Baryonic Features in the Matter Transfer Function

Abstract

We provide scaling relations and fitting formulae for adiabatic cold dark matter cosmologies that account for all baryon effects in the matter transfer function to better than 10% in the large-scale structure regime. They are based upon a physically well-motivated separation of the effects of acoustic oscillations, Compton drag, velocity overshoot, baryon infall, adiabatic damping, Silk damping, and cold-dark-matter growth suppression. We also find a simpler, more accurate, and better motivated form for the zero baryon transfer function than previous works. These descriptions are employed to quantify the amplitude and location of baryonic features in linear theory. While baryonic oscillations are prominent if the baryon fraction exceeds ${\Omega }_0{h}^2+0.2$, the main effect in more conventional cosmologies is a sharp suppression in the transfer function below the sound horizon. We provide a simple but accurate description of this effect and stress that it is not well approximated by a change in the shape parameter $\Gamma$.

20 pages, LaTeX, 7 Postscript figures included. Submitted to ApJ. Electronic versions of formulae are available at http://www.sns.ias.edu/~whu/transfer/transfer.html

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• Probing Cosmic Dawn with Emission Lines: Predicting Infrared and Nebular Line Emission for ALMA and JWST
• Beyond Limber: Efficient computation of angular power spectra for galaxy clustering and weak lensing
• The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II) IV. X-ray Luminosity Function and First Constraints on Cosmological Parameters
• Cosmology in the Next Millennium: Combining MAP and SDSS Data to Constrain Inflationary Models
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modeling of the luminosity and colour dependence in the Data Release 10
• The influence of streaming velocities and Lyman-Werner radiation on the formation of the first stars
• Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
• The Effective Field Theory of Dark Matter and Structure Formation: Semi-Analytical Results
• Improving measurements of H(z) and Da(z) by analyzing clustering anisotropies
• The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey
• The formation of the first cosmic structures and the physics of the z~20 Universe
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• Multiple inflation and the WMAP 'glitches' II. Data analysis and cosmological parameter extraction
• Finding Evidence for Massive Neutrinos using 3D Weak Lensing
• Can late-time extensions solve the $H_0$ and ${\sigma }_8$ tensions?
• Fourier analysis of luminosity-dependent galaxy clustering
• The Galaxy Power Spectrum and Bispectrum in Redshift Space
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Luminosity and Color Dependence and Redshift Evolution
• The New Horizon Run Cosmological N-Body Simulations
• Cosmological Information in the Intrinsic Alignments of Luminous Red Galaxies
• 2D-FFTLog: Efficient computation of real space covariance matrices for galaxy clustering and weak lensing
• Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
• A Cross-Correlation Analysis of Mg II Absorption Line Systems and Luminous Red Galaxies from the SDSS DR5
• The Matryoshka Run (II): Time Dependent Turbulence Statistics, Stochastic Particle Acceleration and Microphysics Impact in a Massive Galaxy Cluster
• Is Double Reionization Physically Plausible?
• Fitting Methods for Baryon Acoustic Oscillations in the Lyman-α Forest Fluctuations in BOSS Data Release 9
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: I. Real Space
• Designing a space-based galaxy redshift survey to probe dark energy
• Galactic rotation curves in hybrid metric-Palatini gravity
• Intrinsic galaxy shapes and alignments II: Modelling the intrinsic alignment contamination of weak lensing surveys
• New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies
• Future CMB tests of dark matter: ultra-light axions and massive neutrinos
• AX-GADGET: a new code for cosmological simulations of Fuzzy Dark Matter and Axion models
• Hubble parameter measurement constraints on dark energy
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
• 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
• Angular Baryon Acoustic Oscillation measure at z=2.225 from the SDSS quasar survey
• Unmasking the Masked Universe: the 2M++ catalogue through Bayesian eyes
• The Spatial Clustering of ROSAT All-Sky Survey AGNs III. Expanded Sample and Comparison with Optical AGNs
• ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• Predicting Future Space Near-IR Grism Surveys using the WFC3 Infrared Spectroscopic Parallels Survey
• The Real Space Power Spectrum of the PSCz Survey from 0.01 to 300 h/Mpc
• Cross-Correlation Lensing: Determining Galaxy and Cluster Mass Profiles from Statistical Weak Lensing Measurements
• Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
• Simulations of Baryon Oscillations
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• Modeling the reconstructed BAO in Fourier space
• Constraining amplitude and slope of the mass fluctuation spectrum using cluster baryon mass function
• Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements
• Evolving Spectra of Pop III Stars: Consequences for Cosmological Reionization
• Average and dispersion of the luminosity-redshift relation in the concordance model
• cosmoabc: Likelihood-free inference via Population Monte Carlo Approximate Bayesian Computation
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Lecture Notes in Cosmology
• A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation
• Small Scale Perturbations in a General MDM Cosmology
• Observational constraints on generalized Proca theories
• The formation of the brightest cluster galaxies in cosmological simulations: the case for AGN feedback
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• The Angular Clustering of WISE-Selected AGN: Different Haloes for Obscured and Unobscured AGN
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
• Cosmological constraints from evolution of cluster baryon mass function at z~0.5
• Fast and accurate mock catalogue generation for low-mass galaxies
• Information content of the non-linear power spectrum: the effect of beat-coupling to large scales
• On the reach of perturbative descriptions for dark matter displacement fields
• Chasing the phantom: A closer look at Type Ia supernovae and the dark energy equation of state
• An analytic model for the bispectrum of galaxies in redshift space
• Lagrangian perturbation theory at one loop order: successes, failures, and improvements
• Closed Universes, de Sitter Space and Inflation
• The Matryoshka Run: Eulerian Refinement Strategy to Study Statistics of Turbulence in Virialized Cosmic Structures
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• The Spatial Clustering of ROSAT All-Sky Survey AGNs II. Halo Occupation Distribution Modeling of the Cross Correlation Function
• High-Redshift Star Formation in a Time-Dependent Lyman-Werner Background
• CosmoBolognaLib: C++ libraries for cosmological calculations
• Primordial Non-Gaussianity from Biased Tracers: Likelihood Analysis of Real-Space Power Spectrum and Bispectrum
• The brief era of direct collapse black hole formation
• Cross-Correlation of spectroscopic and photometric galaxy surveys: cosmology from lensing and redshift distortions
• Linear Redshift Distortions and Power in the PSCz Survey
• Constraining cosmic deceleration-acceleration transition with type Ia supernova, BAO/CMB and H(z) data
• On the impact of $f(Q)$ gravity on the Large Scale Structure
• A Detection of the Baryon Acoustic Oscillation Features in the SDSS BOSS DR12 Galaxy Bispectrum
• Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
• Comparison of dark energy models after Planck 2015
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• Mean-flux Regulated PCA Continuum Fitting of SDSS Lyman-alpha Forest Spectra
• A rigorous EFT-based forward model for large-scale structure
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Chameleon f(R) gravity in the virialized cluster
• Decorrelating the Power Spectrum of Galaxies
• A new light on 21 cm intensity fluctuations from the dark ages
• Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
• Clustering properties of a sterile neutrino dark matter candidate
• Did JWST observe imprints of axion miniclusters or primordial black holes?
• SZE Observables, Pressure Profiles and Center Offsets in Magneticum Simulation Galaxy Clusters
• Effect of Peculiar Motion in Weak Lensing
• Theoretical uncertainty in baryon oscillations
• Looking at cosmic near-infrared background radiation anisotropies
• Lookback time as a test for brane cosmology
• The BOSS-WiggleZ overlap region I: Baryon Acoustic Oscillations
• The Angular Clustering of Infrared-Selected Obscured and Unobscured Quasars
• The cosmological analysis of X-ray cluster surveys: II- Application of the CR-HR method to the XMM archive
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Distribution function approach to redshift space distortions. Part IV: perturbation theory applied to dark matter
• Revisit of the interacting holographic dark energy model after Planck 2015
• The full-sky relativistic correlation function and power spectrum of galaxy number counts: I. Theoretical aspects
• Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case
• The Near-IR Background Intensity and Anisotropies During The Epoch of Reionization
• The influence of structure formation on the cosmic expansion
• On the complementarity of galaxy clustering with cosmic shear and flux magnification
• Large Scale Structures in Kinetic Gravity Braiding Model That Can Be Unbraided
• The evidence of cosmic acceleration and observational constraints
• Faint Lyman-Break galaxies as a crucial test for galaxy formation models
• Running coupling: Does the coupling between dark energy and dark matter change sign during the cosmological evolution?
• Massive neutrinos and cosmic composition
• N-body methods for relativistic cosmology
• Spin Exchange Rates in Electron-Hydrogen Collisions
• Active Galactic Nuclei and their Large-scale Structure: an eROSITA mock catalogue
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Precision modeling of redshift-space distortions from multi-point propagator expansion
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• Geometrical observational bounds on a fractal horizon holographic dark energy
• Halo model description of the non-linear dark matter power spectrum at $k\gg 1$ Mpc${}^{-1}$
• Robust Velocity-induced Acoustic Oscillations at Cosmic Dawn
• A comprehensive comparison of cosmological models from latest observational data
• Scale Dependent Galaxy Bias in the SDSS as a function of Luminosity and Colour
• The Cosmological Impact of Luminous TeV Blazars III: Implications for Galaxy Clusters and the Formation of Dwarf Galaxies
• Dark radiation from particle decay: cosmological constraints and opportunities
• Correlating galaxy colour and halo concentration: A tunable Halo Model of galactic conformity
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• The angular power spectrum of NVSS radio galaxies
• The Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• Quintessence reconstructed: new constraints and tracker viability
• Baryonic Acoustic Oscillations via the Renormalization Group
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
• Cosmological constraints from the CFHTLenS shear measurements using a new, accurate and flexible way of predicting nonlinear mass clustering
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• The galaxy power spectrum: precision cosmology from large scale structure?
• Emulators for the non-linear matter power spectrum beyond $\Lambda$CDM
• Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\Lambda$CDM
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density
• Relaxing the ${\sigma }_8$-tension through running vacuum in the Universe
• Constraining halo occupation properties of X-ray AGNs using clustering of Chandra sources in the Bootes survey region
• Cosmology with Doppler Lensing
• Halo modelling in chameleon theories
• Universal at last? The splashback mass function of dark matter halos
• Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Constraining Modified Gravity and Growth with Weak Lensing
• Unveiling Galaxy Bias via the Halo Model, KiDS and GAMA
• Dark Neutrino interactions phase out the Hubble tension
• Inhomogeneities in the universe
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Generating Log-normal Mock Catalog of Galaxies in Redshift Space
• Cosmological constraints on extended Galileon models
• Observational constraint on generalized Chaplygin gas model
• A Standard Ruler at Cosmic Dawn
• Reconciling the local void with the CMB
• The cosmological background of vector modes
• The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• Backreaction on the luminosity-redshift relation from gauge invariant light-cone averaging
• Reliability of the detection of the Baryon Acoustic Peak
• 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 $0.1$
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• Locally Biased Galaxy Formation and Large Scale Structure
• Determining the Neutrino Mass Hierarchy with Cosmology
• Precision cosmology with a wide area XMM cluster survey
• Testing Gravity Using Large-Scale Redshift-Space Distortions
• The Bispectrum of f(R) Cosmologies
• A New Equation of State for Dark Energy Model
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
• Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
• The Price of Shifting the Hubble Constant
• Theoretical and observational constraints on the HI intensity power spectrum
• The potential of X-ray cluster surveys to constrain primordial non-Gaussianity
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample
• Forecasting the Cosmological Constraints with Anisotropic Baryon Acoustic Oscillations from Multipole Expansion
• Modified Chaplygin Gas as a Unified Dark Matter and Dark Energy Model and Cosmic Constraints
• Bayesian analysis of the dynamic cosmic web in the SDSS galaxy survey
• Testing the Copernican Principle via Cosmological Observations
• Robust and model-independent cosmological constraints from distance measurements
• How clustering dark energy affects matter perturbations
• Is backreaction really small within concordance cosmology?
• Supersonic Relative Velocity Effect on the Baryonic Acoustic Oscillation Measurements
• AIC and BIC for cosmological interacting scenarios
• Toward an accurate mass function for precision cosmology
• Modeling the large-scale redshift-space 3-point correlation function of galaxies
• HICOSMO - Cosmology with a complete sample of galaxy clusters: II. Cosmological results
• Constraining primordial non-Gaussianity via a multitracer technique with surveys by Euclid and Square Kilometre Array
• Introducing SPHINX-MHD: The Impact of Primordial Magnetic Fields on the First Galaxies, Reionization, and the Global 21cm Signal
• Cosmic variance of the galaxy cluster weak lensing signal
• An ideal mass assignment scheme for measuring the Power Spectrum with FFTs
• Resolving Globular Cluster Formation within a Cosmological Context
• Photometric Redshifts for the Dark Energy Survey and VISTA and Implications for Large Scale Structure
• How to Grow a Healthy Merger Tree
• The High Redshift Integrated Sachs-Wolfe Effect
• Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies
• Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Constraints on Cosmological Models and Reconstructing the Acceleration History of the Universe with Gamma-Ray Burst Distance Indicators
• On the road to percent accuracy II: calibration of the non-linear matter power spectrum for arbitrary cosmologies
• Understanding the suppression of structure formation from dark matter$\unicode{x2013}$dark energy momentum coupling
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• Galaxy-CMB and galaxy-galaxy lensing on large scales: sensitivity to primordial non-Gaussianity
• On the incompleteness of the moment and correlation function hierarchy as probes of the lognormal field
• Observational Constraints on Kinetic Gravity Braiding from the Integrated Sachs-Wolfe Effect
• The BACCO simulation project: biased tracers in real space
• Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ
• Cosmological inference from Bayesian forward modelling of deep galaxy redshift surveys
• Lyman-alpha Forest Constraints on Decaying Dark Matter
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• Dark Energy Constraints from Baryon Acoustic Oscillations
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Streaming velocities and the baryon-acoustic oscillation scale
• High redshift cosmography: new results and implication for dark energy
• Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
• Methods for Bayesian power spectrum inference with galaxy surveys
• Cosmological perturbation theory for baryons and dark matter I: one-loop corrections in the RPT framework
• The Two-Point Correlation of Galaxy Groups: Probing the Clustering of Dark Matter Haloes
• Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach
• Combining Probes of Large-Scale Structure with CosmoLike
• Clustering of Luminous Red Galaxies III: Detection of the Baryon Acoustic Peak in the 3-point Correlation Function
• Exploring uncertainties in dark energy constraints using current observational data with Planck 2015 distance priors
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Imprints of the Early Universe on Axion Dark Matter Substructure
• Distribution function approach to redshift space distortions. Part V: perturbation theory applied to dark matter halos
• Accurate Modeling of Weak Lensing with the sGL Method
• Inner cusps of the first dark matter haloes: Formation and survival in a cosmological context
• Measuring Dark Energy with Gamma-Ray Bursts and Other Cosmological Probes
• Pairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matter Model using the Bullet Cluster
• Multiscale Inference of Matter Fields and Baryon Acoustic Oscillations from the Ly-alpha Forest
• TheHaloMod: An online calculator for the halo model
• The contribution of high redshift galaxies to the Near-Infrared Background
• Growth factor parametrization in curved space
• Unveiling the Dynamics of the Universe
• LoCuSS: The infall of X-ray groups onto massive clusters
• Lifting weak lensing degeneracies with a field-based likelihood
• Constraints on the generalized Chaplygin gas model including gamma-ray bursts via a Markov Chain Monte Carlo approach
• The role of HD cooling in primordial star formation
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring H(z) and D_A(z) at z = 0.57 with Clustering Wedges
• Lagrangian or Eulerian; Real or Fourier? Not All Approaches to Large-Scale Structure Are Created Equal
• Constraining baryonic feedback and cosmology with weak-lensing, X-ray, and kinematic Sunyaev-Zeldovich observations
• Is the 2MASS clustering dipole convergent?
• Observational constraints on Myrzakulov gravity
• Cosmic vector for dark energy: constraints from SN, CMB and BAO
• 21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction
• EMMA: an AMR cosmological simulation code with radiative transfer
• Observational constraints on the LLTB model
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• Systematic effects in the sound horizon scale measurements
• Triaxial haloes, intrinsic alignments and the dark matter power spectrum
• Testing Hu-Sawicki f(R) gravity with the Effective Field Theory approach
• Direct Minkowski Functional analysis of large redshift surveys: a new high--speed code tested on the luminous red galaxy Sloan Digital Sky Survey-DR7 catalogue
• Clustering of luminous red galaxies II: small scale redshift space distortions
• Effects of Gravitational Evolution, Biasing, and Redshift Space Distortion on Topology
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: II. Fourier and Redshift Space
• Cosmological constraints of phantom dark energy models
• A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling
• Starobinsky cosmological model in Palatini formalism
• New light on Dark Cosmos
• How does the cosmic large-scale structure bias the Hubble diagram?
• Experimental constraints on the uncoupled Galileon model from SNLS3 data and other cosmological probes
• Bayesian 3d velocity field reconstruction with VIRBIuS
• Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7
• The Acoustic Peak in the Lyman Alpha Forest
• Baryon Oscillations and Dark-Energy Constraints from Imaging Surveys
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Precision cosmology with redshift-space bispectrum: a perturbation theory based model at one-loop order
• Improving geometric and dynamical constraints on cosmology with intrinsic alignments of galaxies
• Particle mesh simulations of the Lyman-alpha forest and the signature of Baryon Acoustic Oscillations in the intergalactic medium
• Observational Constraints on Exponential Gravity
• CFHTLS weak-lensing constraints on the neutrino masses
• Cosmological cross-correlations and nearest neighbor distributions
• Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces
• Three-Point Statistics from a New Perspective
• Dark energy: investigation and modeling
• Assessment of the cosmic distance duality relation using Gaussian Process
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Scale-dependent halo bias from scale-dependent growth
• Cross-correlating WMAP5 with 1.5 million LRGs: a new test for the ISW effect
• On Possible Variation in the Cosmological Baryon Fraction
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Background history and cosmic perturbations for a general system of self-conserved dynamical dark energy and matter
• What is the best way to measure baryonic acoustic oscillations?
• A measurement of the Hubble constant using galaxy redshift surveys
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• Massive Photon and Dark Energy
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• Weighing obscured and unobscured quasar hosts with the CMB
• Cosmic Ballet III: halo spin evolution in the cosmic web
• Power spectrum of halo intrinsic alignments in simulations
• Magnification-Temperature Correlation: the Dark Side of ISW Measurements
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Possible Detection of Baryonic Fluctuations in the Large-Scale Structure Power Spectrum
• Shedding Light on Dark Matter: A Faraday Rotation Experiment to Limit a Dark Magnetic Moment
• The clustering of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future wide-field surveys
• Tension in the Void: Cosmic Rulers Strain Inhomogeneous Cosmologies
• Measuring the neutrino mass from future wide galaxy cluster catalogues
• On the faint-end of the high-$z$ galaxy luminosity function
• What sets the central structure of dark matter haloes?
• Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
• Massive Milky Way Satellites in Cold and Warm Dark Matter: Dependence on Cosmology
• Hints of dark energy anisotropic stress using Machine Learning
• Toward More Realistic Forecasting of Dark Energy Constraints from Galaxy Redshift Surveys
• The growth rate of cosmic structures in the local Universe with the ALFALFA survey
• Cosmological surveys with the Australian Square Kilometre Array Pathfinder
• Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys
• The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\sim 2$
• Cosmological Fluctuations of Short Wavelength
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• The X-ray surface brightness distribution from diffuse gas
• Constraints on growth index parameters from current and future observations
• Early Dark Energy at High Redshifts: Status and Perspectives
• Measuring Redshift-Space Distortions using Photometric Surveys
• The primordial matter power spectrum on sub-galactic scales
• Prospects for Future Binary Black Hole GW Studies in Light of PTA Measurements
• Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks
• Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey
• Perturbation Theory of the Cosmological Log-Density Field
• Clustering of photometric luminous red galaxies I : Growth of Structure and Baryon Acoustic Feature
• Fingerprints of the initial conditions on the density profiles of cold and warm dark matter haloes
• Constraints on small-scale primordial power by annihilation signals from extragalactic dark matter minihalos
• Cosmological observations in a modified theory of gravity (MOG)
• Dark matter voids in the SDSS galaxy survey
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Unified Dark Fluid with Constant Adiabatic Sound Speed and Cosmic Constraints
• Constraining the Baryon-Dark Matter Relative Velocity with the Large-Scale 3-Point Correlation Function of the SDSS BOSS DR12 CMASS Galaxies
• Breaking a dark degeneracy: The gamma-ray signature of early matter domination
• Imprints of Oscillatory Bispectra on Galaxy Clustering
• Lensing Corrections to Features in the Angular Two-Point Correlation Function and Power Spectrum
• A new method for the Alcock-Paczynski test
• Constraining large scale HI bias using redshifted 21-cm signal from the post-reionization epoch
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• On the cross-correlation of sub-mm sources and optically-selected galaxies
• Cosmological distance indicators
• Teleparallel Dark Energy with Purely Non-minimal Coupling to Gravity
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Detectability of Torsion Gravity via Galaxy Clustering and Cosmic Shear Measurements
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• Post-collapse perturbation theory in 1D cosmology -- beyond shell-crossing
• Does small scale structure significantly affect cosmological dynamics?
• From Images to Dark Matter: End-To-End Inference of Substructure From Hundreds of Strong Gravitational Lenses
• Forecasts for Dark Energy Measurements with Future HI Surveys
• How to generate a significant effective temperature for cold dark matter, from first principles
• Target Selection for the DESI Peculiar Velocity Survey
• Non-linear evolution of the BAO scale in alternative theories of gravity
• Scale-dependent Galaxy Bias
• SUNGLASS: A new weak lensing simulation pipeline
• Large Scale Structure Formation in Eddington-inspired Born-Infeld Gravity
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Bayesian forward modelling of cosmic shear data
• The clustering of galaxy clusters in cosmological models with non-Gaussian initial conditions: Predictions for future surveys
• Fractal Dimensions of a Weakly Clustered Distribution and the Scale of Homogeneity
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• Satellite Quenching, Galaxy Inner Density and the Halo Environment
• The Redshift Sensitivities of Dark Energy Surveys
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• Cosmology with 6 parameters in the Stage-IV era: efficient marginalisation over nuisance parameters
• Cosmology with non-minimal derivative couplings: perturbation analysis and observational constraints
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• Galaxy cluster number count data constraints on cosmological parameters
• The 2dF QSO Redshift Survey - XI. The QSO Power Spectrum
• 2-FAST: Fast and accurate computation of projected two-point functions
• Combining FOF and halo-based algorithms for the identification of galaxy groups
• The Reconstructed Power Spectrum in the Zeldovich Approximation
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• Projected Constraints on Modified Gravity Cosmologies from 21 cm Intensity Mapping
• Optimising large galaxy surveys for ISW detection
• BAM: Bias Assignment Method to generate mock catalogs
• Interacting viscous dark fluids
• COSMOS weak-lensing constraints on modified gravity
• Non-linear Galaxy Power Spectrum and Cosmological Parameters
• Prospects for galaxy-mass relations from the 6dF Galaxy Survey
• The Contribution of z<6 Sources to the Spatial Coherence in the Unresolved Cosmic near-Infrared and X-ray Backgrounds
• High Redshift Standard Candles: Predicted Cosmological Constraints
• Relating the structure of dark matter halos to their assembly and environment
• Measuring gravity at cosmological scales
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Galaxy-CMB Cross-Correlation as a Probe of Alternative Models of Gravity
• Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
• Clustering of infrared-bright dust-obscured galaxies revealed by the Hyper Suprime-Cam and WISE
• Cosmological information in Gaussianised weak lensing signals
• Reliability of the dark matter clustering in cosmological N-body simulation on scales below the mean separation length of particles
• The REFLEX II galaxy cluster survey: power spectrum analysis
• Galactic Halos in MONDian Cosmological Simulations
• A Comparative Study of Dark Energy Constraints from Current Observational Data
• Information Content of Higher-Order Galaxy Correlation Functions
• Integrated approach to cosmology: Combining CMB, large-scale structure and weak lensing
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• Understanding `galaxy groups' as a unique structure in the universe
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Effects of baryons on weak lensing peak statistics
• Cosmological constraints on the Generalized Uncertainty Principle from modified Friedmann equations
• Intrinsic alignment of redMaPPer clusters: cluster shape - matter density correlation
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Latest Observational Constraints to the Ghost Dark Energy Model by Using Markov Chain Monte Carlo Approach
• On using the WMAP distance priors in constraining the time evolving equation of state of dark energy
• An optimized correlation function estimator for galaxy surveys
• CMB anisotropies in the presence of a stochastic magnetic field
• Multitracer technique for galaxy bispectrum - An application to constraints on non-local primordial non-Gaussianities -
• Visualizing probabilistic models: Intensive Principal Component Analysis
• Using the Zeldovich dynamics to test expansion schemes
• Weak Lensing Observables in the Halo Model
• The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample
• Observational constraints on cosmic neutrinos and dark energy revisited
• Distance Priors from \emph{Planck} 2015 data
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Acoustic peaks and dips in the CMB power spectrum: observational data and cosmological constraints
• Combining cluster number counts and galaxy clustering
• Machine Learning improved fits of the sound horizon at the baryon drag epoch
• Cosmological Constraints from Hubble parameter $H(z)$ and SN Ia observations
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Testing cold dark matter with the low mass Tully-Fisher relation
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Super-sample covariance approximations and partial sky coverage
• On the Physical Requirements for a Pre-Reionization Origin of the Unresolved Near-Infrared Background
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• The Angular Momentum of Gas in Proto-Galaxies: II -- The Impact of Preheating
• Non-Gaussianity in Large Scale Structure and Minkowski Functionals
• Near term measurements with 21 cm intensity mapping: neutral hydrogen fraction and BAO at z<2
• Baryon Acoustic Oscillations and Dynamical Dark Energy
• Constraining the primordial magnetic field with dwarf galaxy simulations
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Magnification Bias Corrections to Galaxy-Lensing Cross-Correlations
• Low-mass suppression of the satellite luminosity function due to the supersonic baryon--cold-dark-matter relative velocity
• Evolution of primordial magnetic fields during large-scale structure formation
• The effect of baryonic streaming motions on the formation of the first supermassive black holes
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• A Method for Measuring the Bias of High-Redshift Galaxies from Cosmic Variance
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• Anisotropic Fluid Cosmology: an Alternative to Dark Matter?
• Inferring high redshift large-scale structure dynamics from the Lyman-alpha forest
• Accounting for Cosmic Variance in Studies of Gravitationally-Lensed High-Redshift Galaxies in the Hubble Frontier Field Clusters
• A Universe Without Dark Energy: Cosmic Acceleration from Dark Matter-Baryon Interactions
• Exploring the Latest Union2 SNIa Dataset by Using Model-Independent Parametrization Methods
• A New Statistic for Analyzing Baryon Acoustic Oscillations
• Voids in cosmological simulations over cosmic time
• A Study of High-Order Non-Gaussianity with Applications to Massive Clusters and Large Voids
• Holographic Dark Energy with Cosmological Constant
• Galaxy groups in the 2dF galaxy redshift survey: Large Scale Structure with Groups
• Optimized Clustering Estimators for BAO Measurements Accounting for Significant Redshift Uncertainty
• Forecasts of non-Gaussian parameter spaces using Box-Cox transformations
• Fuzzy Dark Matter as a Solution to Reconcile the Stellar Mass Density of High-z Massive Galaxies and Reionization History
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Bayesian Comparison of Interacting Scenarios
• Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• The importance of magnification effects in galaxy-galaxy lensing
• Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
• The effect of photometric redshift uncertainties on galaxy clustering and baryonic acoustic oscillations
• Constraining An Exact Brans-Dicke gravity theory with Recent Observations
• On the accretion history of galaxy clusters: temporal and spatial distribution
• Weak lensing and the Dyer-Roeder approximation
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• A local measurement of the growth rate from peculiar velocities and galaxy clustering correlations in the 6dF Galaxy Survey
• Constraining DGP Gravity from Observational Data
• The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
• 2MASS Constraints on the Local Large-Scale Structure: A Challenge to LCDM?
• Bayesian semi-blind component separation for foreground removal in interferometric 21-cm observations
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• The correlation function of galaxy clusters and detection of baryon acoustic oscillations
• Optimal Weighting Scheme in Redshift-space Power Spectrum Analysis and a Prospect for Measuring the Cosmic Equation of State
• Rejuvenating the Matter Power Spectrum III: The Cosmology Sensitivity of Gaussianized Power Spectra
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• Evidence for an environment-dependent shift in the baryon acoustic oscillation peak
• The dark matter transfer function: free streaming, particle statistics and memory of gravitational clustering
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Power Spectrum Shape from Peculiar Velocity Data
• Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• Modeling the evolution of infrared galaxies : clustering of galaxies in the Cosmic Infrared Background
• Correlations in the (Sub)millimeter background from ACTxBLAST
• A cosmological view of extreme mass-ratio inspirals in nuclear star clusters
• Probability of the most massive cluster under non-Gaussian initial conditions
• Intrinsic alignment statistics of density and velocity fields at large scales: Formulation, modeling, and baryon acoustic oscillation features
• Observational constraint on the varying speed of light theory
• 3-dimensional spherical analyses of cosmological spectroscopic surveys
• Implications of a Scalar Dark Force for Terrestrial Experiments
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales II: Perturbative and numerical analyses of power spectrum and bispectrum
• Impacts of the physical data model on the forward inference of initial conditions from biased tracers
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• Matrix-free Large Scale Bayesian inference in cosmology
• Voids in Lyα Forest Tomographic Maps
• Redshift-space distortions in massive neutrino and evolving dark energy cosmologies
• Relative clustering and the joint halo occupation distribution of red-sequence and blue-cloud galaxies in COMBO-17
• Stellar-to-halo mass relation of cluster galaxies
• Comparison of weak lensing by NFW and Einasto halos and systematic errors
• Perturbation theory challenge for cosmological parameters estimation: Matter power spectrum in real space
• Cosmic velocity--gravity relation in redshift space
• Cosmic Structure Formation with Kinetic Field Theory
• Supermassive Black Hole Merger Rates: Uncertainties from Halo Merger Theory
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• What is the distance to the CMB?
• A comprehensive numerical study on four categories of holographic dark energy models
• Large Scale Clustering of Sloan Digital Sky Survey Quasars: Impact of the Baryon Density and the Cosmological Constant
• Impact of Redshift Information on Cosmological Applications with Next-Generation Radio Surveys
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Inflationary cosmology with Chaplygin gas in Palatini formalism
• Redshift-space streaming velocity effects on the Lyman-$\alpha$ forest baryon acoustic oscillation scale
• A comprehensive investigation on the slowing down of cosmic acceleration
• Have Baryonic Acoustic Oscillations in the galaxy distribution really been measured?
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Gas Loss in Simulated Galaxies as They Fall into Clusters
• Non-linear matter power spectrum from Time Renormalisation Group: efficient computation and comparison with one-loop
• A Flexible Analytic Model of Cosmic Variance in the First Billion Years
• Observational constraints on bimetric gravity
• The homogeneity scale and the growth rate of cosmic structures
• Cluster correlations in redshift space
• How does non-linear dynamics affect the baryon acoustic oscillation?
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Observational Tests of Gauss-Bonnet Like Dark Energy Model
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• Luminous Red Galaxy Clustering at z~0.7 - First Results using AAOmega
• Can Non-Gaussian Cosmological Models Explain the WMAP's High Optical Depth for Reionization?
• Self-Calibrated Cluster Counts as a Probe of Primordial Non-Gaussianity
• Simulations of BAO reconstruction with a quasar Lyman-alpha survey
• Flat-Sky Pseudo-Cls Analysis for Weak Gravitational Lensing
• Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
• Modeling the clustering of dark-matter haloes in resummed perturbation theories
• Two 100 Mpc-scale structures in the 3-D distribution of radio galaxies and their implications
• BAO reconstruction: a swift numerical action method for massive spectroscopic surveys
• Distance Measurements from Supernovae and Dark Energy Constraints
• Dark-Energy Dynamics Required to Solve the Cosmic Coincidence
• Coupling between cold dark matter and dark energy from neutrino mass experiments
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• Search for primordial non-Gaussianity in the quasars of SDSS-III BOSS DR9
• The optimal gravitational softening length for cosmological N-body simulations
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• Large-Scale Velocity Dispersion and the Cosmic Web
• Probing the dynamical behavior of dark energy
• Optimal Reconstruction of Baryon Acoustic Oscillations for DESI 2024
• The Hubble rate in averaged cosmology
• Constraining the halo mass function with observations
• Dynamics of the diffusive DM-DE interaction--dynamical system approach
• Growth of matter perturbations in the extended viscous dark energy models
• Highly-Ionized Oxygen Absorbers in the Intergalactic Medium
• Testing modified gravity models with recent cosmological observations
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Probing high-redshift galaxies with Ly$\alpha$ intensity mapping
• Interacting dark energy from the joint analysis of the power spectrum and bispectrum multipoles with the EFTofLSS
• Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy Survey
• SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of Potential Systematics in Fitting of Baryon Acoustic Feature
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Observational constraints on phantom power-law cosmology
• Fast Generation of Covariance Matrices for Weak Lensing
• Improving reconstruction of the baryon acoustic peak : the effect of local environment
• The Effects of Varying Cosmological Parameters on Halo Substructure
• COMET: Clustering Observables Modelled by Emulated perturbation Theory
• KiDS-450: Enhancing cosmic shear with clipping transformations
• Vorticity generation in the Universe: A perturbative approach
• Prompt cusps and the dark matter annihilation signal
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• Observational Constraints with Recent Data on the DGP Modified Gravity
• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Cosmological model of the interaction between dark matter and dark energy
• Observational constraints on new generalized Chaplygin gas model
• Clustering dark energy and halo abundances
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• Isotropic vs. Anisotropic components of BAO data: a tool for model selection
• Isocurvature modes and Baryon Acoustic Oscillations
• How the Big Bang Ends up Inside a Black Hole
• Generalized covariant prescriptions for averaging cosmological observables
• 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
• The Evolution of Our Local Cosmic Domain: Effective Causal Limits
• Lensing anomaly and oscillations in the primordial power spectrum
• Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
• Monte Carlo Control Loops for cosmic shear cosmology with DES Year 1
• Non-Gaussian errors of baryonic acoustic oscillations
• Cosmological constraints on dark energy models using DESI BAO 2024
• A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
• The Effects of Lyman-Limit Systems on the Evolution and Observability of the Epoch of Reionization
• Shell-crossing in a $\Lambda$CDM Universe
• Soliton Merger Rates and Enhanced Axion Dark Matter Decay
• Generalized Holographic Dark Energy and its Observational Constraints
• Discovery of a new fundamental plane dictating galaxy cluster evolution from gravitational lensing
• Observational constraints on Horava-Lifshitz cosmology
• A new cosmic shear function: Optimised E-/B-mode decomposition on a finite interval
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Higher Order Statistics for Three-dimensional Shear and Flexion
• Strong gravitational lensing constraints on holographic dark energy
• Is ram-pressure stripping an efficient mechanism to remove gas in galaxies?
• Accuracy of cosmological parameters using the baryon acoustic scale
• Precision growth index using the clustering of cosmic structures and growth data
• 3D galaxy clustering with future wide-field surveys: Advantages of a spherical Fourier-Bessel analysis
• PT challenge: Validation of ShapeFit on large-volume, high-resolution mocks
• Detecting the power spectrum turnover with HI intensity mapping
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• The large scale clustering of radio sources
• Covariance of the matter power spectrum including the survey window function effect: N-body simulations vs. fifth-order perturbation theory on grid
• Bulk Flow and Shear Moments of the SFI++ Survey
• Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
• Late time anisotropy as an imprint of cosmological backreaction
• Probing Dark Energy with Baryonic Acoustic Oscillations at High Redshifts
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• A short review on clustering dark energy
• The segregation of baryons and dark matter during halo assembly
• When do cosmic peaks, filaments or walls merge? A theory of critical events in a multi-scale landscape
• Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos
• Non-linear relativistic contributions to the cosmological weak-lensing convergence
• Signatures of Cosmic Reionization on the 21cm 2- and 3-point Correlation Function I: Quadratic Bias Modeling
• New constraints on primordial features from the galaxy two-point correlation function
• Temperature and Entropy Fields of Baryonic Gas in the Universe
• Cosmic slowing down of acceleration using $f_{gas}$
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• Large-scale analysis of the SDSS-III DR8 photometric luminous galaxies angular correlation function
• The Sunyaev-Zeldovich Effect from Quasar Feedback
• Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies
• Hubble constant and sound horizon from the late-time Universe
• Searching for modified gravity with baryon oscillations: from SDSS to wide field multiobject spectroscopy (WFMOS)
• A new model for the full shape of the large-scale power spectrum
• Explicit Bayesian treatment of unknown foreground contaminations in galaxy surveys
• A conventional approach to the dark-energy concept
• Fourier Band-Power E/B-mode Estimators for Cosmic Shear
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Quintessential power-law cosmology: dark energy equation of state
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Reconstructing the baryon acoustic oscillations using biased tracers
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Troubled cosmic flows: turbulence, enstrophy and helicity from the assembly history of the intracluster medium
• Exploring hints for dark energy density evolution in light of recent data
• Low-Redshift Cosmic Baryon Fluid on Large Scales and She-Leveque Universal Scaling
• AGN and QSOs in the eROSITA All-Sky Survey -- Part II: The large-scale structure
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• The BINGO Project VI: HI Halo Occupation Distribution and Mock Building
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• A hierarchical field-level inference approach to reconstruction from sparse Lyman-$\alpha$ forest data
• Evolution of hierarchical clustering in the CFHTLS-Wide since z~1
• Precision Prediction for the Cosmological Density Distribution
• Cosmological implications of the transition from the false vacuum to the true vacuum state
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• The 2MASS galaxy angular power spectrum: Probing the galaxy distribution to Gigaparsec scales
• The bias of dark matter tracers: assessing the accuracy of mapping techniques
• Weak lensing peak count as a probe of f(R) theories
• Resummed Perturbation Theory of Galaxy Clustering
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Gaugessence: a dark energy model with early time radiation-like equation of state
• Constraints on shear and rotation with massive galaxy clusters
• Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data
• Detection of spatial correlations of fundamental plane residuals, and cosmological implications
• Hořava-Lifshitz cosmology in light of new data
• The halo mass of optically-luminous quasars at z=1-2 measured via gravitational deflection of the cosmic microwave background
• Constraints on accelerating universe using ESSENCE and Gold supernovae data combined with other cosmological probes
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• Galaxy correlations and the BAO in a void universe: structure formation as a test of the Copernican Principle
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• Multiverse Dark Matter: SUSY or Axions
• Statistical hierarchy of varying speed of light cosmologies
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• Constraints on Newton's Constant from Cosmological Observations
• The Clustering of X-ray Luminous Quasars
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Testing CCC+TL Cosmology with Observed BAO Features
• Inhomogeneity-induced variance of cosmological parameters
• Hierarchy in the Phase Space and Dark Matter Astronomy
• Spatial Curvature in $f(R)$ Gravity
• Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
• Controlling intrinsic-shear alignment in three-point weak lensing statistics
• Testing the interaction model with cosmological data and gamma-ray bursts
• CFHTLenS: A Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics
• An accurate determination of the Hubble constant from Baryon Acoustic Oscillation datasets
• Vacuum energy as dark matter
• Dark sectors of the Universe: A Euclid survey approach
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• Host Dark Matter Halos of WISE-selected Obscured & Unobscured Quasars: Evidence for Evolution
• Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• Cosmic variance of $H_0$ in light of forthcoming high-redshift surveys
• Cosmological Inference from Galaxy-Clustering Power Spectrum: Gaussianization and Covariance Decomposition
• Extended $\Lambda$CDM model
• Quantum mechanical look at the radioactive-like decay of metastable dark energy
• Dark matter halo occupation: environment and clustering
• Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure
• Understanding the faint red galaxy population using large-scale clustering measurements from SDSS DR7
• Geometrical Diagnostics for Generalized Chaplygin Gas
• Cosmological Parameters from Redshift-Space Correlations
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• From dark matter halos to pre-stellar cores: High resolution follow-up of cosmological Lyman-Werner simulations
• Evidence for baryon acoustic oscillations from galaxy-ellipticity correlations
• Imprints of deviations from the gravitational inverse-square law on the power spectrum of mass fluctuations
• On measuring the absolute scale of baryon acoustic oscillations
• Evolution of density perturbations in large void universe
• Nonlinear Redshift-Space Distortions in the Harmonic-space Galaxy Power Spectrum
• Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
• The power spectrum of galaxy clustering in the APM survey
• High Frequency Cluster Radio Galaxies: Luminosity Functions and Implications for SZE Selected Cluster Samples
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• $f(R)$ gravity modifications: from the action to the data
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Measuring Bulk Flow of Galaxy Clusters using Kinematic Sunyaev-Zel'dovich effect: Prediction for Planck
• Strong lensing modeling in galaxy clusters as a promising method to test cosmography I. Parametric dark energy models
• A scale dependent bias on linear scales: the case for HI intensity mapping at z=1
• Does accelerating universe indicates Brans-Dicke theory
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• Integrated Sachs-Wolfe-galaxy cross-correlation bounds on the two branches of the minimal theory of massive gravity
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Hydrodynamical structure formation in Milgromian cosmology
• A precise symbolic emulator of the linear matter power spectrum
• The Location and Environments of Neutron Star Mergers in an Evolving Universe
• Cold Dark Matter Isocurvature Perturbations: Cosmological Constraints and Applications
• Is the baryon acoustic oscillation peak a cosmological standard ruler?
• Counts of galaxy clusters as cosmological probes: the impact of baryonic physics
• Constraints on the exponential $f(R)$ model from latest Hubble parameter measurements
• CMB-Galaxy correlation in Unified Dark Matter Scalar Field Cosmologies
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Cosmology from Clustering, Cosmic Shear, CMB Lensing, and Cross Correlations: Combining Rubin Observatory and Simons Observatory
• Weak Lensing of Baryon Acoustic Oscillations
• Confronting Tracker Field Quintessence with Data
• Cosmology from weak lensing alone and implications for the Hubble tension
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Robust constraints on dark energy and gravity from galaxy clustering data
• The cosmological free-free signal from galaxy groups and clusters
• Decomposition of Spectra from Redshift Distortion Maps
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Does jackknife scale really matter for accurate large-scale structure covariances?
• A critical discussion on the $H_0$ tension
• Cosmology with decaying cosmological constant -- exact solutions and model testing
• Integrated Cosmological Probes: Extended Analysis
• Energy Scale of Lorentz Violation in Rainbow Gravity
• Effects of biasing on the galaxy power spectrum at large scales
• Inadequacy of internal covariance estimation for super-sample covariance
• Primordial power spectrum and cosmology from black-box galaxy surveys
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Markov-chain reconstruction of the 2dF Galaxy Redshift Survey real-space power spectrum
• Differentiable Cosmological Simulation with Adjoint Method
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• Late time sky as a probe of steps and oscillations in primordial Universe
• The dominant origin of diffuse Ly$\alpha$ halos around LAEs explored by SED fitting and clustering analysis
• Characterizing unknown systematics in large scale structure surveys
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• Easily Interpretable Bulk Flows: Continuing Tension with the Standard Cosmological Model
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Cosmology-informed neural networks to solve the background dynamics of the Universe
• Testing the minimum variance method for estimating large-scale velocity moments
• The clustering of critical points in the evolving cosmic web
• Probing the constancy of the speed of light with future galaxy survey: the case of SKA and Euclid
• Vector perturbations of galaxy number counts
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• Remnants of Galactic subhalos and their impact on indirect dark matter searches
• Eigenmode Analysis of Galaxy Distributions in Redshift Space
• Combining spectroscopic and photometric surveys using angular cross-correlations II: Parameter constraints from different physical effects
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• Optimising cosmic shear surveys to measure modifications to gravity on cosmic scales
• Relation between standard perturbation theory and regularized multi-point propagator method
• Inflation that runs naturally: Gravitational waves and suppression of power at large and small scales
• Constraining the primordial power spectrum from SNIa lensing dispersion
• Using Lagrangian perturbation theory for precision cosmology
• Detecting the Baryons in Matter Power Spectra
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• Model-Independent Measurements of Cosmic Expansion and Growth at z=0.57 Using the Anisotropic Clustering of CMASS Galaxies From the Sloan Digital Sky Survey Data Release 9
• The effect of different observational data on the constraints of cosmological parameters
• Time of flight of ultra-relativistic particles in a realistic Universe: a viable tool for fundamental physics?
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone 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
• RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• BAO scale inference from biased tracers using the EFT likelihood
• Probing dark energy with the next generation X-ray surveys of galaxy clusters
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Accuracy of analytical models of the large-scale matter distribution
• Large-scale structure in mimetic Horndeski gravity
• Acoustic oscillations and viscosity
• Ballistic Dark Matter oscillates above $\Lambda$CDM
• Bayesian power-spectrum inference with foreground and target contamination treatment
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Observational constraints on unified dark matter including Hubble parameter data
• ELG Spectroscopic Systematics Analysis of the DESI Data Release 1
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): On the correct recovery of the count-in-cell probability distribution function
• Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis
• Observational constraints on dark energy cosmological model parameters
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• Modification of the 21-cm power spectrum by X-rays during the epoch of reionisation
• Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae
• Lensing as a Probe of Early Universe: from CMB to Galaxies
• Beyond the growth rate of cosmic structure: Testing modified gravity models with an extra degree of freedom
• Testing the consistency of three-point halo clustering in Fourier and configuration space
• Constraints to Holographic Dark Energy Model via Type Ia Supernovae, Baryon Acoustic Oscillation and WMAP
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• Bispectrum as Baryon Acoustic Oscillation Interferometer
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• Testing averaged cosmology with type Ia supernovae and BAO data
• Baryon acoustic oscillation methods for generic curvature: Application to the SDSS-III Baryon Oscillation Spectroscopic Survey
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Constraints on ${\Omega }_{\mathrm{m}}$ and ${\sigma }_8$ from the potential-based cluster temperature function
• Normalization of the Matter Power Spectrum via Higher-Order Angular Correlations of Luminous Red Galaxies
• New cosmological constraints on the evolution of dark matter energy density
• Validating the Fisher approach for stage IV spectroscopic surveys
• Volume Statistics as a Probe of Large-Scale Structure
• Eccentricity effects on the supermassive black hole gravitational wave background
• Improved cosmological constraints on the curvature and equation of state of dark energy
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Interrelation of the environment of Ly$\alpha$ emitters and massive galaxies at $2<z<4.5$
• Detecting Baryon Acoustic Oscillations
• Which Fundamental Constants for CMB and BAO?
• An updated analysis of two classes of f(R) theories of gravity
• Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• Comparing dark energy models with current observational data
• Recovering a redshift-extended VSL signal from galaxy surveys
• Measuring the luminosity and virial black hole mass dependence of quasar-galaxy clustering at z ~ 0.8
• Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• Mutual Constraints Between Reionization Models and Parameter Extraction From Cosmic Microwave Background Data
• Measuring BAO and non-Gaussianity via QSO clustering
• On the choice of the most suitable indicator for the assembly state of dark matter haloes through cosmic time
• Iterative removal of redshift space distortions from galaxy clustering
• A Second-order bias model for the Logarithmic Halo Mass Density
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Sudden Future Singularity models as an alternative to Dark Energy?
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• A Consistent Comparison of Bias Models using Observational Data
• Topology and geometry of the dark matter web: a multistream view
• Hydrogen Clouds before Reionization: a Lognormal Model Approach
• Fisher matrix predictions for detecting the cosmological 21 cm signal with the Ooty Wide Field Array (OWFA)
• Simulating the Effect of Non-Linear Mode-Coupling in Cosmological Parameter Estimation
• Improving estimates of the growth rate using galaxy-velocity correlations: a simulation study
• Vainshtein Screening in Bimetric Cosmology
• Describing variations of the Fisher-matrix across parameter space
• Probing higher-order primordial non-Gaussianity with galaxy surveys
• An analytic approach to baryon acoustic oscillations
• Cosmological constraints from low-redshift data
• Towards realistic $f(T)$ models with nonminimal torsion-matter coupling extension
• Replacing dark energy by silent virialisation
• The Clustering of Extremely Red Objects
• Constraints on Dark Energy Models Using Late Universe Probes
• A low Hubble Constant from galaxy distribution observations
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Grid-based calculations of redshift-space matter fluctuations from perturbation theory: UV sensitivity and convergence at the field level
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• The Peculiar Velocity Correlation Function
• Cosmic Microwave Background Bispectrum from the Lensing--Rees-Sciama Correlation Reexamined: Effects of Non-linear Matter Clustering
• Using machine learning to compress the matter transfer function $T(k)$
• The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars
• Field-Based Physical Inference From Peculiar Velocity Tracers
• Surveying the dark side
• Signatures of the Baryon Acoustic Oscillations on 21cm Emission Background
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs
• Towards 21-cm Intensity Mapping at $z=2.28$ with uGMRT using the Tapered Gridded Estimator I: Foreground Avoidance
• A generalized mass-to-horizon relation: a new global approach to entropic cosmologies and its connection to $\Lambda$CDM
• A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane
• Extracting high-order cosmological information in galaxy surveys with power spectra
• A GREAT model comparison against the cosmological constant
• Can AGN and galaxy clusters explain the surface brightness fluctuations of the cosmic X-ray background?
• Transient acceleration in $f(T)$ gravity
• Geometric and dynamic distortions in anisotropic galaxy clustering
• A revised density split statistic model for general filters
• Current lookback time-redshift bounds on dark energy
• Constraining thawing and freezing models with cluster number counts
• Updated F(T) gravity constraints from high redshift cosmography
• Efficient Construction of Mock Catalogs for Baryon Acoustic Oscillation Surveys
• f(R) Gravity in an Ellipsoidal Universe
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Isolating the decay rate of cosmological gravitational potential
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• Measuring the Energy Scale of Inflation with Large Scale Structures
• The impact of the Universe's expansion rate on constraints on modified growth of structure
• High Redshift Investigation On The Dark Energy Equation of State
• Effects of NII and H$\alpha$ Line Blending on the WFIRST Galaxy Redshift Survey
• Enhanced n-body annihilation of dark matter and its indirect signatures
• Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe
• Little Red Dots as Direct-collapse Black Hole Nurseries
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• Cosmic magnetic fields with MASCLET: an application to galaxy clusters
• Imprint of thawing scalar fields on large scale galaxy overdensity
• Second-order matter fluctuations via higher-order galaxy correlators
• No evidence for the evolution of mass density power-law index $\gamma$ from strong gravitational lensing observation
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• Dynamics and statefinder analysis of a class of sign-changeable interacting dark energy scenarios
• Biases on cosmological parameter estimators from galaxy cluster number counts
• Prospects in Constraining the Dark Energy Potential
• Lensing smoothing of BAO wiggles
• Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models
• Combining spectroscopic and photometric surveys using angular cross-correlations I: Algorithm and modelling
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• Non-Gaussian CMB and LSS statistics beyond polyspectra
• Dimensionless cosmology
• How accurately can we measure the baryon acoustic oscillation feature?
• Triggering the formation of direct collapse black holes by their congeners
• Interacting generalized ghost dark energy in non-flat universe
• Log-transforming the matter power spectrum
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Forecasting cosmological parameter constraints from near-future space-based galaxy surveys
• Cross-correlations of the Lyman-alpha forest with weak lensing convergence I: Analytical Estimates of S/N and Implications for Neutrino Mass and Dark Energy
• The Phase of the BAO on Observable Scales
• Clustering of CODEX clusters
• Galaxy-QSO Correlation induced by Weak Gravitational Lensing arising from Large-Scale Structure
• Constraining Cosmological Models by the Cluster Mass Function
• Optimising Spectroscopic and Photometric Galaxy Surveys: Same-sky Benefits for Dark Energy and Modified Gravity
• Constraining the emergent dark energy models with observational data at intermediate redshift
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Lyman-alpha Emitters in Ionized Bubbles: Constraining the Environment and Ionized Fraction
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
• Forecasting the power of Higher Order Weak Lensing Statistics with automatically differentiable simulations
• Toward High-Precision Measures of Large-Scale Structure
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• Varying constants entropic--$\Lambda$CDM cosmology
• Parametrizing the transition to the phantom epoch with Supernovae Ia and Standard Rulers
• Discriminating different models of luminosity-redshift distribution
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• Hierarchical Structure Formation and Chemical Evolution of Galaxies
• Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data
• Cosmology with a Decaying Vacuum Energy Parametrization Derived from Quantum Mechanics
• Cluster abundance and large scale structure
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• Fisher Matrix Based Predictions for Measuring the z = 3.35 Binned 21-cm Power Spectrum using the Ooty Wide Field Array (OWFA)
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• Quintessential early dark energy
• Abundance and properties of dark radiation from the cosmic microwave background
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: constraints on the time variation of fundamental constants from the large-scale two-point correlation function
• Towards $21$-cm intensity mapping at $z=2.28$ with uGMRT using the tapered gridded estimator III: Foreground removal
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VI. Effect of massive neutrinos on the cosmological constraints from clusters
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Cosmological constraints from the masses and abundances of L* galaxies
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Dynamical evolutin of quintessence dark energy in collapsing dark matter halos
• Uncertainty in 2-point correlation function estimators and BAO detection in SDSS DR7
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
• Constraints on small-scale primordial density fluctuation from cosmic microwave background through dark matter annihilation
• Figure of Merit and Different Combinations of Observational Data Sets
• Cosmological Constraint and Analysis on Holographic Dark Energy Model Characterized by the Conformal-age-like Length
• Fast, large volume, GPU enabled simulations for the Ly-alpha forest: power spectrum forecasts for baryon acoustic oscillation experiments
• Detecting baryon acoustic oscillations by 3d weak lensing
• Hydrogen Molecules in the Dark Ages Halos: Thermal Emission vs. Resonant Scattering
• Cosmological models with running cosmological term and decaying dark matter
• Cosmology in doubly coupled massive gravity: constraints from SNIa, BAO and CMB
• Dynamical friction in the primordial neutrino sea
• A thermodynamic point of view on dark energy models
• On the concordance of cosmological data in the case of the generalized Chaplygin gas
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• Predictions for measuring the cross power spectrum of the HI 21-cm signal and the Lyman-$\alpha$ forest using OWFA
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• Thermal and Resonant Emission of Dark Ages Halos in the Rotational Lines of HeH${}^{+}$
• Measuring the BAO peak position with different galaxy selections
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Distance-duality in theories with a nonminimal coupling to gravity
• Halo Mass-Concentration Relation at High-Mass End
• Scale-dependent bias from the primordial non-Gaussianity with a Gaussian-squared field
• Tomography-based observational measurements of the halo mass function via the submillimeter magnification bias
• The alignment of galaxies at the Baryon Acoustic Oscillation scale
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• The full-sky Spherical Fourier-Bessel power spectrum in general relativity
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• On the primordial origin of the smoothing excess in the $Planck$ temperature power spectrum in light of LSS data
• A Study on the Baryon Acoustic Oscillation with Topological Data Analysis
• Halo Concentrations and the New Baseline X-ray Luminosity-Temperature and Mass Relations of Galaxy Clusters
• An analytical method to simulate the HI 21-cm visibility signal for intensity mapping experiments
• Halo Model Analysis of Cluster Statistics
• Cosmological constraints on dark energy
• Current cosmological constraints on the curvature, dark energy and modified gravity
• Abundance and evolution of galaxy clusters in cosmological models with massive neutrino
• Is the misalignment of the Local Group velocity and the 2MASS Redshift Survey dipole typical in a LambdaCDM model?
• First and second order cosmological perturbations in light mass Galileon models
• An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
• Scale-dependent Bias from the Reconstruction of Non-Gaussian Distributions
• Cosmic Shear E/B-mode Estimation with Binned Correlation Function Data
• Unravelling cosmic velocity flows: a Helmholtz-Hodge decomposition algorithm for cosmological simulations
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Gravitational Lensing Effects on the Baryonic Acoustic Oscillation Signature in the Redshift-Space Correlation Function
• Starlight from JWST: Implications for star formation and dark matter models
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Towards $21$-cm intensity mapping at $z=2.28$ with uGMRT using the tapered gridded estimator -- IV. Wideband analysis
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Model-Independent Measurement of the Matter-Radiation Equality Scale in DESI 2024
• Signatures of the Baryon Acoustic Oscillations on the Convergence Power Spectrum of Weak lensing by Large Scale Structure
• Tests of Standard Cosmology in Horava Gravity and Bayesian Evidence for a Closed Universe, and the Hubble Tension
• New initial condition of the new agegraphic dark energy model
• Lightcone Averaging and Precision Cosmology
• Constraining Thawing Dark Energy using Galaxy Cluster Number Counts
• Cosmological constraints from multiple tracers in spectroscopic surveys
• How an era of kination impacts substructure and the dark matter annihilation rate
• Machine learning unveils the linear matter power spectrum of modified gravity
• Skewness as a probe of Baryon Acoustic Oscillations
• First test of the consistency relation for the large-scale structure using the anisotropic three-point correlation function of BOSS DR12 galaxies (An explanatory video is available at https://youtu.be/Zi36ooLPhss.)
• 21 cm power spectrum in interacting cubic Galileon model
• Towards $21$-cm intensity mapping at $z=2.28$ with uGMRT using the tapered gridded estimator II: Cross-polarization power spectrum
• Inflationary and phase-transitional primordial magnetic fields in galaxy clusters
• Cosmological evolution of the gravitational entropy of the large-scale structure
• Cosmological implications of different baryon acoustic oscillation data
• Cosmological Implications and Physical Properties of an X-Ray Flux-Limited Sample of Galaxy Clusters
• Symbolic Implementation of Extensions of the $\text{PyCosmo}$ Boltzmann Solver
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Anisotropies in the redshift-space correlations of galaxy groups and clusters II: Analysis of observational cluster samples
• Apparent parity violation in the observed galaxy trispectrum
• Non-local scalar fields inflationary mechanism in light of Planck $2013$
• Cosmic expansion and structure formation in running vacuum cosmologies
• Clustering GCG: a viable option for unified dark matter-dark energy?
• Shape and Spin of Minihaloes: From Large Scales to the Centres
• Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations
• Non minimally coupled condensate cosmologies: matching observational data with phase space
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• Gravitational lensing effects on sub-millimetre galaxy counts
• Modelling Time-varying Dark Energy with Constraints from Latest Observations
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Modified initial power spectrum and too big to fail problem
• Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
• Self-Interacting Dark Matter Scattering Rates Through Cosmic Time
• Cosmological constrains on fast transition Unified Dark Energy/Matter models
• Optimising tomography for weak gravitational lensing surveys
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• Quasi-periodical features in the distribution of Luminous Red Galaxies
• Generalized framework for likelihood-based field-level inference of growth rate from velocity and density fields
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• Perturbations of Cosmological Redshift Drift
• Observational constraint on dynamical evolution of dark energy
• Cosmological Constraint from the 2dF QSO Spatial Power Spectrum
• Gravitational corrections to light propagation in a perturbed FLRW-universe and corresponding weak lensing spectra
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Smoothing the redshift distributions of random samples for the baryon acoustic oscillations : applications to the SDSS-III BOSS DR12 and QPM mock samples
• Revisiting Cardassian Model and Cosmic Constraint
• SIMPLE: Simple Intensity Map Producer for Line Emission
• Effects of dark matter pressure on the ellipticity of cosmic voids
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• Constraints on the $\Lambda$CDM model with redshift tomography
• Intrinsic size correlations in weak lensing
• A direct probe of cosmological power spectra of the peculiar velocity field and the gravitational lensing magnification from photometric redshift surveys
• Simulating the z = 3.35 HI 21-cm visibility signal for the Ooty Wide Field Array(OWFA)
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• Impacts on Cosmological Constraints from Degeneracies
• Two-point statistics without bins: A continuous-function generalization of the correlation function estimator for large-scale structure
• Re-examining the role of curvature in the slowing down acceleration scenario
• Tests of Acoustic Scale Shifts in Halo-based Mock Galaxy Catalogues
• Plasma Suppression of Large Scale Structure Formation in the Universe
• Clustering, Cosmology and a New Era of Black Hole Demographics -- I. The Conditional Luminosity Function of Active Galactic Nuclei
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• X-ray cluster cosmology
• Radiative transfer of Lyman-$\alpha$ photons at cosmic dawn with realistic gas physics
• Numerical convergence of pre-initial conditions on dark matter halo properties
• Impact of photometric redshifts on the galaxy power spectrum and BAO scale in the LSST survey
• Observational constraints on G-corrected holographic dark energy using a Markov chain Monte Carlo method
• Condition for dust evacuation from the first galaxies
• Measuring Cosmological Parameters with the SDSS QSO Spatial Power Spectrum Analysis to Test the Cosmological Principle
• Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
• On the statistical theory of self-gravitating collisionless dark matter flow
• Probing the cosmic acceleration from combinations of different data sets
• Cluster Assembly Times as a Cosmological Test
• Over-cooled haloes at z > 10: a route to form low-mass first stars
• The removal of shear-ellipticity correlations from the cosmic shear signal: Influence of photometric redshift errors on the nulling technique
• The environment-dependence of the growth of the most massive objects in the Universe
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• Constraining dark energy using observational growth rate data
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Cosmological test of an extended quintessence model
• Angular momentum in cluster Spherical Collapse Model
• Investigating the Possibility of a Turning Point in the Dark Energy Equation of State
• Cosmological Model-independent Gamma-ray Bursts Calibration and its Cosmological Constraint to Dark Energy
• What is the origin of the JWST SMBHs?
• Baryon acoustic oscillations with the cross-correlation of spectroscopic and photometric samples
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Addressing the $r_d$ Tension using Late-Time Observational Measurements in a Novel deceleration Parametrization
• A New Probe of the High-z BAO scale: BAO tomography With CMB $\times$ LIM-Nulling Convergence
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Warm Dark Matter versus Bumpy Power Spectra
• Void Lensing in Cubic Galileon Gravity
• Large-scale clustering of buried X-ray AGN: Trends in AGN obscuration and redshift evolution
• Cosmic Void Baryon Acoustic Oscillation Measurement: Evaluation of Sensitivity to Selection Effects
• On the viability of a certain vector-tensor theory of gravitation
• Cosmological consequences of Modified Gravity (MOG)
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• A Model for the Redshift-Space Galaxy 4-Point Correlation Function
• Intensity mapping of post-reionization 21-cm signal and its cross-correlations as a probe of $f(R)$ gravity
• 2D BAO vs 3D BAO: Hints for new physics?
• Extended Fast Action Minimisation method: application to SDSS-DR12 Combined Sample
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• Constraints on the Hubble and matter density parameters with and without modelling the CMB anisotropies
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Refining the nonlinear modelling of primordial oscillatory features
• Squeezing Full-Shape Dynamical Dark Energy Constraints with Galaxy Alignments
• Differentiable Cosmological Hydrodynamics for Field-Level Inference and High Dimensional Parameter Constraints
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
• Matching JWST UV Luminosity Functions with Refined $\Lambda$CDM Halo Models
• Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity
• Cosmic accretion shocks as a tool to measure the dark matter mass of galaxy clusters
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• Probing Quintessence using BAO imprint on the cross-correlation of weak lensing and post-reionization HI 21 cm signal
• Constraining warm dark matter power spectrum using the cross-correlation of HI 21 cm signal and the Lyman-$\alpha$ forest
• The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass
• Redshifted 21-cm emission signal from the halos in Dark Ages
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Can the homogeneity scale be used as a standard ruler?
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• Ellipticity and prolaticity of the initial gravitational-shear field at the position of density maxima
• Power Spectrum Analysis of the 2dF QSO Sample Revisited
• On a quadratic equation of state and a universe mildly bouncing above the Planck temperature
• Beyond boundaries of redshift surveys: assessing mass fluctuations on "super-survey" scales
• Mass - concentration relation and weak lensing peak counts
• Two-point correlation function of density perturbations in a large void universe
• Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
• On the $2^{\text{nd}}$ feature of the matter two-point function
• DUET - The Dark Universe Exploration Telescope
• Cosmological extrapolation of MOND
• Growth rate of matter perturbations as a probe of large-scale magnetism
• Primordial Non-Gaussianity from LAMOST Surveys
• A large change in the predicted number of small halos due to a small amplitude oscillating inflaton potential
• Lowering the Horizon on Dark Energy: A Late-Time Response to Early Solutions for the Hubble Tension
• Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results
• The eventful life journey of galaxy clusters. I. Impact of DM halo and ICM properties on their full assembly histories
• Stability of small-scale baryon perturbations during cosmological recombination
• Confronting the damping of the baryon acoustic oscillations with observation
• Population III star formation: multiple gas phases prevent the use of an equation of state at high densities
• Gravitational potential evolution in Unified Dark Matter Scalar Field Cosmologies: an analytical approach
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Constraints on dark energy evolution
• Data Analysis and Phenomenological Cosmology
• The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
• Numerical implementation of the Cubic Galileon model in PINOCCHIO
• Dark matter haloes: a multistream view
• Modelling the impact of intrinsic size and luminosity correlations on magnification estimation
• Overconstrained dynamics in galaxy redshift surveys
• Lagrangian perturbations theory : Third-order solution for general dark energy models
• The 4MOST-Cosmology Redshift Survey: Target Selection of Bright Galaxies and Luminous Red Galaxies
• Superclusters from velocity divergence fields
• Information content in anisotropic cosmological fields: Impact of different multipole expansion scheme for galaxy density and ellipticity correlations
• High-redshift Galaxies from JWST Observations in More Realistic Dark Matter Halo Models
• The Low Redshift survey at Calar Alto (LoRCA)
• Reionization and CMB non-Gaussianity
• The constraint ability of Hubble parameter by gravitational wave standard sirens on cosmological parameters
• Large-scale periodicity in the distribution of QSO absorption-line systems
• Observing Baryon Oscillations with Cosmic Shear
• Non-linear Matter Spectrum for a Variable Equation of State
• Testing and selecting cosmological models with ultra-compact radio quasars
• Fitting formulae of the reduced-shear power spectrum for weak lensing
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Halo Concentrations and the Fundamental Plane of Galaxy Clusters
• Dark matter cooling during early matter-domination boosts sub-earth halos
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• $H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
• Quasi-periodical components in the radial distributions of cosmologically remote objects
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• Local Limit of Nonlocal Gravity: A Teleparallel Extension of General Relativity
• Updated reduced CMB data and constraints on cosmological parameters
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection
• Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
• CMB B-mode polarization from Thomson scattering in the local universe
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• Action functional of the Cardassian universe
• Cosmological constraints from galaxy clustering
• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• Critical points of the cosmic velocity field and the uncertainties in the value of the Hubble constant
• The mass and galaxy distribution around SZ-selected clusters
• Cosmological perturbation theory using generalized Einstein de Sitter cosmologies
• Cosmic expansion beyond $\Lambda$CDM: Investigating power-law and logarithmic corrections
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• Constraints on the Helium Abundance from Fast Radio Bursts
• Gravitational Lensing of Dark Energy Models and $\Lambda$CDM Using Observational data in Loop Quantum Cosmology
• Global 21 cm signal: a promising probe of primordial features
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks
• The imprints of galaxy cluster internal dynamics on the Sunyaev-Zeldovich effect
• The cusp-halo relation
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• Using dust to constrain dark matter models
• Cosmology with Galaxy Correlations
• Skewness consistency relation in large-scale structure and test of gravity theory
• Predicting the Sufficient-Statistics Power Spectrum for Galaxy Surveys: A Recipe for $P_{A\ast }(k)$
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• Power-spectrum simulations of radial redshift distributions
• An Algorithm to locate the centers of Baryon Acoustic Oscillations
• Gravitational Fluctuations as an Alternative to Inflation II. CMB Angular Power Spectrum
• A Parameter-free Statistical Measurement of Halos with Power Spectra
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Unimodular Theory of Gravity in Light of the Latest Cosmological Data
• Constraint on the growth factor of the cosmic structure from the damping of the baryon acoustic oscillation signature
• On the possibility of Baryon Acoustic Oscillation measurements at redshift $z>7.6$ with the Roman Space Telescope
• A new pressure-parametric cosmological model
• E and B modes of the CMB y-type distortions: polarised kinetic Sunyaev-Zeldovich effect from the reionisation and post-reionisation eras
• Particle production during inflation: constraints expected from redshifted 21 cm observations from the epoch of reionization
• Monopole Fluctuations in Galaxy Surveys
• Metamorphosis of dwarf halo density profile under dark matter decays
• Impact of Large-Scale Structure Systematics on Cosmological Parameter Estimation
• Cosmological constraints from galaxy multi-tracers in the nearby Universe
• On the tomographic cluster clustering as a cosmological probe
• Constraining LTB models with JLA supernovae and BAO
• Model independent calibration for sound horizon combining observations of supernovae and transversal BAO measurements
• A cosmic speed-trap: a gravity-independent test of cosmic acceleration using baryon acoustic oscillations
• Constraining Recent Oscillations in Quintessence Models with Euclid
• Dark aspects of massive spinor electrodynamics
• Estimating the evolution of gas in the Fornax dwarf spheroidal galaxy from its star formation history: an illustrative example
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• A comparison of shrinkage estimators of the cosmological precision matrix
• Mass scaling relations for dark halos from an analytic universal outer density profile
• An implementation of nDGP gravity in Pinocchio
• The Statistics of Cosmological Lyman-alpha Absorption
• Direct Determination of Expansion History Using Redshift Distortions
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Comparison of the linear bias models in the light of the Dark Energy Survey
• Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes
• Primordial fluctuations from deformed quantum algebras
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• The Effect of Corner Modes in the Initial Conditions of Cosmological Simulations
• Testing the Constancy of Type Ia Supernova Luminosities with Gaussian Process
• STRAWBERRY: Finding haloes in the gravitational potential
• Learning from Topology: Cosmological Parameter Estimation from the Large-scale Structure
• The same with less: The cosmic web of warm versus cold dark matter dwarf galaxies
• Morpho-statistical characterisation of the spatial galaxy distribution through Gibbs point processes
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Informational corrections to the early-Universe radiation sector: CET Omega, WIMP freeze-out, and implications for a possible 20 GeV gamma-ray excess
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• A semi-cosmographic approach to study cosmological evolution in phase space
• Ricci cosmology in light of astronomical data
• A gigaparsec-scale local void and the Hubble tension
• The equation and solution of 4-point correlation function of galaxies in Gaussian approximation and its parity-odd part
• Accelerating BAO Scale Fitting Using Taylor Series
• Extracting the BAO scale from BOSS DR12 dataset
• Cosmological Forecasts from the Baryon Acoustic Oscillations in 21cm Intensity Mapping
• Fluids in cosmology
• Does History Repeat Itself? Periodic Time Cosmology
• Solar System Tests of a New Class of $f(z)$ Theory
• Linear perturbations in spherically symmetric dust cosmologies including a cosmological constant
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Constraining cosmology with N-body simulations for future spectroscopic galaxy surveys at $2\le z\le 3$
• Weak lensing of bright standard sirens: prospects for ${\sigma }_8$
• The Diversity of Core Halo Structure in the Fuzzy Dark Matter Model
• Understanding CMB physics through the exploration of exotic cosmological models: a classroom study using CLASS
• Intrinsic alignment boosting: Direct measurement of intrinsic alignments in cosmic shear data
• Motion of the Local Group as a cosmological probe
• Interacting Quintessence and Growth of Structure
• Baryon Acoustic Oscillations from galaxy surveys
• Implications of the cosmic infrared background excess for the cosmic star formation
• Cosmological Constraints on the Undulant Universe
• Layered dark structure with a Structuring Field: A $Z_4$-symmetric Inert Doublet-Singlet realization and implications for the $S_8$ tension
• The Impact of Spectroscopic Redshift Errors on Cosmological Measurements
• From Geometry to Observation: Gravitational Waves and the Raychaudhuri Equation
• On the energy flow of $\lambda$ in Hořava-Lifshitz cosmology
• Benchmarking field-level cosmological inference from galaxy redshift surveys
• Probing dark energy with braneworld cosmology in the light of recent cosmological data
• Quantum geometry from commutators: a Heisenberg-picture framework and a toy application to early structure
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Constraining the lensing dispersion from the angular clustering of binary black hole mergers
• Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey quasar sample: Testing observational systematics on the Baryon Acoustic Oscillation measurement
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data
• Influence of Plasma Collective Effects on Cosmological Evolution
• Probing dark energy using anisotropies in the clustering of post-EoR HI distribution
• Improved Methods for Estimating Peculiar Velocity Correlation Functions Using Volume Weighting
• Interacting dark energy from redshift-space galaxy clustering
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Addressing Dipole Tension via Clustering in $\Lambda$CDM and beyond
• Can we remove the systematic error due to isotropic inhomogeneities?
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• A joint measurement of galaxy luminosity functions and large-scale field densities during the Epoch of Reionization
• Probing small-scale baryon and dark matter isocurvature perturbations with cosmic microwave background anisotropies
• Dynamics of tachyon dark energy on large scales and its imprint on observed galaxy power spectrum
• Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum
• Probing cosmic velocity-density correlations with galaxy luminosity modulations
• Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario
• Testing the effects from dark radiation
• Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Built-in precision: Improving cluster cosmology through the self-calibration of a galaxy cluster sample
• Extended datasamples under the lens of Brane World Theory
• Iterative reconstruction excursions for Baryon Acoustic Oscillations and beyond
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
• Prompt cusps in hierarchical dark matter halos: Implications for annihilation boost
• Tidal adaptive softening and artificial fragmentation in cosmological simulations
• Baryon-photon interactions in Resummed Kinetic Field Theory
• Exploring the constraints on cosmological models with CosmoEJS
• The BAO scale -- how standard is the standard ruler?
• Cosmology from Large Scale Structure
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• The signature of major mergers on the hydrostatic mass bias of galaxy clusters
• Wasserstein Distance in Cosmological Structure Formation: An Optimal Transport Perspective
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics
• Slow neutrinos: non-linearity and momentum-space emulation
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal