The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples

Abstract

We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the Sloan Digital Sky Survey III (SDSS-III). Our results come from the Data Release 11 (DR11) sample, containing nearly one million galaxies and covering approximately $8500$ square degrees and the redshift range $0.2<z<0.7$. We also compare these results with those from the publicly released DR9 and DR10 samples. Assuming a concordance $\Lambda$CDM cosmological model, the DR11 sample covers a volume of 13\,Gpc${}^3$ and is the largest region of the Universe ever surveyed at this density. We measure the correlation function and power spectrum, including density-field reconstruction of the baryon acoustic oscillation (BAO) feature. The acoustic features are detected at a significance of over $7\sigma$ in both the correlation function and power spectrum. Fitting for the position of the acoustic features measures the distance relative to the sound horizon at the drag epoch, $r_d$, which has a value of $r_{d,\mathrm{fid}}=149.28$Mpc in our fiducial cosmology. We find $D_V=(1264\pm 25\mathrm{Mpc})(r_d/r_{d,\mathrm{fid}})$ at $z=0.32$ and $D_V=(2056\pm 20\mathrm{Mpc})(r_d/r_{d,\mathrm{fid}})$ at $z=0.57$. At 1.0 per cent, this latter measure is the most precise distance constraint ever obtained from a galaxy survey. Separating the clustering along and transverse to the line-of-sight yields measurements at $z=0.57$ of $D_A=(1421\pm 20\mathrm{Mpc})(r_d/r_{d,\mathrm{fid}})$ and $H=(96.8\pm 3.4km/s/Mpc)(r_{d,\mathrm{fid}}/r_d)$. Our measurements of the distance scale are in good agreement with previous BAO measurements and with the predictions from cosmic microwave background data for a spatially flat cold dark matter model with a cosmological constant.

40 pages, 29 figures; replaced with final version in journal

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• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• SKA Weak Lensing I: Cosmological Forecasts and the Power of Radio-Optical Cross-Correlations
• Dynamical Dark Matter from Strongly-Coupled Dark Sectors
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Updated Constraints and Forecasts on Primordial Tensor Modes
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
• $\Lambda$CDM or self-interacting neutrinos? - how CMB data can tell the two models apart
• Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• Cosmological limits on neutrino unknowns versus low redshift priors
• Results from the Wilkinson Microwave Anisotropy Probe
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Clustering properties of $g$-selected galaxies at $z\sim 0.8$
• An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
• Time-delay Cosmography: Increased Leverage with Angular Diameter Distances
• Cosmology and the neutrino mass ordering
• Impacts of dark energy on weighing neutrinos after Planck 2015
• Unbiased clustering estimation in the presence of missing observations
• Constraints on the neutrino mass and mass hierarchy from cosmological observations
• Validating estimates of the growth rate of structure with modified gravity simulations
• Testing the equivalence principle on cosmological scales
• HI and cosmological constraints from intensity mapping, optical, and CMB surveys
• Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
• In search of the dark matter dark energy interaction: a kinematic approach
• Cosmological constraints on induced gravity dark energy models
• Cosmological Measurements from Angular Power Spectra Analysis of BOSS DR12 Tomography
• Cosmological parameter inference with Bayesian statistics
• DES13S2cmm: The First Superluminous Supernova from the Dark Energy Survey
• How predictions of cosmological models depend on Hubble parameter data sets
• Neutrino masses and beyond-$\Lambda$CDM cosmology with LSST and future CMB experiments
• Independent Cosmological Constraints from high-z HII Galaxies
• Conjoined constraints on modified gravity from the expansion history and cosmic growth
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• Efficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy Surveys
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• An evaluation of cosmological models from expansion and growth of structure measurements
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• Model independent calibrations of gamma ray bursts using machine learning
• Parametric and nonparametric methods hint dark energy evolution
• On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
• Cosmological implications of scale-independent energy-momentum squared gravity: Pseudo nonminimal interactions in dark matter and relativistic relics
• Measuring the transverse baryonic acoustic scale from the SDSS DR11 galaxies
• How clustering dark energy affects matter perturbations
• Simulations of the OzDES AGN Reverberation Mapping Project
• The Hubble constant from eight time-delay galaxy lenses
• Cosmic viscosity as a remedy for tension between PLANCK and LSS data
• Robust model comparison disfavors power law cosmology
• Acceleration of the universe: a reconstruction of the effective equation of state
• A parametric reconstruction of the cosmological jerk from diverse observational data sets
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Accurate Shear Measurement with Faint Sources
• CFHTLenS and RCSLenS: Testing Photometric Redshift Distributions Using Angular Cross-Correlations with Spectroscopic Galaxy Surveys
• Galaxy and Mass Assembly (GAMA): Redshift Space Distortions from the Clipped Galaxy Field
• Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
• Cosmic Web Reconstruction through Density Ridges: Catalogue
• Observational constraints on dark matter-dark energy scattering cross section
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• Dark Energy and Dark Matter from an additional adiabatic fluid
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Metastable Dark Energy with Radioactive-like Decay
• Galaxy Populations in Massive Galaxy Clusters to z=1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction
• The foreground wedge and 21 cm BAO surveys
• Mass bias evolution in tSZ cluster cosmology
• Optimising the measurement of relativistic distortions in large-scale structure
• Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey
• Fast and Credible Likelihood-Free Cosmology with Truncated Marginal Neural Ratio Estimation
• Positivity Bounds on Dark Energy: When Matter Matters
• Hi intensity mapping with MeerKAT: Primary beam effects on foreground cleaning
• Matter Power Spectrum Covariance Matrix from the DEUS-PUR ΛCDM simulations: Mass Resolution and non-Gaussian Errors
• Planck 2015 constraints on the non-flat XCDM inflation model
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 LRG sample: structure growth rate measurement from the anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0
• Streaming velocities and the baryon-acoustic oscillation scale
• An alternative to the LCDM model: the case of scale invariance
• Cosmological bounds on dark matter-photon coupling
• Gaussian processes reconstruction of modified gravitational wave propagation
• Theoretical Systematics of Future Baryon Acoustic Oscillation Surveys
• Primordial gravitational waves and the H0-tension problem
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• Constraints on dark-matter properties from large-scale structure
• Effective field description of the Anton-Schmidt cosmic fluid
• Cosmic microwave background constraints on secret interactions among sterile neutrinos
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• Designing Horndeski and the effective fluid approach
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Cosmological signatures of ultralight dark matter with an axionlike potential
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Calibrating CHIME, A New Radio Interferometer to Probe Dark Energy
• Testing the effect of $H_0$ on $f{\sigma }_8$ tension using a Gaussian Process method
• Probing cosmology with weak lensing selected clusters I: Halo approach and all-sky simulations
• Simple-graduated dark energy and spatial curvature
• Testing the equation of state for viscous dark energy
• Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with $\Lambda$CDM
• Higgs-Dilaton Cosmology: An inflation - dark energy connection and forecasts for future galaxy surveys
• Is there a concordance value for $H_0$?
• SDSS-IV eBOSS emission-line galaxy pilot survey
• Planck 2015 constraints on spatially-flat dynamical dark energy models
• Neural Network Reconstruction of Late-Time Cosmology and Null Tests
• Horava Gravity in the Effective Field Theory formalism: from cosmology to observational constraints
• Existence of bulk viscous universe in $f(R,T)$ gravity and confrontation with observational data
• Constraining dark matter properties with Cosmic Microwave Background observations
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• Testing Hu-Sawicki f(R) gravity with the Effective Field Theory approach
• On structure formation from a small-scales-interacting dark sector
• Hints of Modified Gravity in Cosmos and in the Lab?
• A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• Improving the precision matrix for precision cosmology
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Cosmological constraints of phantom dark energy models
• Cosmological constraints on dark energy in light of gravitational wave bounds
• Reannihilation of self-interacting dark matter
• Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Cosmological constraints with self-interacting sterile neutrinos
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Mitigating contamination in LSS surveys: a comparison of methods
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Modelling and testing the equation of state for (Early) dark energy
• Observational evidence of galaxy assembly bias
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• A detection of wobbling Brightest Cluster Galaxies within massive galaxy clusters
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• Constraints on modified gravity from Planck 2015: when the health of your theory makes the difference
• Cosmological aspects of a hyperbolic solution in $f(R,T)$ gravity
• COSMIC BIRTH: Efficient Bayesian Inference of the Evolving Cosmic Web from Galaxy Surveys
• Assessment of the cosmic distance duality relation using Gaussian Process
• Connecting neutrino physics with dark matter
• Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\Lambda$CDM cosmology
• Primordial non-Gaussianity from the Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey I: Catalogue Preparation and Systematic Mitigation
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• The Composite Spectrum of BOSS Quasars Selected for Studies of the Lyman-alpha Forest
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Fourier analysis of multi-tracer cosmological surveys
• Geodesics and the magnitude-redshift relation on cosmologically symmetric Finsler spacetimes
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• Dark Catalysis
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Testing cosmic geometry without dynamic distortions using voids
• Regularized cosmological power spectrum and correlation function in modified gravity models
• Measuring cosmic velocities with 21cm intensity mapping and galaxy redshift survey cross-correlation dipoles
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
• Dark Matter properties through cosmic history
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• Large-scale redshift space distortions in modified gravity theories
• Neutrino mass without cosmic variance
• Neutron star merger GW170817 strongly constrains doubly coupled bigravity
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Running the running
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): An unbiased estimate of the growth rate of structure at $⟨\mathbf{z}⟩=0.85$ using the clustering of luminous blue galaxies
• Hints of dark energy anisotropic stress using Machine Learning
• Unified Dark Energy and Dark Matter from Dynamical Space Time
• Unscreening Modified Gravity in the Matter Power Spectrum
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Sterile neutrinos with pseudoscalar self-interactions and cosmology
• Updated observational constraints on quintessence dark energy models
• Unified Superfluid Dark Sector
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence
• How to relax the cosmological neutrino mass bound
• Quintessence's Last Stand?
• Discovery of a massive supercluster system at $z\sim 0.47$
• Cold dark matter plus not-so-clumpy dark relics
• Bayesian Evidences for Dark Energy models in light of current obsevational data
• Using dark energy to suppress power at small scales
• On the road to percent accuracy V: the non-linear power spectrum beyond $\Lambda$CDM with massive neutrinos and baryonic feedback
• The one-loop matter bispectrum as a probe of gravity and dark energy
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Early Dark Energy with Power-law F(R) Gravity
• Cosmological distance indicators
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Relativistic distortions in the large-scale clustering of SDSS-III BOSS CMASS galaxies
• Constraints on the Parameterized Deceleration Parameter in FLRW Universe
• Nonlocal Teleparallel Cosmology
• Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• Unbiased clustering estimates with the DESI fibre assignment
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• Deep Learning the Morphology of Dark Matter Substructure
• New constraints on the distance duality relation from the local data
• From Dark Matter to Galaxies with Convolutional Networks
• HI intensity mapping with MeerKAT: 1/f noise analysis
• Non-linear evolution of the BAO scale in alternative theories of gravity
• Thermodynamical aspects of Bianchi type-I Universe in quadratic form of $f\left(Q\right)$ gravity and observational constraints
• An Axially Symmetric Transitioning models with Observational Constraints
• Growth of matter perturbations in clustered holographic dark energy cosmologies
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• Low redshift observational constraints on tachyon models of dark energy
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• Reconstructing the dark energy potential
• Projected Cosmological Constraints from Strongly Lensed Supernovae with the Roman Space Telescope
• Planck intermediate results. XVI. Profile likelihoods for cosmological parameters
• Deadly dark matter cusps vs faint and extended star clusters: Eridanus II and Andromeda XXV
• Transitioning Universe with hybrid scalar field in Bianchi I space-time
• Cosmic distance inference from purely geometric BAO methods: Linear Point standard ruler and Correlation Function Model Fitting
• A Test of Cosmological Models using high-z Measurements of H(z)
• Probing gravity at large scales through CMB lensing
• Reconstruction of the dark matter-vacuum energy interaction
• Observational constraints of the modified cosmology through Barrow entropy
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Charged Planckian Interacting Dark Matter
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• Unified early and late Universe cosmology through dissipative effects in steep quintessential inflation potential models
• The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
• The massive end of the luminosity and stellar mass functions and clustering from CMASS to SDSS: Evidence for and against passive evolution
• Model selection applied to reconstructions of the Dark Energy
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• Limits on the cosmic neutrino background
• Power law cosmology model comparison with CMB scale information
• Can Holographic dark energy models fit the observational data?
• Testing the distance duality relation using type Ia supernovae and ultracompact radio sources
• High Redshift Standard Candles: Predicted Cosmological Constraints
• Revisiting CMB constraints on dark matter annihilation
• Position-dependent correlation function from the SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 10 CMASS Sample
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• Probing non-standard gravity with the growth index: a background independent analysis
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• Model selection and constraints from Holographic dark energy scenarios
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Optimal Redshift Weighting For Baryon Acoustic Oscillations
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• Testing Einstein's gravity and dark energy with growth of matter perturbations: Indications for new Physics?
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• Power-law cosmology, SN Ia, and BAO
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Correcting for Fibre Assignment Incompleteness in the DESI Bright Galaxy Survey
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Dipolar modulation in the size of galaxies: The effect of Doppler magnification
• The evolution of the [OII], Hβ and [OIII] emission-line luminosity functions over the last nine billions years
• Information Content of Higher-Order Galaxy Correlation Functions
• Statistical Test of Distance--Duality Relation with Type Ia Supernovae and Baryon Acoustic Oscillations
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Machine Learning improved fits of the sound horizon at the baryon drag epoch
• Constraining Anisotropic Cosmological Model in $f(\mathcal{R},{\mathcal{L}}_m)$ Gravity
• Distance Priors from \emph{Planck} 2015 data
• CMB Constraint on Dark Matter Annihilation after Planck 2015
• Alcock-Paczynski Test with Model-independent BAO Data
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Asymmetric Dark Matter Models in SO(10)
• The High-Mass End of the Red Sequence at z~0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function
• Estimating the galaxy two-point correlation function using a split random catalog
• $H_0$ Tension and the Phantom Regime: A Case Study In Terms of an Infrared $f(T)$ Gravity
• Brane with variable tension as a possible solution to the problem of the late cosmic acceleration
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• A new coupled three-form dark energy model and implications for the $H_0$ tension
• Gravitational wave propagation in $f(R)$ models: New parametrizations and observational constraints
• BINGO: a single dish approach to 21cm intensity mapping
• Constraining the curvature density parameter in cosmology
• A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids
• Intensity mapping cross-correlations II: HI halo models including shot noise
• Strongly Lensed Gravitational Waves and Electromagnetic Signals as Powerful Cosmic Rulers
• Confronting interacting dark radiation scenarios with cosmological data
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• Constraining An Exact Brans-Dicke gravity theory with Recent Observations
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Measure of Complexity in Self-Gravitating Systems using Structure Scalars
• Neutrinos secretly converting to lighter particles to please both KATRIN and the cosmos
• Limits on statistical anisotropy from BOSS DR12 galaxies using bipolar spherical harmonics
• Bayesian Comparison of Interacting Scenarios
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Optimized Clustering Estimators for BAO Measurements Accounting for Significant Redshift Uncertainty
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Holographic Dark Energy with Cosmological Constant
• Cosmology with relativistically varying physical constants
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Combining galaxy and 21cm surveys
• Robustness of cosmic neutrino background detection in the cosmic microwave background
• Measuring the reionization optical depth without large-scale CMB polarization
• Cosmological Constraint on the Light Gravitino Mass from CMB Lensing and Cosmic Shear
• Observational constraints on varying neutrino-mass cosmology
• Relieving tensions related to the lensing of CMB temperature power spectra
• Wandering in the Lyman-alpha Forest: A Study of Dark Matter-Dark Radiation Interactions
• The imprint of $f(R)$ gravity on weak gravitational lensing II : Information content in cosmic shear statistics
• Observational constraints and some toy models in $f(Q)$ gravity with bulk viscous fluid
• Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
• Modeling Transit Dark Energy in $f(R,L_m)$-gravity
• Estimating the power spectrum covariance matrix with fewer mock samples
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Searching for scalar gravitational interactions in current and future cosmological data
• Cosmological Constraints on Higgs-Dilaton Inflation
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• Dark Radiation and Inflationary Freedom after Planck 2015
• Redshift-space distortions in massive neutrino and evolving dark energy cosmologies
• Halo nonlinear reconstruction
• Cosmological constraints from HSC survey first-year data using deep learning
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Clustering and Bias Measurements of SDSS Voids
• Neutrino mass and dark energy constraints from redshift-space distortions
• Observational constraints on Tsallis modified gravity
• Prediction of Supernova Rates in Known Galaxy-galaxy Strong-lens Systems
• The BINGO Project II: Instrument Description
• Information Gains from Cosmological Probes
• Inflation Model Selection meets Dark Radiation
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• Status on bidimensional dark energy parameterizations using SNe Ia JLA and BAO datasets
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Light propagation in inhomogeneous and anisotropic cosmologies
• Is there evidence for additional neutrino species from cosmology?
• Disconnected Covariance of 2-point Functions in Large-Scale Structure
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Computing the Small-Scale Galaxy Power Spectrum and Bispectrum in Configuration-Space
• Baryon acoustic oscillations reconstruction using convolutional neural networks
• Linear Point and Sound Horizon as Purely Geometric standard rulers
• Non-parametric reconstruction of interaction in the cosmic dark sector
• Non-linear contributions to angular power spectra
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Inflationary cosmology with Chaplygin gas in Palatini formalism
• Detecting Damped Lyman-$\alpha$ Absorbers with Gaussian Processes
• Cosmological constraints to dark matter with two- and many-body decays
• Collision Avoidance in Next-generation Fiber Positioner Robotic System for Large Survey Spectrograph
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Reconstructing Cosmological Initial Conditions from Late-Time Structure with Convolutional Neural Networks
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski test: galaxy density gradient field
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• J-PAS: Forecasts for dark matter - dark energy elastic couplings
• Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• The sparkling Universe: the coherent motions of cosmic voids
• A comprehensive investigation on the slowing down of cosmic acceleration
• Effect of evolutionary physical constants on type-1a supernova luminosity
• BAO reconstruction: a swift numerical action method for massive spectroscopic surveys
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• Observational Tests of Gauss-Bonnet Like Dark Energy Model
• Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Evaluation of cosmological models in $f(R,T)$ gravity in different dark energy scenario
• Intensity Mapping in the Presence of Foregrounds and Correlated Continuum Emission
• Weak lensing by galaxy troughs with modified gravity
• First experimental constraints on the disformally coupled Galileon model
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• Imprint of DESI fiber assignment on the anisotropic power spectrum of emission line galaxies
• Constraining Logotropic Unified Dark Energy Models
• The effects of massive neutrinos on the linear point of the correlation function
• Evaporating primordial black holes as varying dark energy
• Beating non-linearities: improving the Baryon Acoustic Oscillations with the linear point
• Scalar and tensor perturbations in loop quantum cosmology: High-order corrections
• Mitigating the Impact of the DESI Fiber Assignment on Galaxy Clustering
• The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant
• Cosmology-marginalized approaches in Bayesian model comparison: the neutrino mass as a case study
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• First study of reionization in the Planck 2015 normalized closed $\Lambda$CDM inflation model
• Searching for features of a string-inspired inflationary model with cosmological observations
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• Kiloparsec Mass/Light Offsets in the Galaxy Pair-Ly$\alpha$ Emitter Lens System SDSS\,J1011$+$0143
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski test and volume effect: galaxy two-point correlation function
• Complementing the ground-based CMB Stage-4 experiment on large scales with the PIXIE satellite
• Non-parametric dark energy reconstruction using the tomographic Alcock-Paczynski test
• Observational effects of a running Planck mass
• Using angular pair upweighting to improve 3D clustering measurements
• Constraints on decaying dark matter from weak lensing and cluster counts
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Constraining the dark energy statefinder hierarchy in a kinematic approach
• SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of Potential Systematics in Fitting of Baryon Acoustic Feature
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Type Ia supernova Hubble diagram with near-infrared and optical observations
• Separate Constraints on Early and Late Cosmology
• Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
• Hunting down systematics in baryon acoustic oscillations after cosmic high noon
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• Cosmological constraints on scalar-tensor gravity and the variation of the gravitational constant
• Parameter Inference for Weak Lensing using Gaussian Processes and MOPED
• Stability of Effective Thin-shell Wormholes Under Lorentz Symmetry Breaking Supported by Dark Matter and Dark Energy
• Tracing the cosmic history by Gauss-Bonnet gravity
• Improving reconstruction of the baryon acoustic peak : the effect of local environment
• Cosmological evidence for leptonic asymmetry after Planck
• Surfing gravitational waves: can bigravity survive growing tensor modes?
• The Cepheid distance to the maser-host galaxy NGC 4258: Studying systematics with the Large Binocular Telescope
• A cosmographic analysis of the transition to acceleration using SN-Ia and BAO
• Cosmological constraints on dark energy models using DESI BAO 2024
• Observational Constraints on Dynamical Dark Energy Models
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• The first Hubble diagram and cosmological constraints using superluminous supernova
• Super-CMB fluctuations and the Hubble tension
• A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
• Nonlinear reconstruction of redshift space distortions
• Supermassive Black Holes in the Early Universe
• Broadband distortion modeling in Lyman-$\alpha$ forest BAO fitting
• Constraining extended teleparallel gravity via cosmography: A model-independent approach
• Gaussian Process Approach for Model-Independent Reconstruction of $f(Q)$ Gravity with Direct Hubble Measurements
• Cosmological tests of an axiverse-inspired quintessence field
• The Integrated Sachs-Wolfe Signal from BOSS Super-Structures
• Study on the mapping of dark matter clustering from real space to redshift space
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion
• New general parametrization of quintessence fields and its observational constraints
• Hill crossing during preheating after hilltop inflation
• An improved model of redshift-space distortions around voids: application to quintessence dark energy
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Testing the warmness of dark matter
• Accuracy of cosmological parameters using the baryon acoustic scale
• Measurement of a Cosmographic Distance Ratio with Galaxy and CMB Lensing
• Sub-percent constraints on cosmological temperature evolution
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Transit String Dark Energy Models in $f(Q)$ Gravity
• Cluster counts: calibration issue or new physics?
• SKA-Phase 1 sensitivity for synchrotron radio emission from multi-TeV Dark Matter candidates
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• Effects of electrically charged dark matter on cosmic microwave background anisotropies
• CMB and matter power spectra with non-linear dark-sector interactions
• Constraining the relative velocity effect using the Baryon Oscillation Spectroscopic Survey
• Taking measurements of the kinematic Sunyaev-Zel'dovich effect forward: including uncertainties from velocity reconstruction with forward modeling
• A new calibration method of sub-halo orbital evolution for semi-analytic models
• Gaussianisation for fast and accurate inference from cosmological data
• Suppressing cosmic variance with paired-and-fixed cosmological simulations: average properties and covariances of dark matter clustering statistics
• Impact of the mean pressure profile of galaxy clusters on the cosmological constraints from the $Planck$ tSZ power spectrum
• Late-time acceleration with a scalar field source: Observational constraints and statefinder diagnostics
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Parametric resonance after hilltop inflation caused by an inhomogeneous inflaton field
• New parametrization of the dark-energy equation of state with a single parameter
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• The phenomenology of beyond Horndeski gravity
• Cosmological Tests of Everpresent $\Lambda$
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
• Friedmann cosmology with decaying vacuum density in Brans-Dicke theory
• Testing for New Physics: Neutrinos and the Primordial Power Spectrum
• Extended family of generalized Chaplygin gas models
• Gaugessence: a dark energy model with early time radiation-like equation of state
• Barry and the BAO Model Comparison
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• Constraints on shear and rotation with massive galaxy clusters
• Reconstruction of interaction rate in Holographic dark energy
• Effects of long-wavelength fluctuations in large galaxy surveys
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Observational constraints on $\alpha$-attractor inflationary models with a Higgs-like potential
• Constraining f(R) Gravity with Planck Sunyaev-Zel'dovich Clusters
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• Cosmological implications of the transition from the false vacuum to the true vacuum state
• Redshift drift constraints on holographic dark energy
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Constraining holographic cosmology using Planck data
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Probing the primordial universe with gravitational waves detectors
• Observational constraints on quintessence models of dark energy
• An accurate determination of the Hubble constant from Baryon Acoustic Oscillation datasets
• Extended $\Lambda$CDM model
• Dark sectors of the Universe: A Euclid survey approach
• Planck Satellite Constraints on Pseudo-Nambu--Goldstone Boson Quintessence
• Observational constraints on the oscillating dark energy cosmologies
• Quantifying the accuracy of the Alcock-Paczynski scaling of baryon acoustic oscillation measurements
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• Large scale distribution of total mass versus luminous matter from Baryon Acoustic Oscillations: First search in the SDSS-III BOSS Data Release 10
• 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
• Testing the mapping between redshift and cosmic scale factor
• Null test for cosmic curvature using Gaussian process
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Preparing for advanced LIGO: A Star-Galaxy Separation Catalog for the Palomar Transient Factory
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• Evidence for baryon acoustic oscillations from galaxy-ellipticity correlations
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• Dynamical Dark Matter from Thermal Freeze-Out
• How the Nonbaryonic Dark Matter Theory Grew
• Testing extended Jordan-Brans-Dicke theories with future cosmological observations
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Cosmological parameter inference from galaxy clustering: The effect of the posterior distribution of the power spectrum
• Geometric Biases in Power-Spectrum Measurements
• Central Mass Profiles of the Nearby Cool-core Galaxy Clusters Hydra A and A478
• A note on the relations between thermodynamics, energy definitions and Friedmann equations
• Looking for dark matter trails in colliding galaxy clusters
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• A Faster Fourier Transform? Computing Small-Scale Power Spectra and Bispectra for Cosmological Simulations in $\mathcal{O}(N^2)$ Time
• Blind Observers of the Sky
• Effective equation of state in modified gravity and observational constraints
• Cosmological acceleration
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• Prospect for cosmological parameter estimation using future Hubble parameter measurements
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• The simplest parametrization of equation of state parameter in the scalar field Universe
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• Machine Learning and cosmographic reconstructions of quintessence and the Swampland conjectures
• Resonant bar detector constraints on macro dark matter
• Modelling Non-Linear Effects of Dark Energy
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Dynamical Background
• An 8-mm diameter Fiber Robot Positioner for Massive Spectroscopy Surveys
• Constraints on the exponential $f(R)$ model from latest Hubble parameter measurements
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• The Impact of Non-Gaussianity upon Cosmological Forecasts
• Constraints on decaying early modified gravity from cosmological observations
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Measurement of Redshift Space Power Spectrum for BOSS galaxies and the Growth Rate at redshift 0.57
• Dissipative dark matter and the rotation curves of dwarf galaxies
• A Steep Slope and Small Scatter for the High-Mass End of the L-$\sigma$ Relation at $z\sim 0.55$
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Bounds on Neutrino Mass in Viscous Cosmology
• Impact of ICM disturbances on the mean pressure profile of galaxy clusters: a prospective study of the NIKA2 SZ large program with MUSIC synthetic clusters
• Probing the constancy of the speed of light with future galaxy survey: the case of SKA and Euclid
• Constraints on running vacuum model with $H(z)$ and $f{\sigma }_8$
• Statistical connection of peak counts to power spectrum and moments in weak lensing field
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• 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
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis
• On general features of warm dark matter with reduced relativistic gas
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Hubble tension in a nonminimally coupled curvature-matter gravity model
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Cepheid Variables in the Maser-Host Galaxy NGC 4258
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Comparison of cosmological models using standard rulers and candles
• Mitigating the noise of DESI mocks using analytic control variates
• The Swampland Conjectures and Slow-Roll Thawing Quintessence
• Including parameter dependence in the data and covariance for cosmological inference
• Estimating Cosmological Parameters from the Dark Matter Distribution
• The relation between cosmological redshift and scale factor for photons
• Covariance of the redshift-space matter power spectrum after reconstruction
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• The sparkling Universe: a scenario for cosmic void motions
• Full forward model of galaxy clustering statistics with AbacusSummit lightcones
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Effect of smoothing of density field on reconstruction and anisotropic BAO analysis
• Tachyon inflation in the Large-$N$ formalism
• Radiative stability and observational constraints on dark energy and modified gravity
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Beyond the growth rate of cosmic structure: Testing modified gravity models with an extra degree of freedom
• Baryon acoustic oscillation methods for generic curvature: Application to the SDSS-III Baryon Oscillation Spectroscopic Survey
• Application of the iterative reconstruction to simulated galaxy fields
• Mass Functions, Luminosity Functions, and Completeness Measurements from Clustering Redshifts
• Clustering with general photo-$z$ uncertainties: Application to Baryon Acoustic Oscillations
• Towards optimal estimation of the galaxy power spectrum
• Testing distance duality with CMB anisotropies
• The effects of peculiar velocities in SN Ia environments on the local $H_0$ measurement
• Testing averaged cosmology with type Ia supernovae and BAO data
• Decoding Dark Matter Substructure without Supervision
• Cubic Derivative Interactions and Asymptotic Dynamics of the Galileon Vacuum
• Cosmological constraint on Brans-Dicke Model
• Constraining quantum collapse inflationary models with current data: The semiclassical approach
• Influences of Dark Energy and dark matter on Gravitational Time Advancement
• Quasars as a tracer of large-scale structures in the distant universe
• New parameterization for unified dark matter and dark energy
• A new parametrization for dark energy density and future deceleration
• Theoretical and observational constraints on Tachyon Inflation
• Target Neutrino Mass Precision for Determining the Neutrino Hierarchy
• Comparing dark energy models with current observational data
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data
• A Direct Measurement of the High-Mass End of the Velocity Dispersion Function at $z\sim 0.55$ from SDSS-III/BOSS
• Primordial power spectrum features in phenomenological descriptions of inflation
• Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
• Linear and non-linear perturbations in dark energy models
• Recovering a redshift-extended VSL signal from galaxy surveys
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Neutrino footprint in Large Scale Structure
• Asymmetric dark matter with a spontaneously broken $U(1{)}^{\prime }$: self-interaction and gravitational waves
• Improving estimates of the growth rate using galaxy-velocity correlations: a simulation study
• Geometry and growth contributions to cosmic shear observables
• The Integrated Bispectrum in Modified Gravity Theories
• Cosmological Tests With Strong Gravitational Lenses using Gaussian Processes
• Constraints on Dark Energy Models Using Late Universe Probes
• Reconstruction of the null-test for the matter density perturbations
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs
• A low Hubble Constant from galaxy distribution observations
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Brane inflation and the robustness of the Starobinsky inflationary model
• A GREAT model comparison against the cosmological constant
• Spatial Curvature and Thermodynamics
• Constraints from observational data for a running cosmological constant and warm dark matter with curvature
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• Biased tracer reconstruction with halo mass information
• Cosmological constraints on sterile neutrino oscillations from Planck
• Vainshtein Screening in Bimetric Cosmology
• Bayesian methods for fitting Baryon Acoustic Oscillations in the Lyman-$\alpha$ forest
• Confronting missing observations with probability weights: Fourier space and generalised formalism
• The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Extracting Spectral Index of Intergalactic Magnetic Field from Radio Polarizations
• Spectroscopic QUasar Extractor and redshift (z) EstimatorSQUEzE I: Methodology
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Probing a panoply of curvaton-decay scenarios using CMB data
• Local probes strongly favor $\Lambda$CDM against power-law and $R_h=ct$ universe
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Combined cosmological tests of a bivalent tachyonic dark energy scalar field model
• Constraining power of open likelihoods, made prior-independent
• Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Optimal Weights For Measuring Redshift Space Distortions in Multi-tracer Galaxy Catalogues
• Screening Mechanism and Late-time Cosmology: Role of a Chameleon-Brans-Dicke Scalar Field
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• Environmental screening of dark matter haloes in $f(R)$ gravity
• The cosmic transparency measured with Type Ia supernovae: implications for intergalactic dust
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• A flat FRW model with dynamical $\Lambda$ as function of matter and geometry
• Cosmological constraints of Palatini $f(\mathcal{R})$ gravity
• Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen
• Reconstructing a non-linear interaction in the dark sector with cosmological observations
• HI intensity mapping with the MIGHTEE survey: power spectrum estimates
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• Dynamical systems analysis of the cubic galileon beyond the exponential potential and the cosmological analogue of the vDVZ discontinuity
• Quasars at intermediate redshift are not special; but they are often satellites
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS
• A Robust BAO Extractor
• Efficient Construction of Mock Catalogs for Baryon Acoustic Oscillation Surveys
• Cluster counts. II. Tensions, massive neutrinos, and modified gravity
• No evidence for the evolution of mass density power-law index $\gamma$ from strong gravitational lensing observation
• Assessment of the Systematic Uncertainties in the Cosmological Analysis of the SDSS Supernovae Photometric Sample
• The bias of weighted dark matter halos from peak theory
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• Redshift-space distortions from vector perturbations
• Impact of $1/f$ noise on cosmological parameter constraints for SKA intensity mapping
• Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• Varying constants entropic--$\Lambda$CDM cosmology
• Cosmic Variation of Proton to Electron Mass Ratio with an interacting Higgs Scalar Field
• Exploring the Cosmological Model in $f(R,T^{\varphi })$ Gravity with Observational Constraints
• Intrinsic Alignment as an RSD Contaminant in the DESI Survey
• Consistency of nonlinear interacting ghost dark energy with recent observations
• How accurately can we measure the baryon acoustic oscillation feature?
• Observational constraints on the fractal cosmology
• Cosmological constraints on the neutron lifetime
• Cosmology from HI galaxy surveys with the SKA
• Testing the consistency between cosmological measurements of distance and age
• Cosmological constraints on $\gamma$-gravity models
• Renyi Holographic Dark Energy models in Teleparallel gravity
• Null tests with Gaussian Process
• Interacting dark energy in the dark $SU(2{)}_R$ model
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• On the luminosity distance and the epoch of acceleration
• Spherically Symmetric N-body Simulations with General Relativistic Dynamics
• Running cosmological constant with observational tests
• Effect of observational holes in fractal analysis of galaxy survey masks
• Combining spectroscopic and photometric surveys using angular cross-correlations III: Galaxy bias and stochastisity
• Decaying dark energy in light of the latest cosmological dataset
• Evidence of dark energy in different cosmological observations
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Linear Density Perturbations in Multifield Coupled Quintessence
• Bianchi type-V Transitioning model in Brans-Dicke theory with Observational Constraint
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data
• Constraints on small-scale primordial density fluctuation from cosmic microwave background through dark matter annihilation
• Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
• The Structural and Kinematic Evolution of Central Star Clusters in Dwarf Galaxies and Their Dependence on Dark Matter Halo Profiles
• Cosmological N-body simulations with generic hot dark matter
• Non-minimally coupled quintessence DE model with a cubic galileon term --A Dynamical System Analysis
• Analysis of branon dark matter and extra-dimensional models with AMS-02
• An Effective Field Theory Analysis of the First LUX Dark Matter Search
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• An HSC view of the CMASS galaxy sample. Halo mass as a function of stellar mass, size and Sérsic index
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Roles of sterile neutrinos in particle physics and cosmology
• Can a void mimic the $\Lambda$ in $\Lambda$CDM?
• Measuring the BAO peak position with different galaxy selections
• Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy
• Cosmological models with running cosmological term and decaying dark matter
• Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect
• Reconstruction with velocities
• Distance-duality in theories with a nonminimal coupling to gravity
• Optimal prior for Bayesian inference in a constrained parameter space
• Constraining non-minimally coupled $\beta$-exponential inflation with CMB data
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Quantum collapse as source of the seeds of cosmic structure during the radiation era
• Higher Order Hamiltonian Monte Carlo Sampling for Cosmological Large-Scale Structure Analysis
• Cosmological constraints on ultra-light axion fields
• Modified Equations of State for Dark Energy and Observational Limitations
• Large scale distribution of mass versus light from Baryon Acoustic Oscillations: Measurement in the final SDSS-III BOSS Data Release 12
• Non-linear matter bispectrum in general relativity
• Hubble constant by natural selection: Evolution chips in the Hubble tension
• The gravitational and lensing-ISW bispectrum of 21cm radiation
• Accretion of Self-interacting Scalar Field Dark Matter Onto a Reissner-Nordström Black Hole
• The variation of the fine structure constant: testing the dipole model with thermonuclear supernovae
• The Color and Stellar Mass Dependence of Small-scale Galaxy Clustering in SDSS-III BOSS
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Large-Distance Lens Uncertainties and Time-Delay Measurements of $H_0$
• Cosmology and CPT violating neutrinos
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): testing a new approach to measure the evolution of the structure growth
• Is there another coincidence problem at the reionization epoch?
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• External priors for the next generation of CMB experiments
• Running vacuum model in non-flat universe
• Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
• The viable f(G) gravity models via reconstruction from the observations
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Computing 3 point correlation function randoms counts without the randoms catalogue
• Cold Dark Matter Based on an Analogy with Superconductivity
• Study on the mapping of halo clustering from real space to redshift space
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• On Dark Matter Explanations of the Gamma-Ray Excesses from the Galactic Center and M31
• Posing Constraints on the Free Parameters of a New Model of Dark Energy EoS : Responses Through Cosmological Behaviours
• Determining $H_0$ using a model-independent method
• Implications of multi-axion dark matter on structure formation
• Cosmological bounds on neutrino statistics
• Interacting parametrized post-Friedmann method
• Astrobotics: Swarm Robotics for Astrophysical Studies
• Cosmological implications of different baryon acoustic oscillation data
• Two-point statistics without bins: A continuous-function generalization of the correlation function estimator for large-scale structure
• A new method to test the cosmic distance duality relation using the strongly lensed gravitational waves
• Observational constraint on axion dark matter in a realistic halo profile with gravitational waves
• Evolution of linear perturbations in Lemaître-Tolman-Bondi void models
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• Smoothing the redshift distributions of random samples for the baryon acoustic oscillations : applications to the SDSS-III BOSS DR12 and QPM mock samples
• Halo shapes constrained from a pure sample of central galaxies in KiDS-1000
• The mass-size relation of LRGs from BOSS and DECaLS
• How Similar are the Properties of Quasars with Nearly Identical Ultraviolet Spectra?
• On tachyonic stability priors for dark energy
• What can we learn from higher multipole power spectra of galaxy distribution in redshift space?
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• The Design, Implementation, and Performance of the LZ Calibration Systems
• Degeneracy between nonadiabatic dark energy models and $\Lambda$CDM: ISW effect and the cross correlation of CMB with galaxy clustering data
• Observational constraints on the growth index parameters in $f(Q)$ gravity
• Impact of photometric redshifts on the galaxy power spectrum and BAO scale in the LSST survey
• Constraints on the Combined Models with $R^{2-q}$ Inflation and Viable $f(R)$ Dark Energy
• Tests of Acoustic Scale Shifts in Halo-based Mock Galaxy Catalogues
• Beyond $\Lambda$CDM: Exploring a Dynamical Cosmological Constant Framework Consistent with Late-Time Observations
• Investigating the $w$CDM Model with Latest DESI BAO Observations
• BAO Extractor: bias and redshift space effects
• Analysis cosmological tachyon and fermion model and observation data constraints
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• Brane inflation driven by an arctan potential: CMB constraints and Reheating
• Global asymptotic dynamics of the cubic galileon interacting with dark matter
• Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Deep learning insights into non-universality in the halo mass function
• Enhancing Cosmological Model Selection with Interpretable Machine Learning
• Cosmic Acceleration in an Extended Brans-Dicke-Higgs Theory
• Consistency of the nonflat $\Lambda$CDM model with the new result from BOSS
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Quantum cosmology of quadratic f(R) theories with a FRW metric
• Observational constraints to a unified cosmological model
• Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
• Cosmological constraints on $\Lambda (\alpha )$CDM models with time-varying fine structure constant
• Collision-free motion planning for fiber positioner robots: discretization of velocity profiles
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• Bayesian deep learning for dark energy
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• 2D BAO vs 3D BAO: Hints for new physics?
• Super-Eddington accreting massive black holes explore high-$z$ cosmology: Monte-Carlo simulations
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Cosmological signatures of a Rapid Diluted Energy Density
• Deep learning for cosmological parameter inference from a dark matter halo density field
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• Constraints on Dark Energy from New Observations including Pan-STARRS
• Quantifying the Colour-Dependent Stochasticity of Large-Scale Structure
• Cosmological Perturbations without Inflation
• Barrow holographic dark energy interacting model in the presence of radiation and matter
• Observational constraints using Bayesian statistics and Deep Learning in $f(Q)$ gravity
• Holography and matter creation revisited
• Reconstruction of the scalar field potential in nonmetricity gravity through Gaussian processes
• On the $2^{\text{nd}}$ feature of the matter two-point function
• Extended Fast Action Minimisation method: application to SDSS-DR12 Combined Sample
• Eternal vs singular observers in interacting dark energy-dark matter models
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• Using relativistic effects in large-scale structure to constrain astrophysical properties of galaxy populations
• Spatial variation of fundamental constants: testing models with thermonuclear supernovae
• What is the optimal way to measure the galaxy power spectrum?
• Optimizing BAO measurements with non-linear transformations of Lyman-alpha forest
• Effects of Angular Momentum on Halo Profiles
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Averaged universe confronted with cosmological observations: A fully covariant approach
• Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation
• Bound Dark Matter (BDM) towards solving the Small Scale Structure Problem
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• Data Analysis and Phenomenological Cosmology
• Analytic Study of Cosmological Perturbations in a Unified Model of Dark Matter and Dark Energy with a Sharp Transition
• Performance of Non-Parametric Reconstruction Techniques in the Late-Time Universe
• A simple supergravity model of inflation constrained with Planck 2018 data
• On the origin of the BAOtr-DESI tension
• Effect of Dark Energy Perturbation on Cosmic Voids Formation
• The Low Redshift survey at Calar Alto (LoRCA)
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset
• The establishment of the Standard Cosmological Model through observations
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Scaling of the 1-halo terms with bias
• Improvements in cosmological constraints from breaking growth degeneracy
• Structure Formation in Dark Matter Particle Production Cosmology
• The consistency test on the cosmic evolution
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Quasi-periodical components in the radial distributions of cosmologically remote objects
• Discerning Dark Energy Models with High-Redshift Standard Candles
• Lyra's cosmology of homogeneous and isotropic universe in Brans-Dicke theory
• Testing and selecting cosmological models with ultra-compact radio quasars
• 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 $\Lambda$
• Reducing the Tension Between the BICEP2 and the Planck Measurements: A Complete Exploration of the Parameter Space
• Probing the shape and internal structure of dark matter halos with the halo-shear-shear three-point correlation function
• Observational constraints on inflationary potentials within the quantum collapse framework
• 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
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• Realising effective theories of tribrid inflation: Are there effects from messenger fields?
• Cosmological Perturbations in the 5D Holographic Big Bang Model
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• Anisotropic cosmology in Bumblebee gravity theory
• Hubble Expansion as an Einstein Curvature
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• Decorrelating the errors of the galaxy correlation function with compact transformation matrices
• Developing Micro DC-Brushless Motor Driver and Position Control for Fiber Positioners
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Power-spectrum simulations of radial redshift distributions
• Robust New Statistic for fitting the Baryon Acoustic Feature
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Constraining LTB models with JLA supernovae and BAO
• Phantom scalar field cosmologies constrained by early cosmic measurements
• Traces of Anisotropic Quasi-Regular Structure in the SDSS Data
• Cosmological parameter fittings with the BICEP2 data
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Assessing the Robustness of the CPL Parametrization to Basis and Prior Variations: Insights from DESI DR2 BAO Data
• Reconstructing cosmic evolution with a density parametrization
• Observational constraints on thawing quintessence scalar field model
• Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe
• A new pressure-parametric cosmological model
• Barboza-Alcaniz Equation of State Parametrization : Constraining the Parameters in Different Gravity Theories
• A New f(R) Model in the Light of Local Gravity Test and Late-time Cosmology
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• Mimicking the $\Lambda$CDM Universe through inhomogeneous space-time
• Environment-based selection effects of Planck clusters
• On the possibility of Baryon Acoustic Oscillation measurements at redshift $z>7.6$ with the Roman Space Telescope
• The presence of a Phantom field in a Randall-Sundrum scenario
• Probing the Type 3 interacting dark-energy model using matter pairwise velocity
• Artificial Neural Networks for Galaxy Clustering. Learning from the two-point correlation function of BOSS galaxies
• Exploring the Universe Expansion History with f(R,T) Gravity: Constraints on Cosmological Parameters
• Production and constraints for a massive dark photon at electron-positron colliders
• Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law $f(Q)$ Gravity with Quasars
• Blois 2019: highlights and outlook
• Non-linear effects in early Universe cosmology
• Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
• Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
• Quintessence dark energy model in non-linear $f(Q)$ theory with bulk-viscosity
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• Cosmology and Quantum Field Theory: A study of the Nambu-Jona-Lasinio Model
• Cosmology and Quantum Field Theory II: Study of an extended Nambu-Jona-Lasinio model with a Dynamical Coupling
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Does History Repeat Itself? Periodic Time Cosmology
• Some Classes of Interacting Two-Fluid Model of the Expanding Universe
• 21-cm power spectrum and ionization bias as a probe of long-mode modulated non Gaussian sky
• Interacting Quintessence and Growth of Structure
• On observational signatures of multi-fractional theory
• Redshift in a six-dimensional classical Kaluza-Klein type model
• A neutrino model fit to the CMB power spectrum
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Observations of General Relativity at strong and weak limits
• The Cosmological Effect of CMB/BAO Measurements
• Accelerating BAO Scale Fitting Using Taylor Series
• Robustness of cosmological axion mass limits
• Model independent reconstruction of cosmological accelerated-decelerated phase
• Mitigating the impact of fiber assignment on the measurement of galaxy-lensing cross correlation
• Momentum transfer models of interacting dark energy
• The equation and solution of 4-point correlation function of galaxies in Gaussian approximation and its parity-odd part
• $G_3$ -- interacting scalar tensor dark energy
• SHARP VIII: J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging
• Nonrelativistic superfluids in cosmology from a relativistic approach: Revisiting two formulations of superfluidity
• Gravitational lensing of pulsars as a probe of dark matter halos
• Fast Mock Catalog Generation for Large Scale Structure Modeling
• Fluctuations in the Ginzburg-Landau Theory of Dark Energy: internal (in-)consistencies in PLANCK data set
• Checking T and CPT violation with sterile neutrino
• Scalar field theory for warm dark matter
• Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum
• CMB lensing tomography with clustering estimation of lens redshift distributions
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• On Generalized Theories of Varying Fine Structure Constant
• Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
• Light rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Ray-traced weak lensing convergence in screened modified gravity theories
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• Revisiting dynamics of interacting quintessence
• Dark Radiation and Inflationary Freedom
• Beyond LCDM: Bits join the Dark Side
• Probing dark energy with braneworld cosmology in the light of recent cosmological data
• Bayesian evidence and model selection approach for time-dependent dark energy
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• A novel Cosmic Filament catalogue from SDSS data
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Exploring the constraints on cosmological models with CosmoEJS
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Dark Radiation and Inflationary Freedom
• Cosmological constraints from the density gradient weighted correlation function
• Constraints on energy scales from dark matter decay in a gauged $B-L$ model
• Cosmological Spectral Deconvolution
• Towards degeneracy problem breaking by large scale structures methods
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms