Cosmological parameters from CMB and other data: a Monte-Carlo approach

Abstract

We present a fast Markov Chain Monte-Carlo exploration of cosmological parameter space. We perform a joint analysis of results from recent CMB experiments and provide parameter constraints, including sigma_8, from the CMB independent of other data. We next combine data from the CMB, HST Key Project, 2dF galaxy redshift survey, supernovae Ia and big-bang nucleosynthesis. The Monte Carlo method allows the rapid investigation of a large number of parameters, and we present results from 6 and 9 parameter analyses of flat models, and an 11 parameter analysis of non-flat models. Our results include constraints on the neutrino mass (m_nu < 0.3eV), equation of state of the dark energy, and the tensor amplitude, as well as demonstrating the effect of additional parameters on the base parameter constraints. In a series of appendices we describe the many uses of importance sampling, including computing results from new data and accuracy correction of results generated from an approximate method. We also discuss the different ways of converting parameter samples to parameter constraints, the effect of the prior, assess the goodness of fit and consistency, and describe the use of analytic marginalization over normalization parameters.

Quintessence results now include perturbations. Changes to match version accepted by PRD. MCMC code and data are available at http://cosmologist.info/cosmomc/ along with a B&W printer-friendly version of the paper

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• Planck Constraint on Relic Primordial Black Holes
• Determining the Hubble constant from Hubble parameter measurements
• Isocurvature bounds on axions revisited
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• New Constraints on Oscillations in the Primordial Spectrum of Inflationary Perturbations
• Modelling the Galactic Magnetic Field on the Plane in 2D
• COrE (Cosmic Origins Explorer) A White Paper
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• The SL2S Galaxy-scale Lens Sample. II. Cosmic evolution of dark and luminous mass in early-type galaxies
• Jeans Analysis for Dwarf Spheroidal Galaxies in Wave Dark Matter
• CMB component separation by parameter estimation
• Stringent Limit on Primordial Magnetic Fields from the Cosmic Microwave Background Radiation
• Constraint on neutrino masses from SDSS-III/BOSS Ly$\alpha$ forest and other cosmological probes
• Testing Feedback-Modified Dark Matter Haloes with Galaxy Rotation Curves: Estimation of Halo Parameters and Consistency with $\Lambda$CDM
• Examining the evidence for dynamical dark energy
• Limits on anisotropic inflation from the Planck data
• Constraining Dark Energy with X-ray Galaxy Clusters, Supernovae and the Cosmic Microwave Background
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Signs of neutrino mass in current cosmological datasets
• Type Ia Supernova Light Curve Inference: Hierarchical Bayesian Analysis in the Near Infrared
• Improved Primordial Non-Gaussianity Constraints from Measurements of Galaxy Clustering and the Integrated Sachs-Wolfe Effect
• The Aemulus Project II: Emulating the Halo Mass Function
• The observational status of Galileon gravity after Planck
• On the most constraining cosmological neutrino mass bounds
• Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• A New Photometric Model of the Galactic Bar using Red Clump Giants
• Discovery and Cosmological Implications of SPT-CL J2106-5844, the Most Massive Known Cluster at z > 1
• Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder
• GAMBIT: The Global and Modular Beyond-the-Standard-Model Inference Tool
• Cosmography with strong lensing of LISA gravitational wave sources
• Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope
• Evolution of dark energy reconstructed from the latest observations
• Converting non-relativistic dark matter to radiation
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Bayesian Estimation of CMB Polarization Maps
• Eliminating the optical depth nuisance from the CMB with 21 cm cosmology
• Density perturbations in generalized Einstein scenarios and constraints on nonminimal couplings from the Cosmic Microwave Background
• Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope
• Galaxy-galaxy lensing estimators and their covariance properties
• The Atacama Cosmology Telescope: a measurement of the primordial power spectrum
• Simultaneous Falsification of LCDM and Quintessence with Massive, Distant Clusters
• Cosmological constraints on Brans-Dicke theory
• Alleviating the $H_0$ and ${\sigma }_8$ anomalies with a decaying dark matter model
• Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• HerMES: Deep Galaxy Number Counts from a P(D) Fluctuation Analysis of SPIRE Science Demonstration Phase Observations
• Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG
• Decaying warm dark matter and neutrino masses
• Propagation of cosmic rays in the AMS-02 era
• Scant evidence for thawing quintessence
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Primordial features due to a step in the inflaton potential
• Modelling redshift space distortions in hierarchical cosmologies
• WMAP7 and future CMB constraints on annihilating dark matter: implications for GeV-scale WIMPs
• Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
• Joint CMB and Weak Lensing Analysis; Physically Motivated Constraints on Cosmological Parameters
• Indirect Dark Matter Detection from Dwarf Satellites: Joint Expectations from Astrophysics and Supersymmetry
• Constraints on Supersymmetric Models of Hybrid Inflation
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• AGNfitter: A Bayesian MCMC approach to fitting spectral energy distributions of AGN
• Planck Constraints on Holographic Dark Energy
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the CMB from Two New Analyses of BOOMERANG Observations
• Constraints on the interacting vacuum -- geodesic CDM scenario
• Updated constraints on the cosmic string tension
• A new life for sterile neutrinos: resolving inconsistencies using hot dark matter
• The mass-sheet degeneracy and time-delay cosmography: Analysis of the strong lens RXJ1131-1231
• Sub-millimetre galaxies reside in dark matter halos with masses greater than 3x10^11 solar masses
• Acoustic scale from the angular power spectra of SDSS-III DR8 photometric luminous galaxies
• Constraining Dark Energy Anisotropic Stress
• Constraining Primordial Magnetism
• Detecting the Rise and Fall of the First Stars by Their Impact on Cosmic Reionization
• Cosmic Voids and Void Lensing in the Dark Energy Survey Science Verification Data
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Cosmological Signatures of Interacting Neutrinos
• Adiabatic instability in coupled dark energy-dark matter models
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Warm inflation dissipative effects: predictions and constraints from the Planck data
• A Bayesian model selection analysis of WMAP3
• An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol Surveys
• Grid Based Linear Neutrino Perturbations in Cosmological N-body Simulations
• Implications of the Cosmic Background Imager Polarization Data
• How well do we understand cosmological recombination?
• H0LiCOW XII. Lens mass model of WFI2033-4723 and blind measurement of its time-delay distance and $H_0$
• Coupled dark matter-dark energy in light of near Universe observations
• Measuring the Speed of Dark: Detecting Dark Energy Perturbations
• Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results
• Dark Photon Oscillations in Our Inhomogeneous Universe
• Systematic Uncertainties In Constraining Dark Matter Annihilation From The Cosmic Microwave Background
• Cluster Density Profiles as a Test of Modified Gravity
• Model-Independent Reconstruction of the Primordial Power Spectrum from WMAP Data
• Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio
• Probing for dynamics of dark energy and curvature of universe with latest cosmological observations
• KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics-I: Inference from Analytical Prediction of High Signal-to-Noise Ratio Convergence Peaks
• Emulating Simulations of Cosmic Dawn for 21cm Power Spectrum Constraints on Cosmology, Reionization, and X-ray Heating
• Neutrino masses and their ordering: Global Data, Priors and Models
• Can we avoid dark energy?
• Position-dependent power spectrum of the large-scale structure: a novel method to measure the squeezed-limit bispectrum
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• Testing chameleon gravity with the Coma cluster
• Observing Dark Energy Dynamics with Supernova, Microwave Background and Galaxy Clustering
• Maximum Likelihood algorithm for parametric component separation in CMB experiments
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Luminosity and stellar mass dependence of galaxy clustering at 0.5<z<1.1
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model
• Cosmological Constraints on DGP Braneworld Gravity with Brane Tension
• Neutrinos help reconcile Planck measurements with both Early and Local Universe
• Pseudoscalar - sterile neutrino interactions: reconciling the cosmos with neutrino oscillations
• Observational constraints on holographic dark energy with varying gravitational constant
• Early recombination as a solution to the $H_0$ tension
• Scale-dependent galaxy bias, CMB lensing-galaxy cross-correlation, and neutrino masses
• The impacts of dark matter particle annihilation on recombination and the anisotropies of the cosmic microwave background
• Relic Neutrinos, thermal axions and cosmology in early 2014
• Precision cosmology defeats void models for acceleration
• Constraint on Coupled Dark Energy Models from Observations
• Neutrino and axion hot dark matter bounds after WMAP-7
• Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological constraints from the full shape of the clustering wedges
• Calibrating the cosmic distance scale ladder: the role of the sound horizon scale and the local expansion rate as distance anchors
• Black hole formation and slow-roll inflation
• Testing modified gravity with Planck: the case of coupled dark energy
• Cosmological Axion and neutrino mass constraints from Planck 2015 temperature and polarization data
• Cosmological parameters from WMAP 5-year temperature maps
• Constraints on the Sound Speed of Dynamical Dark Energy
• Particle Production During Inflation: Observational Constraints and Signatures
• Updated constraints on massive neutrino self-interactions from cosmology in light of the $H_0$ tension
• Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0{w}_a$CDM cosmological parameterization result
• Constraining The Early-Universe Baryon Density And Expansion Rate
• The dark degeneracy and interacting cosmic components
• How early is early dark energy?
• The 1-1000 micron SEDs of far-infrared galaxies
• Pre-inflationary universe in loop quantum cosmology
• Selected topics in scalar-tensor theories and beyond
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• Using the tilted flat-$\Lambda$CDM and the untilted non-flat $\Lambda$CDM inflation models to measure cosmological parameters from a compilation of observational data
• The Mass Distribution and Assembly of the Milky Way from the Properties of the Magellanic Clouds
• Bayesian Analysis of Inflation: Parameter Estimation for Single Field Models
• Cosmic Shear Measurements with DES Science Verification Data
• Decaying dark matter and the tension in ${\sigma }_8$
• Bayesian evidence as a tool for comparing datasets
• Features of holographic dark energy under the combined cosmological constraints
• Beyond six parameters: extending $\Lambda$CDM
• The Statistical Significance of the Low CMB Mulitipoles
• Neutrino physics from precision cosmology
• Cosmological Constraints From Weak Lensing Peak Statistics With CFHT Stripe 82 Survey
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• Testing the Isotropy of the Universe with Type Ia Supernovae
• The outer halo globular cluster system of M31 - II. Kinematics
• Revisiting Generalized Chaplygin Gas as a Unified Dark Matter and Dark Energy Model
• Bayesian analysis of spatial-dependent cosmic-ray propagation: astrophysical background of antiprotons and positrons
• Primordial Neutrinos
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• A New Look at Massive Clusters: weak lensing constraints on the triaxial dark matter halos of Abell 1689, Abell 1835, & Abell 2204
• Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension
• Constraints on massive sterile neutrino species from current and future cosmological data
• Precision Epoch of Reionization studies with next-generation CMB experiments
• Limits on Dark Radiation, Early Dark Energy, and Relativistic Degrees of Freedom
• Field theoretic interpretations of interacting dark energy scenarios and recent observations
• Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations
• WMAPping inflationary physics
• A preference for a non-zero neutrino mass from cosmological data
• Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Comparing Brane Inflation to WMAP
• The Beginning and Evolution of the Universe
• Present and future evidence for evolving dark energy
• Dark matter profiles and annihilation in dwarf spheroidal galaxies: prospectives for present and future gamma-ray observatories - I. The classical dSphs
• Distance Priors from Planck and Dark Energy Constraints from Current Data
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Cosmological constraints on a decomposed Chaplygin gas
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• Addendum to: Global constraints on absolute neutrino masses and their ordering
• Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data
• Dynamics of Interacting Quintessence Models: Observational Constraints
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Cosmological Parameters from Pre-Planck CMB Measurements
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• Evidence for interacting dark energy from BOSS
• Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
• Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map
• Dark energy with non-adiabatic sound speed: initial conditions and detectability
• Observational bounds on the cosmic radiation density
• Implications of the Higgs Boson Discovery for mSUGRA
• anesthetic: nested sampling visualisation
• WMAP and Inflation
• Observational signatures of Jordan-Brans-Dicke theories of gravity
• Interacting Dark Energy in a closed universe
• The Foundation Supernova Survey: Measuring Cosmological Parameters with Supernovae from a Single Telescope
• Improved Models for Cosmic Infrared Background Anisotropies: New Constraints on the IR Galaxy Population
• New constraints on time-dependent variations of fundamental constants using Planck data
• Cosmological parameter estimation using Very Small Array data out to l=1500
• Cosmic reionization after Planck II: contribution from quasars
• Non-Baryonic Dark Matter in Cosmology
• Constraints on dark matter annihilation from CMB observations before Planck
• Cosmic acceleration in dust only Universe via energy-momentum powered gravity
• Model-independent constraints on reionization from large-scale CMB polarization
• Radio Counterparts of Compact Binary Mergers detectable in Gravitational Waves: A Simulation for an Optimized Survey
• Reconstructing the primordial power spectrum - a new algorithm
• The kSZ effect as a test of general radial inhomogeneity in LTB cosmology
• Quantitative study of the AMS-02 electron/positron spectra: implications for the pulsar and dark matter properties
• From Planck data to Planck era: Observational tests of Holographic Cosmology
• CMB and BBN constraints on evaporating primordial black holes revisited
• Multiple inflation and the WMAP 'glitches' II. Data analysis and cosmological parameter extraction
• Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Reionization optical depth determination from Planck HFI data with ten percent accuracy
• Improved constraints on cosmic microwave background secondary anisotropies from the complete 2008 South Pole Telescope data
• Planck Early Results: The Planck View of Nearby Galaxies
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• Neutrino Dark Energy -- Revisiting the Stability Issue
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• Constraining dark matter late-time energy injection: decays and p-wave annihilations
• Asymmetric Dark Matter and Dark Radiation
• Cosmological Information in the Intrinsic Alignments of Luminous Red Galaxies
• Simulating the Spitzer mid-IR color-color diagrams
• Approximate Bayesian Computation for Forward Modeling in Cosmology
• The Lyman-alpha forest and WMAP year three
• Matching current observational constraints with nonminimally coupled dark energy
• Bayesian model selection and isocurvature perturbations
• Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae
• Axion hot dark matter bounds after Planck
• Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
• Upper limits on neutrino masses from the 2dFGRS and WMAP: the role of priors
• Asymmetric Inelastic Inert Doublet Dark Matter from Triplet Scalar Leptogenesis
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the Halo Occupation Distribution model for Emission Line Galaxies
• The phenomenological approach to modeling the dark energy
• Impact of neutrino properties on the estimation of inflationary parameters from current and future observations
• Fables of reconstruction: controlling bias in the dark energy equation of state
• Improved Measurements of the CMB Power Spectrum with ACBAR
• Reconstructing Gravity on Cosmological Scales
• Dark Coupling and Gauge Invariance
• Measuring neutrino masses with a future galaxy survey
• Designing a space-based galaxy redshift survey to probe dark energy
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• A Model Of Inflationary Cosmology Without Singularity
• Relieving the $H_0$ tension with a new interacting dark energy model
• Redshift Dependence of the CMB Temperature from S-Z Measurements
• Constraints on Cosmological Parameters from the 500 deg${}^2$ SPTpol Lensing Power Spectrum
• Using BBN in cosmological parameter extraction from CMB: a forecast for Planck
• Estimating Cosmological Parameter Covariance
• Exploring the Superimposed Oscillations Parameter Space
• SED fitting with Markov Chain Monte Carlo: Methodology and Application to z=3.1 Lyman Alpha Emitting Galaxies
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• New CMB constraints for Abelian Higgs cosmic strings
• New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
• Discovering anomaly-mediated supersymmetry at the LHC
• Sterile Neutrinos: Cosmology vs Short-BaseLine Experiments
• CosmoHammer: Cosmological parameter estimation with the MCMC Hammer
• Connecting massive galaxies to dark matter halos in BOSS - I. Is galaxy color a stochastic process in high-mass halos?
• Observational constraints on the tilted spatially-flat and the untilted nonflat $\varphi$CDM dynamical dark energy inflation models
• Constraints on primordial gravitational waves from the Cosmic Microwave Background
• Future CMB Constraints on Early, Cold, or Stressed Dark Energy
• Structure formation constraints on the Jordan-Brans-Dicke theory
• Dark sectors with dynamical coupling
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
• Cosmographic reconstruction of $f(\mathcal{T})$ cosmology
• CMB Constraints on a Stochastic Background of Primordial Magnetic Fields
• Cosmic microwave background with Brans-Dicke gravity II: constraints with the WMAP and SDSS data
• Estimation of cosmological parameters using adaptive importance sampling
• A Profile Likelihood Analysis of the Constrained MSSM with Genetic Algorithms
• Observational constraints on variable equation of state parameters of dark matter and dark energy after Planck
• Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
• The intergalactic medium thermal history at redshift z=1.7--3.2 from the Lyman alpha forest: a comparison of measurements using wavelets and the flux distribution
• Testing coupled dark energy with large scale structure observation
• Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
• Intrinsic alignments of galaxies in the MassiveBlack-II simulation: analysis of two-point statistics
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• CIGALEMC: Galaxy Parameter Estimation using a Markov Chain Monte Carlo Approach with Cigale
• Testing the dark energy with gravitational lensing statistics
• Evidence for Emergent Dark Energy
• Effects of a Primordial Magnetic Field on Low and High Multipoles of the CMB
• New constraints on parametrised modified gravity from correlations of the CMB with large scale structure
• Neutrinos in Physics and Astrophysics
• The parameter space in Galileon gravity models
• Localizing compact binary inspirals on the sky using ground-based gravitational wave interferometers
• Constraining $f(R)$ Gravity Theory Using Weak Lensing Peak Statistics from the Canada-France-Hawaii-Telescope Lensing Survey
• Cosmological Constraints on Horndeski Gravity in Light of GW170817
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• All-inclusive interacting dark sector cosmologies
• Constraints on coupled dark energy using CMB data from WMAP and SPT
• Hunting Down the Best Model of Inflation with Bayesian Evidence
• Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS
• Increasing Neff with particles in thermal equilibrium with neutrinos
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Testing General Relativity at Cosmological Scales: Implementation and Parameter Correlations
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Cosmological Hints of Modified Gravity ?
• Fast cosmological parameter estimation using neural networks
• Reconciling $H_0$ tension in a six parameter space?
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Constraints on a mixed inflaton and curvaton scenario for the generation of the curvature perturbation
• Complementarity of Weak Lensing and Peculiar Velocity Measurements in Testing General Relativity
• Constraints on f(R) Cosmology in the Palatini Formalism
• The large-scale properties of simulated cosmological magnetic fields
• Testing models of vacuum energy interacting with cold dark matter
• Decaying particles and the reionization history of the Universe
• MAXIPOL: Cosmic Microwave Background Polarimetry Using a Rotating Half-Wave Plate
• How flat can you get? A model comparison perspective on the curvature of the Universe
• Direct reconstruction of the quintessence potential
• Deep 3 GHz Number Counts from a P(D) Fluctuation Analysis
• Updated constraints on amplitude and tilt of the tensor primordial spectrum
• Neutrino Mass Bounds in the era of Tension Cosmology
• Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Constraining interacting dark energy models with latest cosmological observations
• Resolving Cosmic Neutrino Structure: A Hybrid Neutrino N-body Scheme
• On the Validity of Cosmological Fisher Matrix Forecasts
• Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach
• Models of the Primordial Standard Clock
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• Bayesian model selection without evidences: application to the dark energy equation-of-state
• Quantifying dimensionality: Bayesian cosmological model complexities
• Neutrino Masses from Cosmological Probes
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Cosmology Based on f(R) Gravity Admits 1 eV Sterile Neutrinos
• Model selection applied to reconstruction of the Primordial Power Spectrum
• The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM
• On Minimally-Parametric Primordial Power Spectrum Reconstruction and the Evidence for a Red Tilt
• Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
• Probing Dark Energy with Supernovae: Exploiting Complementarity with the Cosmic Microwave Background
• A re-analysis of the three-year WMAP temperature power spectrum and likelihood
• Global fits of the dark matter-nucleon effective interactions
• Revealing the Nature of Dark Energy Using Bayesian Evidence
• WMAP Constraints on Decaying Cold Dark Matter
• Properties of Galactic cirrus clouds observed by BOOMERanG
• First Constraint on the Neutrino-Induced Phase Shift in the BAO Spectrum
• Mapping Growth and Gravity with Robust Redshift Space Distortions
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• Constraints on braneworld inflation from CMB anisotropies
• Neutrino mass hierarchy and electron neutrino oscillation parameters with one hundred thousand reactor events
• On the impact of $f(Q)$ gravity on the Large Scale Structure
• Brane inflation and the WMAP data: a Bayesian analysis
• Improving time-delay cosmography with spatially resolved kinematics
• Wiggly Whipped Inflation
• Inflation with moderately sharp features in the speed of sound: GSR and in-in formalism for power spectrum and bispectrum
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• Updated constraints on $f(\mathcal{R})$ gravity from cosmography
• H0 tension or T0 tension?
• Observational constraints on patch inflation in noncommutative spacetime
• No new cosmological concordance with massive sterile neutrinos
• New Constraints on the Primordial Magnetic Field
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?
• Comparison of sampling techniques for Bayesian parameter estimation
• Constraining Gravity at the Largest Scales through CMB Lensing and Galaxy Velocities
• Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data
• Robustness of dark energy phenomenology across different parameterizations
• Model-independent cosmological constraints from the CMB
• Falsifying Paradigms for Cosmic Acceleration
• Probing kinematics and fate of the Universe with linearly time-varying deceleration parameter
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Whipped inflation
• Constraint on the abundance of primordial black holes in dark matter from Planck data
• On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond $\Lambda$CDM
• The effect of Limber and flat-sky approximations on galaxy weak lensing
• Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples
• The Search for a Primordial Magnetic Field
• Updated CMB, X- and gamma-ray constraints on majoron dark matter
• Is there concordance within the concordance $\Lambda$CDM model?
• Nonlinear growth in modified gravity theories of dark energy
• Cosmological Constraints on Newton's Constant
• On the Viability of Bianchi Type VIIh Models with Dark Energy
• Quantum Gravity in the Sky: Interplay between fundamental theory and observations
• DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
• Breaking the spell of Gaussianity: forecasting with higher order Fisher matrices
• An improved cosmological bound on the thermal axion mass
• Constraining the time variation of Newton's constant $G$ with gravitational-wave standard sirens and supernovae
• Dark Matter CMB Constraints and Likelihoods for Poor Particle Physicists
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• Natural Inflation: Consistency with Cosmic Microwave Background Observations of Planck and BICEP2
• Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2
• Swampland Conjectures and Late-Time Cosmology
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• Testing the Copernican principle by constraining spatial homogeneity
• The Differential Rotation of Kappa1 Ceti as Observed by MOST
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Cosmological lepton asymmetry with a nonzero mixing angle θ_{13}
• Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
• Observational Constraints on Gauge Field Production in Axion Inflation
• Analyze This! A Cosmological Constraint Package for CMBEASY
• Measuring the speed of cosmological gravitational waves
• The Cosmic Microwave Background and the Ionization History of the Universe
• Cosmological Bound on the QCD Axion Mass, Redux
• Constraints on Neutrino Masses from Weak Lensing
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
• Revisiting cosmological bounds on sterile neutrinos
• CMB Polarization Systematics, Cosmological Birefringence and the Gravitational Waves Background
• MGCAMB with massive neutrinos and dynamical dark energy
• Early dark energy from zero-point quantum fluctuations
• Is a step in the primordial spectral index favored by CMB data ?
• Addendum to "Superimposed Oscillations in the WMAP Data?"
• Effects of modified gravity on B-mode polarization
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• A measurement of the Hubble constant from angular diameter distances to two gravitational lenses
• Cosmological discordances: a new measure, marginalization effects, and application to geometry vs growth current data sets
• The cosmology of sub-MeV dark matter freeze-in
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
• Cosmological constraints on dark matter models with velocity-dependent annihilation cross section
• Constraints on the Primordial Power Spectrum from High Resolution Lyman-alpha Forest Spectra and WMAP
• Large-scale structure phenomenology of viable Horndeski theories
• A Bayesian analysis of the primordial power spectrum
• Cosmological Constraints on Decoupled Dark Photons and Dark Higgs
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• Updated Constraints and Forecasts on Primordial Tensor Modes
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Soundness of Dark Energy properties
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• The Shape of the Primordial Power Spectrum: A Last Stand Before Planck
• Late time transitions in the quintessence field and the $H_0$ tension
• Impacts of dark energy on weighing neutrinos: mass hierarchies considered
• Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
• Exponential Potentials for Tracker Fields
• Testing 3+1 and 3+2 neutrino mass models with cosmology and short baseline experiments
• $\Lambda$CDM or self-interacting neutrinos? - how CMB data can tell the two models apart
• A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
• Correlated isocurvature perturbations from mixed inflaton-curvaton decay
• Primordial Non-Gaussianity and the NRAO VLA Sky Survey
• Low & High scale MSSM inflation, gravitational waves and constraints from Planck
• A comprehensive comparison of cosmological models from latest observational data
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Bayesian emulator optimisation for cosmology: application to the Lyman-alpha forest
• Improved limits on short-wavelength gravitational waves from the cosmic microwave background
• CMB Polarization B-mode Delensing with SPTpol and Herschel
• Probing Dark Energy Using Its Density Instead of Its Equation of State
• Observational constraints on braneworld inflation: the effect of a Gauss-Bonnet term
• Comparison of statistical sampling methods with ScannerBit, the GAMBIT scanning module
• Cosmological limits on neutrino unknowns versus low redshift priors
• Planck Constraints on Monodromy Inflation
• Cosmography: Supernovae Union2, Baryon Acoustic Oscillation, Observational Hubble Data and Gamma Ray Bursts
• First Observational Tests of Eternal Inflation: Analysis Methods and WMAP 7-Year Results
• Mass, velocity anisotropy, and pseudo phase-space density profiles of Abell 2142
• WMAP5 constraints on the unified model of dark energy and dark matter
• Testing Low-Redshift Cosmic Acceleration with Large-Scale Structure
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Oscillations in the inflaton potential: Complete numerical treatment and comparison with the recent and forthcoming CMB datasets
• MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio
• An MCMC approach to extracting the global 21-cm signal during the cosmic dawn from sky-averaged radio observations
• Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\varphi$CDM dark energy inflation cosmologies
• Constraints on the cosmic neutrino background
• Revealing the effects of curvature on the cosmological models
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Constraints on Primordial Magnetic Fields from Planck combined with the South Pole Telescope CMB B-mode polarization measurements
• Quintessence reconstructed: new constraints and tracker viability
• Impacts of dark energy on weighing neutrinos after Planck 2015
• Constraints on the neutrino mass and mass hierarchy from cosmological observations
• Cosmology and the neutrino mass ordering
• Cosmological parameters, shear maps and power spectra from CFHTLenS using Bayesian hierarchical inference
• Updating constraints on f(T) teleparallel cosmology and the consistency with Big Bang Nucleosynthesis
• The Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest
• Constraints on the Brans-Dicke gravity theory with the Planck data
• Correlated adiabatic and isocurvature CMB fluctuations in the wake of the WMAP
• Einstein's Universe: Cosmological structure formation in numerical relativity
• Anisotropic dark matter distribution functions and impact on WIMP direct detection
• Constraining the helium abundance with CMB
• A Constraint on Planck-scale Modifications to Electrodynamics with CMB polarization data
• The spin expansion for binary black hole merger: new predictions and future directions
• Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data
• The impact of AGN feedback and baryonic cooling on galaxy clusters as gravitational lenses
• The exact numerical treatment of inflationary models
• Observational Constraints on Oscillating Dark-Energy Parametrizations
• Testing CPT Symmetry with CMB Measurements
• CMB photons shedding light on dark matter
• Evolution of high-energy particle distribution in Supernova Remnants
• Emulators for the non-linear matter power spectrum beyond $\Lambda$CDM
• Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Confronting General Relativity with Further Cosmological Data
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• HST Emission Line Galaxies at z ~ 2: Comparing Physical Properties of Lyman Alpha and Optical Emission Line Selected Galaxies
• The galaxy power spectrum: precision cosmology from large scale structure?
• Testing the isotropy of the Universe by using the JLA compilation of type-Ia supernovae
• Are cosmological neutrinos free-streaming?
• Constraints on the Evolution of the Primordial Magnetic Field from the Small-Scale Cosmic Microwave Background Angular Anisotropy
• Dark Energy Constraints after Planck
• Post-$Planck$ constraints on interacting vacuum energy
• Constraining cosmology and ionization history with combined 21 cm power spectrum and global signal measurements
• Dark matter vs. astrophysics in the interpretation of AMS-02 electron and positron data
• Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
• Reconstruction of the Dark Energy equation of state
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Constraining Warm Inflation with CMB data
• astroABC: An Approximate Bayesian Computation Sequential Monte Carlo sampler for cosmological parameter estimation
• Primordial Features from Linear to Nonlinear Scales
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Connecting Synchrotron, Cosmic Rays, and Magnetic Fields in the Plane of the Galaxy
• Cosmological parameter inference with Bayesian statistics
• iCosmo: an Interactive Cosmology Package
• Dark matter searches in the gamma-ray extragalactic background via cross-correlations with galaxy catalogues
• Squeezing the window on isocurvature modes with the Lyman-alpha forest
• Dark Neutrino interactions phase out the Hubble tension
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• WMAP constraints on inflationary models with global defects
• Dissecting the high-z interstellar medium through intensity mapping cross-correlations
• Constraining Lorentz violation with cosmology
• Can Dark Matter Decay in Dark Energy?
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• A low CMB variance in the WMAP data
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Do current cosmological observations rule out all Covariant Galileons?
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
• New observational constraints on $f(T)$ cosmology from radio quasars
• Coupled dark energy with perturbed Hubble expansion rate
• A Markov Chain Monte Carlo for Galactic Cosmic Ray physics: I. Method and results for the Leaky Box Model
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• Testing for double inflation with WMAP
• Efficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy Surveys
• Light sterile neutrinos after BICEP-2
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• ExoFit: Orbital Parameters of Extra-solar Planets from Radial Velocities
• Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume
• Reconciling the local void with the CMB
• BayesCLUMPY: Bayesian Inference with Clumpy Dusty Torus Models
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Testing extreme-axion wave dark matter using the BOSS Lyman-Alpha forest data
• The CMB Quadrupole depression produced by early fast-roll inflation: MCMC analysis of WMAP and SDSS data
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Crossing SNe Ia and BAO observational constraints with local ones in hybrid metric-Palatini gravity
• Isocurvature forecast in the anthropic axion window
• Overcoming the Circular Problem for γ-ray Bursts in Cosmological Global Fitting Analysis
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• First results from the Very Small Array -- IV. Cosmological parameter estimation
• Joint QSO-CMB constraints on reionization history
• Forecasting the Bayes factor of a future observation
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• The last stand before MAP: cosmological parameters from lensing, CMB and galaxy clustering
• Constraining Monodromy Inflation
• Galaxy-Galaxy Lensing in the DES Science Verification Data
• {\sc CosmoNet}: fast cosmological parameter estimation in non-flat models using neural networks
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• Efficient Cosmological Parameter Estimation with Hamiltonian Monte Carlo
• Modified Chaplygin Gas as a Unified Dark Matter and Dark Energy Model and Cosmic Constraints
• Reionization constraints using Principal Component Analysis
• Constraints on neutrino and dark radiation interactions using cosmological observations
• Connecting early and late epochs by f(z)CDM cosmography
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space
• Constraining the dark energy equation of state with double source plane strong lenses
• Forecasts for CMB μ- and i-type spectral distortion constraints on the primordial power spectrum on scales 8 < k < 10^4 Mpc^-1 with the future Pixie-like experiments
• Using correlations between CMB lensing and large-scale structure to measure primordial non-Gaussianity
• B-modes and the Nature of Inflation
• Calibrating the Planck Cluster Mass Scale with CLASH
• An evaluation of cosmological models from expansion and growth of structure measurements
• Model independent inference of the expansion history and implications for the growth of structure
• Early Structure Formation Constraints on the Ultra-Light Axion in the Post-Inflation Scenario
• Cosmological constraints on an exponential interaction in the dark sector
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies
• Post-WMAP Assessment of Infrared Cutoff in the Primordial Spectrum from Inflation
• A double take on early and interacting dark energy from JWST
• The impact of a new median statistics $H_0$ prior on the evidence for dark radiation
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
• Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• On what scale should inflationary observables be constrained?
• Combining Planck with Large Scale Structure gives strong neutrino mass constraint
• A search for sterile neutrinos with the latest cosmological observations
• The nature of the unresolved extragalactic soft CXB
• Dynamical models for the Sculptor dwarf spheroidal in a Lambda CDM universe
• Measuring the primordial power spectrum: Principal component analysis of the cosmic microwave background
• A New Class of Parametrization for Dark Energy without Divergence
• WIMP astronomy and particle physics with liquid-noble and cryogenic direct-detection experiments
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Measuring the cosmological bulk flow using the peculiar velocities of supernovae
• Constraints on secret neutrino interactions after Planck
• Neutrino mass constraint with the Sloan Digital Sky Survey power spectrum of luminous red galaxies and perturbation theory
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Cosmic microwave anisotropies from BPS semilocal strings
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• A Bayesian view of the current status of dark matter direct searches
• Primordial Black Holes, Eternal Inflation, and the Inflationary Parameter Space after WMAP5
• The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies
• Challenging bulk viscous unified scenarios with cosmological observations
• The High Redshift Integrated Sachs-Wolfe Effect
• Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Can cosmology detect hierarchical neutrino masses?
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• How Well Can Future CMB Missions Constrain Cosmic Inflation?
• Cosmological constraints on neutrino plus axion hot dark matter
• Quantifying concordance of correlated cosmological data sets
• Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing
• HelMod in the works: from direct observations to the local interstellar spectrum of cosmic-ray electrons
• The Monopole Moment of the Three-Point Correlation Function of the 2-degree Field Galaxy Redshift Survey
• Cosmological constraints on coupled dark energy
• Universal features of quantum bounce in loop quantum cosmology
• Smoothing spline primordial power spectrum reconstruction
• Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State
• Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lyman-alpha Emitters in COSMOS and GOODS-N
• Testing dark energy paradigms with weak gravitational lensing
• Cosmological constraints on slow-roll inflation: an update
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Galileons on Trial
• Signatures of a Graviton Mass in the Cosmic Microwave Background
• New cosmological bounds on hot relics: Axions $\&$ Neutrinos
• Cosmic Microwave Background constraints for global strings and global monopoles
• Pippi - painless parsing, post-processing and plotting of posterior and likelihood samples
• Searching for Oscillations in the Primordial Power Spectrum: Perturbative Approach (Paper I)
• From Cavendish to PLANCK: Constraining Newton's Gravitational Constant with CMB Temperature and Polarization Anisotropy
• A combined analysis of 3D Weak Lensing, Lyman-alpha forest and WMAP year three data
• Cosmic ray propagation and dark matter in light of the latest AMS-02 data
• Probing elastic interactions in the dark sector and the role of $S_8$
• Observational constraints on Gauss-Bonnet cosmology
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Can Non-standard Recombination Resolve the Hubble Tension?
• Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
• Compatibility of Planck and BICEP2 in the Light of Inflation
• Efficient Evaluation of Cosmological Angular Statistics
• Lyman-alpha Forest Constraints on Decaying Dark Matter
• Novel cosmological bounds on thermally-produced axion-like particles
• Hints of Isocurvature Perturbations in the Cosmic Microwave Background?
• Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946
• Anisotropy of the Universe via the Pantheon supernovae sample revisited
• AIC, BIC, Bayesian evidence against the interacting dark energy model
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• Mass bias evolution in tSZ cluster cosmology
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Structural and dynamical modeling of WINGS clusters. II. The orbital anisotropies of elliptical, spiral and lenticular galaxies
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Bias and scatter in the Hubble diagram from cosmological large-scale structure
• Do the cosmological observational data prefer phantom dark energy?
• A fake Interacting Dark Energy detection?
• Cosmic string parameter constraints and model analysis using small scale Cosmic Microwave Background data
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• Complete Reionization Constraints from Planck 2015 Polarization
• Polyspectra searches for sharp oscillatory features in cosmic microwave sky data
• Spatial curvature and cosmological tests of general relativity
• Constraints on Scalar and Tensor spectra from $N_{eff}$
• The WiggleZ Dark Energy Survey: Final Data Release and the Metallicity of UV-Luminous Galaxies
• Constraints on dark-matter properties from large-scale structure
• WMAP, neutrino degeneracy and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation
• Multi-wavelength constraints on the inflationary consistency relation
• Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Dark Radiation and interacting scenarios
• Measuring the Properties of Dark Energy with Photometrically Classified Pan-STARRS Supernovae. I. Systematic Uncertainty from Core-Collapse Supernova Contamination
• The resilience of the Etherington-Hubble relation
• Current Observational Constraints on Cosmic Doomsday
• Primordial gravitational waves and the H0-tension problem
• Emergent Dark Energy, neutrinos and cosmological tensions
• Markov chain Monte Carlo analysis of Bianchi VII_h models
• Joint deprojection of Sunyaev-Zeldovich and X-ray images of galaxy clusters
• Null Signal for the Cosmic Anisotropy in the Pantheon Supernovae Data
• Determining Cosmological Parameters with Latest Observational Data
• A cross-correlation study of the Fermi-LAT $\gamma$-ray diffuse extragalactic signal
• Updating constraints on inflationary features in the primordial power spectrum with the Planck data
• Information Gain on Reheating: the One Bit Milestone
• Large-scale (in-) stability Analysis of an Exactly Solved Coupled Dark-Energy Model
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
• Cosmic microwave background constraints on secret interactions among sterile neutrinos
• The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties
• Limits on Defects Formation and Hybrid Inflationary Models with Three-Year WMAP Observations
• Exploring uncertainties in dark energy constraints using current observational data with Planck 2015 distance priors
• Testing the effect of $H_0$ on $f{\sigma }_8$ tension using a Gaussian Process method
• Inflationary Potential Reconstruction for a WMAP Running Power Spectrum
• Future CMB cosmological constraints in a dark coupled universe
• Evidence for extra radiation? Profile likelihood versus Bayesian posterior
• Growth factor parametrization in curved space
• New limits on Early Dark Energy from the South Pole Telescope
• Constraints on the generalized Chaplygin gas model including gamma-ray bursts via a Markov Chain Monte Carlo approach
• Cosmological parameter estimation and Bayesian model comparison using VSA data
• Analytic Methods for Cosmological Likelihoods
• Reconstruction of the Primordial Power Spectrum by Direct Inversion
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Taking Bigger Metropolis Steps by Dragging Fast Variables
• Search for Compensated Isocurvature Perturbations with Planck Power Spectra
• Unveiling the Dynamics of the Universe
• Probing the neutrino mass hierarchy with CMB weak lensing
• An Extended action for the effective field theory of dark energy: a stability analysis and a complete guide to the mapping at the basis of EFTCAMB
• $\nu \mathrm{CO}N\mathrm{CEPT}$: Cosmological neutrino simulations from the non-linear Boltzmann hierarchy
• Testing Hu-Sawicki f(R) gravity with the Effective Field Theory approach
• Do observations prove that cosmological neutrinos are thermally distributed?
• Constraining inflation with future galaxy redshift surveys
• Cluster-Void Degeneracy Breaking: Dark Energy, Planck and the Largest Cluster & Void
• Large scale anomalies in the CMB and non-Gaussianity in bouncing cosmologies
• Rico: An Accurate Cosmological Recombination Code
• Impact of the non-Gaussian covariance of the weak lensing power spectrum and bispectrum on cosmological parameter estimation
• Features in the primordial power spectrum? A frequentist analysis
• Contribution to the Diffuse Radio Background from Extragalactic Radio Sources
• Cosmological constraints on a light non-thermal sterile neutrino
• Analytical Solutions to the Mass-Anisotropy Degeneracy with Higher Order Jeans Analysis: A General Method
• Signatures of Self-Interacting Dark Matter in the Matter Power Spectrum and the CMB
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the ${\Omega }_m$-${\sigma }_8$ plane
• Horava Gravity in the Effective Field Theory formalism: from cosmology to observational constraints
• Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments
• Constraints on primordial isocurvature perturbations and spatial curvature by Bayesian model selection
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• How Cold is Cold Dark Matter?
• The Adiabatic Instability on Cosmology's Dark Side
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Is cosmology compatible with sterile neutrinos?
• Constraining Fundamental Physics with Future CMB Experiments
• What do we know about cosmography
• EFTCAMB/EFTCosmoMC: massive neutrinos in dark cosmologies
• Cosmological constraints on non-standard inflationary quantum collapse models
• Breaking Beta: A comparison of mass modelling methods for spherical systems
• Predictions of just-enough inflation
• Probing CPT Violation with CMB Polarization Measurements
• A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• 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
• CosRayMC: a global fitting method in studying the properties of the new sources of cosmic e${}^{\pm }$ excesses
• Planck confronts large scale structure: methods to quantify discordance
• Measurement of CIB power spectra over large sky areas from Planck HFI maps
• Prospects for direct detection of dark matter in an effective theory approach
• Latest astronomical constraints on some nonlinear parametric dark energy models
• Evidence for bouncing evolution before inflation after BICEP2
• Cosmological Parameters from pre-Planck CMB Measurements: a 2017 Update
• CFHTLS weak-lensing constraints on the neutrino masses
• Constraints on a Stochastic Background of Primordial Magnetic Fields with WMAP and South Pole Telescope data
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Observational Constraints on Exponential Gravity
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Experimental constraints on the uncoupled Galileon model from SNLS3 data and other cosmological probes
• Probing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data
• Bayesian Evidence against Harrison-Zel'dovich spectrum in tension cosmology
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Contribution of domain wall networks to the CMB power spectrum
• Is the $H_0$ tension suggesting a 4th neutrino's generation?
• Prospects for Constraining Neutrino Mass Using Planck and Lyman-Alpha Forest Data
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• Suppressing the impact of a high tensor-to-scalar ratio on the temperature anisotropies
• MultiModeCode: An efficient numerical solver for multifield inflation
• Is the Harrison-Zel'dovich spectrum coming back? ACT preference for $n_s\sim 1$ and its discordance with Planck
• Modified Gravity Constraints from the Full Shape Modeling of Clustering Measurements from DESI 2024
• Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
• Constraints on modified gravity from Planck 2015: when the health of your theory makes the difference
• Constraints on the CMB temperature redshift dependence from SZ and distance measurements
• 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
• Revisiting Studies of the Statistical Property of a Strong Gravitational Lens System and Model-independent Constraint on the Curvature of the Universe
• Space Telescope and Optical Reverberation Mapping Project. XII. Broad-Line Region Modeling of NGC 5548
• Probing nuclear rates with Planck and BICEP2
• Propagating Speed of Primordial Gravitational Waves
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• nestcheck: diagnostic tests for nested sampling calculations
• Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
• Constraints on quintessence scalar field models using cosmological observations
• Probing Dark Matter with Future CMB Measurements
• Convolutional Neural Networks on the HEALPix sphere: a pixel-based algorithm and its application to CMB data analysis
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• Observational Constraint in $f(R,T)$ gravity from the cosmic chronometers and some standard distance measurement parameters
• Bayesian Analysis of Inflation III: Slow Roll Reconstruction Using Model Selection
• Testing CPT Symmetry with CMB Measurements: Update after WMAP5
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• MAXIPOL: Data Analysis and Results
• Testable dark energy predictions from current data
• Does Current Data Prefer a Non-minimally Coupled Inflaton?
• Probing the Effective Number of Neutrino Species with Cosmic Microwave Background
• Coupled Quintessence and the Halo Mass Function
• A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing
• Bayesian inflationary reconstructions from Planck 2018 data
• What is the best way to measure baryonic acoustic oscillations?
• Cosmic Ray Astronomy
• Gravity in the infrared and effective nonlocal models
• Lensing convergence and the neutrino mass scale in galaxy redshift surveys
• A measurement of the Hubble constant using galaxy redshift surveys
• Standard-siren cosmology using gravitational waves from binary black holes
• New Constraints on variations of the fine structure constant from CMB anisotropies
• Statistical methods for cosmological parameter selection and estimation
• Dark Radiation candidates after Planck
• Joint analysis of the thermal Sunyaev-Zeldovich effect and 2MASS galaxies: Probing gas physics in the local Universe and beyond
• How robust are inflation model and dark matter constraints from cosmological data?
• Tensions between direct measurements of the lens power spectrum from Planck data
• Game of cones: A nulling strategy for modelling lensing convergence in cones with large deviation theory
• SWIPE: a bolometric polarimeter for the Large-Scale Polarization Explorer
• Testing Einstein Gravity with Cosmic Growth and Expansion
• A Multi-Parameter Investigation of Gravitational Slip
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• HERUS: The Far-IR/Submm Spectral Energy Distributions of Local ULIRGs & Photometric Atlas
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Constraining the shape of the CMB: a Peak-by-Peak analysis
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Bayesian evidence for the tensor-to-scalar ratio $r$ and neutrino masses $m_{\nu }$: Effects of uniform vs logarithmic priors
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis
• Running the running
• TDCOSMO. IX. Systematic comparison between lens modelling software programs: time delay prediction for WGD 2038-4008
• An analysis of star formation with Herschel in the Hi-GAL Survey. I. The Science Demonstration Phase Fields
• Constraining Modified Gravity with Euclid
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Markov Chain Monte Carlo joint analysis of Chandra X-ray imaging spectroscopy and Sunyaev-Zeldovich Effect data
• New constraints on the observable inflaton potential from WMAP and SDSS
• Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology
• Constraints and tensions in testing general relativity from Planck and CFHTLenS including intrinsic alignment systematics
• Cosmological Constraints on Decaying Dark Matter
• $\mu$-Distortions or Running: A Guaranteed Discovery from CMB Spectrometry
• A Revised SALT2 Surface for Fitting Type Ia Supernova Light Curves
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• On the local variation of the Hubble constant
• Testing Cosmology with Cosmic Sound Waves
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Dynamical Dark sectors and Neutrino masses and abundances
• Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
• WMAP 3-year primordial power spectrum
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Addressing $H_0$ tension with emergent dark radiation in unitary gravity
• Planck priors for dark energy surveys
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Nongaussianity from Particle Production During Inflation
• Reconstruction of broad features in the primordial spectrum and inflaton potential from Planck
• Searching for a dipole modulation in the large-scale structure of the Universe
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Phenomenology of Large Scale Structure in scalar-tensor theories: joint prior covariance of $w_{\text{DE}}$, $\Sigma$ and $\mu$ in Horndeski
• Modeling Dark Photon Oscillations in Our Inhomogeneous Universe
• Testing chirality of primordial gravitational waves with Planck and future CMB data: no hope from angular power spectra
• Ruling out the power-law form of the scalar primordial spectrum
• Planck and BICEP/Keck Array 2018 constraints on primordial gravitational waves and perspectives for future B-mode polarization measurements
• Inflation model constraints from data released in 2015
• Latest inflation model constraints from cosmic microwave background measurements
• Early Dark Energy at High Redshifts: Status and Perspectives
• Constraints on growth index parameters from current and future observations
• Probing dark energy with redshift-drift
• Sterile neutrinos with pseudoscalar self-interactions and cosmology
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Constraints on Kinetically Modified Inflation from WMAP5
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Low power on large scales in just enough inflation models
• Model independent constraints on transition redshift
• Probing the cosmic web: inter-cluster filament detection using gravitational lensing
• WMAP 7 Constraints on Oscillations in the Primordial Power Spectrum
• Model-Independent Constraints on Lorentz Invariance Violation via the Cosmographic Approach
• Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?
• The trouble with Hubble: Local versus global expansion rates in inhomogeneous cosmological simulations with numerical relativity
• Cosmological parameters after WMAP5: forecasts for Planck and future galaxy surveys
• Neutrino mass from future high redshift galaxy surveys: sensitivity and detection threshold
• Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey
• Unified Dark Fluid with Constant Adiabatic Sound Speed and Cosmic Constraints
• On the road to percent accuracy V: the non-linear power spectrum beyond $\Lambda$CDM with massive neutrinos and baryonic feedback
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Fast Cosmological Parameter Estimation from Microwave Background Temperature and Polarization Power Spectra
• Using dark energy to suppress power at small scales
• Impact of polarised extragalactic sources on the measurement of CMB B-mode anisotropies
• U(e3) from physics above the GUT scale
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Natural Inflation After Planck 2018
• Constraints on the Nambu-Goto cosmic string contribution to the CMB power spectrum in light of new temperature and polarisation data
• CMB anomalies from an inflationary model in string theory
• Fractal initial conditions and natural parameter values in hybrid inflation
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• POLOCALC: a Novel Method to Measure the Absolute Polarization Orientation of the Cosmic Microwave Background
• Joint resonant CMB power spectrum and bispectrum estimation
• Massive neutrino self-interactions and inflation
• Dark Energy and Fate of the Universe
• General framework for cosmological dark matter bounds using $N$-body simulations
• Exploring Parameter Constraints on Quintessential Dark Energy: the Pseudo-Nambu Goldstone Boson Model
• Constraining large scale HI bias using redshifted 21-cm signal from the post-reionization epoch
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Unifying darko-lepto-genesis with scalar triplet inflation
• Herschel-ATLAS: Statistical Properties of Galactic Cirrus in the GAMA-9 Hour Science Demonstration Phase Field
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Evidence for CII diffuse line emission at redshift $z\sim 2.6$
• Reconcile the AMS-02 positron fraction and Fermi-LAT/HESS total $e^{\pm }$ spectra by the primary electron spectrum hardening
• First Galaxy-Galaxy Lensing Measurement of Satellite Halo Mass in the CFHT Stripe-82 Survey
• Reconstruction of the neutrino mass as a function of redshift
• Combined cosmological and solar system constraints on chameleon mechanism
• Friction in Gravitational Waves: a test for early-time modified gravity
• Revisiting CMB constraints on Warm Inflation
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Future weak lensing constraints in a dark coupled universe
• Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Cornering the Planck $A_{lens}$ tension with future CMB data
• Holography and the scale-invariance of density fluctuations
• Do joint CMB and HST data support a scale invariant spectrum?
• Prospects for precision cosmology with the 21 cm signal from the dark ages
• What do WMAP and SDSS really tell about inflation?
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• The joint large-scale foreground-CMB posteriors of the 3-year WMAP data
• Bayesian component separation and CMB estimation for the 5-year WMAP temperature data
• Constraining the dark fluid
• Inflation in the closed FLRW model and the CMB
• Constraining dynamical dark energy with a divergence-free parametrization in the presence of spatial curvature and massive neutrinos
• Primordial features and Planck polarization
• Single-field inflation constraints from CMB and SDSS data
• Constraining the Primordial Magnetic Field from Cosmic Microwave Background Anisotropies at Higher Multipoles
• Precise cosmological parameter estimation using CosmoRec
• CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data
• What the small angle CMB really tells us about the curvature of the Universe
• CMB anisotropy and BBN constraints on pre-recombination decay of dark matter to visible particles
• Observational constraints on K-inflation models
• Tight constraints on F- and D-term hybrid inflation scenarios
• The Gauss-Legendre Sky Pixelization for the CMB polarization (GLESP-pol). Errors due to pixelization of the CMB sky
• Constraints on primordial magnetic fields from magnetically-induced perturbations: current status and future perspectives with LiteBIRD and future ground based experiments
• Model-independent constraints on Lorentz invariance violation: implication from updated Gamma-ray burst observations
• A 31 GHz Survey of Low-Frequency Selected Radio Sources
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Reconstruction of the dark matter-vacuum energy interaction
• Parametrized modified gravity constraints after Planck
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Reconciling Hubble Constant Discrepancy from Holographic Dark Energy
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• Planck intermediate results. XVI. Profile likelihoods for cosmological parameters
• Projected Cosmological Constraints from Strongly Lensed Supernovae with the Roman Space Telescope
• When Did Cosmic Acceleration Start ?
• Uncovering the History of Cosmic Inflation from Anomalies in Cosmic Microwave Background Spectra
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Observing Trans-Planckian Signatures in the Cosmic Microwave Background
• Quintessence with Yukawa Interaction
• Improved determination of the WIMP mass from direct detection data
• Redshift drift exploration for interacting dark energy
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Impact of theoretical priors in cosmological analyses: the case of single field quintessence
• $\nu$Galileon: modified gravity with massive neutrinos as a testable alternative to $\Lambda$CDM
• On the Classification of UGC1382 as a Giant Low Surface Brightness Galaxy
• Reconstruction of the primordial power spectra with Planck and BICEP2
• Microwave background constraints on inflationary parameters
• Principal reconstructed modes of dark energy and gravity
• New Parametrization for the Scale Dependent Growth Function in General Relativity
• Strong Gravitational Lens Inversion: A Bayesian Approach
• Simultaneous constraints on the number and mass of relativistic species
• Energy-momentum correlations for Abelian Higgs cosmic strings
• Accelerating Large-Scale-Structure data analyses by emulating Boltzmann solvers and Lagrangian Perturbation Theory
• 21-cm constraints on spinning primordial black holes
• Probing the Local Velocity Distribution of WIMP Dark Matter with Directional Detectors
• Galaxy cluster number count data constraints on cosmological parameters
• Neutrino and Dark Radiation properties in light of latest CMB observations
• Copula Cosmology: Constructing a Likelihood Function
• Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• Figures of merit and constraints from testing General Relativity using the latest cosmological data sets including refined COSMOS 3D weak lensing
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Early Universe Constraints on Time Variation of Fundamental Constants
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Inflation and Alternatives with Blue Tensor Spectra
• Cosmic Discordance: Detection of a modulation in the primordial fluctuation spectrum
• Bianchi I meets the Hubble diagram
• Revisiting CMB constraints on dark matter annihilation
• Lensing-like tensions in the Planck legacy release
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Point-Source Power in 3 Year Wilkinson Microwave Anisotropy Probe Data
• Revisiting the Constraint on the Helium Abundance from CMB
• Observational Constraints on Accelerating Brane Cosmology with Exchange between the Bulk and Brane
• 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
• Statistics of X-ray flares of Sagittarius A*: evidence for solar-like self-organized criticality phenomenon
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
• The HI content of dark matter halos at $z\approx 0$ from ALFALFA
• A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• CMB Beam Systematics: Impact on Lensing Parameter Estimation
• Can Planck-scale physics be seen in the cosmic microwave background ?
• Cosmology with fast radio bursts in the era of SKA
• Constraining the initial conditions of the Universe using large scale structure
• Dark Energy coupling with electromagnetism as seen from future low-medium redshift probes
• COSMOS weak-lensing constraints on modified gravity
• Latest Observational Constraints to the Ghost Dark Energy Model by Using Markov Chain Monte Carlo Approach
• New Limits on Coupled Dark Energy from Planck
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• KiDS-1000: Constraints on the intrinsic alignment of luminous red galaxies
• Superplot: a graphical interface for plotting and analysing MultiNest output
• A measurement of the CMB E-mode angular power spectrum at subdegree scales from 670 square degrees of POLARBEAR data
• The Fine Structure Constant and the CMB Damping Scale
• BAMBI: blind accelerated multimodal Bayesian inference
• Cosmic Magnetism in Centimeter and Meter Wavelength Radio Astronomy
• Primordial Neutrinos, Cosmological Perturbations in Interacting Dark-Energy Model: CMB and LSS
• Cosmological CPT Violation, Baryon/Leptogenesis and CMB Polarization
• Detecting relic gravitational waves in the CMB: Optimal parameters and their constraints
• Robust Strong Lensing Time Delay Estimation
• Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data
• Maximum likelihood, parametric component separation and CMB B-mode detection in suborbital experiments
• The Luminosity Function and Formation Rate of A Complete Sample of Long Gamma-Ray Bursts
• Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
• Kinematic Modelling of Disc Galaxies using Graphics Processing Units
• Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster?
• A Comparative Study of Dark Energy Constraints from Current Observational Data
• Observational constraints on early dark energy
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• The REFLEX II galaxy cluster survey: power spectrum analysis
• On using the WMAP distance priors in constraining the time evolving equation of state of dark energy
• Reducing the $H_0$ tension with generalized Proca theory
• Measuring the tilt of primordial gravitational-wave power spectrum from observations
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Redshift evolution of cosmic birefringence in CMB anisotropies
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Constraining the evolution of the CMB temperature with SZ measurements from Planck data
• Equation of State of Dark Matter after Planck Data
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Aligned natural inflation with modulations
• Observational constraints on cosmic neutrinos and dark energy revisited
• Testing quantum gravity effects with latest CMB observations
• Including birefringence into time evolution of CMB: current and future constraints
• Background reionization history from omniscopes
• CMB Constraint on Dark Matter Annihilation after Planck 2015
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Figures of merit for present and future dark energy probes
• Magnification bias in galaxy surveys with complex sample selection functions
• New Constraints On The Dark Energy Equation of State
• Are Light Sterile Neutrinos Preferred or Disfavored by Cosmology?
• Affine parameterization of the dark sector: costraints from WMAP5 and SDSS
• Primordial Helium Abundance from CMB: a constraint from recent observations and a forecast
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• Properties and use of CMB power spectrum likelihoods
• Precise Estimation of Cosmological Parameters Using a More Accurate Likelihood Function
• Testing gravity using the growth of large scale structure in the Universe
• CosmoPower-JAX: high-dimensional Bayesian inference with differentiable cosmological emulators
• Reconstructing physical parameters from template gravitational wave spectra at LISA: first order phase transitions
• No H_0 Assistance from Assisted Quintessence
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Determining the core radio luminosity function of radio AGNs via copula
• Implications on cosmic ray injection and propagation parameters from Voyager/ACE/AMS-02 nucleus data
• LikeDM: likelihood calculator of dark matter detection
• The Dark Side of the Universe after Planck
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Dark Radiation in extended cosmological scenarios
• Extending the generalized Chaplygin gas model by using geometrothermodynamics
• Cosmological parameter estimation with free-form primordial power spectrum
• Microphysics of Early Dark Energy
• Impacts of dark energy on weighing neutrinos after DESI BAO
• Weighing Neutrinos in $f(R)$ gravity
• Neutrinos secretly converting to lighter particles to please both KATRIN and the cosmos
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• The age-redshift relation for Luminous Red Galaxies in the Sloan Digital Sky Survey
• On quantifying and resolving the BICEP2/Planck tension over gravitational waves
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
• Dynamics and cosmological constraints on Brans-Dicke cosmology
• Theoretical Accuracy in Cosmological Growth Estimation
• The Deep Diffuse Extragalactic Radio Sky at 1.75 GHz
• Constraints on Brane Inflation and Cosmic Strings
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• Blue Gravity Waves from BICEP2 ?
• The Angular Power Spectra of Photometric SDSS LRGs
• Viscous Dark Energy In Bianchi Type V Space-Time
• Fitting string inflation to real cosmological data: the Fibre Inflation case
• Prospects of constraining reionization model parameters using Minkowski tensors and Betti numbers
• Holographic Dark Energy with Cosmological Constant
• Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II
• Power-law solution for homogeneous and isotropic universe in $f(R,T)$ gravity
• Constraining the kinetically dominated Universe
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Constraints on massive sterile plus active neutrino species in non minimal cosmologies
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• Studies on cosmic ray nuclei with Voyager, ACE and AMS-02: I. local interstellar spectra and solar modulation
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• Cosmological constraints on general, single field inflation
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• Dark MaGICC: the effect of Dark Energy on galaxy formation. Cosmology does matter
• Model marginalized constraints on neutrino properties from cosmology
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Bayesian Comparison of Interacting Scenarios
• On the stability conditions for theories of modified gravity in presence of matter fields
• Searching for primordial localized features with CMB and LSS spectra
• Direct Wavelet Expansion of the Primordial Power Spectrum
• COMAP Early Science: VII. Prospects for CO Intensity Mapping at Reionization
• Accelerated Bayesian inference using deep learning
• Cosmic Inflation at the Crossroads
• Is the $w_0{w}_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
• Cosmology with Superluminous Supernovae
• Primordial Standard Clock Models and CMB Residual Anomalies
• Dark Matter and Dark Energy from a single scalar field and CMB data
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Origin of Delta N_eff as a Result of an Interaction between Dark Radiation and Dark Matter
• Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
• The Impact of Observing Strategy on Cosmological Constraints with LSST
• Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg${}^2$ SPT-SZ and Planck Gravitational Lensing Map
• Perceiving the equation of state of Dark Energy while living in a Cold Spot
• Probing the dynamics of dark energy with divergence-free parametrizations: A global fit study
• On the road to discovery of relic gravitational waves: The TE and BB Correlations in the cosmic microwave background radiation
• CMB power spectrum of Nambu-Goto cosmic strings
• Observational constraints on varying neutrino-mass cosmology
• The Limited Accuracy of Linearized Gravity
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Alleviating the tension at low multipole through Axion Monodromy
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Detecting and distinguishing topological defects in future data from the CMBPol satellite
• Complete WMAP Constraints on Bandlimited Inflationary Features
• Cosmological parameter estimation using Particle Swarm Optimization (PSO)
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• Varying couplings in the early universe: correlated variations of $\alpha$ and $G$
• Zero-point quantum fluctuations in cosmology
• CMB Constraints on Principal Components of the Inflaton Potential
• Sources of $H_0$-tensions in dark energy scenarios
• What $\xi$? Cosmological constraints on the non-minimal coupling constant
• Impact of systematics on cosmological parameters from future Galaxy Clusters surveys
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Cosmological searches for a non-cold dark matter component
• New Constraints on the running-mass inflation model
• Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra
• Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
• Dark Radiation and Inflationary Freedom after Planck 2015
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Euclid: Superluminous supernovae in the Deep Survey
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• Can modified gravity models reconcile the tension between CMB anisotropy and lensing maps in Planck-like observations?
• Neutrino mass and dark energy constraints from redshift-space distortions
• MCMC Using Ensembles of States for Problems with Fast and Slow Variables such as Gaussian Process Regression
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• An exploration of an early gravity transition in light of cosmological tensions
• Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
• Searching for Cosmic Strings in CMB Anisotropy Maps using Wavelets and Curvelets
• The Cosmic Neutrino Background and the Age of the Universe
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Dark Matter Interactions, Helium, and the CMB
• A comprehensive numerical study on four categories of holographic dark energy models
• Current and Future Constraints on Primordial Magnetic Fields
• Testing standard and non-standard neutrino physics with cosmological data
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Observational Constraints on Constant Roll Inflation
• The $H_0$ Tension in Non-flat QCDM Cosmology
• Probing Dark Energy Dynamics from Current and Future Cosmological Observations
• Barred spiral galaxies in modified gravity theories
• Comparing multi-field primordial feature models with the Planck data
• Is there evidence for additional neutrino species from cosmology?
• Testing non-minimally coupled inflation with CMB data: a Bayesian analysis
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift space distortions between redshift 0.8 and 2.2
• CMB Lensing Constraints on Dark Energy and Modified Gravity Scenarios
• Computing the Small-Scale Galaxy Power Spectrum and Bispectrum in Configuration-Space
• Binning is Sinning (Supernova Version): The Impact of Self-Calibration in Cosmological Analyses with Type Ia Supernovae
• Constraining the time variation of the coupling constants from cosmic microwave background: effect of Λ_{QCD}
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• Stellar graveyards: Clustering of compact objects in globular clusters NGC 3201 and NGC 6397
• Post-Planck Dark Energy Constraints
• On the degeneracy between primordial tensor modes and cosmic strings in future CMB data from Planck
• New Constraints on the Early Expansion History
• Cosmological tests of quintessence in quantum gravity
• Optimal constraint on g_NL from CMB
• On the current status of Modified Gravity
• Bayesian data analysis tools for atomic physics
• Directional dependence of LCDM cosmological parameters
• Modeling Extragalactic Foregrounds and Secondaries for Unbiased Estimation of Cosmological Parameters From Primary CMB Anisotropy
• Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
• Strong Bounds on Sum of Neutrino Masses in a 12 Parameter Extended Scenario with Non-Phantom Dynamical Dark Energy ($w(z)\ge -1$)
• New MGCAMB tests of gravity with CosmoMC and Cobaya
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• Reconstructing the history of dark energy using maximum entropy
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the growth rate of structure from the small-scale clustering of the luminous red galaxy sample
• Inflationary Freedom and Cosmological Neutrino Constraints
• A comprehensive investigation on the slowing down of cosmic acceleration
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Did Boomerang hit MOND?
• An optimal estimator for resonance bispectra in the CMB
• Two Component Model of Dark Energy
• Do the observational data favor a local void?
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• Non-adiabatic Evolution of Primordial Perturbations and non-Gaussinity in Hybrid Approach of Loop Quantum Cosmology
• Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data
• Potential Impact of Global Navigation Satellite Services on Total Power HI Intensity Mapping Surveys
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum
• The present and future of the most favoured inflationary models after $Planck$ 2015
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Modified Cosmology Models from Thermodynamical Approach
• Distance Measurements from Supernovae and Dark Energy Constraints
• Complementarity of Peculiar Velocity Surveys and Redshift Space Distortions for Testing Gravity
• Lensing power spectrum of the Cosmic Microwave Background with deep polarization experiments
• Steve: A hierarchical Bayesian model for Supernova Cosmology
• Uncertainty on w from large-scale structure
• Understanding parameter differences between analyses employing nested data subsets
• The cosmological constant and general isocurvature initial conditions
• Intensity Mapping in the Presence of Foregrounds and Correlated Continuum Emission
• Inflationary spectra with inverse-volume corrections in loop quantum cosmology and their observational constraints from Planck 2015 data
• Reconstruction of the primordial power spectrum from CMB data
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• CMB constraints on $\beta$-exponential inflationary models
• Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
• How covariant is the galaxy luminosity function?
• BAO reconstruction: a swift numerical action method for massive spectroscopic surveys
• A systematic study on the cosmic ray antiproton flux
• Constraint on $f(R)$ Gravity through the Redshift Space Distortion
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Tickling the CMB damping tail: scrutinizing the tension between the ACT and SPT experiments
• Robust Simulation-Based Inference in Cosmology with Bayesian Neural Networks
• Likelihood-free Cosmological Constraints with Artificial Neural Networks: An Application on Hubble Parameters and SNe Ia
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• An application of extreme value statistics to the most massive galaxy clusters at low and high redshifts
• Discordances in cosmology and the violation of slow-roll inflationary dynamics
• Reconciling the Quasar Microlensing Disc Size Problem with a Wind Model of Active Galactic Nucleus
• Using the cluster mass function from weak lensing to constrain neutrino masses
• Searching for features of a string-inspired inflationary model with cosmological observations
• Constraining Cut-off Physics in the Cosmic Microwave Background
• Dark energy and cosmic curvature: Monte-Carlo Markov Chain approach
• Tensors, non-Gaussianities, and the future of potential reconstruction
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• The Polarization of the Cosmic Microwave Background Due to Primordial Gravitational Waves
• CosmicNet I: Physics-driven implementation of neural networks within Boltzmann-Einstein solvers
• Constraining the substructure of dark matter haloes with galaxy-galaxy lensing
• Testing modified gravity models with recent cosmological observations
• Cosmological model with decaying vacuum energy law from principles of quantum mechanics
• What Can We Learn by Combining the Skew Spectrum and the Power Spectrum?
• An Integrated Analysis of Radial Velocities in Planet Searches
• Galactic cosmic-ray model in the light of AMS-02 nuclei data
• The look-elsewhere effect from a unified Bayesian and frequentist perspective
• Constraints on variation in $\alpha$ and $m_e$ from WMAP 7-year data
• Baryons still trace dark matter: probing CMB lensing maps for hidden isocurvature
• Does Quartessence Ease Tensions?
• Constraints on inflation revisited: An analysis including the latest local measurement of the Hubble constant
• Exploring Cosmic Origins with CORE: Cluster Science
• Quantum Cosmology and the Evolution of Inflationary Spectra
• Non-minimal Derivative Coupling Scalar Field and Bulk Viscous Dark Energy
• Cosmology-marginalized approaches in Bayesian model comparison: the neutrino mass as a case study
• Features in the primordial spectrum: new constraints from WMAP7+ACT data and prospects for Planck
• Correcting correlation functions for redshift-dependent interloper contamination
• Reionization and dark matter decay
• Cosmological constraints on Galileon dark energy with broken shift symmetry
• How SN Ia host-galaxy properties affect cosmological parameters
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• The differential rotation of epsilon Eri from MOST data
• Isocurvature modes and Baryon Acoustic Oscillations
• Scaling Transformations and the Origins of Light Relics Constraints from Cosmic Microwave Background Observations
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• Axion cold dark matter: status after Planck and BICEP2
• A comment on power-law inflation with a dark radiation component
• Constraints on decaying dark matter from weak lensing and cluster counts
• Fast Bayesian inference for slow-roll inflation
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Observational constraints on new generalized Chaplygin gas model
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Anomalies in the CMB from a cosmic bounce
• Cosmological Alfvén waves in the recent CMB data, and the observational bound on the primordial vector perturbation
• ETHOS -- An effective parametrization and classification for structure formation: the non-linear regime at $z\gtrsim 5$
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• An MCMC Fitting Method for Triaxial Dark Matter Haloes
• Constraints on Resonant Particle Production during Inflation from the Matter and CMB Power Spectra
• Cosmological Constraints from the eBOSS Lyman-$\alpha$ Forest using the PRIYA Simulations
• Inflationary Features and Shifts in Cosmological Parameters from Planck 2015 Data
• GLASS: Generator for Large Scale Structure
• Constraints on the spatially dependent cosmic-ray propagation model from Bayesian Analysis
• CMB lensing and primordial squeezed non-Gaussianity
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Cosmology with Photometric Surveys of Type Ia Supernovae
• Boundary Inflation and the WMAP Data
• Constraint on noncommutative spacetime from PLANCK data
• CMB likelihood approximation by a Gaussianized Blackwell-Rao estimator
• The Dark Energy Survey Supernova Program: Cosmological biases from supernova photometric classification
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• Constraints on time variation of fine structure constant from WMAP-3yr data
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• A global fit study on the new agegraphic dark energy model
• Will Nonlinear Peculiar Velocity and Inhomogeneous Reionization Spoil 21cm Cosmology from the Epoch of Reionization?
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• Efficient optimal non-Gaussian CMB estimators with polarisation
• The first Hubble diagram and cosmological constraints using superluminous supernova
• Intelligent Design: On the Emulation of Cosmological Simulations
• Computation of the Halo Mass Function Using Physical Collapse Parameters: Application to Non-Standard Cosmologies
• Measuring growth index in a universe with sterile neutrinos
• Cosmological evidence for leptonic asymmetry after Planck
• A Monte Carlo Approach to Evolution of the Far-Infrared Luminosity Function with BLAST
• Updated constraints from the PLANCK experiment on modified gravity
• Impact of reionization on CMB polarization tests of slow-roll inflation
• Observational Constraints on Interacting Dark Matter Model Without Dark Energy
• Polarization Predictions for Inflationary CMB Power Spectrum Features
• The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
• Inflation in a two 3-form fields scenario
• A Conditional Luminosity Function Model of the Cosmic Far-Infrared Background Anisotropy Power Spectrum
• Constraints on the solid dark universe model
• Surfing gravitational waves: can bigravity survive growing tensor modes?
• WMAP 5-year constraints on time variation of $\alpha$ and $m_e$ in a detailed recombination scenario
• Testing gravity theories using tensor perturbations
• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• Generalized Holographic Dark Energy and its Observational Constraints
• Disentangling dark energy and cosmic tests of gravity from weak lensing systematics
• Hubble constant difference between CMB lensing and BAO measurements
• Response of distance measures to the equation of state
• Observational hints on the Big Bounce
• Testing flatness of the universe with probes of cosmic distances and growth
• Sound speed of scalar field dark energy: weak effects and large uncertainties
• Accuracy of cosmological parameters using the baryon acoustic scale
• A Bayesian analysis of inflationary primordial spectrum models using Planck data
• Consistency check of ΛCDM phenomenology
• Bayesian analysis of the break in DAMPE lepton spectra
• Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
• Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion
• Observational Constraints on the Averaged Universe
• Probability distribution function of the aperture mass field with large deviation theory
• Higher-Curvature Corrections and Tensor Modes
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• Model-independent test for the cosmic distance duality relation with Pantheon and eBOSS DR16 quasar sample
• Optimal parameterizations for observational constraints on thawing dark energy
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Observational constraints on conformal time symmetry, missing matter and double dark energy
• Forecast for weighing neutrinos in cosmology with SKA
• Scalar Field Oscillations Contributing to Dark Energy
• Determining neutrino properties using future galaxy redshift surveys
• Model independent constraints on mass-varying neutrino scenarios
• Strong gravitational lensing constraints on holographic dark energy
• Growth Index after the Planck Results
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• CMBfit: Rapid WMAP likelihood calculations with normal parameters
• Confronting the concordance model of cosmology with Planck data
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• Large-scale analysis of the SDSS-III DR8 photometric luminous galaxies angular correlation function
• PINGU and the neutrino mass hierarchy: Statistical and systematic aspects
• Prospects of Future CMB Anisotropy Probes for Primordial Black Holes
• Viscous Generalized Chaplygin Gas as a Unified Dark Fluid: Including Perturbation of Bulk Viscosity
• Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe
• The $\nu$ generation: present and future constraints on neutrino masses from cosmology and laboratory experiments
• Dark Radiation after Planck
• Exploring cosmic origins with CORE: effects of observer peculiar motion
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• Can we test Dark Energy with Running Fundamental Constants ?
• Optimal Redshift Weighting For Redshift Space Distortions
• Echoes of Inflationary First-Order Phase Transitions in the CMB
• The WMAP normalization of inflationary cosmologies
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• Possible indication for non-zero neutrino mass and additional neutrino species from cosmological observations
• Multi-tasking the growth of cosmological structures
• Physics of the cosmic microwave background anisotropy
• Isocurvature perturbations in extra radiation
• A model-independent fit to Planck and BICEP2 data
• Cluster counts: calibration issue or new physics?
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Constraints on cosmological birefringence from Planck and Bicep2/Keck data
• Bayesian Model Averaging in Astrophysics: A Review
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
• Gaussianisation for fast and accurate inference from cosmological data
• High-resolution temporal constraints on the dynamics of dark energy
• Bayesian analysis of inflationary features in Planck and SDSS data
• Exploring the "$L$--$\sigma$" relation of HII galaxies and giant extragalactic HII regions acting as standard candles
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data
• How to constrain inflationary parameter space with minimal priors
• Parameter estimation with Sandage-Loeb test
• Changes in the halo formation rates due to features in the primordial spectrum
• Current constraints on deviations from General Relativity using binning in redshift and scale
• Constraining neutrino masses with the ISW-galaxy correlation function
• A new model for the full shape of the large-scale power spectrum
• Relic gravitational waves: latest revisions and preparations for new data
• Data-constrained reionization and its effects on cosmological parameters
• Physical component analysis of galaxy cluster weak gravitational lensing data
• RELIKE: Reionization Effective Likelihood from Planck 2018 Data
• Primordial Magnetic Field Effects on the CMB and Large Scale Structure
• Hubble constant and sound horizon from the late-time Universe
• Constraining holographic inflation with WMAP
• Smoothed Particle Inference: A Kilo-Parametric Method for X-ray Galaxy Cluster Modeling
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• Quantum Gravity and the Large Scale Anomaly
• Revisiting a pre-inflationary radiation era and its effect on the CMB power spectrum
• The variance of the locally measured Hubble parameter explained with different estimators
• A search for sterile neutrinos in interacting dark energy models using DESI baryon acoustic oscillations and DES supernovae data
• Observational Constraints on Warm Inflation in Loop Quantum Cosmology
• Acceleration in Friedmann cosmology with torsion
• On the running of the spectral index to all orders: a new model dependent approach to constrain inflationary models
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• AGN and QSOs in the eROSITA All-Sky Survey -- Part II: The large-scale structure
• Constraining the Variation of G by Cosmic Microwave Background Anisotropies
• Hint of a truncated primordial spectrum from the CMB large-scale anomalies
• Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Observational constraints on tachyon and DBI inflation
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• Fast and robust Bayesian Inference using Gaussian Processes with GPry
• Constraining interacting dark energy models with the halo concentration-mass relation
• Delayed Recombination and Cosmic Parameters
• Extracting the Dark Matter Profile of a Relaxed Galaxy Cluster
• Cosmological Tests of Everpresent $\Lambda$
• A mixture evolution scenario of the AGN radio luminosity function. II. Do low- and high-power radio-loud AGNs evolve differently?
• Probing for the Cosmological Parameters with PLANCK Measurement
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• Unified Dark Fluid with Constant Adiabatic Sound Speed: Including Entropic Perturbations
• Reconstructing dark energy with model independent methods after DESI DR2 BAO
• X-ray Cluster Constraints on Non-Gaussianity
• Testing $f(R)$ dark energy model with the large scale structure
• Constraints on Superconducting Cosmic Strings from Early Reionization
• Constraining Cosmological Parameters with Observational Data Including Weak Lensing Effects
• Observational constraints on $\alpha$-attractor inflationary models with a Higgs-like potential
• Sensitivity forecasts for the cosmological recombination radiation in the presence of foregrounds
• Should we doubt the cosmological constant?
• Inflationary generalized Chaplygin gas and dark energy in the light of the Planck and BICEP2 experiments
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Confronting DGP Braneworld Gravity with Cosmic Observations after Planck Data
• Constraining holographic cosmology using Planck data
• Constrained Cluster Parameters from Sunyaev-Zel'dovich Observations
• K-mouflage Imprints on Cosmological Observables and Data Constraints
• Galactic googly: the rotation-metallicity bias in the inner stellar halo of the Milky Way
• Barry and the BAO Model Comparison
• A Constraint On the Integrated Mass Power Spectrum out to z = 1100 from Lensing of the Cosmic Microwave Background
• Constraints on Newton's Constant from Cosmological Observations
• A Dark Energy model from Generalized Proca Theory
• Back to the features: assessing the discriminating power of future CMB missions on inflationary models
• Does Planck 2015 polarization favor high redshift reionization?
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• AMS-02 Positron Excess and Indirect Detection of Three-body Decaying Dark Matter
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Cascading Dark Energy
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• Photometric classification and redshift estimation of LSST Supernovae
• Constraining f(R) Gravity with Planck Sunyaev-Zel'dovich Clusters
• Neutrino Anisotropies after Planck
• Probing dynamics of dark energy with latest observations
• Inflationary vs. Reionization Features from Planck 2015 Data
• Accurate Extra-Galactic Distances and Dark Energy: Anchoring the Distance Scale with Rotational Parallaxes
• The impact of neutrino masses on the determination of dark energy properties
• Planck Satellite Constraints on Pseudo-Nambu--Goldstone Boson Quintessence
• Galaxy Clusters as a probe of early dark energy
• Early dark energy and its interaction with dark matter
• Topology of large scale structure as test of modified gravity
• A tomographic test of cosmological principle using the JLA compilation of type Ia supernovae
• The Curious Case of Lyman Alpha Emitters: Growing Younger from z ~ 3 to z ~ 2?
• A new pressure-parametrization unified dark fluid model
• Cosmological discordances III: more on measure properties, Large-Scale-Structure constraints, the Hubble constant and Planck
• Parameterizing and Measuring Dark Energy Trajectories from Late-Inflatons
• Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant
• Predictions for the CMB from an anisotropic quantum bounce
• Effects of CMB temperature uncertainties on cosmological parameter estimation
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• Cosmological CPT Violation and CMB Polarization Measurements
• Principal component analysis of the primordial tensor power spectrum
• Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
• Quantifying the impact of future Sandage-Loeb test data on dark energy constraints
• Testing the interaction model with cosmological data and gamma-ray bursts
• Revised WMAP constraints on neutrino masses and other extensions of the minimal $\Lambda$CDM model
• Update constraints on neutrino mass and mass hierarchy in light of dark energy models
• Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
• Probing the primordial universe with gravitational waves detectors
• Dark matter in disk galaxies I: a Markov Chain Monte Carlo method and application to DDO 154
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• The scalar perturbation spectral index n_s: WMAP sensitivity to unresolved point sources
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• Probing spatial variation of the fine-structure constant using the CMB
• Cosmic Anisotropy and Fast Radio Bursts
• BoloCalc: a sensitivity calculator for the design of Simons Observatory
• The Schrödinger-Poisson method for Large-Scale Structure
• Bayesian correction of $H(z)$ data uncertainties
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
• The Local Value of $H_0$ in an Inhomogeneous Universe
• Hybrid Natural Inflation
• Cosmological parameter inference from galaxy clustering: The effect of the posterior distribution of the power spectrum
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• $\alpha$-attractor inflation: Models and predictions
• The traces of anisotropic dark energy in light of Planck
• Disentangling a group of lensed submm galaxies at z~2.9
• Signatures of Cosmic Ray Heating in 21-cm Observables
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• New Constraints on Anisotropic Rotation of CMB Polarization
• Does accelerating universe indicates Brans-Dicke theory
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• Fermi Large Area Telescope observations of the supernova remnant HESS J1731-347
• Constraint on the primordial gravitational waves from the joint analysis of BICEP2 and Planck HFI 353 GHz dust polarization data
• How Flat is Our Universe Really?
• Fast Analytic Computation of Cosmic String Power Spectra
• Cosmological Constraints on Dissipative Models of Inflation
• Harrison-Z'eldovich primordial spectrum is consistent with observations
• Properties and uncertainties of scalar field models of dark energy with barotropic equation of state
• Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
• Cold Dark Matter Isocurvature Perturbations: Cosmological Constraints and Applications
• Low scale gravity as the source of neutrino masses?
• Pulsar interpretation of the lepton spectra measured by AMS-02
• Observational Constraints on Growth Index with Cosmography
• Constraints on Quintessence From Using Cosmological Data
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Dynamical Background
• The Group Evolution Multiwavelength Study (GEMS): The near-infrared luminosity function of nearby galaxy groups
• Dark Matter - Dark Energy coupling biasing parameter estimates from CMB data
• Phenomenological approaches of inflation and their equivalence
• Study of warm inflationary models and their parameter estimation from CMB
• Constraints on decaying early modified gravity from cosmological observations
• Constraints on neutrino density and velocity isocurvature modes from WMAP-9 data
• Cosmic microwave background anisotropies in the timescape cosmology
• The preferentially magnified active nucleus in IRAS F10214+4724 - II. Spatially resolved cold molecular gas
• Current constraints on Cosmological Parameters from Microwave Background Anisotropies
• Precision cosmology with a combination of wide and deep Sunyaev-Zeldovich cluster surveys
• The effect of asymmetric beams in the Wilkinson Microwave Anisotropy Probe experiment
• Evidence for horizon-scale power from CMB polarization
• Characterizing unknown systematics in large scale structure surveys
• Principal components of dark energy with SNLS supernovae: the effects of systematic errors
• Featuring the primordial power spectrum: new constraints on interrupted slow-roll from CMB and LRG data
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Parameter Estimation from Improved Measurements of the CMB from QUaD
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Lepton Models for TeV Emission from SNR RX J1713.7-3946
• What is the amplitude of the Gravitational Waves background expected in the Starobinsky model ?
• Testing one-zone synchrotron-self-Compton models with spectral energy distributions of Mrk 421
• Cold dark energy constraints from the abundance of galaxy clusters
• Constraints on features in the inflationary potential from future Euclid data
• MG-MAMPOSSt: A code to test modifications of gravity with the dynamics of galaxy clusters
• Photons and Baryons before Atoms: Improving the Tight-Coupling Approximation
• Impact of general reionization scenarios on extraction of inflationary parameters
• Detecting relic gravitational waves in the CMB: Comparison of different methods
• Breaking Be: a sterile neutrino solution to the cosmological lithium problem
• Constraints on the location of $\gamma$-ray emitting region for a sample of blazars with radio core-shift measurements
• The Cosmic Neutrino Background Anisotropy - Linear Theory
• Leavers and remainers: Galaxies split by group-exit
• Light Sterile Neutrinos and Inflationary Freedom
• Non-comoving Cosmology
• Lifting Primordial Non-Gaussianity Above the Noise
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Time variation of the fine structure constant in the early universe and the Bekenstein model
• Testing dark energy using pairs of galaxies in redshift space
• Quintessence versus phantom dark energy: the arbitrating power of current and future observations
• No evidence for the blue-tilted power spectrum of relic gravitational waves
• Inflation that runs naturally: Gravitational waves and suppression of power at large and small scales
• Disentangling redshift-space distortions and nonlinear bias using the 2D power spectrum
• Effect of Redshift Distributions of Fast Radio Bursts on Cosmological Constraints
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• HSTPROMO Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco
• Reconstructing Quintessence
• Joining bits and pieces of reionization history
• An elusive dark central mass in the globular cluster M4
• Consistency of the Planck CMB data and $\Lambda$CDM cosmology
• Time variation of the electron mass in the early universe and the Barrow-Magueijo model
• Cosmological parameter estimation from CMB and X-ray clusters after Planck
• Optical Characterization of the SPT-3G Focal Plane
• Robust predictions for an oscillatory bispectrum in Planck 2015 data from transient reductions in the speed of sound of the inflaton
• Cosmological constraints on the generalized holographic dark energy
• Observational constraints on scalar field models of dark energy with barotropic equation of state
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Prospects for Dark Energy Evolution: a Frequentist Multi-Probe Approach
• Parameterizing the Power Spectrum: Beyond the Truncated Taylor Expansion
• Spatial and temporal tuning in void models for acceleration
• The effect of different observational data on the constraints of cosmological parameters
• Cosmological parameter estimation: impact of CMB aberration
• Cosmic microwave background constraints on light dark matter candidates
• Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Stability and the Gauge Problem in Non-Perturbative Cosmology
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Anisotropic Baryon Acoustic Oscillations measurements in Fourier-space with optimal redshift weights
• On the impact of large angle CMB polarization data on cosmological parameters
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• Probing the Neutrino Mass Hierarchy beyond $\Lambda$CDM Model
• Relic gravitational waves in the light of 7-year Wilkinson Microwave Anisotropy Probe data and improved prospects for the Planck mission
• Constraints on running vacuum model with $H(z)$ and $f{\sigma }_8$
• Symmetry and anti-symmetry of the CMB anisotropy pattern
• Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters
• Improved model-independent constraints on the recombination era and development of a direct projection method
• 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
• More Evidence for the Redshift Dependence of Color from the JLA Supernova Sample Using Redshift Tomography
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Hierarchical scaling and biasing
• A novel CMB polarization likelihood package for large angular scales built from combined WMAP and Planck LFI legacy maps
• Observational constraints on unified dark matter including Hubble parameter data
• Diagnostic and Comparative Analysis of Dark Energy Models with $q(z)$ Parametrizations
• BeyondPlanck XI. Bayesian CMB analysis with sample-based end-to-end error propagation
• Forecasting neutrino masses from galaxy clustering in the Dark Energy Survey combined with the Planck Measurements
• Cosmological Bounds on sub-GeV Dark Vector Bosons from Electromagnetic Energy Injection
• Constraining Cosmic Expansion and Gravity with Galaxy Redshift Surveys
• Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator
• Constraining quantum collapse inflationary models with CMB data
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• Maximum Entropy deconvolution of Primordial Power Spectrum
• Cosmological forecasts on thermal axions, relic neutrinos and light elements
• Model-independent constraints on modified gravity from current data and from the Euclid and SKA future surveys
• Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription
• Impact of Point Source Clustering on Cosmological Parameters with CMB Anisotropies
• Probing the Seesaw Mechanism with Cosmological Data
• Emitting Electron Spectra and Acceleration Processes in the Jet of PKS 0447-439
• Relationship between the CMB, SZ Cluster Counts, and Local Hubble Parameter Measurements in a Simple Void Model
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
• Estimating Cosmological Parameters from the Dark Matter Distribution
• Differentiating dark interactions with perturbation
• From model dynamics to oscillating dark energy parameterisation
• Improving the Calibration of Type Ia Supernovae Using Late-time Lightcurves
• Is Cosmology Compatible with Blue Gravity Waves ?
• A novel model-marginalized cosmological bound on the QCD axion mass
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• Stable indications of relic gravitational waves in Wilkinson Microwave Anisotropy Probe data and forecasts for the Planck mission
• Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
• Current constraints on early and stressed dark energy models and future 21 cm perspectives
• Probing Primordial Non-Gaussianity with Weak Lensing Minkowski Functionals
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• CMB anomalies and the effects of local features of the inflaton potential
• Dark Matter Annihilation into Four-Body Final States and Implications for the AMS Antiproton Excess
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• Effects of neutrino mass and asymmetry on cosmological structure formation
• Cosmological constraint on Brans-Dicke Model
• Cosmological Constraints on the Higgs Boson Mass
• Direct cosmological inference from three-dimensional correlations of the Lyman-$\alpha$ forest
• Tachyon inflation in the Large-$N$ formalism
• BeyondPlanck VI. Noise characterization and modelling
• Constraining quantum collapse inflationary models with current data: The semiclassical approach
• Application of Bayesian model averaging to measurements of the primordial power spectrum
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• Probing for Dynamics of Dark-Energy in Mass Varying Neutrinos: Cosmic Microwave Background Radiation and Large Scale Structure
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Direct comparison of sterile neutrino constraints from cosmological data, ${\nu }_e$ disappearance data and ${\nu }_{\mu }\to {\nu }_e$ appearance data in a $3+1$ model
• Improved cosmological constraints on the curvature and equation of state of dark energy
• Cosmological constraints in the presence of ionizing and resonance radiation at recombination
• Testing averaged cosmology with type Ia supernovae and BAO data
• Confronting Kähler moduli inflation with CMB data
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Path Integral Marginalization for Cosmology: Scale Dependent Galaxy Bias & Intrinsic Alignments
• Constraints to Holographic Dark Energy Model via Type Ia Supernovae, Baryon Acoustic Oscillation and WMAP
• Gravitational Waves: A Test for Modified Gravity
• Evolution of High-Energy Particle Distribution in Mature Shell-Type Supernova Remnants
• The Inflationary Gravity Waves in light of recent Cosmic Microwave Background Anisotropies data
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Testing distance duality with CMB anisotropies
• Cosmological neutrino mass limit and the dynamics of dark energy
• Constraining Light Gravitino Mass from Cosmic Microwave Background
• Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae
• Cubic Derivative Interactions and Asymptotic Dynamics of the Galileon Vacuum
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• Statistical challenges in the search for dark matter
• Negative running prevents eternal inflation
• Theoretical and observational constraints on Tachyon Inflation
• Test of consistency between Planck and WMAP
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Impact of the damping tail on neutrino mass constraints
• Flat Tree-level Inflationary Potentials in Light of CMB and LSS Data
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Physics Beyond The Standard Model with Circular Polarization in the CMB and CMB-21cm Cross-Correlation
• Detectability of Cosmic Dark Flow in the Type Ia Supernova Redshift-Distance Relation
• Precision measurements of large scale structure with future type Ia supernova surveys
• Uncorrelated estimates of the primordial power spectrum
• Cosmological Tests with the FSRQ Gamma-ray Luminosity Function
• Detecting dark photon dark matter with Gaia-like astrometry observations
• Constraining exotic dark matter models with the dark ages 21-cm signal
• Testing the cosmic conservation of photon number with type Ia supernovae and ages of old objects
• The Reactor Anomaly after Daya Bay and RENO
• Constraints on Modified Gravity from ACT and SPT
• Mean shift cluster recognition method implementation in the nested sampling algorithm
• Closing up the cluster tension?
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic measurement of structure growth and expansion rate from anisotropic galaxy clustering in Fourier space
• Linear and non-linear perturbations in dark energy models
• Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
• Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
• Comparing dark energy models with current observational data
• Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys
• Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
• Speeding Up Cosmological Boltzmann Codes
• A mixture evolution scenario of the AGN radio luminosity function
• Primordial power spectrum features in phenomenological descriptions of inflation
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• Isocurvature perturbations and tensor mode in light of Planck and BICEP2
• Can dark matter-dark energy interaction alleviate the Cosmic Coincidence Problem?
• Dark Energy From Fifth Dimensional Brans-Dicke Theory
• Precision Primordial ${}^4$He Measurement with CMB Experiments
• New model of axion monodromy inflation and its cosmological implications
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Post-Born corrections to the one-point statistics of (CMB) lensing convergence obtained via large deviation theory
• The Impact of Assuming Flatness in the Determination of Neutrino Properties from Cosmological Data
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• Lensed Cosmic Microwave Background Constraints on Post-General Relativity Parameters
• SUSY Predictions and SUSY Tools at the LHC
• Model independent approaches to reionization in the analysis of upcoming CMB data
• Bayesian evidence of non-standard inflation: isocurvature perturbations and running spectral index
• Data analysis methods for the cosmic microwave background
• Reconstructing Probability Distributions with Gaussian Processes
• Weighing neutrinos in the presence of a running primordial spectral index
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• Galaxy rotation curves using a non-parametric regression method: core, cusp and fuzzy scalar field dark matter models
• Estimating the tensor-to-scalar ratio and the effect of residual foreground contamination
• Lensing covariance on cut sky and SPT-Planck lensing tensions
• Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• Bayesian approach to constraining the properties of ionized bubbles during reionization
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• Likelihood, Fisher information, and systematics of cosmic microwave background experiments
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• Measuring kinematic anisotropies with pulsar timing arrays
• Cosmological constraints on sterile neutrino oscillations from Planck
• Cluster Probes of Dark Energy Clustering
• A generalized method of constraining Warm Inflation with CMB data
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• An optimal basis system for cosmology: data analysis and new parameterisation
• Fibre inflation and precision CMB data
• Bayesian methods for fitting Baryon Acoustic Oscillations in the Lyman-$\alpha$ forest
• Foreground influence on primordial non-Gaussianity estimates: needlet analysis of WMAP 5-year data
• Flow-Based Likelihoods for Non-Gaussian Inference
• Brane inflation and the robustness of the Starobinsky inflationary model
• A dark energy view of inflation
• CMB Lens Sample Covariance and Consistency Relations
• Edges and Endpoints in 21-cm Observations from Resonant Photon Production
• Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR
• Lorentz invariance violation in the neutrino sector: a joint analysis from big bang nucleosynthesis and the cosmic microwave background
• Quantifying the CMB Degeneracy Between the Matter Density and Hubble Constant in Current Experiments
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Small field models with gravitational wave signature supported by CMB data
• Constraints on single-field inflation with WMAP, SPT and ACT data -- A last-minute stand before Planck
• Measuring the spectral running from cosmic microwave background and primordial black holes
• The Impact of Prior Assumptions on Bayesian Estimates of Inflation Parameters and the Expected Gravitational Waves Signal from Inflation
• Efficient ILC analysis on polarization maps after EB leakage correction
• Was there an early reionization component in our universe?
• How much primordial tensor mode is allowed?
• Detecting relic gravitational waves in the CMB: The contamination caused by the cosmological birefringence
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• The dark side of curvature
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• Is gravity getting weaker at low z? Observational evidence and theoretical implications
• Correlations between cosmic strings and extra relativistic species
• Investigation of CMB constraints for dark matter-helium scattering
• Cluster counts. II. Tensions, massive neutrinos, and modified gravity
• Large Scale Traces of Solar System Cold Dust on CMB Anisotropies
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• The Multi-Tracer Optimal Estimator applied to VIPERS
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• The 21-cm Signal from the Cosmological Epoch of Recombination
• Observational status of the Galileon model general solution from cosmological data and gravitational waves
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Dynamic changes of emitting electron distribution in the jet of 3C 279: signatures of acceleration and cooling
• OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Forecast and analysis of the cosmological redshift drift
• Predicted Constraints on Cosmic String Tension from Planck and Future CMB Polarization Measurements
• Nontrivial Geometries: Bounds on the Curvature of the Universe
• Probing a panoply of curvaton-decay scenarios using CMB data
• Dynamical systems analysis of the cubic galileon beyond the exponential potential and the cosmological analogue of the vDVZ discontinuity
• Local interstellar spectra and solar modulation of cosmic ray electrons and positrons
• Constraints on Models with a Break in the Primordial Power Spectrum
• A flexible method for estimating luminosity functions via Kernel Density Estimation
• Dark Matter In Disk Galaxies II: Density Profiles as Constraints on Feedback Scenarios
• Cosmological Constraints on Scalar Field Dark Matter
• How robust are the parameter constraints extending the $\Lambda$CDM model?
• Dark Energy Scaling from Dark Matter to Acceleration
• Constraints on Generalized Dark Energy from Recent Observations
• CMB polarization as a tool to constrain the optical properties of the Universe
• The interaction of neutrinos with Phantom, Quintessence, and Quintum scalar fields and its effect on the formation of structures in the early Universe
• Confronting Dark Energy Anisotropic Stress
• Topology of Large-Scale Structures of Galaxies in Two Dimensions - Systematic Effects
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• Constraints on brane inflation after Planck 2015: Impacts of the latest local measurement of the Hubble constant
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• Lensing-induced morphology changes in CMB temperature maps in modified gravity theories
• Probing for variation of neutrino mass with current observations
• Observational constraints on the energy scale of inflation
• Effect of damped oscillations in the inflationary potential
• Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
• Spatial curvature sensitivity to local $H_0$ from the Cepheid distance ladder
• Interacting generalized ghost dark energy in non-flat universe
• How CMB and large-scale structure constrain chameleon interacting dark energy
• Impact of $1/f$ noise on cosmological parameter constraints for SKA intensity mapping
• Unified Model for Inflation and Dark Energy with Planck-Scale Pseudo-Goldstone Bosons
• Cosmological constraints on a unified dark matter-energy scalar field model with fast transition
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Constraining the reionization history with CMB and spectroscopic observations
• Testing the nature of Dark Energy with Precision Cosmological constraints
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
• From heaviness to lightness during inflation
• Inflaton or Curvaton? Constraints on Bimodal Primordial Spectra from Mixed Perturbations
• Constraints on a special running vacuum model
• Low-$\ell$ power suppression in punctuated inflation
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• Tensors, BICEP2, prior dependence, and dust
• Reionization in the dark and the light from Cosmic Microwave Background
• Towards a Solution to the H0 Tension: the Price to Pay
• Mass-varying neutrino in light of cosmic microwave background and weak lensing
• Subdegree Sunyaev-Zel'dovich Signal from Multifrequency BOOMERanG observations
• Constraints on the Tensor-to-Scalar ratio for non-power-law models
• Cosmological constraints on the neutron lifetime
• Weighing neutrinos in $f(R)$ gravity in light of BICEP2
• Retrieving cosmological information from small-scale CMB foregrounds I. The thermal Sunyaev Zel'dovich effect
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• On the question of measuring spatial curvature in an inhomogeneous universe
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• The contribution of the kinematic Sunyaev-Zel'dovich Effect from the Warm Hot Intergalactic Medium to the Five-Year WMAP Data
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Likelihood of the Power Spectrum in Cosmological Parameter Estimation
• Constraining Hybrid Natural Inflation with recent CMB data
• Reactor sterile neutrinos, dark energy and the age of the universe
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• The Hubble tension in the non-flat Super-$\Lambda \mathrm{CDM}$ model
• Trident: A three-pronged galaxy survey. I. Lyman alpha emitting galaxies at z~2 in GOODS North
• The impact of theoretical assumptions in the determination of the neutrino effective number from future CMB measurements
• Assessing non-linear models for galaxy clustering III: Theoretical accuracy for Stage IV surveys
• Pairwise velocities in the "Running FLRW" cosmological model
• Galaxy power spectrum and biasing results from the LOFAR Two-metre Sky Survey (first data release)
• The Bayes factor surface for searches for new physics
• Combining Optical and X-ray Observations of Galaxy Clusters to Constrain Cosmological Parameters
• A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: constraints on the time variation of fundamental constants from the large-scale two-point correlation function
• The Impact of Primordial Magnetic Fields on Future CMB Bounds on Inflationary Gravitational Waves
• Non-Gaussian signatures of general inflationary trajectories
• Testing inflationary consistency relations by the potential CMB observations
• LINX: A Fast, Differentiable, and Extensible Big Bang Nucleosynthesis Package
• Running cosmological constant with observational tests
• Constraints on small-scale primordial density fluctuation from cosmic microwave background through dark matter annihilation
• Cosmology at the boundary of de Sitter using the dS/QFT correspondence
• New insights on $\nu$-DM Interactions
• Explaining low l anomalies in the CMB power spectrum with resonant superstring excitations during inflation
• Probing cosmology with weak lensing selected clusters II: Dark energy and f(R) gravity models
• Shan--Chen interacting vacuum cosmology
• Classification algorithms applied to structure formation simulations
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Constraining the Break of Spatial Diffeomorphism Invariance with Planck Data
• Cosmological N-body simulations with generic hot dark matter
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• Fast and effortless computation of profile likelihoods using CONNECT
• Observational consequences of the Standard Model Higgs inflation variants
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• Reconstruction of Baryon Fraction in Intergalactic Medium through Dispersion Measurements of Fast Radio Bursts
• A fast method of reionization parameter space exploration using GPR trained SCRIPT
• Possible Evidence for Planck-Scale Resonant Particle Production during Inflation from the CMB Power Spectrum
• Efficient exploration of reionization parameters for the upcoming 21 cm observations using a photon conserving semi-numerical model SCRIPT
• The Effective Fluid approach for Modified Gravity and its applications
• The role of the diffusive protons in the gamma-ray emission of supernova remnant RX J1713.7$-$3946 --- a two-zone model
• X-ray galaxy clusters abundance and mass temperature scaling
• Constraining non-minimally coupled $\beta$-exponential inflation with CMB data
• The power spectrum of systematics in cosmic shear tomography and the bias on cosmological parameters
• Constraints on sterile neutrinos and the cosmological tensions
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Constraining ultra slow roll inflation using cosmological datasets
• Probing the intergalactic medium during the Epoch of Reionization using 21-cm signal power spectra
• Determination of the Kinematic Parameters from SNe Ia and Cosmic Chronometers
• The Dark Energy Cosmic Clock: A New Way to Parametrise the Equation of State
• Cosmological data and indications for new physics
• Astrophysical information from the Rayleigh-Jeans Tail of the CMB
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Relic Neutrino Degeneracies and Their Impact on Cosmological Parameters
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• Constraining Perturbative Early Dark Energy with Current Observations
• SCoPE: An efficient method of Cosmological Parameter Estimation
• The Tilt of Primordial Gravitational Waves Spectra from BICEP2
• No stable dissipative phantom scenario in the framework of a complete cosmological dynamics
• Optimal prior for Bayesian inference in a constrained parameter space
• Late-time acceleration with steep exponential potentials
• Probing local non-Gaussianities within a Bayesian framework
• Self-consistent redshift estimation using correlation functions without a spectroscopic reference sample
• Parametric tension between even and odd multipole data of WMAP power spectrum: unaccounted contamination or missing parameters?
• Current cosmological constraints on the curvature, dark energy and modified gravity
• Weighing neutrinos using high redshift galaxy luminosity functions
• Cosmological tests of gravity with latest observations
• A model independent constraint on the temporal evolution of the speed of light
• Short Distance Physics and Initial State Effects on the CMB Power Spectrum
• Measuring the temperature and profiles of Lyman-$\alpha$ absorbers
• How real-time cosmology can distinguish between different anisotropic models
• How does pressure gravitate? Cosmological constant problem confronts observational cosmology
• The Impact of Secondary non-Gaussianities in the CMB on Cosmological Parameter Estimation
• Quantum collapse as source of the seeds of cosmic structure during the radiation era
• WMAP Constraints On K-Inflation
• Cosmological Parameters from CMB Maps without Likelihood Approximation
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Cosmology and neutrino masses - an update
• Probing the primordial power spectra with inflationary priors
• CMB Neutrino Mass Bounds and Reionization
• Optimising Inflationary Features the Bayesian Way
• Constraints on Running of Non-Gaussianity from Large Scale Structure Probes
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Fast numerical method to generate halo catalogs in modified gravity (part I): second-order Lagrangian Perturbation Theory
• Observational evidence for Early Dark Energy as a unified explanation for Cosmic Birefringence and the Hubble tension
• Large-Scale Polarized Foreground Component Separation for Planck
• Probing the Weak Gravity Conjecture in the Cosmic Microwave Background
• An Extended Zel'dovich Model for the Halo Mass Function
• Global neutrino parameter estimation using Markov Chain Monte Carlo
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
• Running vacuum model in non-flat universe
• New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): testing a new approach to measure the evolution of the structure growth
• Posterior sampling for inverse imaging problems on the sphere in seismology and cosmology
• Detection of relic gravitational waves in the CMB: Prospects for CMBPol mission
• Constraints on electromagnetic form factors of sub-GeV dark matter from the Cosmic Microwave Background anisotropy
• Is there another coincidence problem at the reionization epoch?
• Optimized Large-Scale CMB Likelihood And Quadratic Maximum Likelihood Power Spectrum Estimation
• CMB Optical Depth Measurements: Past, Present, Future
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• Ultra faint dwarf galaxies: an arena for testing dark matter versus modified gravity
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Late transient acceleration of the universe in string theory on $S^1/Z_2$
• Interacting parametrized post-Friedmann method
• Specific Effect of Peculiar Velocities on Dark-Energy Constraints from Type Ia Supernovae
• Optimising Boltzmann codes for the Planck era
• Probing Ricci dark energy model with perturbations by using WMAP seven-year cosmic microwave background measurements, BAO and Type Ia supernovae
• Constraining Warm Dark Matter with high-$z$ supernova lensing
• Detection of transplanckian effects in the cosmic microwave background
• Limits on Entanglement Effects in the String Landscape from Planck and BICEP/Keck Data
• Testing LTB Void Models Without the Cosmic Microwave Background or Large Scale Structure: New Constraints from Galaxy Ages
• Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
• Testing the cosmic distance duality relation with baryon acoustic oscillations and supernovae data
• Can we distinguish early dark energy from a cosmological constant?
• Cosmological Constraints from Fourier Phase Statistics
• Small-scale CMB anisotropies induced by the primordial magnetic fields
• On Weak Lensing Shape Noise
• Lens covariance effects on likelihood analyses of CMB power spectra
• Kinetic powers of the relativistic jets in Mrk 421 and Mrk 501
• Cosmological implications of different baryon acoustic oscillation data
• Implications for cosmology from Ground-based Cosmic Microwave Background observations
• A field-level emulator for modified gravity
• Cosmology when living near the Great Attractor
• Constraints on the multi-lognormal magnetic fields from the observations of the cosmic microwave background and the matter power spectrum
• Can power spectrum observations rule out slow-roll inflation?
• Understanding large scale CMB anomalies with the generalized non-minimal derivative coupling during inflation
• Cosmological Constraints on Rapid Roll Inflation
• Constraining galaxy-halo connection with high-order statistics
• Systematic effects in the measurement of polarization by the PLANCK telescope
• Local interstellar spectra and solar modulation of cosmic ray proton and Helium
• The primordial "f_NL" non-Gaussianity, and perturbations beyond the present horizon
• Constraining Decaying Dark Matter
• Validating galaxy clustering models with Fixed & Paired and Matched-ICs simulations: application to Primordial Non-Gaussianities
• Planck constraints on neutrino isocurvature density perturbations
• Reconstruction of Reionization History through Dispersion Measure of Fast Radio Bursts
• Cosmology in a certain vector-tensor theory of gravitation
• Freezing Out Early Dark Energy
• Dark Twilight Joined with the Light of Dawn to Unveil the Reionization History
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• CMB observations from the CBI and VSA: A comparison of coincident maps and parameter estimation methods
• Constraints on the cosmological parameters from BICEP2, Planck and WMAP
• Constraints on Dark Energy state equation with varying pivoting redshift
• A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
• The BINGO Project IX: Search for Fast Radio Bursts -- A Forecast for the BINGO Interferometry System
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• How accurately can we measure the hydrogen 2S->1S transition rate from the cosmological data?
• CMB Anisotropy Constraints on Flat-Lambda and Open CDM Cosmogonies from DMR, UCSB South Pole, Python, ARGO, MAX, White Dish, OVRO, and SuZIE Data
• Revisiting Cardassian Model and Cosmic Constraint
• Cosmic Microwave Background Anisotropy numerical solution (CMBAns) I: An introduction to $C_l$ calculation
• Cosmological implications of the KATRIN experiment
• Likelihood analysis of small field polynomial models of inflation yielding a high Tensor-to-Scalar ratio
• Constraints on dark energy from TDCOSMO & SLACS lenses
• Strong Gravitational Lensing and Its Cosmic Constraints
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Chameleon Early Dark Energy and the Hubble Tension
• Constraining cosmological scaling solutions of a Galileon field
• On the Injection of Relativistic Electrons in the Jet of 3C 279
• Observational constraints on running vacuum model
• Constraints on non-thermal Dark Matter from Planck lensing extraction
• Constraining the redshifts of TeV BL Lac objects
• The catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST
• Self-Calibrating the Look-Elsewhere Effect: Fast Evaluation of the Statistical Significance Using Peak Heights
• Agnostic cosmology in the CAMEL framework
• Cosmological constrains on fast transition Unified Dark Energy/Matter models
• Correlations between $\gamma$-ray luminosity and magnetization of the jet as well as relativistic electron injection power:cases for Mrk 421, 3C 454.3 and 3C 279
• The measurements of matter density perturbations amplitude from cosmological data
• The primordial information content of Rayleigh Anisotropies
• Impacts on Cosmological Constraints from Degeneracies
• An Informational Approach to Cosmological Parameter Estimation
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• Constraints on the Combined Models with $R^{2-q}$ Inflation and Viable $f(R)$ Dark Energy
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Primordial power spectrum versus extension parameters beyond the standard model
• Learn-As-You-Go Acceleration of Cosmological Parameter Estimates
• The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• Statistical Uncertainties of the $N_{\text{DW}}=1$ QCD Axion Mass Window from Topological Defects
• Solar modulation of AMS-02 daily proton and Helium fluxes with modified force field approximation models
• The ultimate frontier of 21cm cosmology
• Re-examining the role of curvature in the slowing down acceleration scenario
• Interacting Barrow Holographic Dark Energy in Non-flat Universe
• Isolating the linear signal when making redshift space distortion measurements
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• A New Fast Monte Carlo Code for Solving Radiative Transfer Equations based on Neumann Solution
• Testing consistency of ${\Omega }_b{h}^2$ in the Planck data
• Observational constraint on dynamical evolution of dark energy
• Old Dark Energy
• Searching for oscillations in the primordial power spectrum
• Observational constraints on the growth index parameters in $f(Q)$ gravity
• On Dark Energy Isocurvature Perturbation
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• Constraints on the Sunyaev-Zel'dovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
• Reconstruction of a direction-dependent primordial power spectrum from Planck CMB data
• Improving CMB non-Gaussianity estimators using tracers of local structure
• Expansion and Growth of Structure Observables in a Macroscopic Gravity Averaged Universe
• Sampling the Probability Distribution of Type Ia Supernova Lightcurve Parameters in Cosmological Analysis
• What can be learned about dark energy evolution?
• Primordial Gravitational Waves Measurements and Anisotropies of CMB Polarization Rotation
• Testing for Features in the Primordial Power Spectrum
• Reconstructing thawing quintessence with multiple datasets
• Higgs Inflation: constraining the top quark mass and breaking the $H_0$-${\sigma }_8$ correlation
• Constraints on cosmic birefringence using $E$-mode polarisation
• Cosmological test of an extended quintessence model
• Model-Independent Dark Energy Measurements from DESI DR2 and Planck 2015 Data
• Markov Chain Beam Randomization: a study of the impact of PLANCK beam measurement errors on cosmological parameter estimation
• Brane inflation driven by an arctan potential: CMB constraints and Reheating
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Ionization from Cosmic Strings at Cosmic Dawn
• Measuring the scalar induced gravitational waves from observations
• Climbing out of the shadows: building the distance ladder with black hole images
• Inflation in de Sitter spacetime and CMB large scales anomaly
• Closing in on the large-scale CMB power asymmetry
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• Effects of Neutrino Masses and Asymmetries on Dark Matter Halo Assembly
• Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
• Modern Cosmology: Interactive Computer Simulations that use Recent Observational Surveys
• Probing for cosmological parameters with LAMOST measurement
• Precision of future experiments measuring primordial tensor fluctuation
• Cosmological constraints on $\Lambda (\alpha )$CDM models with time-varying fine structure constant
• Do current observations support transient acceleration of our universe?
• B-mode Power Spectrum of CMB via Polarized Compton Scattering
• Investigating the Possibility of a Turning Point in the Dark Energy Equation of State
• Reionization and Cosmic Dawn: theory and simulations
• Reconciling the light component and all-particle cosmic ray energy spectra at the knee
• More about a successful vector-tensor theory of gravitation
• Cosmological Parameters from a re-analysis of the WMAP-7 low resolution maps
• Constraining Brans-Dicke cosmology with the CSST galaxy clustering spectroscopic survey
• Thermal gravitational-wave background in the general pre-inflationary scenario
• Constraining primordial black holes in dark matter with kinematics of dwarf galaxies
• Using the Markov Chain Monte Carlo method to study the physical properties GeV-TeV BL Lac objects
• Consistency of the nonflat $\Lambda$CDM model with the new result from BOSS
• Measuring primordial gravitational waves from CMB B-modes in cosmologies with generalized expansion histories
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• Cosmic constraint on the unified model of dark sectors with or without a cosmic string fluid in the varying gravitational constant theory
• Probing Lepton Asymmetry with 21 cm Fluctuations
• Cosmic Microwave Background constraints of decaying dark matter particle properties
• Principal component analysis of the reionization history from Planck 2015 data
• SED fitting with MCMC: methodology and application to large galaxy surveys
• Optimal strategy for polarization modulation in the LSPE-SWIPE experiment
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Current and Future constraints on single-field $\alpha$-Attractor model
• Inflation after WMAP3
• Isocurvature modes: joint analysis of the CMB power spectrum and bispectrum
• Probing the cosmic acceleration from combinations of different data sets
• Non-trivial time crystal-like ground state for gravitational perturbation in quadratic gravity
• Probing Quintessence Potential with Future Cosmological Surveys
• Reconstruction of inflationary scenarios in non-conservative unimodular gravity
• What does a cosmological experiment really measure? Covariant posterior decomposition with normalizing flows
• Unified dark fluid with fast transition: including entropic perturbations
• Understanding selection effects in observed samples of cataclysmic variables
• Density perturbations from both the inflaton and the curvaton
• Dark Energy Search with Supernovae
• Nonlinear structure formation in Bound Dark Energy
• Constraining dark energy using observational growth rate data
• Scrutinizing coupled vector dark energy in light of data
• Improved Cosmological Parameter Constraints from CMB and H(z) Data
• Cosmological Model-independent Gamma-ray Bursts Calibration and its Cosmological Constraint to Dark Energy
• Measuring the extragalactic background light from very high energy gamma-ray observations of blazars
• Reconstructing the dark matter and dark energy interaction scenarios from observations
• Structure Formation Constraints on Sommerfeld-Enhanced Dark Matter Annihilation
• Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
• Dark energy as an elastic strain fluid
• Constraints on primordial non-Gaussianity using multitracer technique for skew spectrum
• Testing Dvali-Gabadadze-Porrati Gravity with Planck
• Dark Matter in the Alternative Left Right Model
• Small field models of inflation that predict a tensor-to-scalar ratio $r=0.03$
• Estimates of unresolved point sources contribution to WMAP 5
• Constraining cosmic reionization by combining the kinetic Sunyaev-Zel'dovich and the 21 cm power spectra
• Revisiting the cosmological bias due to local gravitational redshifts
• COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions
• A Constrained NILC method for CMB B mode observations
• Local energy-momentum conservation in scalar-tensor-like gravity with generic curvature invariants
• Observational constraints on inflection point quintessence with a cubic potential
• Super-Eddington accreting massive black holes explore high-$z$ cosmology: Monte-Carlo simulations
• Constraints on Dark Energy from New Observations including Pan-STARRS
• Investigating the Origin of CMB Large-Scale Features Using LiteBIRD and CMB-S4
• A very extended reionization epoch ?
• Signature of short distance physics on inflation power spectrum and CMB anisotropy
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Numerical solution of the exact background collisional Boltzmann equation for dark matter-baryon scattering
• Testing the Consistence of Gamma Ray Burst Data-set and Supernovae Union2
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Parameters and pitfalls in dark energy models with time varying equation of state
• Bayesian error propagation for neural-net based parameter inference
• Observational constraints on tachyonic chameleon dark energy model
• BICEP's acceleration
• Joint constraint on primordial gravitational waves and polarization rotation angle with current CMB polarization data
• Implication of the PAMELA antiproton data for dark matter indirect detection at LHC
• Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• Cosmic Void Baryon Acoustic Oscillation Measurement: Evaluation of Sensitivity to Selection Effects
• Cosmological constraints for the Cosmic Defect theory
• A Bayesian estimate of the CMB-large-scale structure cross-correlation
• Exponential quintessence with momentum coupling to dark matter
• EIG - II. Intriguing characteristics of the most extremely isolated galaxies
• The Simons Observatory: Assessing the Impact of Dust Complexity on the Recovery of Primordial $B$-modes
• Constraints on the primordial gravitational waves with variable sound speed from current CMB data
• The spectral energy distribution of the Carina nebula from far infrared to radio wavelengths
• Mapping the Cosmological Confidence Ball Surface
• Compressing combined probes: redshift weights for joint lensing and clustering analyses
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• A new way to test the WIMP dark matter models
• Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation
• Observational constraints on dynamical dark energy with pivoting redshift
• Numerical search for a potential planet sculpting the young disc of HD 115600
• Averaged universe confronted with cosmological observations: A fully covariant approach
• Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation
• The Low Redshift survey at Calar Alto (LoRCA)
• Comparison of Supernovae datasets Constraints on Dark Energy
• Calculating Bayesian evidence for inflationary models using CONNECT
• Planck and WMAP constraints on generalised Hubble flow inflationary trajectories
• A note on the initial conditions within the effective field theory approach of cosmic acceleration
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Scale and redshift dependent limits on cosmic neutrino properties
• Cosmological constraints on Lorentz invariance violation in the neutrino sector
• Data Analysis and Phenomenological Cosmology
• Discerning Dark Energy Models with High-Redshift Standard Candles
• Fourier imaging of non-linear structure formation
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• On the horizons in a viable vector-tensor theory of gravitation
• Constraining spatial variations of the fine-structure constant in symmetron models
• How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
• Updated reduced CMB data and constraints on cosmological parameters
• Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff
• Constraints on the phase transition of Early Dark Energy with the CMB anisotropies
• Reionization history and CMB parameter estimation
• A simple supergravity model of inflation constrained with Planck 2018 data
• The Accelerated Recombination, and the ACBAR and WMAP data
• Perturbation in an interacting dark universe
• Beyond Fisher Forecasting for Cosmology
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Thawing Quintessence: Priors, evidence, and likely trajectories
• Constraining primordial tensor features with the anisotropies of the Cosmic Microwave Background
• A flexible parameterization to test early physics solutions to the Hubble tension with future CMB data
• Euclid preparation. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey
• Primordial neutrinos fade to gray: constraints from cosmological observables
• The reconstruction of dark energy with Ridge Regression Approach
• Suppression of scalar power on large scales and associated bispectra
• Measuring the modified gravitational waves propagation beyond general relativity from CMB observations
• Lognormal semi-numerical simulations of the Lyman-$\alpha$ forest: comparison with full hydrodynamic simulations
• Sample variance in N--body simulations and impact on tomographic shear predictions
• Updated observational constraints on $\varphi$CDM dynamical dark energy cosmological models
• Pixel space convolution for cosmic microwave background experiments
• Constraining primordial vector mode from B-mode polarization
• Cosmic Constraints to wCDM Model from Strong Gravitational Lensing
• Cosmic Reionization Study : Principle Component Analysis After Planck
• Caching and Interpolated Likelihoods: Accelerating Cosmological Monte Carlo Markov Chains
• Breaking the degeneracy between polarization efficiency and cosmological parameters in CMB experiments
• Measuring our peculiar velocity from spectroscopic redshift surveys
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Cosmological constraints from galaxy clustering
• Constraints on Extragalactic Background Light using TeV Observations of BL Lacertae objects
• Future constraints on variations of the fine structure constant from combined CMB and weak lensing measurements
• CMB Anomalies from Imperfect Dark Energy: Confrontation with the Data
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• On the prior dependence of constraints on the tensor-to-scalar ratio
• Measuring the primordial gravitational waves from cosmic microwave background and stochastic gravitational wave background observations
• Probing Cosmic Acceleration by Using Model-Independent Parametrizations and Three Kinds of Supernova Statistics Techniques
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Observational constraints on inflationary potentials within the quantum collapse framework
• Non-linear coupling in the dark sector as a running vacuum model
• A Brachistochrone Approach to Reconstruct the Inflaton Potential
• Power law $\alpha$-Starobinsky inflation
• Statistical Nuances in BAO Analysis: Likelihood Formulations and Non-Gaussianities
• Cosmological Perturbations in the 5D Holographic Big Bang Model
• Accelerating LISA inference with Gaussian processes
• Non-Affine Extensions of the Raychaudhuri Equation in the K-essence Framework
• Forecasting of the time-dependent fluxes of antiprotons in the AMS-02 era
• Modern Bayesian Sampling Methods for Cosmological Inference: A Comparative Study
• Probing the matter and dark energy sources in a viable Big Rip model of the Universe
• The CMB Derivatives of Planck's Beam Asymmetry
• The two-and three-point correlation functions of the polarized five-year WMAP sky maps
• Reducing the Tension Between the BICEP2 and the Planck Measurements: A Complete Exploration of the Parameter Space
• Constraining CMB physical processes using Planck 2018 data
• Superimposed Oscillations in Brane Inflation
• Cosmic microwave background constraints on the tensor-to-scalar ratio
• Cosmology with Higher-Derivative Gravities
• Model-independent Reconstruction of UV Luminosity Function and Reionization Epoch
• A Semiblind Reconstruction of the History of Effective Number of Neutrinos Using CMB Data
• Neutrino physics from future weak lensing surveys
• A unification of RDE model and XCDM model
• Measuring the primordial curvature perturbations from the scalar induced gravitational waves
• Bayesian analysis of multiple direct detection experiments
• Mixing Bispectrum Multipoles Under Geometric Distortions
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Cosmic microwave background constraints on a decaying cosmological term related to the thermal evolution
• Reanalysis of the Systematic Uncertainties in Cosmic-Ray Antiproton Flux
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• Improved Gibbs samplers for Cosmic Microwave Background power spectrum estimation
• Conformally de Sitter space from anisotropic SD3-brane of type IIB string theory
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Searches for sterile neutrinos (and other light particles)
• Gaussbock: Fast parallel-iterative cosmological parameter estimation with Bayesian nonparametrics
• Red Density Perturbations and Inflationary Gravitational Waves
• Partition function approach to non-Gaussian likelihoods: Formalism and expansions for weakly non-Gaussian cosmological inference
• Effect of the field self-interaction of General Relativity on the Cosmic Microwave Background Anisotropies
• Constraints on the Helium Abundance from Fast Radio Bursts
• Constraints on Tensor to Scalar Ratio using WKB Approximation
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• On the possibility of Baryon Acoustic Oscillation measurements at redshift $z>7.6$ with the Roman Space Telescope
• Numerical Analysis of the Primordial Power Spectrum for (Small Field) Inflationary Potentials
• Cosmoglobe: Towards end-to-end CMB cosmological parameter estimation without likelihood approximations
• Are all perturbations created equal? An analysis of the WMAP 5- and 7-year data without inflationary prejudice
• Cosmology of Single Species Hidden Dark Matter
• Do data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Scalar field models of dark energy with barotropic equation of state: properties and observational constraints from different datasets
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Observational effects of the early episodically dominating dark energy
• Dark matter search with CMB: a study of foregrounds
• Sunyaev-Zel'dovich contribution in CMB analysis
• Estimating Cosmological Parameters and Reconstructing Hubble Constant with Artificial Neural Networks: A Test with covariance matrix and mock H(z)
• Minimal parameterizations for modified gravity
• The BINGO/ABDUS Project: Forecast for cosmological parameters from a mock Fast Radio Bursts survey
• Bayes and present dark matter direct search status
• Neutrino emission from dark matter annihilation/decay in light of cosmic $e^{\pm }$ and $\bar{p}$ data
• Constraints on Dark Matter annihilation and Its Equation of State after Planck Data
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Linear and non-linear Modified Gravity forecasts with future surveys
• Axion hot dark matter bounds
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Lensing anomalies from the epoch of reionisation
• Probing solar modulation of AMS-02 time-dependent D, ${}^3$He and ${}^4$He fluxes with modified force field approximation
• Weighing Neutrinos with Large-Scale Structure
• Discrete treatment of inverse Compton scattering: implications on parameter estimation in gamma-ray astronomy
• Cosmological parameter fittings with the BICEP2 data
• The running of featureful primordial power spectra
• A Multifrequency approach of the cosmological parameter estimation in presence of extragalactic point sources
• Mildly mixed coupled models vs. WMAP7 data
• Optimization of the half wave plate configuration for the LSPE-SWIPE experiment
• Cosmological Constraints on Radion Evolution in the Universal Extra Dimension Model
• Probing the primordial Universe from the low-multipole CMB data
• Amplitudes of thermal and kinetic Sunyaev-Zel'dovich signals from small-scale CMB anisotropies
• Detecting the neutrino mass and mass hierarchy from global data
• Cosmic microwave background constraints on coupled dark matter
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• An Inflationary Scenario Taking into Account of Possible Dark Energy Effects in the Early Universe
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• Testing the CMB Data for Systematic Effects
• Tensor Tilt from Primordial B-modes
• Combined $13\times 2$-point analysis of the Cosmic Microwave Background and Large-Scale Structure: implications for the $S_8$-tension and neutrino mass constraints
• Non-adiabatic instability in coupled dark sectors
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• The virial mode $k_v$ approach to Structure Formation with Warm Dark Matter
• Stacking catalog sources in WMAP data
• A measurement of the intrahalo light fraction with near-infrared background anisotropies
• Observable predictions of generalised inflationary scenarios
• Results and forecasts on cosmic inflation from weak lensing
• Reexamine the dark matter scenario accounting for the positron excess in a new cosmic ray propagation model
• Observational constraints on the second-order primordial power spectrum: Exploring a Continuous Spontaneous Localization inspired inflationary model
• Bayesian analysis of the backreaction models
• Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
• Neutrino mass limits and decaying dark matter: background evolution versus perturbations
• Inflation Story: slow-roll and beyond
• Probing the last scattering surface through the recent and future CMB observations
• Constraints on the birth of the universe and origin of cosmic dark flow
• Cosmological measurements from the CMB and BAO are insensitive to the tail probability in the assumed likelihood
• LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Non-linear structure formation in the "Running FLRW" cosmological model
• Phenomenological constraints on low-scale gravity
• Cosmology in warped massive gravity
• CMB Constraint on Radion Evolution in the Brane World Scenario
• The large-scale monopole of the power spectrum in a Euclid-like survey: wide-angle effects, lensing, and the `finger of the observer'
• Mixed Inflaton and Spectator Field Models: CMB constraints and $\mu$ distortion
• A data compression and optimal galaxy weights scheme for Dark Energy Spectroscopic Instrument and weak lensing datasets
• Tracing the environmental history of observed galaxies via extended fast action minimization method
• Robustness of cosmological axion mass limits
• Limits in late time conversion of cold dark matter into dark radiation
• Sequential Kalman Tuning of the $t$-preconditioned Crank-Nicolson algorithm: efficient, adaptive and gradient-free inference for Bayesian inverse problems
• Is PLANCK consistent with primordial deuterium measurements ?
• From WMAP to Planck: Exact reconstruction of 4- and 5-dimensional inflationary potential from high precision CMB measurements
• Quasi-matter Bounce Cosmology in Light of Planck
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Excess B-modes extracted from the Planck polarization maps
• Studies of Extragalactic Background Light with TeV BL Lac Objects
• Reconstruction of Tsallis Holographic Dark Energy via Modified Non-Metric Gravity: An $f(Q,C)$ Approach
• Does History Repeat Itself? Periodic Time Cosmology
• Cosmological solutions for model with a $1/H^2$ term
• Mitigation of nonlinear galaxy bias with a theoretical-error likelihood
• Neutrino masses from CMB B-mode polarization and cosmic growth rate
• Observational constraints on massive gravity
• Initial Conditions in the Effective Field Theory of Inflation
• Selected Topics in Numerical Methods for Cosmology
• Cosmological Parameter Estimation: Method
• Refitting cosmological data with neutrino mass and degeneracy
• Implications of $f(R)$ gravity on late-time cosmic structure growth through a complete description of density perturbations
• Conformal Killing Gravity: New Constraints from DESI DR2 BAO datasets
• Search for dark Higgs inflaton with curvature couplings at LHC experiments
• Forecasting constraints from the cosmic microwave background on eternal inflation
• Constraints on the generalized natural inflation after Planck 2018
• Cosmic tango between the very small and the very large: Addressing CMB anomalies through Loop Quantum Cosmology
• Can dark energy explain a high growth index?
• Observational constraints on the modified cosmology inspired by string T-duality
• Signatures of primordial gravitational waves in matter power spectrum
• A Python compressed low-$\ell$ Planck likelihood for temperature and polarization
• Probing Systematic Bias in Low-Redshift Type Ia Supernova Measurements by Cross Analyzing Surface Brightness and Hubble Residuals
• Cosmological Model Independent Constraints on Lorentz Invariance Violation with Updated Gamma-Ray Burst Observations: An Artificial Neural Network Approach
• Constraint on Neutrino Statistics from Cosmological Data
• Massive neutrinos and dark energy
• Pico: Parameters for the Impatient Cosmologist
• Interpreting deviations between AR-VTG and GR
• The CMB angular power spectrum via component separation: a study on Planck data
• Beetroots: spatially-regularized Bayesian inference of physical parameter maps -- Application to Orion
• A saddle-point finder and its application to the spin foam model
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Bayesian Inversion of Stokes Profiles
• CMB at small scales: Cosmology from tSZ power spectrum
• Nearly scale-invariant power spectrum and quantum cosmological perturbations in the gravity's rainbow scenario
• From Geometry to Observation: Gravitational Waves and the Raychaudhuri Equation
• Origin & evolution of the Universe
• Stochastic Electron Acceleration in SNR RX J1713.7-3946
• Geometric formulation of $k$-essence and late-time acceleration
• Exploring trans-Planckian physics and the curvature effect by primordial power spectrum with WMAP five-year data
• Constraints on the Modified Emergent Dark Energy Model Using DESI DR2 BAO
• HOLISMOKES -- XVIII. Cosmology with strongly lensed type II supernovae: Effects of instrumental setups on $H_0$
• Intrinsic alignments of galaxies in multiple projections
• Perturbations In Some Dark Energy Models
• Removing systematics-induced 21-cm foreground residuals by cross-correlating filtered data
• Can Gibbons-Hawking Radiation and Inflation Arise Due to Spacetime Quanta?
• Robust posterior inference when statistically emulating forward simulations
• Measuring the speed of scalar induced gravitational waves from observations
• Exploring the constraints on cosmological models with CosmoEJS
• Testing the cosmic distance duality relation using model-independent approach
• Implications of a high growth index on the variation of $G$
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra
• Accelerating reionization constraints: An ANN-emulator framework for the SCRIPT Semi-numerical Model
• Insights for Early Dark Energy with Big Bang Nucleosynthesis
• Constraining beyond $\Lambda$CDM models with 21cm intensity mapping forecast observations combined with latest CMB data
• Cosmological constraints on viable $f(R)$ models using weak lensing
• The impact of the locally measured Hubble parameter on the mass of Sterile neutrino
• Fluctuations in the Ginzburg-Landau Theory of Dark Energy: internal (in-)consistencies in PLANCK data set
• Recent results and perspectives on cosmology and fundamental physics from microwave surveys
• Dark Matter Recoupling
• Neutrino physics from Cosmology
• The Parameter-Level Performance of Covariance Matrix Conditioning in Cosmic Microwave Background Data Analyses
• Integrated Markov Chain Monte Carlo (MCMC) analysis of primordial non-Gaussianity (f_NL) in the recent CMB data
• Optimisation of the Population Monte Carlo algorithm: Application to constraining isocurvature models with cosmic microwave background data
• Confronting phantom inflation with Planck data
• Calibrating Bayesian Tension Statistics using Neural Ratio Estimation
• Bayesian evidence and model selection approach for time-dependent dark energy
• Revisiting observational constraints on coupled exponential quintessence with energy and momentum transfers: degeneracy with massive neutrinos
• Running the small-correlated-against-large estimator at scale: Applications of small-scale CMB lensing estimators on realistic simulations
• Optimizing Observational Strategy for Future Fgas Constraints
• Consistency of Planck Data With Power-Law Primordial Scalar Power Spectrum
• On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
• Dipole of the luminosity distance as a test for dark energy models
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• APES: Approximate Posterior Ensemble Sampler
• Smoothed quantum fluctuations and CMB observations
• Lookback time and Chandra constrains on cosmological parameters
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Testing the Anton-Schmidt dark energy model with the DESI DR2 measurements
• No preference for generalized emergent dark energy from current cosmological data
• Unified Model for Inflation and the Dark Side of the Universe
• Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology
• pylevin: Efficient numerical integration of integrals containing up to three Bessel functions
• Quintessence reconstruction of interacting HDE in a non-flat universe
• Finite inflation in curved space
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS