Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample

Abstract

The spectroscopic Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) galaxy sample represents the final set of galaxies observed using the original SDSS target selection criteria. We analyse the clustering of galaxies within this sample, including both the Luminous Red Galaxy (LRG) and Main samples, and also include the 2-degree Field Galaxy Redshift Survey (2dFGRS) data. Baryon Acoustic Oscillations are observed in power spectra measured for different slices in redshift; this allows us to constrain the distance--redshift relation at multiple epochs. We achieve a distance measure at redshift z=0.275, of r_s(z_d)/D_V(0.275)=0.1390+/-0.0037 (2.7% accuracy), where r_s(z_d) is the comoving sound horizon at the baryon drag epoch, D_V(z)=[(1+z)^2D_A^2cz/H(z)]^(1/3), D_A(z) is the angular diameter distance and H(z) is the Hubble parameter. We find an almost independent constraint on the ratio of distances D_V(0.35)/D_V(0.2)=1.736+/-0.065, which is consistent at the 1.1sigma level with the best fit Lambda-CDM model obtained when combining our z=0.275 distance constraint with the WMAP 5-year data. The offset is similar to that found in previous analyses of the SDSS DR5 sample, but the discrepancy is now of lower significance, a change caused by a revised error analysis and a change in the methodology adopted, as well as the addition of more data. Using WMAP5 constraints on Omega_bh^2 and Omega_ch^2, and combining our BAO distance measurements with those from the Union Supernova sample, places a tight constraint on Omega_m=0.286+/-0.018 and H_0 = 68.2+/-2.2km/s/Mpc that is robust to allowing curvature and non-Lambda dark energy. This result is independent of the behaviour of dark energy at redshifts greater than those probed by the BAO and supernova measurements. (abridged)

22 pages, 16 figures, minor changes to match version published in MNRAS

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• Observational constraints on a logarithmic scalar field dark energy model and black hole mass evolution in the Universe
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Reconstruction and constraining of the jerk parameter from OHD and SNe Ia observations
• How predictions of cosmological models depend on Hubble parameter data sets
• Reconstruction of the Dark Energy equation of state
• Cosmography beyond standard candles and rulers
• Potential-driven Galileon inflation
• Constraints on the shapes of galaxy dark matter haloes from weak gravitational lensing
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Reconciling the local void with the CMB
• Numerical resolution limits on subhalo abundance matching
• New observational constraints on $f(T)$ cosmology from radio quasars
• Complete dark energy scenario in $f(Q)$ gravity
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• On the Density profile slope of Clusters of Galaxies
• Linear growth of structure in massive bigravity
• Cosmological constraints on extended Galileon models
• The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements
• Efficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy Surveys
• Hubble parameter data constraints on dark energy
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• The Sommerfeld enhancement for scalar particles and application to sfermion co-annihilation regions
• Current constraints on the epoch of cosmic acceleration
• Primordial backgrounds of relic gravitons
• Shear and rotation in Chaplygin cosmology
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• A New Equation of State for Dark Energy Model
• Constraining the dark energy equation of state with double source plane strong lenses
• Model independent calibrations of gamma ray bursts using machine learning
• Modified Chaplygin Gas as a Unified Dark Matter and Dark Energy Model and Cosmic Constraints
• Exhausting the Information: Novel Bayesian Combination of Photometric Redshift PDFs
• A model of interacting holographic dark energy at the Ricci's scale
• Forecasting the Cosmological Constraints with Anisotropic Baryon Acoustic Oscillations from Multipole Expansion
• Measuring the transverse baryonic acoustic scale from the SDSS DR11 galaxies
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• A New Class of Parametrization for Dark Energy without Divergence
• Barrow Entropy Cosmology: an observational approach with a hint of stability analysis
• Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
• Large-Scale Structure of the Universe as a Cosmic Standard Ruler
• The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies
• Right-Handed Neutrinos as the Dark Radiation: Status and Forecasts for the LHC
• The Atacama Cosmology Telescope: Physical Properties of Sunyaev-Zel'dovich Effect Clusters on the Celestial Equator
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• Neutrino mass constraint with the Sloan Digital Sky Survey power spectrum of luminous red galaxies and perturbation theory
• AIC and BIC for cosmological interacting scenarios
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• Cosmic acceleration without dark energy: Background tests and thermodynamic analysis
• Modified Supergravity and Early Universe: the Meeting Point of Cosmology and High-Energy Physics
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• $f(R)$-gravity from Killing Tensors
• Constrained $f(Q,T)$ gravity accelerating cosmological model and its dynamical system analysis
• Structure formation in cosmologies with oscillating dark energy
• Clustering of Photometric Luminous Red Galaxies II: Cosmological Implications from the Baryon Acoustic Scale
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
• Metastable Dark Energy with Radioactive-like Decay
• Matter bispectrum in cubic Galileon cosmologies
• Testing dark energy paradigms with weak gravitational lensing
• Constraints on Cosmological Models and Reconstructing the Acceleration History of the Universe with Gamma-Ray Burst Distance Indicators
• Surface Density of dark matter haloes on galactic and cluster scales
• The foreground wedge and 21 cm BAO surveys
• Constraining the expansion rate of the Universe using low-redshift ellipticals as cosmic chronometers
• Observational constraints on a holographic, interacting dark energy model
• Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• From a Bounce to the Dark Energy Era with $F(R)$ Gravity
• Streaming velocities and the baryon-acoustic oscillation scale
• High redshift cosmography: new results and implication for dark energy
• Cosmic string parameter constraints and model analysis using small scale Cosmic Microwave Background data
• Chaotic inflation in modified gravitational theories
• Systematic biases on galaxy haloes parameters from Yukawa-like gravitational potentials
• New holographic reconstruction of scalar field dark energy models in the framework of chameleon Brans-Dicke cosmology
• Gauss-Bonnet dark energy by Lagrange multipliers
• Constant sound speed and its thermodynamical interpretation in $f(Q)$ gravity
• Cosmographic parameters in model-independent approaches
• The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties
• Speeding up $N$-body simulations of modified gravity: Chameleon screening models
• Revisit of cosmic age problem
• Can all cosmological observations be accurately interpreted with a unique geometry?
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Distribution function approach to redshift space distortions. Part V: perturbation theory applied to dark matter halos
• Future CMB cosmological constraints in a dark coupled universe
• Observational constraints on non-flat dynamical dark energy cosmological models
• Probing the neutrino mass hierarchy with CMB weak lensing
• Cosmology with nonminimal kinetic coupling and a power-law potential
• Constraints on the generalized Chaplygin gas model including gamma-ray bursts via a Markov Chain Monte Carlo approach
• Linear growth in power law $f(T)$ gravity
• Testing the equation of state for viscous dark energy
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• New limits on Early Dark Energy from the South Pole Telescope
• Nonlinear Power Spectrum from Resummed Perturbation Theory: a Leap Beyond the BAO Scale
• Constraining inflation with future galaxy redshift surveys
• 21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction
• Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• Phantom cosmological model with observational constraints in $f(Q)$ gravity
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• Starobinsky cosmological model in Palatini formalism
• 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
• Constraints on dark energy from H II starburst galaxy apparent magnitude versus redshift data
• Accelerating expansion of the universe in modified symmetric teleparallel gravity
• From Big to Little Rip in modified F(R,G) gravity
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• EFTCAMB/EFTCosmoMC: massive neutrinos in dark cosmologies
• Cosmic acceleration in non-flat $f(T)$ cosmology
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Phantom dark energy as an effect of bulk viscosity
• Observational Constraints on Exponential Gravity
• Modelling and testing the equation of state for (Early) dark energy
• Quasi-dilaton non-linear massive gravity: Investigations of background cosmological dynamics
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Accelerating Universe scenario in anisotropic $f\left(Q\right)$ cosmology
• Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope
• Dark energy: investigation and modeling
• Primordial non-Gaussianity from the Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey I: Catalogue Preparation and Systematic Mitigation
• Applications of Bayesian model averaging to the curvature and size of the Universe
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• On the surface density of dark matter haloes
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Generalization of Regular Black Holes in General Relativity to $f(R)$ Gravity
• Investigating the dark energy phenomenon in $f(R,L_m)$ cosmological models with observational constraints
• Halo clustering and g_{NL}-type primordial non-Gaussianity
• Coupled Quintessence and the Halo Mass Function
• Standard-siren cosmology using gravitational waves from binary black holes
• The Effect of Weak Lensing on Distance Estimates from Supernovae
• Testable dark energy predictions from current data
• Cosmography of f(R) - brane cosmology
• Dark energy from primordial inflationary quantum fluctuations
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Exploring stable models in $f(R;T;R_{\mu \nu }{T}^{\mu \nu })$ gravity
• Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• Viscous cosmology in the Weyl-type $f(Q,T)$ gravity
• A new test of $f(R)$ gravity with the cosmological standard rulers in radio quasars
• Tension in the Void: Cosmic Rulers Strain Inhomogeneous Cosmologies
• Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey
• Galaxy and Mass Assembly (GAMA): The evolution of bias in the radio source population to z ~ 1.5
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• Cosmology with matter diffusion
• Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
• Constraints and tensions in testing general relativity from Planck and CFHTLenS including intrinsic alignment systematics
• Cosmic acceleration from modified gravity with Palatini formalism
• Dynamical symmetries and observational constraints in scalar field cosmology
• Dark matter-dark energy interaction for a time-dependent equation of state
• Priors on the effective Dark Energy equation of state in scalar-tensor theories
• Cosmological investigations of (extended) nonlinear massive gravity schemes with non-minimal coupling
• Consistency of inflation and preheating in F(R) supergravity
• Cosmological surveys with the Australian Square Kilometre Array Pathfinder
• Unified Dark Energy and Dark Matter from Dynamical Space Time
• Deuterium at high-redshift: Primordial abundance in the zabs = 2.621 damped Ly-alpha system towards CTQ247
• Analytic rotating black hole solutions in $N$-dimensional $f(T)$ gravity
• Testing the Etherington's distance duality relation at higher redshifts: the combination of radio quasars and gravitational waves
• Neutrino Cosmology after WMAP and LHC7
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Light Sterile Neutrinos in Cosmology and Short-Baseline Oscillation Experiments
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Young and turbulent: the early life of massive galaxy progenitors
• Clustering of photometric luminous red galaxies I : Growth of Structure and Baryon Acoustic Feature
• Unified Dark Fluid with Constant Adiabatic Sound Speed and Cosmic Constraints
• FLRW cosmological models with quark and strange quark matters in f(R,T) gravity
• Model-Independent Constraints on Lorentz Invariance Violation via the Cosmographic Approach
• Unbiased methods for removing systematics from galaxy clustering measurements
• Sneutrino Hybrid Inflation and Nonthermal Leptogenesis
• Dark Energy and Fate of the Universe
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Linearisation with Cosmological Perturbation Theory
• Early Dark Energy with Power-law F(R) Gravity
• Non-minimal kinetic coupling and the phenomenology of dark energy
• Regarding the Line-of-Sight Baryonic Acoustic Feature in the Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey Luminous Red Galaxy Samples
• A new method for the Alcock-Paczynski test
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• An Axially Symmetric Transitioning models with Observational Constraints
• Thermodynamical aspects of Bianchi type-I Universe in quadratic form of $f\left(Q\right)$ gravity and observational constraints
• Future weak lensing constraints in a dark coupled universe
• (Lack of) Cosmological evidence for dark radiation after Planck
• Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant
• The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < z < 1.46
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• Classical and Quantum Solutions in Brans-Dicke Cosmology with a Perfect Fluid
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data
• Emergence of the mass discrepancy-acceleration relation from dark matter-baryon interactions
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Quintessence Universe and cosmic acceleration in $f(Q,T)$ gravity
• Parametrized modified gravity constraints after Planck
• Observational constraints on non-minimally coupled Galileon model
• Secondary infall model and dark matter scaling relations in intermediate redshift early - type galaxies
• Statistical and systematic errors in redshift-space distortion measurements from large surveys
• Dark matter scaling relations in intermediate z haloes
• Multi-Point Propagators for Non-Gaussian Initial Conditions
• Phantom cosmology in an Extended Theory of Gravity
• Figures of merit and constraints from testing General Relativity using the latest cosmological data sets including refined COSMOS 3D weak lensing
• Cosmic distance duality and cosmic transparency
• Galaxy cluster number count data constraints on cosmological parameters
• Cosmology with non-minimal derivative couplings: perturbation analysis and observational constraints
• Shedding Light on Dark Matter at Colliders
• Unified Dark Matter scalar field models with fast transition
• Interacting viscous dark fluids
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Testing the distance duality relation with present and future data
• Constraining Variations in the Fine Structure Constant in the presence of Early Dark Energy
• Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
• High Redshift Standard Candles: Predicted Cosmological Constraints
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Latest Observational Constraints to the Ghost Dark Energy Model by Using Markov Chain Monte Carlo Approach
• The radial acceleration relation in galaxy clusters
• The REFLEX II galaxy cluster survey: power spectrum analysis
• Robustness to systematics for future dark energy probes
• A Comparative Study of Dark Energy Constraints from Current Observational Data
• Power-law cosmology, SN Ia, and BAO
• Gravitational Waves in Viable f(R) Models
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Comparison of Recent SnIa datasets
• Dark energy from scalar field with Gauss Bonnet and non-minimal kinetic coupling
• Confronting the relaxation mechanism for a large cosmological constant with observations
• Estimating the galaxy two-point correlation function using a split random catalog
• New Constraints On The Dark Energy Equation of State
• Cosmological constraints on dark energy in $f(Q)$ gravity: A parametrized perspective
• Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement
• Figures of merit for present and future dark energy probes
• Observational constraints on cosmic neutrinos and dark energy revisited
• Can $f(T)$ models play a bridge between early and late time Universe?
• Bulk viscous matter and the cosmic acceleration of the universe in $f(Q,T)$ gravity
• The full Fisher matrix for galaxy surveys
• Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?
• Super-sample covariance approximations and partial sky coverage
• Smoothing the $H_0$ tension with a dynamical dark energy model
• The Dark Side of the Universe after Planck
• A New $Om(z)$ Diagnostic of Dark Energy in General Relativity Theory
• Are Light Sterile Neutrinos Preferred or Disfavored by Cosmology?
• Late-time cosmology in $f(Q,L_m)$ gravity: Analytical solutions and observational fits
• Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Agegraphic dark energy: growth index and cosmological implications
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• Bayesian Comparison of Interacting Scenarios
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• One-loop corrections, uncertainties and approximations in neutralino annihilations: Examples
• Constraints on interacting dark energy models from galaxy Rotation Curves
• Big Bang nucleosynthesis with a stiff fluid
• Big Rip and Little Rip solutions in scalar model with kinetic and Gauss Bonnet couplings
• Weighing Neutrinos in $f(R)$ gravity
• Constraining $f(Q,L_m)$ gravity with bulk viscosity
• Constraining Entropic Cosmology
• Hanbury Brown-Twiss interferometry and second-order correlations of inflaton quanta
• Dynamics and cosmological constraints on Brans-Dicke cosmology
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• Exploring the Latest Union2 SNIa Dataset by Using Model-Independent Parametrization Methods
• A Robust Measure of Cosmic Structure beyond the Power-Spectrum: Cosmic Filaments and the Temperature of Dark Matter
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Geodesic Deviation Equation in $f(R,T)$ Gravity
• Exploring accelerated expansion in the universe: A study of $f(Q,T)$ gravity with parameterized EoS and cosmological constraints
• The correlation function of galaxy clusters and detection of baryon acoustic oscillations
• Beyond delta: Tailoring marked statistics to reveal modified gravity
• Supernova light-curve fitters and Dark Energy
• Modeling Transit Dark Energy in $f(R,L_m)$-gravity
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• Observational analysis of late-time acceleration in $f(Q,L_m)$ gravity
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Statefinder diagnosis and the interacting ghost model of dark energy
• Observational constraints on Tsallis modified gravity
• Cosmology in massive gravity
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• Zero-point quantum fluctuations in cosmology
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Evolution of Dark Energy Perturbations in Scalar-Tensor Cosmologies
• Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
• Characterisation of the non-Gaussianity of radio and IR point-sources at CMB frequencies
• Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra
• Highlights and Discoveries from the Chandra X-ray Observatory
• Prediction of Supernova Rates in Known Galaxy-galaxy Strong-lens Systems
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• Observational constraints on the equation of state of viscous fluid in $f(R,T)$ gravity
• Testing for dynamical dark energy models with redshift-space distortions
• Quantitative acoustic models for superfluid circuits
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• The effect of redshift-space distortions on projected 2-pt clustering measurements
• Constraining dark energy fluctuations with supernova correlations
• Testing standard and non-standard neutrino physics with cosmological data
• $H_0$ Tension in Torsion-based Modified Gravity
• Is there evidence for additional neutrino species from cosmology?
• Inflationary cosmology with Chaplygin gas in Palatini formalism
• Cosmological constraints for an Eddington-Born-Infeld field
• W-WIMP Annihilation as a Source of the Fermi Bubbles
• Post-Planck Dark Energy Constraints
• Generalized Chaplygin gas and accelerating universe in $f(Q,T)$ gravity
• Breaking parameter degeneracy in interacting dark energy models from observations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Observational constrained $F(R,\mathcal{G})$ gravity cosmological model and the dynamical system analysis
• Background cosmological dynamics in $f(R)$ gravity and observational constraints
• A comprehensive investigation on the slowing down of cosmic acceleration
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Have Baryonic Acoustic Oscillations in the galaxy distribution really been measured?
• Exploring late-time cosmic acceleration: A study of a linear $f(T)$ cosmological model using observational data
• Cosmological implications of the constant jerk parameter in $f(Q,T)$ gravity theory
• Implications from simulated strong gravitational lensing systems: constraining cosmological parameters using Gaussian Processes
• Gravitational quantum effects on power spectra and spectral indices with higher-order corrections
• How does non-linear dynamics affect the baryon acoustic oscillation?
• Reconstruction of the primordial power spectrum from CMB data
• Weyl type $f(Q,T)$ gravity observational constrained cosmological model
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
• The distinctions between $\Lambda$CDM and $f(T)$ gravity according Noether symmetry
• Simulations of BAO reconstruction with a quasar Lyman-alpha survey
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Do Observations Favour Galileon Over Quintessence?
• Cosmological Structure Formation in Decaying Dark Matter Models
• Noether symmetries and boundary terms in extended Teleparallel gravity cosmology
• Statistical properties of the dark matter haloes of dwarf galaxies and correlations with the environment
• Data Analysis of three parameter models of deceleration parameter in FRW Universe
• Dark Energy from Gauss-Bonnet and non-minimal couplings
• Weak gravitational lensing effects on cosmological parameters and dark energy from gamma-ray bursts
• Dynamics of the diffusive DM-DE interaction--dynamical system approach
• LHC Phenomenology and Cosmology of String-Inspired Intersecting D-Brane Models
• Cosmological model with decaying vacuum energy law from principles of quantum mechanics
• Interaction between viscous varying modified cosmic Chaplygin gas and Tachyonic fluid
• Analysis of accretion disk around a black hole in dRGT massive gravity
• Evolution of spherical overdensities in holographic dark energy models
• Bouncing cosmology in modified gravity with higher-order Gauss-Bonnet curvature term
• Growth of matter perturbations in the extended viscous dark energy models
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant
• Probing the dynamical behavior of dark energy
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Testing modified gravity models with recent cosmological observations
• BAO cosmography
• Phase Transitions in 4D Gauss-Bonnet-de Sitter Black Holes
• Constraining viscous dark energy equation of state in $f(R,L_m)$ gravity
• Increasing the Lensing Figure of Merit through Higher Order Convergence Moments
• Constraining massive gravity with recent cosmological data
• Constraints on Lema\^ıtre-Tolman-Bondi models from Observational Hubble Parameter data
• Testing nonstandard cosmological models with SNLS3 supernova data and other cosmological probes
• Weak Lensing by Line-of-sight Halos as the Origin of Flux-ratio Anomalies in Quadruply Lensed QSOs
• Statistical Classification Techniques for Photometric Supernova Typing
• Quantum Corrections in Galileons from Matter Loops
• Cosmological model of the interaction between dark matter and dark energy
• Gravitino LSP and leptogenesis after the first LHC results
• Impacts of satellite galaxies on the redshift-space distortions
• Connecting inflation with late cosmic acceleration by particle production
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• Cosmic age test in inhomogeneous cosmological models mimicking $\Lambda$CDM on the light cone
• Observational constraints on new generalized Chaplygin gas model
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
• Reheating in 3-form inflation
• Observational constraints on phantom power-law cosmology
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Constraining the cosmological model of modified $f(Q)$ gravity: Phantom dark energy and observational insights
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Probing the dark-matter halos of cluster galaxies with weak lensing
• Formulation and constraints on decaying dark matter with finite mass daughter particles
• Updated constraints from the PLANCK experiment on modified gravity
• Broadband distortion modeling in Lyman-$\alpha$ forest BAO fitting
• The $\Lambda$CDM growth rate of structure revisited
• Cosmological constraints on dark energy models using DESI BAO 2024
• Generalized Holographic Dark Energy and its Observational Constraints
• 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
• Cosmology and thermodynamics of FRW universe with bulk viscous stiff fluid
• MeV dark matter in the 3+1+1 model
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• Cosmological evidence for leptonic asymmetry after Planck
• Revealing modified gravity signal in matter and halo hierarchical clustering
• Measuring growth index in a universe with sterile neutrinos
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• Non-Gaussian errors of baryonic acoustic oscillations
• Observational Constraints on Dynamical Dark Energy Models
• A cosmographic analysis of the transition to acceleration using SN-Ia and BAO
• A global fit study on the new agegraphic dark energy model
• Observational constraints on decaying vacuum dark energy model
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Does $\Lambda$CDM really be in tension with the Hubble diagram data?
• Cosmological Parameter Determination in Free-Form Strong Gravitational Lens Modeling
• Effects of New Viscosity Model on Cosmological Evolution
• Cosmology with nonminimal kinetic coupling and a Higgs-like potential
• Galaxy cluster angular size data constraints on dark energy
• Statefinder Analysis of Symmetric Teleparallel Cosmology
• A new Tolman test of a cosmic distance duality relation at 21 cm
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Observational Constraints on the Averaged Universe
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Bouncing cosmological models in $f(R,L_m)$ gravity
• Consistency check of ΛCDM phenomenology
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Growth of spherical overdensities in scalar-tensor cosmologies
• Horava-Lifshitz cosmology with generalized Chaplygin gas
• Isocurvature perturbations in extra radiation
• Exact Cosmology in Myrzakulov Gravity
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• Isotropic compact stars in 4D Einstein-Gauss-Bonnet gravity
• Possible indication for non-zero neutrino mass and additional neutrino species from cosmological observations
• Relations between canonical and non-canonical inflation
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• The WiggleZ Dark Energy Survey: constraining the evolution of Newton's constant using the growth rate of structure
• Cosmic slowing down of acceleration using $f_{gas}$
• Cosmological Constraints on the Gravitational Interactions of Matter and Dark Matter
• Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Probing modified gravity theories with the Sandage-Loeb test
• Do cosmological data rule out $f(\mathcal{R})$ with $w\ne -1$?
• Relic gravitational waves: latest revisions and preparations for new data
• Cosmological Tests of Everpresent $\Lambda$
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• The Accelerating Universe
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Exploring hints for dark energy density evolution in light of recent data
• Bouncing cosmologies and stability analysis in symmetric teleparallel $f(Q)$ gravity
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies
• Quintessential power-law cosmology: dark energy equation of state
• Constraining holographic inflation with WMAP
• A conventional approach to the dark-energy concept
• Dark Radiation and Decaying Matter
• Testing Verlinde's emergent gravity in early-type galaxies
• Probing large-scale magnetism with the Cosmic Microwave Background
• Modeling cosmic acceleration with a generalized varying deceleration parameter
• Constraints on anisotropic properties of the universe in $f(Q,T)$ gravity theory
• Unified Dark Fluid with Constant Adiabatic Sound Speed: Including Entropic Perturbations
• Cosmological implications of the transition from the false vacuum to the true vacuum state
• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Halo based reconstruction of the cosmic mass density field
• Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
• Constraints on dark energy from the Lyα forest baryon acoustic oscillations measurement of the redshift 2.3 Hubble parameter
• Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Anisotropic f(Q) gravity model with bulk viscosity
• A new $f(Q)$ cosmological model with $H(z)$ quadratic expansion
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• Observational constraints on the oscillating dark energy cosmologies
• Quantum mechanical look at the radioactive-like decay of metastable dark energy
• A comprehensive parametrization approach for the Hubble parameter in scalar field dark energy models
• The stellar mass function and star formation rate-stellar mass relation of galaxies at z ~ 4 - 7
• Investigating early and late-time epochs in $f(Q)$ gravity
• Observational constraints on a generalized equation of state model
• Exploring Universe acceleration through observational constraints via Hubble parameter reconstruction
• Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant
• Future dynamics in f(R) theories
• Higher-Order Gauss-Bonnet Cosmology
• Effective dark energy equation of state in interacting dark energy models
• Testing the interaction model with cosmological data and gamma-ray bursts
• Vacuum energy as dark matter
• Non-Gaussian isocurvature perturbations in dark radiation
• Non-minimal kinetic coupling and Chaplygin gas cosmology
• Stellar Mass and color dependence of the three-point correlation function of galaxies in the local universe
• Obstacles to Constructing de Sitter Space in String Theory
• Traversable holographic dark energy wormholes constrained by astronomical observations
• Study of the charged super-Chandrasekhar limiting mass white dwarfs in the $f(R,\mathcal{T})$ gravity
• Galaxy Peculiar Velocities From Large-Scale Supernova Surveys as a Dark Energy Probe
• A 3% Determination of $H_0$ at Intermediate Redshifts
• Is the Cosmic Transparency Spatially Homogeneous?
• Properties and uncertainties of scalar field models of dark energy with barotropic equation of state
• Harrison-Z'eldovich primordial spectrum is consistent with observations
• Cosmological acceleration
• Evidence for baryon acoustic oscillations from galaxy-ellipticity correlations
• Does DESI DR2 challenge $\Lambda$CDM paradigm ?
• The traces of anisotropic dark energy in light of Planck
• The signature of the scattering between dark sectors in large scale cosmic microwave background anisotropies
• Time and distance constraints on accelerating cosmological models
• Reduced modified Chaplygin gas cosmology
• Two scalar field cosmology from coupled one-field models
• Does accelerating universe indicates Brans-Dicke theory
• CMB dipoles and other low-order multipoles in the quasispherical Szekeres model
• On measuring the absolute scale of baryon acoustic oscillations
• Pulse-wise Amati correlation in Fermi GRBs
• Tension between SN and BAO: current status and future forecasts
• BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures
• Inflationary susceptibilities, duality and large-scale magnetic fields generation
• Observational constraints on the generalized $\alpha$ attractor model
• Dark energy from cosmological fluids obeying a Shan-Chen non-ideal equation of state
• Measuring the Geometry of the Universe from Weak Gravitational Lensing behind Galaxy Groups in the HST COSMOS survey
• Cosmology with decaying cosmological constant -- exact solutions and model testing
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Testing $f(R)$ Gravity With Scale Dependent Cosmic Void Velocity Profiles
• Robust constraints on dark energy and gravity from galaxy clustering data
• Cosmological constraints on dynamical dark energy model in $F(Q)$ gravity
• Spherical collapse model in agegraphic dark energy cosmologies
• Homogeneous Gödel-type solutions in hybrid metric-Palatini gravity
• Confronting Tracker Field Quintessence with Data
• Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
• Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum
• Featuring the primordial power spectrum: new constraints on interrupted slow-roll from CMB and LRG data
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• Observational Viability of an Inflation Model with E-Model non-Minimal Derivative Coupling
• Discrimination between Lambda-CDM, quintessence, and modified gravity models using wide area surveys
• General dynamical properties of cosmological models with nonminimal kinetic coupling
• Late time cosmological scenarios from scalar field with Gauss Bonnet and non-minimal kinetic couplings
• Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
• Observational constraints on scalar field models of dark energy with barotropic equation of state
• The COSMOS Density Field: A Reconstruction Using Both Weak Lensing and Galaxy Distributions
• On the Trans-Planckian Censorship Conjecture and the Generalized Non-Minimal Coupling
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• Modelling non-linear evolution using Lagrangian Perturbation Theory (LPT) re-expansions
• Using newest VLT-KMOS HII Galaxies and other cosmic tracers to test the $\Lambda$CDM tension
• Cosmological models with squared trace in modified gravity
• Study of parametrized dark energy models with a general non-canonical scalar field
• On the role of shear in cosmological averaging
• The clustering of critical points in the evolving cosmic web
• Constraining the interacting dark energy models from weak gravity conjecture and recent observations
• Quintessence versus phantom dark energy: the arbitrating power of current and future observations
• Using Lagrangian perturbation theory for precision cosmology
• The effect of different observational data on the constraints of cosmological parameters
• Raytracing simulations of coupled dark energy models
• Cosmological parameter estimation from CMB and X-ray clusters after Planck
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Cosmological constraints on the new holographic dark energy model with action principle
• The ages of stellar populations in a warm dark matter universe
• Observational constraints on unified dark matter including Hubble parameter data
• Future CMB ISW-Lensing bispectrum constraints on modified gravity in the Parameterized Post-Friedmann formalism
• Can the degeneracies in the gravity sector be broken?
• Observational constraints on assisted k-inflation
• Probing interactions within the dark matter sector via extra radiation contributions
• Observational Constraints on Hybrid Scale Factor in f(Q,T) Gravity with Anisotropic Space-Time
• Scalar cosmological perturbations from inflationary black holes
• Observational constraints on dark energy cosmological model parameters
• Quintessence-like features in the late-time cosmological evolution of $f(Q)$ symmetric teleparallel gravity
• Bubble of nothing decays of unstable theories
• Type Ia supernova parameter estimation: a comparison of two approaches using current datasets
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• On the effect of the degeneracy between w_0 and w_a
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• The role of curvature in the slowing down acceleration scenario
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Diagnostic and Comparative Analysis of Dark Energy Models with $q(z)$ Parametrizations
• Phenomenology of Gravitational Aether as a solution to the Old Cosmological Constant Problem
• Phantom crossing dark energy in Horndeski's theory
• Interacting agegraphic dark energy model in tachyon cosmology coupled to matter
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Constraining Thawing Quintessence
• Constraints to Holographic Dark Energy Model via Type Ia Supernovae, Baryon Acoustic Oscillation and WMAP
• Cubic Derivative Interactions and Asymptotic Dynamics of the Galileon Vacuum
• The D-material universe
• Dynamics and constraints of the dissipative Liouville cosmology
• de Sitter Decays to Infinity
• Is the CMB telling us that dark matter is weaker than weakly interacting?
• An interacting model for the cosmological dark sector
• Modified cosmology in $f(Q,L_m)$ gravity
• Clustering with general photo-$z$ uncertainties: Application to Baryon Acoustic Oscillations
• Structure formation in dark energy cosmologies described by PADE parameterization
• Exact Scalar-Tensor Cosmological Models
• Possible dark energy imprints in gravitational wave spectrum of mixed neutron-dark-energy stars
• Non-Canonical Inflation in Supergravity
• Post-inflationary thermal histories and the refractive index of relic gravitons
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• A critical assessment of some inhomogeneous pressure Stephani models
• Improved cosmological constraints on the curvature and equation of state of dark energy
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• Detecting Baryon Acoustic Oscillations
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Holographic dark energy described at the Hubble length
• Cosmological Constraints on the Higgs Boson Mass
• Cosmological constraint on Brans-Dicke Model
• Future constraints on the Hu-Sawicki modified gravity scenario
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Constraining Galileon gravity from observational data with growth rate
• Weinberg's Higgs portal confronting recent LUX and LHC results together with upper limits on B^+ and K^+ decay into invisibles
• Observational constraints to a phenomenological $f\left(R,\nabla R\right)$-model
• Estimating the uncorrelated dark energy evolution in the Planck era
• Constraint propagation equations of the 3+1 decomposition of f(R) gravity
• The tension on the cosmological parameters from different observational data
• Cosmology with viscous generalized Chaplygin gas in $f(Q)$ gravity
• The Cosmological Parameters 2014
• Dark Energy From Fifth Dimensional Brans-Dicke Theory
• Dependence on supernovae light-curve processing in void models
• Chebyshev cosmography in the framework of extended symmetric teleparallel theory
• Lyman-tomography of cosmic infrared background fluctuations with Euclid: probing emissions and baryonic acoustic oscillations at z>10
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• The Age-Redshift Relation For Luminous Red Galaxies Obtained From the Full Spectrum Fitting and Its Cosmological Implications
• Baryonic effects in cosmic shear tomography: PCA parametrization and importance of extreme baryonic models
• Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
• New parameterization for unified dark matter and dark energy
• An updated analysis of two classes of f(R) theories of gravity
• Uncorrelated estimates of the primordial power spectrum
• The complementarity of the redshift drift
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• Model-independent estimation of the cosmography parameters using cosmic chronometers
• Using machine learning to compress the matter transfer function $T(k)$
• Late time acceleration in a slow moving galileon field
• Line confusion in spectroscopic surveys and its possible effects: Shifts in Baryon Acoustic Oscillations position
• Parameter Estimation with BEAMS in the presence of biases and correlations
• $f(\mathcal{G},\text{T})$ Gravity Bouncing Universe with Cosmological Parameters
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• Observational constraints on a cosmological model with Lagrange multipliers
• Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs
• Third quantization of $f(R)$-type gravity
• Exact Scalar-Tensor Cosmological Solutions via Noether Symmetry
• The Impact of Assuming Flatness in the Determination of Neutrino Properties from Cosmological Data
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• Coupled quintessence with a possible transient accelerating phase
• Is dark energy evolving?
• Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH
• Figures of Merit for Testing Standard Models: Application to Dark Energy Experiments in Cosmology
• Probing the course of cosmic expansion with a combination of observational data
• ISW-Galaxy Cross Correlation:A probe of Dark Energy clustering and distribution of Dark Matter tracers
• Updated F(T) gravity constraints from high redshift cosmography
• Constraints on $\Lambda (t)$CDM models as holographic and agegraphic dark energy with the observational Hubble parameter data
• Systematics in the Gamma Ray Bursts Hubble diagram
• The Stellar Masses of ~40,000 UV Selected Galaxies from the WiggleZ Survey at 0.3<z<1.0: Analogues of Lyman Break Galaxies?
• Exploring cosmological evolution and constraints in $f(T)$ teleparallel gravity
• Effects of NII and H$\alpha$ Line Blending on the WFIRST Galaxy Redshift Survey
• Constraining thawing and freezing models with cluster number counts
• Schwarzschild Lecture 2014: HectoMAPping The Universe
• Geometric and dynamic distortions in anisotropic galaxy clustering
• High Redshift Investigation On The Dark Energy Equation of State
• Baryonic matter perturbations in decaying vacuum cosmology
• Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models
• Relic density calculations beyond tree-level, exact calculations versus effective couplings: the ZZ final state
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• Bulk viscous cosmological model in $f(T,\mathcal{T})$ modified gravity
• Observation constraints on scalar field cosmological model in Anisotropic universe
• Squared torsion $f(T,\mathcal{T})$ gravity and its cosmological implications
• It's a dark, dark world: Background evolution of interacting $\varphi$CDM models beyond simple exponential potentials
• Interacting generalized ghost dark energy in non-flat universe
• A Reconstruction of Quintessence Dark Energy
• Uneven flows: On cosmic bulk flows, local observers, and gravity
• Deviation From ΛCDM With Cosmic Strings Networks
• Forecasting cosmological parameter constraints from near-future space-based galaxy surveys
• Constraints on $\Lambda (t)$-cosmology with power law interacting dark sectors
• Disentangling star formation and merger growth in the evolution of Luminous Red Galaxies
• Weighing neutrinos in $f(R)$ gravity in light of BICEP2
• Consistency of nonlinear interacting ghost dark energy with recent observations
• The radial acceleration relation and dark baryons in MOND
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Light mass galileon and late time acceleration of the Universe
• Cosmic acceleration from coupling of baryonic and dark matter components: Analysis and diagnostics
• Observational constraints on the fractal cosmology
• Glauber theory and the quantum coherence of curvature inhomogeneities
• Observational constraints on the energy scale of inflation
• Cosmology in Brans-Dicke-de Rham-Gabadadze-Tolley massive gravity
• A new approach to cosmological perturbations in f(R) models
• Observational constrained Weyl type $f(Q,T)$ gravity cosmological model and the dynamical system analysis
• Constraints on a special running vacuum model
• Likelihood of the Power Spectrum in Cosmological Parameter Estimation
• Dark Energy Perturbations Revisited
• Probing Weyl-type $f(Q,T)$ gravity: Cosmological implications and constraints
• Third quantization of $f(R)$-type gravity II - General $f(R)$ case -
• Multiple $\Lambda$CDM cosmology with string landscape features and future singularities
• Testing the consistency between cosmological measurements of distance and age
• Fast, large volume, GPU enabled simulations for the Ly-alpha forest: power spectrum forecasts for baryon acoustic oscillation experiments
• Do we need wavelets in the late Universe?
• Decaying dark matter mimicking time-varying dark energy
• Uncertainty in 2-point correlation function estimators and BAO detection in SDSS DR7
• Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data
• Future evolution in a backreaction model and the analogous scalar field cosmology
• Designing Future Dark Energy Space Missions: II. Photometric Redshift of Space Weak Lensing Optimized Survey
• Cosmological constraints on Agegraphic dark energy in DGP braneworld gravity
• Cosmology With Axionic-quintessence Coupled with Dark Matter
• Evidence of dark energy in different cosmological observations
• Detecting baryon acoustic oscillations by 3d weak lensing
• Figure of Merit and Different Combinations of Observational Data Sets
• Revisiting cosmic acceleration with DESI BAO
• Cosmology with a Decaying Vacuum Energy Parametrization Derived from Quantum Mechanics
• A power-law coupled three-form dark energy model
• Dynamical Analysis of Scalar Field Cosmologies with Spatial Curvature
• Cosmic acceleration and phantom crossing in $f(T)$-gravity
• Bulk viscous matter in $f(T)$ gravity: A path to cosmic acceleration
• Multi-fluid cosmology: An illustration of fundamental principles
• Cosmic jerk parameter in symmetric teleparallel cosmology
• Observational Constraints on Axions as Quintessence in String Theory
• Observational consequences of the Standard Model Higgs inflation variants
• DBI Galileon and Late time acceleration of the universe
• Multistate scalar field dark matter and its correlation with galactic properties
• Viscous fluid cosmology in symmetric teleparallel gravity
• Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect
• Quintessential and phantom power-law solutions in scalar tensor model of dark energy
• The Chandra X-Ray Observatory: Progress Report and Highlights
• An Introduction into the Theory of Cosmological Structure Formation
• Unified dark matter and dark energy description in a chiral cosmological model
• A thermodynamic point of view on dark energy models
• No stable dissipative phantom scenario in the framework of a complete cosmological dynamics
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Bulk viscous fluid in symmetric teleparallel cosmology: theory versus experiment
• Current cosmological constraints on the curvature, dark energy and modified gravity
• Dynamical analysis for a scalar-tensor model with kinetic and non-minimal couplings
• Cosmological constraints on dark energy
• Scaling cosmology with variable dark-energy equation of state
• Gravitational lensing in WDM cosmologies: The cross section for giant arcs
• Cosmological models with running cosmological term and decaying dark matter
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• Phase space analysis for a scalar-tensor model with kinetic and Gauss-Bonnet couplings
• Cosmological constraints on $f(Q)$ gravity models in the non-coincident formalism
• New initial condition of the new agegraphic dark energy model
• Viable dark energy models using pseudo-Nambu-Goldstone bosons
• Exact Solutions in Modified Gravity Models
• Joint analysis of X-ray and Sunyaev Zel'dovich observations of galaxy clusters using an analytic model of the intra-cluster medium
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Cosmological analytic solutions with reduced relativistic gas
• The parameter space of Cubic Galileon models for cosmic acceleration
• Gradient expansion, curvature perturbations and magnetized plasmas
• Aether-quasi-dilaton massive gravity
• Probing the primordial power spectra with inflationary priors
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Cosmology with a Continuous Tower of Scalar Fields
• Relativistic cosmology number densities in void-Lemaitre-Tolman-Bondi models
• Machine learning unveils the linear matter power spectrum of modified gravity
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Window effect in the power spectrum analysis of a galaxy redshift survey
• Large scale distribution of mass versus light from Baryon Acoustic Oscillations: Measurement in the final SDSS-III BOSS Data Release 12
• Resonant non-Gaussianity with equilateral properties
• Square-Root parametrization of dark energy in $f(Q)$ cosmology
• Assessing the foundation and applicability of some dark energy fluid models in the Dirac-Born-Infeld framework
• Challenges in Constraining Gravity with Cosmic Voids
• Constraining Temporal Oscillations of Cosmological Parameters Using Type Ia Supernovae
• Cosmological implications of different baryon acoustic oscillation data
• Can we distinguish early dark energy from a cosmological constant?
• Energy conditions in $f(Q,L_m)$ gravity
• Galaxy Zoo Morphology and Photometric Redshifts in the Sloan Digital Sky Survey
• Extra relativistic degrees of freedom without extra particles using Planck data
• Probing Ricci dark energy model with perturbations by using WMAP seven-year cosmic microwave background measurements, BAO and Type Ia supernovae
• Modelling Time-varying Dark Energy with Constraints from Latest Observations
• On the canonical formalism of $f(R)$-type gravity using Lie derivatives
• Modern Cosmology, an Amuse-Gueule
• Fast analytical calculation of the random pair counts for realistic survey geometry
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• Testing LTB Void Models Without the Cosmic Microwave Background or Large Scale Structure: New Constraints from Galaxy Ages
• Cosmology of Dirac-Born-Infeld dRGT massive gravity
• Fuzzy Supernova Templates II: Parameter Estimation
• Reconstructing FHDE with Scalar and Gauge Fields
• Bootstrapping from inflationary magnetogenesis to CMB initial conditions
• Stability analysis of agegraphic dark energy in Brans-Dicke cosmology
• Non minimally coupled condensate cosmologies: matching observational data with phase space
• A matter-dominated cosmological model with variable $G$ and $\Lambda$. Confrontation of theoretical predictions with observational data
• Modified initial power spectrum and too big to fail problem
• Reassessing Dust's Role in Forming the CMB
• Constraints on Dark Energy state equation with varying pivoting redshift
• Revisiting Cardassian Model and Cosmic Constraint
• A coupled generalized three-form dark energy model
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Structure formation in clustering DBI dark energy model with constant sound speed
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• Constraints on the $\Lambda$CDM model with redshift tomography
• A search for nontoroidal topological lensing in the Sloan Digital Sky Survey quasar catalog
• Analysis cosmological tachyon and fermion model and observation data constraints
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• Quasi-periodical features in the distribution of Luminous Red Galaxies
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Reconciling BICEP2 and Planck results with right-handed Dirac neutrinos in the fundamental representation of grand unified E_6
• Primordial power spectrum versus extension parameters beyond the standard model
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Scalar field description of a parametric model of dark energy
• How accurately can we measure the hydrogen 2S->1S transition rate from the cosmological data?
• Consistency analysis of a Dark Matter velocity dependent force as an alternative to the Cosmological Constant
• Observational constraints to a unified cosmological model
• Modern Cosmology: Interactive Computer Simulations that use Recent Observational Surveys
• Constraining dark energy using observational growth rate data
• Measuring primordial gravitational waves from CMB B-modes in cosmologies with generalized expansion histories
• Chi-square versus median statistics in SNIa data analysis
• Probing the cosmic acceleration from combinations of different data sets
• Effects of particle creation rate in two-fluid interacting cosmologies
• The evolution of Luminous Red Galaxies in the Sloan Digital Sky Survey 7th data release
• Simulation studies of dark energy clustering induced by the formation of dark matter halos
• Dynamics of dark energy in the gravitational fields of matter inhomogeneities
• The Bianchi type-V Dark Energy Cosmology in Self Interacting Brans Dicke Theory of Gravity
• Unified dark fluid with fast transition: including entropic perturbations
• Observational constraints on G-corrected holographic dark energy using a Markov chain Monte Carlo method
• Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model
• Holographic dark energy at the Ricci scale
• Computing Accurate Age and Distance Factors in Cosmology
• Scalar field dark energy: Insights into cosmological evolution and black hole accretion
• Cosmological Model-independent Gamma-ray Bursts Calibration and its Cosmological Constraint to Dark Energy
• Novel aspects of C-theories in Cosmology
• Scalar-tensor extension of the $\Lambda$CDM model
• Transient Accelerating Scalar Models with Exponential Potential
• Baryon acoustic oscillations with the cross-correlation of spectroscopic and photometric samples
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Angular systematics-free cosmological analysis of galaxy clustering in configuration space
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• The coincidence problem in $f(R)$ gravity models
• Observational constraints on viscous cosmology in $f(T,L_m)$ gravity
• Second order invariants and holography
• Consistency of $f(R)$ gravity models around solar polytropes
• Eternal vs singular observers in interacting dark energy-dark matter models
• Probing Lambda-DGP Braneworld Model
• Cosmological Study in Myrzakulov $F(R,T)$ Quasi-dilaton Massive Gravity
• Towards a sound massive cosmology
• Constraining hybrid potential scalar field cosmological model in Lyra's geometry with recent observational data
• Dark energy as an elastic strain fluid
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• Accelerated expansion induced by Dark Matter with two charges
• A new method to probe the mass density and the cosmological constant using configuration entropy
• Bias of reconstructing the dark energy equation of state from the Pad$\acute{e}$ cosmography
• Complementary cosmological tests of RSII brane models
• Modeling dark energy through an Ising fluid with network interactions
• Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?
• Spectral Distortion in a Radially Inhomogeneous Cosmology
• Impact of dark energy on the equation of state in light of the latest cosmological data
• Observational constraints on tachyonic chameleon dark energy model
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia, BAO, CMB, H(z) and X-ray gas mass fraction
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• Cosmological aspects of a vector field model
• Voids and Halos in Voids statistics as a probe of the Expansion History of the Universe
• Testing and selecting cosmological models with ultra-compact radio quasars
• Constrain the linear scalar perturbation theory of Cotton gravity
• The Low Redshift survey at Calar Alto (LoRCA)
• Quasi-periodical components in the radial distributions of cosmologically remote objects
• Probing Dark Energy Properties in $fQ,C)$ Gravity with FLRW Cosmological Models
• Accelerated expansion of the Universe a la the Stueckelberg mechanism
• Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset
• Cosmological dynamics of interacting dark energy and dark matter in $f(Q)$ gravity
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• Spectator Higgs, large-scale gauge fields and the non-minimal coupling to gravity
• New parameterizations of generalized Chaplygin gas model constrained at background and perturbation levels
• Structure Formation in Dark Matter Particle Production Cosmology
• Oscillating solutions of the matter density contrast in Horndeski's theory
• A Study of Universal Thermodynamics in Massive Gravity: Modified Entropy on the Horizons
• Non-singular bouncing cosmology in $f(T,\mathcal{T})$ gravity with energy condition violations
• Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• Dynamical Oscillations in Dark Energy: Joint Constraints on the $w_{sin}$CDM Model from DESI, OHD, and Supernova Samples
• Cosmological constraints on Lorentz invariance violation in the neutrino sector
• Non-linear Matter Spectrum for a Variable Equation of State
• Exact solutions in a scalar-tensor model of dark energy
• Observational constraints on a Yang-Mills condensate dark energy model
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• Cosmic Evolution of the Kantowski-Sachs Universe in the Context of a Bulk Viscous String in Teleparallel Gravity
• New measures to test modified gravity cosmologies
• Cosmological Evolution of Viscous Dark Energy in f(Q,C) Gravity: Two-Fluid Approach
• Gravitational energy as dark energy: Average observational quantities
• Estimations of the cosmological parameters from the observational variation of the fine structure constant
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Constraints on dark energy evolution
• Updated reduced CMB data and constraints on cosmological parameters
• Holographic description of unified early and late universe in viscous mimetic gravity
• Effects of high-order operators in non-relativistic Lifshitz holography
• Assessing the viability of successful reconstruction of the dynamics of dark energy using varying fundamental couplings
• Future constraints on variations of the fine structure constant from combined CMB and weak lensing measurements
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Effect of lensing magnification on type Ia supernova cosmology
• Secondary graviton spectra, second-order correlations and Bose-Einstein enhancement
• Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 $<$ z $<$ 0.45 -- status update
• Cosmic expansion beyond $\Lambda$CDM: Investigating power-law and logarithmic corrections
• Power-law expansion and Higgs-type potential in a scalar-tensor model
• Cosmological constraints in symmetric teleparallel gravity with bulk viscosity
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• Neutrino physics from future weak lensing surveys
• A unification of RDE model and XCDM model
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• Bounce and Collapse in the Slotheonic Universe
• Non-Affine Extensions of the Raychaudhuri Equation in the K-essence Framework
• Hubble Expansion as an Einstein Curvature
• Constraining Chaplygin models using diffuse supernova neutrino background
• Power-spectrum simulations of radial redshift distributions
• The ergodicity bias in the observed galaxy distribution
• Cosmology in a model with Lagrange multiplier, and Gauss-Bonnet and non-minimal kinetic couplings
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Linear perturbations spectra for dynamical dark energy inspired by modified gravity
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Viscous fluid dynamics with decaying vacuum energy density
• Observational constraints and dynamical analysis of Kaniadakis horizon-entropy cosmology
• Quintessence like behavior of symmetric teleparallel dark energy: Linear and nonlinear model
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Observable predictions of generalised inflationary scenarios
• A pressure parametric dark energy model
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• A class of transient acceleration models consistent with Big Bang Cosmology
• Generalized second law of thermodynamics in massive gravity
• Degeneracy and Discreteness in Cosmological Model Fitting
• A cosmic speed-trap: a gravity-independent test of cosmic acceleration using baryon acoustic oscillations
• Metallicity and kinematical clues to the formation of the Local Group
• Traces of Anisotropic Quasi-Regular Structure in the SDSS Data
• Reconstructing cosmic evolution with a density parametrization
• Indirect dark matter searches at ultrahigh energy neutrino detectors
• Inflation and late time acceleration designed by Stueckelberg massive photon
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• Mimetic Tensor-Vector-Scalar Cosmology: Incorporating Dark Matter, Dark Energy and Stiff Matter
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Cuscuton-like contribution to dark energy evolution
• Dynamical Shortcomings in the Generalized SU(2) Proca Theory: Challenges for Cosmic Acceleration
• Finite scale factor and future singularities
• The Hubble flow: an observer's perspective
• QSO Selection and Photometric Redshifts with Neural Networks
• Off-diagonal solutions in Einsteingravity modeling f(R) gravity and dynamical darkenergy vs Lambda CDM cosmology
• Thermodynamics and holography of tachyon cosmology
• Monopole Fluctuations in Galaxy Surveys
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• The general expression for $f(T)$ in a charged cylindrical spacetime with diverse dimensions
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Accelerating and decelerating cosmology from spinor and scalar fields non-minimally coupled with f(R) gravity
• Constraints on a scalar-tensor model with Gauss-Bonnet coupling from SN Ia and BAO observations
• Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law $f(Q)$ Gravity with Quasars
• Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Cluster optical depth and pairwise velocity estimation using machine learning
• Cosmology of Quasi-Dilaton Massive Gravity with Non-minimal Kinetic Coupling
• Cosmology in energy-momentum squared symmetric teleparallel gravity
• Holographic Dark Energy with Torsion
• Motion of the Local Group as a cosmological probe
• On the fairness of the main galaxy sample of SDSS
• Robustness of cosmological axion mass limits
• On observational signatures of multi-fractional theory
• Static, Cylindrically Symmetric Spacetimes in the Coincident f(Q) Gravity
• Observational constraints on massive gravity
• Observations of General Relativity at strong and weak limits
• The Cosmological Effect of CMB/BAO Measurements
• Model independent reconstruction of cosmological accelerated-decelerated phase
• Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Cosmic expansion history analysis with Hubble parametrization in $Q^n$ gravity
• Probing cosmic velocity-density correlations with galaxy luminosity modulations
• Fluctuation of the Hubble parameter
• Cosmic velocity, density and halo mass function: Insights from deep learning
• Coupling dark-baryonic matter density profile for vacuum decay scenarios
• How BAO measurements can fail to detect quintessence
• Observational consequences of a dark interaction model
• Dynamical friction shear and rotation in Chaplygin cosmology
• Can we remove the systematic error due to isotropic inhomogeneities?
• Exploring the constraints on cosmological models with CosmoEJS
• Constraints on a vacuum energy from both SNIa and CMB temperature observations
• Dark Radiation and Inflationary Freedom
• Effective $\Lambda$CDM model emerging from $f(Q,T)$ under a special EOS limit in symmetric cosmology with Bayesian and ANN observational constraints
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Studying the stochasticity in astrophysical signals
• Cosmological solutions of Tensor-Vector theories of gravity with varying the space-time-matter coupling constant
• Evaluation of the neutron background in CsI target for WIMP direct detection when using a reactor neutrino detector as a neutron veto system
• Friedmann-free limits on spatial curvature
• From Geometry to Observation: Gravitational Waves and the Raychaudhuri Equation
• Energy conditions and entropy density of the universe
• Dark Radiation and Inflationary Freedom
• Neutrino matter with PLANCK
• On the accelerated expansion of the cosmos
• Effective Approaches in and Beyond the MSSM : applications to Higgs Physics and Dark Matter observables
• $\Lambda$CDM-like models with future singularities
• Investigating Graviton Mass Effects on Black Hole Lensing in dRGT Massive Gravity
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• Dipole of the luminosity distance as a test for dark energy models
• Anisotropic evolution of D-dimensional FRW spacetime
• Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology
• Testing the effects from dark radiation
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• The model-independent degeneracy-breaking point in cosmological models with interacting Dark Energy and Dark Matter
• Quintessence reconstruction of interacting HDE in a non-flat universe
• On the absence of a universal surface density, and a maximum Newtonian acceleration in dark matter haloes: consequences for MOND