The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications

Abstract

We present a power spectrum analysis of the final 2dF Galaxy Redshift Survey, employing a direct Fourier method. The sample used comprises 221,414 galaxies with measured redshifts. We investigate in detail the modelling of the sample selection. A new angular mask is derived, based on revisions to the photometric calibration. The redshift selection function is determined by dividing the survey according to rest-frame colour, and deducing a self-consistent treatment of k-corrections and evolution for each population. The covariance matrix for the power-spectrum estimates is determined using two different approaches to the construction of mock surveys which are used to demonstrate that the input cosmological model can be correctly recovered. We are confident that the 2dFGRS power spectrum can be used to infer the matter content of the universe. On large scales, our estimated power spectrum shows evidence for the `baryon oscillations' that are predicted in CDM models. Fitting to a CDM model, assuming a primordial $n_s=1$ spectrum, $h=0.72$ and negligible neutrino mass, the preferred parameters are ${\Omega }_{M}h=0.168\pm 0.016$ and a baryon fraction ${\Omega }_b/{\Omega }_M=0.185\pm 0.046$ (1$\sigma$ errors). The value of ${\Omega }_{M}h$ is $1\sigma$ lower than the $0.20\pm 0.03$ in our 2001 analysis of the partially complete 2dFGRS. This shift is largely due to the signal from the newly-sampled regions of space, rather than the refinements in the treatment of observational selection. This analysis therefore implies a density significantly below the standard ${\Omega }_M=0.3$: in combination with CMB data from WMAP, we infer ${\Omega }_M=0.231\pm 0.021$. (Abridged.)

Updated to match the in press MNRAS version. P(k) data and covariance matrix available at http://www.mso.anu.edu.au/2dFGRS/Public/Release/PowSpec

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• Constraints on the Sound Speed of Dynamical Dark Energy
• Particle Production During Inflation: Observational Constraints and Signatures
• Constraining The Early-Universe Baryon Density And Expansion Rate
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• Viscous dark fluid universe
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• f(R) Gravity with Torsion: The Metric-Affine Approach
• Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of ${\sigma }_8$
• Cosmic Emulation: Fast Predictions for the Galaxy Power Spectrum
• The Hubble Constant
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Assessment of the Information Content of the Power Spectrum and Bispectrum
• Relic gravitational waves and their detection
• A new approach to simulating collisionless dark matter fluids
• Baryon acoustic signature in the clustering of density maxima
• Revealing the galaxy-halo connection in IllustrisTNG
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• Cosmological constraints on a decomposed Chaplygin gas
• Dynamics of Interacting Quintessence Models: Observational Constraints
• Effects of dark sectors' mutual interaction on the growth of structures
• Some remarks on the dynamical systems approach to fourth order gravity
• The Physics and Early History of the Intergalactic Medium
• An optimal FFT-based anisotropic power spectrum estimator
• Statistical Analysis of Galaxy Surveys-II. The 3-point galaxy correlation function measured from the 2dFGRS
• Universal fitting formulae for baryon oscillation surveys
• Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
• Accelerating f(T) gravity models constrained by recent cosmological data
• The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with 3-point correlation functions
• Observational bounds on the cosmic radiation density
• On the connectivity of the cosmic web: theory and implications for cosmology and galaxy formation
• Recovering a MOND-like acceleration law in mimetic gravity
• Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields
• Voids as a Precision Probe of Dark Energy
• Improving measurements of H(z) and Da(z) by analyzing clustering anisotropies
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• The phase space density of fermionic dark matter haloes
• High Energy Positrons and the WMAP Haze from Exciting Dark Matter
• Measuring dark energy with the $E_{\mathrm{iso}}-E_{\mathrm{p}}$ correlation of gamma-ray bursts using model-independent methods
• Variability selected high-redshift quasars on SDSS Stripe 82
• Cosmological parameter constraints for Horndeski scalar-tensor gravity
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from the Third Data Release Quasar Lens Catalog
• Why multi-tracer surveys beat cosmic variance
• The New Horizon Run Cosmological N-Body Simulations
• A Scale-Dependent Power Asymmetry from Isocurvature Perturbations
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• Modeling the angular correlation function and its full covariance in Photometric Galaxy Surveys
• Improved Measurements of the CMB Power Spectrum with ACBAR
• Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
• On the co-existence of matter dominated and accelerating solutions in f(G)-gravity
• Internal space structure generalization of the quintom cosmological scenario
• Thermal history of the plasma and high-frequency gravitons
• Measuring neutrino masses with a future galaxy survey
• 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
• Investigating dark energy experiments with principal components
• The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: final Emission Line Galaxy Target Selection
• The Art of Lattice and Gravity Waves from Preheating
• 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
• Baryon Acoustic Oscillations from the SDSS DR10 galaxies angular correlation function
• Angular Baryon Acoustic Oscillation measure at z=2.225 from the SDSS quasar survey
• Statistics of Voids in the 2dF Galaxy Redshift Survey
• Constraints on the identity of the dark matter from strong gravitational lenses
• ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD
• Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
• Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study
• CMB Constraints on a Stochastic Background of Primordial Magnetic Fields
• Satellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matter
• The Weak Lensing Signal and the Clustering of BOSS Galaxies I: Measurements
• Predicting Future Space Near-IR Grism Surveys using the WFC3 Infrared Spectroscopic Parallels Survey
• Simulations of Baryon Oscillations
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• Comparing approximate methods for mock catalogues and covariance matrices I: correlation function
• nIFTy Cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics
• Wide Angle Effects in Future Galaxy Surveys
• Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements
• Dark energy perturbations and cosmic coincidence
• A General Analysis of Direct Dark Matter Detection: From Microphysics to Observational Signatures
• Observational Evidence of the Accelerated Expansion of the Universe
• Dynamics of f(R)-cosmologies containing Einstein static models
• A clear and measurable signature of modified gravity in the galaxy velocity field
• Evaluating backreaction with the peak model of structure formation
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
• On the Validity of Cosmological Fisher Matrix Forecasts
• Information content of the non-linear power spectrum: the effect of beat-coupling to large scales
• Fast and accurate mock catalogue generation for low-mass galaxies
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• An analytic model for the bispectrum of galaxies in redshift space
• Cosmological perturbation theory in 1+1 dimensions
• On Minimally-Parametric Primordial Power Spectrum Reconstruction and the Evidence for a Red Tilt
• Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
• Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• Spherical collapse model in dark energy cosmologies
• Mapping Growth and Gravity with Robust Redshift Space Distortions
• The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample
• Power spectrum for the Bose-Einstein condensate dark matter
• Estimation of Primordial Spectrum with post-WMAP 3 year data
• New Constraints on the Primordial Magnetic Field
• Probing the Early Universe with Axion Physics and Gravitational Waves
• A new framework for studying spherically symmetric static solutions in f(R) gravity
• Cosmological dynamics with non-linear interactions
• Fast simulations for intensity mapping experiments
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Nonlinear growth in modified gravity theories of dark energy
• Galaxy Formation in WDM Cosmology
• An exact quantification of backreaction in relativistic cosmology
• Exact solutions of three dimensional black holes: Einstein gravity vs F(R) gravity
• Revisiting the Baryon Fractions of Galaxy Clusters: A Comparison with WMAP 3-year Results
• The Search for a Primordial Magnetic Field
• Magnetized CMB observables: a dedicated numerical approach
• Near-ultraviolet Spectroscopy of Star-forming Galaxies from eBOSS: Signatures of Ubiquitous Galactic-scale Outflows
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5
• Scientific Synergy Between LSST and Euclid
• DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
• Observational Requirements for Lyman-alpha Forest Tomographic Mapping of Large-Scale Structure at z ~ 2
• An improved cosmological bound on the thermal axion mass
• Spherical collapse model with shear and angular momentum in dark energy cosmologies
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Clarifying the effects of interacting dark energy on linear and nonlinear structure formation processes
• Cosmological Evolution in f(R,T) theory with Collisional Matter
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions
• Simulating Redshift-Space Distortions for Galaxy Pairs with Wide Angular Separation
• The Santiago-Harvard-Edinburgh-Durham void comparison II: unveiling the Vainshtein screening using weak lensing
• Constraining the Dark Energy Equation of State with HII Galaxies
• Empirical H-alpha emitter count predictions for dark energy surveys
• Galaxy clustering from COMBO-17: The halo occupation distribution at <z>=0.6
• On the complementarity of galaxy clustering with cosmic shear and flux magnification
• The Redshift Space Momentum Power Spectrum II: measuring the growth rate from the combined 2MTF and 6dFGSv surveys
• Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case
• Anatomy of luminosity functions: the 2dFGRS example
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• Massive neutrinos and cosmic composition
• Gravitational lensing in fourth order gravity
• Evidence for cosmological particle creation?
• Determining the WIMP mass using direct detection experiments
• Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
• Probing the Epoch of Early Baryonic Infall Through 21cm Fluctuations
• Galaxy Groups in the 2dFGRS: the number density of groups
• Reionization and Galaxy Formation in Warm Dark Matter Cosmologies
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Can dark energy be expressed as a power series of the Hubble parameter?
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• Early galaxy formation in warm dark matter cosmologies
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• Scale Dependent Galaxy Bias in the SDSS as a function of Luminosity and Colour
• Looking for interactions in the cosmological dark sector
• Dark Energy in Practice
• Cosmology of neutrinos and extra light particles after WMAP3
• Dark Energy: Recent Developments
• Quintessence reconstructed: new constraints and tracker viability
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations
• Einstein's Universe: Cosmological structure formation in numerical relativity
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. I. Which Environment Affects Galaxy Evolution?
• Kinetic k-essence ghost dark energy model
• Cosmological hydrogen recombination: The effect of extremely high-n states
• Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\Lambda$CDM
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• On the Luminosity Dependence of the Galaxy Pairwise Velocity Dispersion
• The galaxy power spectrum: precision cosmology from large scale structure?
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Cosmography beyond standard candles and rulers
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Are cosmological neutrinos free-streaming?
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Independent Cosmological Constraints from high-z HII Galaxies
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• Constraining Lorentz violation with cosmology
• Interacting Dark Energy in f(T) cosmology : A Dynamical System analysis
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• Density Perturbations for Running Cosmological Constant
• Higher-order gravity and the cosmological background of gravitational waves
• The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements
• Statistical methods in cosmology
• Red Giants in the Small Magellanic Cloud. I. Disk and Tidal Stream Kinematics
• Bayesian analysis of Friedmannless cosmologies
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• Constraining dark energy with gamma-ray bursts
• Overcoming the Circular Problem for γ-ray Bursts in Cosmological Global Fitting Analysis
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• Reliability of the detection of the Baryon Acoustic Peak
• Reconstructing a general inflationary action
• BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space
• A cosmological concordance model with dynamical vacuum term
• Gravitational energy as dark energy: Concordance of cosmological tests
• B-modes and the Nature of Inflation
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample
• Large-Scale Structure of the Universe as a Cosmic Standard Ruler
• Active galactic nuclei and massive galaxy cores
• Measuring the transverse baryonic acoustic scale from the SDSS DR11 galaxies
• How clustering dark energy affects matter perturbations
• Galaxy redshift surveys selected by neutral hydrogen using FAST
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
• Determining the WIMP mass from a single direct detection experiment, a more detailed study
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• Cosmic microwave anisotropies from BPS semilocal strings
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering
• Dynamical analysis on $f(R,\mathcal{G})$ cosmology
• Anisotropic perturbations due to dark energy
• Constraint on the Effective Number of Neutrino Species from the WMAP and SDSS LRG Power Spectra
• The High Redshift Integrated Sachs-Wolfe Effect
• Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
• Cosmological constraints on neutrino plus axion hot dark matter
• The cosmological constant as an eigenvalue of f(R)-gravity Hamiltonian constraint
• How closely do baryons follow dark matter on large scales?
• An iterative reconstruction of cosmological initial density fields
• Can a galaxy redshift survey measure dark energy clustering?
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• Imprint of galaxy clustering in the cosmic gamma-ray background
• The cosmology of an holographic induced gravity model with curvature effects
• Remarks on the formulation of the cosmological constant/dark energy problems
• Matter Power Spectrum Covariance Matrix from the DEUS-PUR ΛCDM simulations: Mass Resolution and non-Gaussian Errors
• The foreground wedge and 21 cm BAO surveys
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• Methods for Bayesian power spectrum inference with galaxy surveys
• Theoretical Systematics of Future Baryon Acoustic Oscillation Surveys
• Streaming velocities and the baryon-acoustic oscillation scale
• Evolution of density perturbations in decaying vacuum cosmology
• Determining Cosmological Parameters with Latest Observational Data
• Can all cosmological observations be accurately interpreted with a unique geometry?
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Bayesian optimal reconstruction of the primordial power spectrum
• Cosmographic parameters in model-independent approaches
• Transient cosmic acceleration from interacting fluids
• Attractive Lagrangians for Noncanonical Inflation
• The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
• Unified dark fluid in Brans-Dicke theory
• 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
• Response function of the large-scale structure of the universe to the small scale inhomogeneities
• 21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction
• Oscillations in the dark energy EoS: new MCMC lessons
• Systematic effects in the sound horizon scale measurements
• A New Test of the Statistical Nature of the Brightest Cluster Galaxies
• Superclusters of galaxies in the 2dF redshift survey. III. The properties of galaxies in superclusters
• Ruling out the Modified Chaplygin Gas Cosmologies
• Duty Cycle and the Increasing Star Formation History of z>=6 Galaxies
• F(R) gravity's rainbow and its Einstein counterpart
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multi-tracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate
• Large-Scale Structure Observables in General Relativity
• Dynamical Dark Energy simulations: high accuracy Power Spectra at high redshift
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: II. Fourier and Redshift Space
• Is cosmology compatible with sterile neutrinos?
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• Baryon Oscillations and Consistency Tests for Photometrically-Determined Redshifts of Very Faint Galaxies
• The Acoustic Peak in the Lyman Alpha Forest
• Improving Photometric Redshift Estimation using GPz: size information, post processing and improved photometry
• Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7
• Particle mesh simulations of the Lyman-alpha forest and the signature of Baryon Acoustic Oscillations in the intergalactic medium
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Dark energy records in lensed cosmic microwave background
• Cross-correlating WMAP5 with 1.5 million LRGs: a new test for the ISW effect
• Primordial non-Gaussianity from the Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey I: Catalogue Preparation and Systematic Mitigation
• Generalization of Regular Black Holes in General Relativity to $f(R)$ Gravity
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• On the signature of $z\sim 0.6$ superclusters and voids in the Integrated Sachs-Wolfe effect
• Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope
• The nonlinear matter power spectrum
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• Appeasing the Phantom Menace?
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• What is the best way to measure baryonic acoustic oscillations?
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Effects of cosmological model assumptions on galaxy redshift survey measurements
• Mass Function of Rich Galaxy Clusters and Its Constraint on sigma_8
• Fourier analysis of multi-tracer cosmological surveys
• Exploring stable models in $f(R;T;R_{\mu \nu }{T}^{\mu \nu })$ gravity
• Is the evidence for dark energy secure?
• Cosmic perturbations with running G and Lambda
• Hierarchical clustering in chameleon $f(R)$ gravity
• Cosmography of f(R) - brane cosmology
• Galaxy and Mass Assembly (GAMA): The evolution of bias in the radio source population to z ~ 1.5
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Cosmology with matter diffusion
• The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
• Planck intermediate results. XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• Realizing Scale-invariant Density Perturbations in Low-energy Effective String Theory
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Too small to succeed? Lighting up massive dark matter subhaloes of the Milky Way
• Testing gravity with motion of satellites around galaxies: Newtonian gravity against Modified Newtonian Dynamics
• Redshift Measurement and Spectral Classification for eBOSS Galaxies with the Redmonster Software
• Model independent constraints on the cosmological expansion rate
• $f(R,T)=f(R)+\lambda T$ gravity models as alternatives to cosmic acceleration
• Beyond consistency test of gravity with redshift-space distortions at quasi-linear scales
• Cosmological surveys with the Australian Square Kilometre Array Pathfinder
• How well will ton-scale dark matter direct detection experiments constrain minimal supersymmetry?
• Observational tests of non-adiabatic Chaplygin gas
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
• Constraining warm dark matter with cosmic shear power spectra
• The Cosmological Mean Density and its Local Variations Probed by Peculiar Velocities
• FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
• Nongaussianity from Particle Production During Inflation
• Hubble Space Telescope Observations of Nine High-Redshift ESSENCE Supernovae
• Cosmological Constraints on Decaying Dark Matter
• Age constraints on the cosmic equation of state
• Predicting Hα emission line galaxy counts for future galaxy redshift surveys
• Early Dark Energy at High Redshifts: Status and Perspectives
• Toward understanding rich superclusters
• Analytic rotating black hole solutions in $N$-dimensional $f(T)$ gravity
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
• Astrophysical constraints on extended gravity models
• Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\mathrm{eff}}$=0.85 from the final dataset
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Probing deviations from General Relativity with the Euclid spectroscopic survey
• Cosmological observations in a modified theory of gravity (MOG)
• Phantom-Like Behavior in $f(R)$-Gravity
• Unbiased methods for removing systematics from galaxy clustering measurements
• Cosmological dynamics of fourth order gravity: A compact view
• A step towards testing general relativity using weak gravitational lensing and redshift surveys
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Pairwise-Inverse-Probability and Angular Correction for Fibre Collisions in Clustering Measurements
• Linearisation with Cosmological Perturbation Theory
• Cosmological distance indicators
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Reconstruction of the neutrino mass as a function of redshift
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Regarding the Line-of-Sight Baryonic Acoustic Feature in the Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey Luminous Red Galaxy Samples
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• Lensing Corrections to Features in the Angular Two-Point Correlation Function and Power Spectrum
• First Detection of the BAO Signal from Early DESI Data
• Baryon effects on void statistics in the EAGLE simulation
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• Subhalo statistics of galactic halos: beyond the resolution limit
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
• Non-linear evolution of the BAO scale in alternative theories of gravity
• Holography and the scale-invariance of density fluctuations
• Selection Functions in Astronomical Data Modeling, with the Space Density of White Dwarfs as Worked Example
• Revisiting the WMAP - NVSS angular cross correlation. A skeptic's view
• HI intensity mapping with MeerKAT: 1/f noise analysis
• Scale-dependent Galaxy Bias
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• On the implementation of the spherical collapse model for dark energy models
• Fractal Dimensions of a Weakly Clustered Distribution and the Scale of Homogeneity
• Quintessence with Yukawa Interaction
• When Did Cosmic Acceleration Start ?
• Environment and the cosmic evolution of star formation
• The Redshift Sensitivities of Dark Energy Surveys
• Cosmic distance inference from purely geometric BAO methods: Linear Point standard ruler and Correlation Function Model Fitting
• Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
• Separating out the Alcock-Paczynski Effect on 21cm Fluctuations
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• 3D Spherical Analysis of Baryon Acoustic Oscillations
• New H-band Galaxy Number Counts: A Large Local Hole in the Galaxy Distribution?
• Relativistic Modified Newtonian Dynamics from String Theory?
• Power Spectrum Estimation from Peculiar Velocity Catalogues
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• Early Universe Constraints on Time Variation of Fundamental Constants
• Information Content of Higher-Order Galaxy Correlation Functions
• The evolution of the [OII], Hβ and [OIII] emission-line luminosity functions over the last nine billions years
• The REFLEX II galaxy cluster survey: power spectrum analysis
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• Composite dark energy: cosmon models with running cosmological term and gravitational coupling
• Cosmic Magnetism in Centimeter and Meter Wavelength Radio Astronomy
• Primordial Neutrinos, Cosmological Perturbations in Interacting Dark-Energy Model: CMB and LSS
• Combining perturbation theories with halo models for the matter bispectrum
• Estimating the galaxy two-point correlation function using a split random catalog
• Matter Power Spectrum for the Generalized Chaplygin Gas Model: The Newtonian Approach
• Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology
• Supernova tests of the timescape cosmology
• Constraints on the cosmic expansion rate at redshift 2.3 from the Lyman-$\alpha$ forest
• Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement
• Testing gaussianity, homogeneity and isotropy with the cosmic microwave background
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• The full Fisher matrix for galaxy surveys
• Asymmetric Gravitational Lenses in TeVeS and Application to the Bullet Cluster
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?
• Halo Mass Functions in Early Dark Energy Cosmologies
• Cosmological Constant Problems and Renormalization Group
• Cosmological constraints on general, single field inflation
• Agegraphic dark energy: growth index and cosmological implications
• Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey
• Machine Learning for Observational Cosmology
• Photometric Redshifts from SDSS Images with an Interpretable Deep Capsule Network
• Luminosity distance and anisotropic sky-sampling at low redshifts: a numerical relativity study
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• Observational tests for Λ(t)CDM cosmology
• Analysis of galactic tides and stars on CDM microhalos
• Dynamics and Non-Gaussianity in the Weak-Dissipative Warm Inflation Scenario
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Geodesic Deviation Equation in $f(R,T)$ Gravity
• Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Reionisation in sterile neutrino cosmologies
• Effects of Cosmological Constant on Clustering of Galaxies
• Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
• Estimating the power spectrum covariance matrix with fewer mock samples
• CoLoRe: fast cosmological realisations over large volumes with multiple tracers
• The most general fourth order theory of Gravity at low energy
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• Semi-analytical approach to magnetized temperature autocorrelations
• Spectral Evolution in High Redshift Quasars from the Final BOSS Sample
• Evolution of density perturbations in decaying vacuum cosmology: The case of non-zero perturbations in the cosmological term
• Small-scale galaxy clustering in the EAGLE simulation
• Casimir effect in Extended Theories of Gravity
• Power Spectrum Shape from Peculiar Velocity Data
• Cluster Ellipticities as a Cosmological Probe
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• Chameleonic Generalized Brans--Dicke model and late-time acceleration
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales II: Perturbative and numerical analyses of power spectrum and bispectrum
• An entirely analytical cosmological model
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• The Cosmic Neutrino Background and the Age of the Universe
• Expansion schemes for gravitational clustering: computing two-point and three-point functions
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• Signatures of clumpy dark matter in the global 21 cm background signal
• Backreaction in Cosmology
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Redshift-space streaming velocity effects on the Lyman-$\alpha$ forest baryon acoustic oscillation scale
• Measuring large-scale structure with quasars in narrow-band filter surveys
• Testing gravity with $E_G$: mapping theory onto observations
• Initial Conditions for Non-Canonical Inflation
• The effect of redshift-space distortions on projected 2-pt clustering measurements
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Dissipative Liouville Cosmology: A Case Study
• Cosmology with cosmic web environments I. Real-space power spectra
• Effective growth of matter density fluctuations in the running LCDM and LXCDM models
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Cosmological Constraints on Isocurvature and Tensor Perturbations
• Cosmological models with a Hybrid Scale Factor
• Non-Gravitational Contributions to the Clustering of Ly-alpha Selected Galaxies: Implications for Cosmological Surveys
• Statefinder diagnosis for holographic dark energy in the DGP braneworld
• Abell 2744: Too much substructure for Lambda CDM?
• How does non-linear dynamics affect the baryon acoustic oscillation?
• Forecasting neutrino masses from combining KATRIN and the CMB: Frequentist and Bayesian analyses
• Large-scale galaxy correlations as a test for dark energy
• Reconstructing the history of dark energy using maximum entropy
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Gravitational quantum effects on power spectra and spectral indices with higher-order corrections
• What determines large scale galaxy clustering: halo mass or local density?
• Non-adiabatic Chaplygin gas
• 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
• Inflation from D3-brane motion in the background of D5-branes
• The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• The Post-Newtonian Limit of f(R)-gravity in the Harmonic Gauge
• Evolution in the bias of faint radio sources to z ~ 2.2
• The effects of massive neutrinos on the linear point of the correlation function
• The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
• Matter power spectrum for the generalized Chaplygin gas model: The relativistic case
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Simulations of BAO reconstruction with a quasar Lyman-alpha survey
• Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
• Luminous Red Galaxy Clustering at z~0.7 - First Results using AAOmega
• BAO reconstruction: a swift numerical action method for massive spectroscopic surveys
• The spatial distribution of Milky Way satellites, gaps in streams and the nature of dark matter
• Basics of inflationary cosmology
• Galaxy redshift surveys with sparse sampling
• Gravitational energy and cosmic acceleration
• Exploring Large-scale Structure with Billions of Galaxies
• Expansion history and f(R) modified gravity
• Supernovae and Cosmology
• Keck spectroscopy of z=1-3 ULIRGs from the Spitzer SWIRE survey
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
• Using the cluster mass function from weak lensing to constrain neutrino masses
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• Coupling between cold dark matter and dark energy from neutrino mass experiments
• The Polarization of the Cosmic Microwave Background Due to Primordial Gravitational Waves
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Galaxy surveys, inhomogeneous reionization, and dark energy
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• A Slight Excess of Large Scale Power from Moments of the Peculiar Velocity Field
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Optimal Reconstruction of Baryon Acoustic Oscillations for DESI 2024
• Generalized CMB initial conditions with pre-equality magnetic fields
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Constraining massive gravity with recent cosmological data
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• Self-accelerating the normal DGP branch
• Precision Measurements of Higher-Order Angular Galaxy Correlations Using 11 Million SDSS Galaxies
• Stealth Acceleration and Modified Gravity
• Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
• Quasinormal modes of black holes absorbing dark energy
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• The thermal Sunyaev-Zel'dovich Signature of Baryons in the Local Universe
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Hunting down systematics in baryon acoustic oscillations after cosmic high noon
• Holographic Dark Energy from a Modified GBIG Scenario
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Cosmological model of the interaction between dark matter and dark energy
• A model for the metallicity evolution of damped Lyman-alpha systems
• Constraints on the Primordial Magnetic Field from ${\sigma }_8$
• The Evolution of Our Local Cosmic Domain: Effective Causal Limits
• Broadband distortion modeling in Lyman-$\alpha$ forest BAO fitting
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• Statistical Analysis of Galaxy Surveys-IV: An objective way to quantify the impact of superstructures on galaxy clustering statistics
• Non-Gaussian errors of baryonic acoustic oscillations
• DBI N-flation
• Galaxy Luminosities in 2PIGG groups
• Inflating an Inhomogeneous Universe
• Cosmological tests of modified gravity: constraints on $F(R)$ theories from the galaxy clustering ratio
• Cosmological constraints on dark energy models using DESI BAO 2024
• 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
• Unified Dark Fluid and Cosmic Transit Models in Brans-Dicke Theory
• Dark energy parameterizations and their effect on dark halos
• WMAP 5-year constraints on time variation of $\alpha$ and $m_e$ in a detailed recombination scenario
• A model independent approach to the study of $f(R)$ cosmologies with expansion histories close to $\Lambda$CDM
• Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
• Modelling redshift-space distortion in the post-reionization $\mathrm{HI}$ 21-cm power spectrum
• Consistency check of ΛCDM phenomenology
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• DM haloes in the fifth-force cosmology
• Dark Energy: A Unifying View
• Covariance matrices for halo number counts and correlation functions
• Neutrino masses and mixings in the baryon triality constrained minimal supersymmetric standard model
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• An improved model of redshift-space distortions around voids: application to quintessence dark energy
• Model independent constraints on mass-varying neutrino scenarios
• Using the Topology of Large Scale Structure to constrain Dark Energy
• Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
• Gravitational Lensing with Three-Dimensional Ray Tracing
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Probing Dark Energy with Baryonic Acoustic Oscillations at High Redshifts
• Peculiar Velocities into the Next Generation: Cosmological Parameters From Large Surveys without Bias from Nonlinear Structure
• Bulk Flow and Shear Moments of the SFI++ Survey
• Connected structure in the 2dFGRS
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Constraining the relative velocity effect using the Baryon Oscillation Spectroscopic Survey
• Holographic kinetic k-essence model
• Modified GBIG Scenario as an Alternative for Dark Energy
• Canceling out intensity mapping foregrounds
• Galaxy peculiar velocities and evolution-bias
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• Constraints on oscillating dark energy models
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• High-resolution temporal constraints on the dynamics of dark energy
• Constraints on CDM cosmology from galaxy power spectrum, CMB and SNIa evolution
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• AGN and QSOs in the eROSITA All-Sky Survey -- Part II: The large-scale structure
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Cosmic strings interacting with dark strings
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• Searching for modified gravity with baryon oscillations: from SDSS to wide field multiobject spectroscopy (WFMOS)
• Probing for the Cosmological Parameters with PLANCK Measurement
• Noether gauge symmetry for the Bianchi type I model in f(T) gravity
• A new model for the full shape of the large-scale power spectrum
• Reconstructing the baryon acoustic oscillations using biased tracers
• Statistical coverage for supersymmetric parameter estimation: a case study with direct detection of dark matter
• How well can (renormalized) perturbation theory predict dark matter clustering properties?
• Analytical and EZmock covariance validation for the DESI 2024 results
• Primordial Magnetic Field Effects on the CMB and Large Scale Structure
• On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
• k-essence in the DGP brane-world cosmology
• Testing CCC+TL Cosmology with Observed BAO Features
• Large scale structure and ISW effect in decaying vacuum cosmology
• Typical density profile for warm dark matter haloes
• Astrophysical Tests of Dark Matter Self-Interactions
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Resummed Perturbation Theory of Galaxy Clustering
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• Cross-correlating 21 cm and galaxy surveys: implications for cosmology and astrophysics
• The Variation of the Galaxy Luminosity Function with Group Properties
• The 2MASS galaxy angular power spectrum: Probing the galaxy distribution to Gigaparsec scales
• Barry and the BAO Model Comparison
• Velocity and mass bias in the distribution of dark matter halos
• RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
• Density-dependent clustering: I. Pulling back the curtains on motions of the BAO peak
• Best values of parameters for interacting HDE with GO IR-cutoff in Brans-Dicke cosmology
• Constraints on the neutrino mass and the primordial magnetic field from the matter density fluctuation parameter ${\sigma }_8$
• $\Lambda$CDM is alive and well
• Evolution of the Phase-Space Density of Dark Matter Halos and Mixing Effects in Merger Events
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• Future dynamics in f(R) theories
• Large scale distribution of total mass versus luminous matter from Baryon Acoustic Oscillations: First search in the SDSS-III BOSS Data Release 10
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• The impact of neutrino masses on the determination of dark energy properties
• Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis
• Quantifying the accuracy of the Alcock-Paczynski scaling of baryon acoustic oscillation measurements
• The Standard Cosmological Model
• Observational constraints on the oscillating dark energy cosmologies
• Non-Gaussian Error in Galaxy Survey (Part 1)
• The Unsettled Number: Hubble's Tension
• Optimal ISW detection and joint likelihood for cosmological parameter estimation
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• Holographic dark energy with the sign-changeable interaction term
• Enhanced Inflation in the Dirac-Born-Infeld framework
• Removing BAO-peak Shifts with Local Density Transforms
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• On measuring the absolute scale of baryon acoustic oscillations
• The assembly bias of emission line galaxies
• Photometric Selection of Emission Line Galaxies, Clustering Analysis and a Search for the ISW effect
• Is the baryon acoustic oscillation peak a cosmological standard ruler?
• Tension between SN and BAO: current status and future forecasts
• The effect of dark strings on semilocal strings
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• Numerical investigation of lenses with substructures using the perturbative method
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• Weak Lensing Effects on the Galaxy Three-Point Correlation Function
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• Constraints on Quintessence From Using Cosmological Data
• Effects of biasing on the galaxy power spectrum at large scales
• Improved calculation of relic gravitational waves
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• Homogeneous Gödel-type solutions in hybrid metric-Palatini gravity
• Time variation of the fine structure constant in the early universe and the Bekenstein model
• The clustering of dark matter halos: scale-dependent bias on quasi-linear scales
• Confronting Tracker Field Quintessence with Data
• Spherical collapse model in agegraphic dark energy cosmologies
• Dissipative dark matter and the rotation curves of dwarf galaxies
• The Impact of Non-Gaussianity upon Cosmological Forecasts
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Interacting Tsallis and Rényi Holographic Dark Energy with Hybrid Expansion Law
• Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
• Neutrino spin oscillations in conformally gravity coupling models and quintessence surrounding a black hole
• Extending Recovery of the Primordial Matter Power Spectrum
• What it takes to measure a fundamental difference between dark matter and baryons: the halo velocity anisotropy
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Testing dark matter warmness and quantity via the reduced relativistic gas model
• Constraints on dark energy models from radial baryon acoustic scale measurements
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• 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
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Anisotropic Baryon Acoustic Oscillations measurements in Fourier-space with optimal redshift weights
• A Complete Cosmological Scenario in Teleparallel Gravity
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Phase Space Analysis and Thermodynamics of Interacting Umami Chaplygin gas in FRW Universe
• Raytracing simulations of coupled dark energy models
• Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity
• On the Emergence of Accelerating Cosmic Expansion in f(R) Theories of Gravity
• Topology of large-scale structure in the 2dF Galaxy Redshift Survey
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Conservative Estimates of the Mass of the Neutrino from Cosmology
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Extragalactic Point Source Search in WMAP 61 and 94 GHz Data
• Accurate Baryon Acoustic Oscillations reconstruction via semi-discrete optimal transport
• Topology of non-linear structure in the 2dF Galaxy Redshift Survey
• The Clustering Of Galaxies Around Radio-Loud AGNs
• Perturbations for transient acceleration
• Gravitational collapse in the Schrödinger-Poisson system
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Using Lagrangian perturbation theory for precision cosmology
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• Time variation of the electron mass in the early universe and the Barrow-Magueijo model
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• RHDE models in FRW Universe with two IR cut-offs with redshift parametrization
• BE-HaPPY: Bias Emulator for Halo Power Spectrum including massive neutrinos
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Growth of perturbations in dark energy parametrization scenarios
• A candidate relativistic tidal disruption event at 340 Mpc
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Constraints on a scale-dependent bias from galaxy clustering
• Estimating Cosmological Parameters from the Dark Matter Distribution
• Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
• Maximum Likelihood Random Galaxy Catalogues and Luminosity Function Estimation
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
• Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390
• QCD modified ghost scalar field dark energy models
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Probing Dark Energy Inhomogeneities with Supernovae
• Covariance of the redshift-space matter power spectrum after reconstruction
• Statistical recovery of the BAO scale from multipoles of the beam-convolved 21cm correlation function
• Baryon acoustic oscillation methods for generic curvature: Application to the SDSS-III Baryon Oscillation Spectroscopic Survey
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Structure formation in dark energy cosmologies described by PADE parameterization
• Cosmological neutrino mass limit and the dynamics of dark energy
• fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• The physical foundations for the geometric structure of relativistic theories of gravitation. From General Relativity to Extended Theories of Gravity through Ehlers-Pirani-Schild approach
• Detecting Baryon Acoustic Oscillations
• Probing for Dynamics of Dark-Energy in Mass Varying Neutrinos: Cosmic Microwave Background Radiation and Large Scale Structure
• Evolution of dark matter velocity dispersion
• Redshift-space correlation functions in large galaxy cluster surveys
• Volume Statistics as a Probe of Large-Scale Structure
• Clustering with general photo-$z$ uncertainties: Application to Baryon Acoustic Oscillations
• Asymptotic cosmological regimes in scalar-torsion gravity with a perfect fluid
• Interacting Holographic Dark Energy, the Present Accelerated Expansion and Black Holes
• Neutrino pair annihilation ($\nu \bar{\nu }\to e^{-}{e}^{+}$) in the presence of quintessence surrounding a black hole
• Dark Matter from the Inflaton Field
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• Reducing the Variance of Redshift Space Distortion Measurements from Mock Galaxy Catalogues with Different Lines of Sight
• Application of the iterative reconstruction to simulated galaxy fields
• Direct cosmological inference from three-dimensional correlations of the Lyman-$\alpha$ forest
• Properties of the exact analytic solution of the growth factor and its applications
• Delayed Recombination and Standard Rulers
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Cosmological aspects of a unified dark energy and dust dark matter model
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Studying the Intervention of an Unusual Term in $f(T)$ Gravity via Noether Symmetry
• The clustering of baryonic matter. II: halo model and hydrodynamic simulations
• Strongly Coupled Dark Energy with Warm dark matter vs. LCDM
• New parameterization for unified dark matter and dark energy
• Distance Probes of Dark Energy
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• The Nature of the Faint Low-Frequency Radio Source Population
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Observational constraints to a phenomenological $f\left(R,\nabla R\right)$-model
• Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations
• Bayesian methods for fitting Baryon Acoustic Oscillations in the Lyman-$\alpha$ forest
• The study of the angular and spatial distribution of radio selected AGNs and star-forming galaxies in the ELAIS N1 field
• Satellites in the field and lens galaxies: SDSS/COSMOS vs. SLACS/CLASS
• Weighing neutrinos in the presence of a running primordial spectral index
• Line confusion in spectroscopic surveys and its possible effects: Shifts in Baryon Acoustic Oscillations position
• Observational Constraints on Undulant Cosmologies
• Noether Symmetries of a Modified Model in Teleparallel Gravity and a New Approach for Exact Solutions
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Signatures of the Baryon Acoustic Oscillations on 21cm Emission Background
• The impact and mitigation of broad absorption line quasars in Lyman$-\alpha$ forest correlations
• Interacting Dark Energy: Dynamical System Analysis
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• From Little Bangs to the Big Bang
• Topological phantom AdS black holes in $F(R)$ gravity
• Cosmological homogeneity scale estimates are dressed
• GRB Hubble diagram and constraints on a Λ(t)CDM model
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• Surveying the dark side
• Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs
• Observing trans-Planckian ripples in the primordial power spectrum with future large scale structure probes
• MEDUSA: Minkowski functionals estimated from Delaunay tessellations of the three-dimensional large-scale structure
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Plasma dark matter direct detection
• Observations of the High Redshift Universe
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Phenomenology of BAO evolution from Lagrangian to Eulerian Space
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• Fast generation of weak lensing maps by the inverse-Gaussianization method
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• Dark sector evolution in Horndeski models
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• The dark side of curvature
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• Shell-like structures in our cosmic neighbourhood
• Baryonic matter perturbations in decaying vacuum cosmology
• Planting a Lyman alpha forest on AbacusSummit
• Dynamical Dark Energy model parameters with or without massive neutrinos
• ISW-Galaxy Cross Correlation:A probe of Dark Energy clustering and distribution of Dark Matter tracers
• Analysis of spin directions of galaxies in the DESI Legacy Survey
• Field Theory of the Correlation Function of Mass Density Fluctuations for Self-Gravitating Systems
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Power-law solutions and accelerated expansion in scalar-tensor theories
• Effects of NII and H$\alpha$ Line Blending on the WFIRST Galaxy Redshift Survey
• Performance study of Lagrangian methods: reconstruction of large scale peculiar velocities and baryonic acoustic oscillations
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• DM particles: how warm they can be?
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Galactic satellite systems in CDM, WDM and SIDM
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• Wide Field Surveys and Astronomical Discovery Space
• Observational constrained Weyl type $f(Q,T)$ gravity cosmological model and the dynamical system analysis
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Braneworld Black Holes
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• New evidence and analysis of cosmological-scale asymmetry in galaxy spin directions
• Interacting holographic dark energy models: A general approach
• The $k$-essence scalar field in the context of Supernova Ia Observations
• Prospects in Constraining the Dark Energy Potential
• Constraints on Generalized Dark Energy from Recent Observations
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Spherical collapse of dark matter haloes in tidal gravitational fields
• Probing for variation of neutrino mass with current observations
• Consistency of nonlinear interacting ghost dark energy with recent observations
• How accurately can we measure the baryon acoustic oscillation feature?
• Optimising Spectroscopic and Photometric Galaxy Surveys: Same-sky Benefits for Dark Energy and Modified Gravity
• Comparing teh holographic principle inspired dark energy models
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Non-Perturbative Yang-Mills Condensate as Dark Energy
• The miniJPAS survey quasar selection II: Machine learning classification with photometric measurements and uncertainties
• Dynamic analysis of noncanonical warm inflation
• Uncovering substructure with wavelets: proof of concept using Abell 2744
• Holographic dilatonic model of dark energy
• Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
• Probing signatures of bounce inflation with current observations
• Cosmologies with variable parameters and dynamical cosmon: implications on the cosmic coincidence problem
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Cosmological dynamics of a non-minimally coupled bulk scalar field in DGP setup
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Evidence of dark energy in different cosmological observations
• Baryogenesis through Asymmetric Hawking Radiation from Primordial Black Holes as Dark Matter
• Viscous dark fluid Universe: a unified model of the dark sector?
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• Fast, large volume, GPU enabled simulations for the Ly-alpha forest: power spectrum forecasts for baryon acoustic oscillation experiments
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Interacting holographic tachyon model of dark energy
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Short Distance Physics and Initial State Effects on the CMB Power Spectrum
• Cosmological constraints on dark energy
• Gravitational lensing in WDM cosmologies: The cross section for giant arcs
• Field Equation of Correlation Function of Mass Density Fluctuation for Self-Gravitating Systems
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• The Skeleton: Connecting Large Scale Structures to Galaxy Formation
• Cosmological Analysis of Modified Holographic Ricci Dark Energy in Chern-Simons Modified Gravity
• Field Equation of Correlation Function of Mass Density Fluctuation for Self-Gravitating Systems
• Massive Neutrinos in Cosmology
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Measuring the BAO peak position with different galaxy selections
• Shear and vorticity in the spherical collapse of dark matter haloes
• Strong lensing, cosmology and lensing halos
• Measuring galaxy [OII] emission line doublet with future ground-based wide-field spectroscopic surveys
• X-ray Clusters of Galaxies as Cosmological Tools
• Locating the Baryon Acoustic Peak
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Using 3D and 2D analysis for analyzing large-scale asymmetry in galaxy spin directions
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• Testing the statistical isotropy of large scale structure with multipole vectors
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• No stable dissipative phantom scenario in the framework of a complete cosmological dynamics
• Evolution of the cosmic matter density field with a primordial magnetic field
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Global neutrino parameter estimation using Markov Chain Monte Carlo
• An extension of the cosmological standard model with a bounded Hubble expansion rate
• Constraining Thawing Dark Energy using Galaxy Cluster Number Counts
• Window effect in the power spectrum analysis of a galaxy redshift survey
• Analytical solutions of the geodesic equation in the space-time of a black hole surrounded by perfect fluid in Rastall theory
• Dark Energy as a Critical Period in Binary Motion: Bounds from Multi-scale Binaries
• Cosmological surveys with multi-object spectrographs
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Skewness as a probe of Baryon Acoustic Oscillations
• Large scale distribution of mass versus light from Baryon Acoustic Oscillations: Measurement in the final SDSS-III BOSS Data Release 12
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Holographic field theory models of dark energy in interaction with dark matter
• Observational Constraints on Visser's Cosmological Model
• On fast Generation of Cosmological Random Fields
• Model Selection with Baryonic Acoustic Oscillations in the Lyman-alpha Forest
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Assessing the foundation and applicability of some dark energy fluid models in the Dirac-Born-Infeld framework
• Analysis of $\sim 10^6$ spiral galaxies from four telescopes shows large-scale patterns of asymmetry in galaxy spin directions
• Ghost dark energy with sign-changeable interaction term
• Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Fast analytical calculation of the random pair counts for realistic survey geometry
• Stability analysis of agegraphic dark energy in Brans-Dicke cosmology
• Probing the azimuthal environment of galaxies around clusters. From cluster core to cosmic filaments
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• Posing Constraints on the Free Parameters of a New Model of Dark Energy EoS : Responses Through Cosmological Behaviours
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• Modelling Time-varying Dark Energy with Constraints from Latest Observations
• What have we learned from observational cosmology ?
• Facilities for Dark Energy Investigations
• Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations
• Giga-z: A 100,000 Object Superconducting Spectrophotometer for LSST Follow-up
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• Evolution mapping II: describing statistics of the non-linear cosmic velocity field
• Simultaneous constraints on bias, normalization and growth index through power spectrum measurements
• Cosmic evolution in the background of non-minimal coupling in $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ Gravity
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Let there be Light: the Emergence of Structure out of the Dark Ages in the Early Universe
• A new test of gravity -- I: Introduction to the method
• Astrophysics in 2005
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Hubble flow variations as a test for inhomogeneous cosmology
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• Does spatial flatness forbid the turnaround epoch of collapsing structures?
• The DAMIC-M Low Background Chamber
• Improved two-point correlation function estimates using glass-like distributions as a reference sample
• Smoothing the redshift distributions of random samples for the baryon acoustic oscillations : applications to the SDSS-III BOSS DR12 and QPM mock samples
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• Structure formation in clustering DBI dark energy model with constant sound speed
• The importance of the cosmic web and halo substructure for power spectra
• New Inflation vs. Chaotic Inflation, Higher Degree Potentials and the Reconstruction Program in light of WMAP3
• The Cosmology of Asymmetric Brane Modified Gravity
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• Unveiling the Universe with Emerging Cosmological Probes
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Multi-wavelength consensus of large-scale linear bias
• Two-point statistics without bins: A continuous-function generalization of the correlation function estimator for large-scale structure
• Forward modeling of galaxy kinematics in slitless spectroscopy
• Effects of tidal gravitational fields in clustering dark energy models
• Constraining Parameters for the Accelerating Universe in $f(R,{\mathcal{L}}_m)$ Gravity
• Interactions in the dark sector of the Universe
• Effects of particle creation rate in two-fluid interacting cosmologies
• Angular systematics-free cosmological analysis of galaxy clustering in configuration space
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Testing for Features in the Primordial Power Spectrum
• Reconstructing thawing quintessence with multiple datasets
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Complementarity of Future Dark Energy Probes
• Slow-roll reconstruction for running spectral index
• Large-scale asymmetry in galaxy spin directions -- analysis of galaxies with spectra in DES, SDSS, and DESI Legacy Survey
• Model Selection using Baryon Acoustic Oscillations in the Final SDSS-IV Release
• Constraints on the cosmic distance duality relation with simulated data of gravitational waves from the Einstein Telescope
• The evolution of Luminous Red Galaxies in the Sloan Digital Sky Survey 7th data release
• A Possible Late Time $\Lambda$CDM-like Background Cosmology in Relativistic MOND Theory
• Probing for cosmological parameters with LAMOST measurement
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Cosmic acceleration from second order gauge gravity
• Gravitational instability of the primordial plasma: anisotropic evolution of structure seeds
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Self-gravitating systems in Extended Gravity
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Isocurvature initial conditions for second order Boltzmann solvers
• Probing the Neutrino Mass through the Cross Correlation between the Rees-Sciama Effect and Weak Lensing
• A left and right truncated Schechter luminosity function for quasars
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Clustering Measurements of broad-line AGNs: Review and Future
• A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)
• Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
• Dark energy as an elastic strain fluid
• A comprehensive analysis of the compact phase space for Hu-Sawicki $f(R)$ dark energy models including spatial curvature
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• 2D BAO vs 3D BAO: Hints for new physics?
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Nucleation regions in the Large-Scale Structure I. A catalogue of cores in nearby rich superclusters
• A Model for the Redshift-Space Galaxy 4-Point Correlation Function
• Relaxing cosmological constraints on current neutrino masses
• Non-Linearly Interacting Ghost Dark Energy in Brans-Dicke Cosmology
• Bayesian large-scale structure inference and cosmic web analysis
• Cosmological consequences of Modified Gravity (MOG)
• Numerical Analysis of Galactic Rotation Curves
• Ray-tracing log-normal simulation for weak gravitational lensing: application to the cross-correlation with galaxies
• Late-time power-law stages of cosmological evolution in teleparallel gravity with nonminimal coupling
• A Well-Behaved f(R) Gravity Model in Planetary Motions
• Sub-eV upper limits on neutrino masses from cosmology
• Galaxy And Mass Assembly (GAMA): $\mathbf{z}\sim 0$ Galaxy Luminosity Function down to $\mathbf{L}\sim 10^6{\mathbf{L}}_{\odot }$ via Clustering Based Redshift Inference
• The Effect of Lensing on the Large-Scale CMB Anisotropy
• Cosmic Void Baryon Acoustic Oscillation Measurement: Evaluation of Sensitivity to Selection Effects
• Measurement of the baryonic acoustic oscillation scale in 21 cm intensity fluctuations during the reionisation era
• Multipole analysis on gyroscopic precession in $f(R)$ gravity with irreducible Cartesian tensors
• An introduction to the dark energy problem
• White Noise from Dark Matter: 21 cm Observations of Early Baryon Collapse
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• High-order 2MASS galaxy correlation functions: Probing the primordial density field and the linearity of galaxy bias
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Barrow holographic dark energy interacting model in the presence of radiation and matter
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Locations of Satellite Galaxies in the Two-Degree Field Galaxy Redshift Survey
• Scaling of the 1-halo terms with bias
• Scaling attractors for quintessence in flat universe with cosmological term
• Tracing the assembly histories of galaxy clusters in the nearby universe
• The establishment of the Standard Cosmological Model through observations
• Observing Baryon Oscillations with Cosmic Shear
• Effective field theory of coupled dark energy and dark matter
• The 4MOST-Cosmology Redshift Survey: Target Selection of Bright Galaxies and Luminous Red Galaxies
• Optimizing BAO measurements with non-linear transformations of Lyman-alpha forest
• Lognormal semi-numerical simulations of the Lyman-$\alpha$ forest: comparison with full hydrodynamic simulations
• Primordial Non-Gaussianity from LAMOST Surveys
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Universal conditional distribution function of [OII] luminosity of galaxies, and prediction for the [OII] luminosity function at redshift $z<3$
• On the origin of the BAOtr-DESI tension
• The Cosmic Lens All-Sky Survey parent population - I. Sample selection and number counts
• Dynamical Oscillations in Dark Energy: Joint Constraints on the $w_{sin}$CDM Model from DESI, OHD, and Supernova Samples
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Precession shift in curvature based Extended Theories of Gravity and Quintessence fields
• Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data
• Gödel-type solutions in $f(R,T,R_{\mu \nu }{T}^{\mu \nu }$) gravity
• Analytic Study of Cosmological Perturbations in a Unified Model of Dark Matter and Dark Energy with a Sharp Transition
• Early dark energy in the pre- and post-recombination epochs
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Euclid preparation. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey
• Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
• Constraints on dark energy evolution
• Small cosmological constant in seesaw mechanism with breaking down SUSY
• Power-law solutions for TeVeS
• Upper limits on neutrino masses from cosmology
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Effects of high-order operators in non-relativistic Lifshitz holography
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Mixing Bispectrum Multipoles Under Geometric Distortions
• Structure in Galaxy Distribution. III. Fourier Transforming the Universe
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis
• On the cosmological viability of the Hu-Sawicki type modified induced gravity
• Stochastic Order Redshift Technique (SORT): a simple, efficient and robust method to improve cosmological redshift measurements
• The Evolution of the Baryon Distribution in the Universe from Cosmological Simulations
• Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering
• The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks
• A New Approach to Testing Dark Energy Models by Observations
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Cosmic Microwave Background Polarization
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• Cosmology with Galaxy Correlations
• Euclid: Fast two-point correlation function covariance through linear construction
• Cosmological constraints from galaxy clustering
• Primordial fluctuations from deformed quantum algebras
• Modelling the covariance matrix for the power spectra before and after the BAO reconstruction
• Tighter bounds on a hypothetical graviton screening mass from the gravitational wave observation GW150914 at LIGO
• Constraint on the growth factor of the cosmic structure from the damping of the baryon acoustic oscillation signature
• Dark Energy Survey: DESI-Independent Angular BAO Measurement
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Some remarks on the observational constraints on the self-interacting scalar field model for dark energy
• Observable predictions of generalised inflationary scenarios
• A cosmic speed-trap: a gravity-independent test of cosmic acceleration using baryon acoustic oscillations
• Hubble Diagrams in the Jordan and Einstein Frames
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Barboza-Alcaniz Equation of State Parametrization : Constraining the Parameters in Different Gravity Theories
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Data-driven Cosmology from Three-dimensional Light Cones
• The reach of next-to-leading-order perturbation theory for the matter bispectrum
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Photo-z optimization for measurements of the BAO radial direction
• Angular Diameter Distance Measurement with Galaxy Clustering in the Multipole Space
• Axion hot dark matter bounds
• Cosmological constraints from galaxy multi-tracers in the nearby Universe
• The general expression for $f(T)$ in a charged cylindrical spacetime with diverse dimensions
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• On the possibility of Baryon Acoustic Oscillation measurements at redshift $z>7.6$ with the Roman Space Telescope
• Holographic Principle and the Second Law in Stephani Cosmology Revisited
• Observational constraints on thawing quintessence scalar field model
• Investigating the Redshift Evolution of Lensing Galaxy Density Slopes via Model-Independent Distance Ratios
• A new test for the Galactic formation and evolution -- prediction for the orbital eccentricity distribution of the halo stars
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Non-vacuum relativistic extensions of MOND using metric theories of gravity with curvature-matter couplings and their applications to the accelerated expansion of the Universe without dark components
• Non-linear effects in early Universe cosmology
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Cosmology behind the mask: Constraining the parameters of $\Lambda$CDM with the unmasked galaxy density field from VIPERS
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Production and constraints for a massive dark photon at electron-positron colliders
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Cosmology with CMB anisotropy
• Phase space of multi-fluid universe in $F(T)$-gravity and some enhancements for the oscillating interaction model
• Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
• Where galaxies really come from
• Observations of General Relativity at strong and weak limits
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• Irreversible Thermodynamics of the Universe: Constraints from Planck Data
• Dynamics of Solutions of $f(R)$ Theory
• An "Ultrasonic Image" of the Embryonic Universe: CMB Polarization Tests of the Inflationary Paradigm
• Challenges to the cosmological constant model following results from the Dark Energy Survey
• Massive neutrinos and dark energy
• The mass and redshift dependence of halo star clustering
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• A comprehensive dynamical and phenomenological analysis of structure growth in curvature-modulated coupled quintessence scenario
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Accelerating BAO Scale Fitting Using Taylor Series
• Artificial Neural Networks for Galaxy Clustering. Learning from the two-point correlation function of BOSS galaxies
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Gödel-type solutions in hybrid metric-Palatini gravity
• Newtonian Approach to the Matter Power Spectrum of the Generalized Chaplygin Gas
• Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
• Comparing LambdaCDM, wCDM, and w0waCDM models with DESI DR2 BAO: Redshift-Resolved Diagnostics and the Role of rd
• Testing modified (Horndeski) gravity by combining intrinsic galaxyalignments with cosmic shear
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• $\Lambda$CDM, $\Lambda$DGP and extended phantom-like cosmologies
• Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
• Cosmological Calculations on the GPU
• Solving small-scale clustering problems in approximate lightcone mocks
• Cosmology of Cubic Poincaré Gauge gravity
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• Skewness as a Probe of Gravity: Real and Redshift Space Counts-In-Cells
• A Deep Dive into f(R) Gravity Theory
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Mixed constraints to inflationary models
• Coupling dark-baryonic matter density profile for vacuum decay scenarios
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference
• Constraining effective neutrino species with bispectrum of large scale structures
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• HINORA, a method for detecting ring-like structures in 3D point distributions I: application to the Local Volume Galaxy catalogue
• Cosmological quests in the CMB sky
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB
• Post-Newtonian N-Body Dynamics in Extended Theories of Gravity
• Testing the CCC+TL cosmology with cosmic-chronometer measurements of the Hubble parameter
• A novel Cosmic Filament catalogue from SDSS data
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• Testing General Relativity on Galactic Scales via DESI-BAO and Strong Lensing: Circumventing Assumptions on the Hubble Constant, Sound Horizon, and Dark Energy
• The BAO scale -- how standard is the standard ruler?
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging
• A Bayesian estimator for peculiar velocity correction in cosmological inference from supernovae data
• Confusing dark matter particle properties with modifications to General Relativity
• An emulation-based model for the projected correlation function
• `Standard' Cosmological model & beyond with CMB
• Quintessence reconstruction of interacting HDE in a non-flat universe
• A Spectrum of Cosmological Rips and Their Observational Signatures
• Manifestations of String Theory in Astrophysical Data and at the LHC
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment