-correlations
• Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency
• Intrinsic and extrinsic gravitational flexions
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• Gaussbock: Fast parallel-iterative cosmological parameter estimation with Bayesian nonparametrics
• Predicting the Sufficient-Statistics Power Spectrum for Galaxy Surveys: A Recipe for $P_{A\ast }(k)$
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• Neutrino physics from future weak lensing surveys
• Cosmological constraints from galaxy clustering
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• Gravitational stability of dark energy in galaxies and clusters of galaxies
• Kinetic field theory: Non-linear cosmic power spectra in the mean-field approximation
• Precision Cosmology and Hubble tension in the era of LSS surveys
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Mildly mixed coupled models vs. WMAP7 data
• Covariance of the One-Dimensional Mass Power Spectrum
• Cosmological Implications of a Neutrino Mass Detection
• Self-similarity and stable clustering in a family of scale-free cosmologies
• Scalar-field quintessence by cosmic shear: CFHT data analysis and forecasts for DUNE
• Constraining Recent Oscillations in Quintessence Models with Euclid
• Impact of reproduction-mobility trade-off on biodiversity in rock-paper-scissors models in changing environmental conditions
• Introduction to Higher Order Spatial Statistics in Cosmology
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Cosmological Constraints on Neutrino Masses in a Second-Order CPL Dark Energy Model
• Linear and non-linear Modified Gravity forecasts with future surveys
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Large-scale structure and the intrinsic alignment of galaxies
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• On the origin of transient features in cosmological N-Body Simulations
• Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-Power Spectrum
• Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics
• oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization
• An Optimally Weighted Estimator of the Linear Power Spectrum Disentangling the Growth of Density Perturbations Across Galaxy Surveys
• Estimating power spectrum of discrete cosmic momentum field with fast Fourier transform
• Non-screening of the Cosmological Background in K-mouflage modified gravity
• A systematic study of projection biases in the Weak Lensing analysis of cosmic shear and the combination of galaxy clustering and galaxy-galaxy lensing
• KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
• Gravity heats the Universe
• Non-linear structure formation in the "Running FLRW" cosmological model
• Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
• AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
• Intrinsic alignment boosting: Direct measurement of intrinsic alignments in cosmic shear data
• Cosmic shear beyond 2-point statistics: Accounting for galaxy intrinsic alignment with projected tidal fields
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Cosmic magnification on high-redshift submillimeter galaxies
• Massive neutrinos and interacting dark matter look alike through the lens of lensing
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• Power Spectrum Emulators from Neural Networks and Tree-Based Methods
• Etherington duality breaking: gravitational lensing in non-metric spacetimes versus intrinsic alignments
• Exploring Inflationary Initial State With Large Scale Structure Observations
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Weak lensing deflection of three-point correlation functions
• Multi-wavelength spectroscopic probes: prospects for primordial non-Gaussianity and relativistic effects
• Cosmology with Gravitational Lensing
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• Clustering of the extreme: A theoretical description of weak lensing critical points power spectra in the mildly nonlinear regime
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• Universality of the halo mass function in modified gravity cosmologies
• Cosmic Dipoles from Large-Scale Structure Surveys
• Neural Network Acceleration of Large-scale Structure Theory Calculations
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Indicator Power Spectra: Surgical Excision of Non-linearities and Covariance Matrices for Counts in Cells
• How to embed any likelihood into SBI: Application to Planck + Stage IV galaxy surveys and Dynamical Dark Energy
• Dark energy model selection with current and future data
• Towards a universal model for the density profiles of dark matter haloes
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• Clustering properties of TGSS radio sources
• On the sensitivity of weak gravitational lensing to the cosmic expansion function
• Cosmological constraints from clustering properties of galaxy clusters
• Testing growth rate dependence in cosmological perturbation theory using scale-free models
• Hybrid $P_{\ell }(k)$: general, unified, non-linear matter power spectrum in redshift space
• Compact star forming galaxies as the progenitors of compact quiescent galaxies: clustering result
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Fast Sampling of Cosmological Initial Conditions with Gaussian Neural Posterior Estimation
• Mapping the dark matter using weak lensing
• High redshift galaxies in the ALHAMBRA survey: II. strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z <= 4.5 by PDF analysis
• Stable Clustering Ansatz, Consistency Relations and Gravity Dual of Large-Scale Structure
• Constraining the growth rate on linear scales by combining SKAO and DESI surveys
• CMB lensing tomography with clustering estimation of lens redshift distributions
• A simple prediction of the nonlinear matter power spectrum in Brans-Dicke gravity from linear theory
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Variational autoencoder for generating realistic $N$-body simulations for dark matter halos
• Particle loads for cosmological simulations with equal-mass dark matter and baryonic particles
• Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
• Skew-spectra: a generalization to spin-$s$
• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
• Reconstructing spatially-varying multiplicative bias for Stage IV weak lensing galaxy surveys with a quadratic estimator
• Probing power spectrum enhancement at small scales with the SKA