Efficient Computation of CMB anisotropies in closed FRW models

Abstract

We implement the efficient line of sight method to calculate the anisotropy and polarization of the cosmic microwave background for scalar and tensor modes in almost-Friedmann-Robertson-Walker models with positive spatial curvature. We present new results for the polarization power spectra in such models.

4 pages, 1 figure. Corrected/updated references. Accepted by ApJ. For the F90 source code see http://www.mrao.cam.ac.uk/~aml1005/cmb/

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• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample
• Neutrino masses and cosmological parameters from a Euclid-like survey: Markov Chain Monte Carlo forecasts including theoretical errors
• Challenges to the DGP Model from Horizon-Scale Growth and Geometry
• Probing modifications of General Relativity using current cosmological observations
• Xspect, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars
• gevolution: a cosmological N-body code based on General Relativity
• Observational constraints on the curvaton model of inflation
• Constraints on f(R) gravity from probing the large-scale structure
• Angular Power Spectra of the Millimeter Wavelength Background Light from Dusty Star-forming Galaxies with the South Pole Telescope
• Growth of perturbations in dark matter coupled with quintessence
• Non-commutative inflation and the CMB
• Self-Consistent Cosmological Simulations of DGP Braneworld Gravity
• Probing neutrino masses with CMB lensing extraction
• The Global 21-cm Signal in the Context of the High-z Galaxy Luminosity Function
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogues and Measurement of the isotropic BAO between redshift 0.6 and 1.1 for the Emission Line Galaxy Sample
• Exploring Cosmic Origins with CORE: Inflation
• Punctuated inflation and the low CMB multipoles
• Gaussian covariance matrices for anisotropic galaxy clustering measurements
• Impact of massive neutrinos on nonlinear matter power spectrum
• CMB temperature lensing power reconstruction
• Massive Neutrinos and Magnetic Fields in the Early Universe
• Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman-$\alpha$ flux power spectrum
• Rotation of Linear Polarization Plane and Circular Polarization from Cosmological Pseudoscalar Fields
• FAST-PT: a novel algorithm to calculate convolution integrals in cosmological perturbation theory
• New constraints on $f(R)$ gravity from clusters of galaxies
• Planck Data Reconsidered
• How to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cosmological Simulations
• One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
• Neutrino mass in cosmology: status and prospects
• Large Fluctuations in the High-Redshift Metagalactic Ionizing Background
• Cosmology of Mass-Varying Neutrinos Driven by Quintessence: Theory and Observations
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization
• Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters
• N-Body Simulations for Coupled Scalar Field Cosmology
• No large-angle correlations on the non-Galactic microwave sky
• Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces
• Bayesian Analysis of Inflation II: Model Selection and Constraints on Reheating
• Minimally Parametric Power Spectrum Reconstruction from the Lyman-alpha Forest
• Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
• Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies
• Bayesian analysis of sparse anisotropic universe models and application to the 5-yr WMAP data
• The nonlinear matter and velocity power spectra in f(R) gravity
• Constraining Primordial non-Gaussianity with Bispectrum and Power Spectum from Upcoming Optical and Radio Surveys
• The dark degeneracy: On the number and nature of dark components
• Constraining slow-roll inflation with WMAP and 2dF
• KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
• Exploring Cosmic Origins with CORE: Cosmological Parameters
• Probing Cosmology with Weak Lensing Peak Counts
• Neutrino cosmology and Planck
• Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
• Obtaining the CMB anomalies with a bounce from the contracting phase to inflation
• Combining perturbation theories with halo models
• An alternative to the cosmological 'concordance model'
• The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy
• KiDS-1000 Cosmology: constraints beyond flat $\Lambda$CDM
• CMB constraints on cosmic strings and superstrings
• Constraints on millicharged particles from Planck
• New Light Species and the CMB
• The Mira-Titan Universe II: Matter Power Spectrum Emulation
• Probing polarization states of primordial gravitational waves with CMB anisotropies
• Detection of Baryon Acoustic Oscillation Features in the Large-Scale 3-Point Correlation Function of SDSS BOSS DR12 CMASS Galaxies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample
• The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys
• CMB polarization features from inflation versus reionization
• Planck Constraint on Relic Primordial Black Holes
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• Measurements of H(z) and D_A(z) from the Two-Dimensional Two-Point Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
• Improved Constraints on Cosmic Birefringence from the WMAP and Planck Cosmic Microwave Background Polarization Data
• CMB Constraints on Primordial non-Gaussianity from the Bispectrum (f_{NL}) and Trispectrum (g_{NL} and τ_{NL}) and a New Consistency Test of Single-Field Inflation
• Jeans Analysis for Dwarf Spheroidal Galaxies in Wave Dark Matter
• Stringent Limit on Primordial Magnetic Fields from the Cosmic Microwave Background Radiation
• Limits on anisotropic inflation from the Planck data
• Constraining Dark Energy with X-ray Galaxy Clusters, Supernovae and the Cosmic Microwave Background
• Constraint on neutrino masses from SDSS-III/BOSS Ly$\alpha$ forest and other cosmological probes
• Parametrized Post-Friedmann Signatures of Acceleration in the CMB
• Non-Gaussian information from weak lensing data via deep learning
• On the most constraining cosmological neutrino mass bounds
• Imprint of Inhomogeneous Hydrogen Reionization on the Temperature Distribution of the Intergalactic Medium
• Improved Primordial Non-Gaussianity Constraints from Measurements of Galaxy Clustering and the Integrated Sachs-Wolfe Effect
• Forward Modeling of Large-Scale Structure: An open-source approach with Halotools
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder
• Separate Universe Simulations
• Parameter constraints from cross-correlation of CMB lensing with galaxy clustering
• A Lower Bound of Star Formation Activity in Ultra-high Redshift Galaxies Detected with JWST: Implications for Stellar Populations and Radiation Sources
• Cosmological information in the redshift-space bispectrum
• Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of N-body Simulations and Analytic Models
• Supermassive black holes in the EAGLE Universe. Revealing the observables of their growth
• Interpreting ALMA Observations of the ISM During the Epoch of Reionisation
• Spherical collapse in quintessence models with zero speed of sound
• Double Inflation and the Low CMB Quadrupole
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: galaxy clustering measurements in the low redshift sample of Data Release 11
• Modeling Biased Tracers at the Field Level
• Converting non-relativistic dark matter to radiation
• Evolution of dark energy reconstructed from the latest observations
• Cosmological Simulations of Normal-Branch Braneworld Gravity
• Simultaneous Falsification of LCDM and Quintessence with Massive, Distant Clusters
• Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• Modelling the line-of-sight contribution in substructure lensing
• Halo Profiles and the Concentration-Mass Relation for a ΛCDM Universe
• CMB Lensing Power Spectrum Biases from Galaxies and Clusters using High-angular Resolution Temperature Maps
• Alleviating the $H_0$ and ${\sigma }_8$ anomalies with a decaying dark matter model
• Density perturbations in generalized Einstein scenarios and constraints on nonminimal couplings from the Cosmic Microwave Background
• Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope
• Detection of the kinematic Sunyaev-Zel'dovich effect with DES Year 1 and SPT
• Asymmetric galaxy correlation functions
• Gauge-ready formulation of the cosmological kinetic theory in generalized gravity theories
• Halo assembly bias and the tidal anisotropy of the local halo environment
• Decaying warm dark matter and neutrino masses
• Probing Cosmology with Weak Lensing Minkowski Functionals
• Simulations of Baryon Acoustic Oscillations II: Covariance matrix of the matter power spectrum
• Cosmology with photometric redshift surveys
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Joint CMB and Weak Lensing Analysis; Physically Motivated Constraints on Cosmological Parameters
• Induced two-photon decay of the 2s level and the rate of cosmological hydrogen recombination
• Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
• Large-scale BAO signatures of the smallest galaxies
• On the road to percent accuracy: nonlinear reaction of the matter power spectrum to dark energy and modified gravity
• Primordial features due to a step in the inflaton potential
• Constraints on Supersymmetric Models of Hybrid Inflation
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Planck Constraints on Holographic Dark Energy
• A Simplified Approach to General Scalar-Tensor Theories
• Information content of weak lensing power spectrum and bispectrum: including the non-Gaussian error covariance matrix
• Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
• Combining cosmological datasets: hyperparameters and Bayesian evidence
• Cosmic Calibration: Constraints from the Matter Power Spectrum and the Cosmic Microwave Background
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release
• CMB Polarization Systematics Due to Beam Asymmetry: Impact on Inflationary Science
• Constraints on primordial non-Gaussianity from 800,000 photometric quasars
• Updated constraints on the cosmic string tension
• Constraints on the interacting vacuum -- geodesic CDM scenario
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts
• The 6dF Galaxy Velocity Survey: Cosmological constraints from the velocity power spectrum
• CMB lensing tomography with the DES Science Verification galaxies
• Acoustic scale from the angular power spectra of SDSS-III DR8 photometric luminous galaxies
• Primordial black holes and gravitational waves from parametric amplification of curvature perturbations
• Observing the tail of reionization: neutral islands in the $z=5.5$ Lyman-$\alpha$ Forest
• Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension
• Constraining Primordial Magnetism
• Population III.1 and III.2 gamma-Ray Bursts: Constraints on the event rate for future radio and X-ray surveys
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Cosmological Signatures of Interacting Neutrinos
• Warm inflation dissipative effects: predictions and constraints from the Planck data
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• 21 cm signal from cosmic dawn: Imprints of spin temperature fluctuations and peculiar velocities
• Fisher for complements: Extracting cosmology and neutrino mass from the counts-in-cells PDF
• Current cosmological constraints from a 10 parameter CMB analysis
• Coupled dark matter-dark energy in light of near Universe observations
• Measuring the Speed of Dark: Detecting Dark Energy Perturbations
• Zooming in on accretion - I. The structure of halo gas
• Adiabatic initial conditions for perturbations in interacting dark energy models
• Dark Photon Oscillations in Our Inhomogeneous Universe
• Constraining Isocurvature Initial Conditions with WMAP 3-year data
• Small-Angle CMB Temperature Anisotropies Induced by Cosmic Strings
• The Age of the Universe and the Cosmological Constant Determined from Cosmic Microwave Background Anisotropy Measurements
• Systematic Uncertainties In Constraining Dark Matter Annihilation From The Cosmic Microwave Background
• Impact of post-Born lensing on the CMB
• Baryons, Neutrinos, Feedback and Weak Gravitational Lensing
• Emulating Simulations of Cosmic Dawn for 21cm Power Spectrum Constraints on Cosmology, Reionization, and X-ray Heating
• Anomalous CMB polarization and gravitational chirality
• High angular resolution Sunyaev-Zel'dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis
• The influence of non-uniform reionization on the CMB
• Neutrino masses and their ordering: Global Data, Priors and Models
• Reconstructing Patchy Reionization from the Cosmic Microwave Background
• Cosmic flows in the nearby Universe: new peculiar velocities from SNe and cosmological constraints
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Maximum Likelihood algorithm for parametric component separation in CMB experiments
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• Are sterile neutrinos consistent with clusters, the CMB and MOND?
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• Can we avoid dark energy?
• Unbiased constraints on ultralight axion mass from dwarf spheroidal galaxies
• The Subhalo Mass Function and Ultralight Bosonic Dark Matter
• Constraining the primordial initial mass function with stellar archaeology
• Matter power spectrum: from Ly$\alpha$ forest to CMB scales
• Cosmological Constraints on DGP Braneworld Gravity with Brane Tension
• What do we really know about Dark Energy?
• Peculiar velocity effects in high-resolution microwave background experiments
• The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies
• Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
• Pseudoscalar - sterile neutrino interactions: reconciling the cosmos with neutrino oscillations
• Emulating the CFHTLenS Weak Lensing data: Cosmological Constraints from moments and Minkowski functionals
• Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835
• Early recombination as a solution to the $H_0$ tension
• Scale-dependent galaxy bias, CMB lensing-galaxy cross-correlation, and neutrino masses
• The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures
• Sterile neutrino dark matter: A tale of weak interactions in the strong coupling epoch
• Probability Distribution Functions of Cosmological Lensing: Convergence, Shear, and Magnification
• Relic Neutrinos, thermal axions and cosmology in early 2014
• Cosmological perturbation theory at three-loop order
• The impacts of dark matter particle annihilation on recombination and the anisotropies of the cosmic microwave background
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: the low redshift sample
• Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
• Precision cosmology defeats void models for acceleration
• Curvature vs Distances: testing the FLRW cosmology
• Constraint on Coupled Dark Energy Models from Observations
• Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
• Testing modified gravity with Planck: the case of coupled dark energy
• Computing the Three-Point Correlation Function of Galaxies in $\mathcal{O}(N^2)$ Time
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological constraints from the full shape of the clustering wedges
• 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
• Constraints on the Sound Speed of Dynamical Dark Energy
• Cosmological Axion and neutrino mass constraints from Planck 2015 temperature and polarization data
• The large-scale 3-point correlation function of the SDSS BOSS DR12 CMASS galaxies
• Cosmological parameters from WMAP 5-year temperature maps
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Are peculiar velocity surveys competitive as a cosmological probe?
• Self-Consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations
• Bayesian Analysis of Inflation: Parameter Estimation for Single Field Models
• 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
• HI intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies
• Decaying dark matter and the tension in ${\sigma }_8$
• Cosmological Tests of General Relativity with Future Tomographic Surveys
• The Abacus Cosmos: A Suite of Cosmological N-body Simulations
• The significance of the integrated Sachs-Wolfe effect revisited
• The Atacama Cosmology Telescope: Cross-Correlation of CMB Lensing and Quasars
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• Cosmological Constraints From Weak Lensing Peak Statistics With CFHT Stripe 82 Survey
• The effect of foreground subtraction on cosmological measurements from Intensity Mapping
• Large Opacity Variations in the High-Redshift Lyman-alpha Forest: the Signature of Relic Temperature Fluctuations from Patchy Reionization
• The Gaussian streaming model and Lagrangian effective field theory
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• The Outer Rim Simulation: A Path to Many-Core Supercomputers
• Weak lensing of the CMB
• Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension
• The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• CMB power spectra from cosmic strings: predictions for the Planck satellite and beyond
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies
• Field theoretic interpretations of interacting dark energy scenarios and recent observations
• Constraints on massive sterile neutrino species from current and future cosmological data
• Halo bias in mixed dark matter cosmologies
• Limits on Dark Radiation, Early Dark Energy, and Relativistic Degrees of Freedom
• Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations
• Assessment of the Information Content of the Power Spectrum and Bispectrum
• Interacting radiation after Planck and its implications for the Hubble Tension
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): a cosmological forecast
• Baryon acoustic signature in the clustering of density maxima
• A preference for a non-zero neutrino mass from cosmological data
• Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors
• The inner structure of haloes in Cold+Warm dark matter models
• Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations
• POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields
• Constraining sterile neutrino cosmologies with strong gravitational lensing observations at redshift z~0.2
• The full contribution of a stochastic background of magnetic fields to CMB anisotropies
• The assembly bias of dark matter haloes to higher orders
• Analytic model for the matter power spectrum, its covariance matrix, and baryonic effects
• Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data
• Evidence for interacting dark energy from BOSS
• 21-cm Fluctuations from Charged Dark Matter
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties
• Cosmological Parameters from Pre-Planck CMB Measurements
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Robust Cosmological Bounds on Neutrinos and their Combination with Oscillation Results
• Decoding the X-ray Properties of Pre-Reionization Era Sources
• An improved fitting formula for the dark matter bispectrum
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• The imprint of neutrinos on clustering in redshift-space
• The splashback radius of halos from particle dynamics. I. The SPARTA algorithm
• New Interpretable Statistics for Large Scale Structure Analysis and Generation
• Inflationary Cosmological Perturbations of Quantum-Mechanical Origin
• Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
• Detecting a Lorentz-Violating Field in Cosmology
• Survey geometry and the internal consistency of recent cosmic shear measurements
• Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
• No galaxy left behind: accurate measurements with the faintest objects in the Dark Energy Survey
• Evolution of cosmological dark matter perturbations
• Dark energy with non-adiabatic sound speed: initial conditions and detectability
• The 6dF Galaxy Survey: Bulk Flows on $50-70h^{-1}$ Mpc scales
• Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time
• Interacting Dark Energy in a closed universe
• Initial Conditions for Accurate N-Body Simulations of Massive Neutrino Cosmologies
• Observational signatures of Jordan-Brans-Dicke theories of gravity
• WMAP and Inflation
• Can we measure the neutrino mass hierarchy in the sky?
• Voids as a Precision Probe of Dark Energy
• Can 21-cm observations discriminate between high-mass and low-mass galaxies as reionization sources?
• New constraints on time-dependent variations of fundamental constants using Planck data
• 2MTF VI. Measuring the velocity power spectrum
• The impact of massive neutrinos on the abundance of massive clusters
• Model-independent constraints on reionization from large-scale CMB polarization
• Constraints on dark matter annihilation from CMB observations before Planck
• A direct measurement of the linear bias of mid-infrared-selected quasars at z~1 using cosmic microwave background lensing
• Reionization optical depth determination from Planck HFI data with ten percent accuracy
• Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements
• Multiple inflation and the WMAP 'glitches' II. Data analysis and cosmological parameter extraction
• Cosmological consequences of an adiabatic matter creation process
• Analytic marginalization over CMB calibration and beam uncertainty
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• From Planck data to Planck era: Observational tests of Holographic Cosmology
• Galaxy clustering, photometric redshifts and diagnosis of systematics in the DES Science Verification data
• Recovering 3D clustering information with angular correlations
• Measuring the spectrum of primordial gravitational waves with CMB, PTA and Laser Interferometers
• Axion hot dark matter bounds after Planck
• Cosmic history of viable exponential gravity: Equation of state oscillations and growth index from inflation to dark energy era
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment
• Constraining dark matter late-time energy injection: decays and p-wave annihilations
• A CMB lensing mass map and its correlation with the cosmic infrared background
• Halo-model signatures from 380,000 SDSS Luminous Red Galaxies with photometric redshifts
• Asymmetric Dark Matter and Dark Radiation
• Improved Measurements of the CMB Power Spectrum with ACBAR
• Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
• Dark Coupling and Gauge Invariance
• Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approximation
• Evidence for suppression of structure growth in the concordance cosmological model
• The phenomenological approach to modeling the dark energy
• Neutrino constraints from future nearly all-sky spectroscopic galaxy surveys
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background by Galaxy Clusters Using Data from the South Pole Telescope
• Reconstructing Gravity on Cosmological Scales
• Polarised radio filaments outside the Galactic plane
• Upper limits on neutrino masses from the 2dFGRS and WMAP: the role of priors
• Exploring the Superimposed Oscillations Parameter Space
• A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
• Sensitivity and foreground modelling for large-scale CMB B-mode polarization satellite missions
• Fitting Methods for Baryon Acoustic Oscillations in the Lyman-α Forest Fluctuations in BOSS Data Release 9
• A Measurement of the Correlation of Galaxy Surveys with CMB Lensing Convergence Maps from the South Pole Telescope
• Constraints on Cosmological Parameters from the 500 deg${}^2$ SPTpol Lensing Power Spectrum
• A comparison of cosmological Boltzmann codes: are we ready for high precision cosmology?
• Designing a space-based galaxy redshift survey to probe dark energy
• Using BBN in cosmological parameter extraction from CMB: a forecast for Planck
• Neutrino clustering in growing neutrino quintessence
• Non-Gaussianity from isocurvature perturbations
• The High-$z$ Universe Confronts Warm Dark Matter: Galaxy Counts, Reionization and the Nature of Dark Matter
• Observational issues in loop quantum cosmology
• New CMB constraints for Abelian Higgs cosmic strings
• Cross-correlation between the CMB lensing potential measured by Planck and high-z sub-mm galaxies detected by the Herschel-ATLAS survey
• New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• AX-GADGET: a new code for cosmological simulations of Fuzzy Dark Matter and Axion models
• CosmoHammer: Cosmological parameter estimation with the MCMC Hammer
• The 0.1<z<1.65 evolution of the bright end of the [OII] luminosity function
• Some aspects of generalized modified gravity models
• Observational constraints on the tilted spatially-flat and the untilted nonflat $\varphi$CDM dynamical dark energy inflation models
• Higher order corrections to the large scale matter power spectrum in the presence of massive neutrinos
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
• Constraints on primordial gravitational waves from the Cosmic Microwave Background
• Dark sectors with dynamical coupling
• Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
• Fingerprinting dark energy
• Baryon Acoustic Oscillations from the SDSS DR10 galaxies angular correlation function
• Future CMB Constraints on Early, Cold, or Stressed Dark Energy
• CMB polarization power spectra contributions from a network of cosmic strings
• Satellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matter
• Estimation of cosmological parameters using adaptive importance sampling
• IGM Constraints from the SDSS-III/BOSS DR9 Ly-alpha Forest Flux Probability Distribution Function
• CMB Constraints on a Stochastic Background of Primordial Magnetic Fields
• Cosmological performance of SKA HI galaxy surveys
• Planck 2015 constraints on the non-flat $\Lambda$CDM inflation model
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• 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
• The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• New constraints on parametrised modified gravity from correlations of the CMB with large scale structure
• Joint constraints on cosmology and the impact of baryon feedback: combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• All-inclusive interacting dark sector cosmologies
• The 2-degree Field Lensing Survey: design and clustering measurements
• The Atacama Cosmology Telescope: Constraints on Cosmic Birefringence
• Dark Sky Simulations: Early Data Release
• Large-Scale Clustering of Cosmic Voids
• Cosmological Constraints on Horndeski Gravity in Light of GW170817
• Average and dispersion of the luminosity-redshift relation in the concordance model
• An analytical approximation of the scalar spectrum in the ultra-slow-roll inflationary models
• Hunting Down the Best Model of Inflation with Bayesian Evidence
• Relaxing Cosmological Neutrino Mass Bounds with Unstable Neutrinos
• Reionization on Large Scales III: Predictions for Low-ell Cosmic Microwave Background Polarization and High-ell Kinetic Sunyaev-Zel'dovich Observables
• Fast Large Scale Structure Perturbation Theory using 1D FFTs
• Super-Sample Signal
• The pre-inflationary vacuum in the cosmic microwave background
• Increasing Neff with particles in thermal equilibrium with neutrinos
• High-redshift radio galaxies: a potential new source of 21-cm fluctuations
• Testing General Relativity at Cosmological Scales: Implementation and Parameter Correlations
• Cosmological tests of General Relativity: a principal component analysis
• Where are the Low-Mass Population III Stars ?
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Cosmological Hints of Modified Gravity ?
• Homogeneity and isotropy in the 2MASS Photometric Redshift catalogue
• Fast cosmological parameter estimation using neural networks
• Frequency-Dependent Constraints on Cosmic Birefringence from the LFI and HFI Planck Data Release 4
• Reconciling $H_0$ tension in a six parameter space?
• Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-Square-Degree Survey
• Arguments against using $h^{-1}\mathrm{Mpc}$ units in observational cosmology
• Primordial Non-Gaussianity in the Cosmic Microwave Background
• Testing models of vacuum energy interacting with cold dark matter
• Updated constraints on amplitude and tilt of the tensor primordial spectrum
• Neutrino Mass Bounds in the era of Tension Cosmology
• Galaxy Bispectrum from Massive Spinning Particles
• FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory
• How flat can you get? A model comparison perspective on the curvature of the Universe
• Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure
• Missing Thermal Energy of the Intracluster Medium
• N-body simulations with generic non-Gaussian initial conditions I: Power Spectrum and halo mass function
• Primordial power spectrum from Planck
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• RCSLenS: Testing gravitational physics through the cross-correlation of weak lensing and large-scale structure
• Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample
• Bayesian model selection without evidences: application to the dark energy equation-of-state
• Cosmological constraints on neutrino self-interactions with a light mediator
• Closed Universes, de Sitter Space and Inflation
• Near optimal bispectrum estimators for large-scale structure
• The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
• Dark Radiation Emerging After Big Bang Nucleosynthesis?
• Phenomenology of Modified Gravity at Recombination
• The Impact of Stochastic Primordial Magnetic Fields on the Scalar Contribution to Cosmic Microwave Background Anisotropies
• SILVERRUSH. VI. A simulation of Ly$\alpha$ emitters in the reionization epoch and a comparison with Subaru Hyper Suprime-Cam survey early data
• Neutrino Masses from Cosmological Probes
• Model selection applied to reconstruction of the Primordial Power Spectrum
• Cosmology Based on f(R) Gravity Admits 1 eV Sterile Neutrinos
• Analytic approach to the CMB polarizations generated by relic gravitational waves
• Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
• Probing primordial features with future galaxy surveys
• On Minimally-Parametric Primordial Power Spectrum Reconstruction and the Evidence for a Red Tilt
• CMB lensing and primordial non-Gaussianity
• Characterization of the BICEP Telescope for High-Precision Cosmic Microwave Background Polarimetry
• CosmoBolognaLib: C++ libraries for cosmological calculations
• The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM
• Planck 2015 results. XII. Full Focal Plane simulations
• The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
• First Constraint on the Neutrino-Induced Phase Shift in the BAO Spectrum
• Non-Gaussianity from Cosmic Magnetic Fields
• Bianchi Model CMB Polarization and its Implications for CMB Anomalies
• WMAP Constraints on Decaying Cold Dark Matter
• A User's Guide to Extracting Cosmological Information from Line-Intensity Maps
• The state of the dark energy equation of state circa 2023
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• Mapping Growth and Gravity with Robust Redshift Space Distortions
• Cosmology in Extended Parameter Space with DESI Data Release 2 Baryon Acoustic Oscillations: A 2$\sigma$+ Detection of Nonzero Neutrino Masses with an Update on Dynamical Dark Energy and Lensing Anomaly
• On the impact of $f(Q)$ gravity on the Large Scale Structure
• Standard Clock in Primordial Density Perturbations and Cosmic Microwave Background
• Inflation with moderately sharp features in the speed of sound: GSR and in-in formalism for power spectrum and bispectrum
• The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
• A Detection of the Baryon Acoustic Oscillation Features in the SDSS BOSS DR12 Galaxy Bispectrum
• Brane inflation and the WMAP data: a Bayesian analysis
• No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data
• Wiggly Whipped Inflation
• Constraints on braneworld inflation from CMB anisotropies
• A parametrization of the growth index of matter perturbations in various Dark Energy models and observational prospects using a Euclid-like survey
• Structure Formation by Fifth Force I: N-Body vs. Linear Simulations
• Cosmic voids in modified gravity models with massive neutrinos
• Error analysis of quadratic power spectrum estimates for CMB polarization: sampling covariance
• Eddington-Born-Infeld gravity and the large scale structure of the Universe
• Observational constraints on patch inflation in noncommutative spacetime
• Comparison of sampling techniques for Bayesian parameter estimation
• Dark Energy Survey Year 3 Results: Optimizing the Lens Sample in Combined Galaxy Clustering and Galaxy-Galaxy Lensing Analysis
• Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data
• Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Observable-to-Mass-and-Redshift Relations of Galaxy Clusters and Groups with Weak-Lensing Mass Calibration from the Hyper Suprime-Cam Subaru Strategic Program Survey
• The State Equation of the Yang-Mills field Dark Energy Models
• Model-independent cosmological constraints from the CMB
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• Early mass varying neutrino dark energy: Nugget formation and Hubble anomaly
• High-redshift post-reionization cosmology with 21cm intensity mapping
• CMB Delensing Beyond the B Modes
• Whipped inflation
• Non-linear evolution of the cosmic neutrino background
• Exploring Cosmic Origins with CORE: B-mode Component Separation
• CMB constraints on primordial black hole dark matter
• Fast simulations for intensity mapping experiments
• Improved simulation of non-Gaussian temperature and polarization CMB maps
• A new light on 21 cm intensity fluctuations from the dark ages
• Updated CMB, X- and gamma-ray constraints on majoron dark matter
• Horizon Run 4 Simulation: Coupled Evolution of Galaxies and Large-scale Structures of the Universe
• Is there concordance within the concordance $\Lambda$CDM model?
• Boltzmann hierarchy for interacting neutrinos I: formalism
• Cosmology with the Square Kilometre Array
• The separate and combined effects of baryon physics and neutrino free-streaming on large-scale structure
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• Clustering properties of a sterile neutrino dark matter candidate
• Simulations of Weak Gravitational Lensing - II : Including Finite Support Effects in Cosmic Shear Covariance Matrices
• Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples
• Quantum Gravity in the Sky: Interplay between fundamental theory and observations
• DeepCMB: Lensing Reconstruction of the Cosmic Microwave Background with Deep Neural Networks
• Swampland Conjectures and Late-Time Cosmology
• Spherical collapse and halo mass function in f(R) theories
• Constraining $f(R)$ gravity by the Large Scale Structure
• The BOSS-WiggleZ overlap region I: Baryon Acoustic Oscillations
• A simulation pipeline for the Planck mission
• Testing the Copernican principle by constraining spatial homogeneity
• The Lyman-$\alpha$ forest as a diagnostic of the nature of the dark matter
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• Scale-dependent bias in the BAO-scale intergalactic neutral hydrogen
• Cosmological Forecasts for Combined and Next Generation Peculiar Velocity Surveys
• Scientific Synergy Between LSST and Euclid
• The Cosmic Microwave Background and the Ionization History of the Universe
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Isolating relativistic effects in large-scale structure
• General relativistic corrections to $N$-body simulations and the Zel'dovich approximation
• Reconstruction of the Primordial Power Spectrum using Temperature and Polarisation Data from Multiple Experiments
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• Observational constraints on interacting Tsallis holographic dark energy models
• Matter Power Spectrum in Hidden Neutrino Interacting Dark Matter Models: A Closer Look at the Collision Term
• Cosmological lepton asymmetry with a nonzero mixing angle θ_{13}
• Analyze This! A Cosmological Constraint Package for CMBEASY
• Cosmological Bound on the QCD Axion Mass, Redux
• Constraints on Neutrino Masses from Weak Lensing
• Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
• Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
• Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
• The Trispectrum in the Effective Field Theory of Large Scale Structure
• MGCAMB with massive neutrinos and dynamical dark energy
• Towards a measurement of the spectral runnings
• The Non-Gaussian Halo Mass Function with fNL, gNL and tauNL
• Simple foreground cleaning algorithm for detecting primordial B-mode polarization of the cosmic microwave background
• Early dark energy from zero-point quantum fluctuations
• Revisiting cosmological bounds on sterile neutrinos
• A 14 $h^{-3}$ Gpc${}^3$ study of cosmic homogeneity using BOSS DR12 quasar sample
• New approach for precise computation of Lyman-alpha forest power spectrum with hydrodynamical simulations
• The Future of Primordial Features with Large-Scale Structure Surveys
• Addendum to "Superimposed Oscillations in the WMAP Data?"
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• Single-Field Consistency Relations of Large Scale Structure. Part III: Test of the Equivalence Principle
• Parity violation of primordial magnetic fields in the CMB bispectrum
• A 2500 square-degree CMB lensing map from combined South Pole Telescope and Planck data
• Large-scale structure phenomenology of viable Horndeski theories
• Weak Lensing Light-Cones in Modified Gravity simulations with and without Massive Neutrinos
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Shrinkage Estimation of the Power Spectrum Covariance Matrix
• Cosmological constraints on dark matter models with velocity-dependent annihilation cross section
• A Bayesian analysis of the primordial power spectrum
• SKA Weak Lensing I: Cosmological Forecasts and the Power of Radio-Optical Cross-Correlations
• The cosmology of sub-MeV dark matter freeze-in
• Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
• Spatial Curvature Falsifies Eternal Inflation
• Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
• The full-sky relativistic correlation function and power spectrum of galaxy number counts: I. Theoretical aspects
• Super-resolution emulator of cosmological simulations using deep physical models
• N-body methods for relativistic cosmology
• The Cosmic Microwave Background in an Inhomogeneous Universe - why void models of dark energy are only weakly constrained by the CMB
• Can we actually constrain $f_{\mathrm{NL}}$ using the scale-dependent bias effect? An illustration of the impact of galaxy bias uncertainties using the BOSS DR12 galaxy power spectrum
• First season QUaD CMB temperature and polarization power spectra
• Late time transitions in the quintessence field and the $H_0$ tension
• Soundness of Dark Energy properties
• An Intensity Mapping Detection of Aggregate CO Line Emission at 3 mm
• The Shape of the Primordial Power Spectrum: A Last Stand Before Planck
• Correlated isocurvature perturbations from mixed inflaton-curvaton decay
• Theoretical Priors On Modified Growth Parametrisations
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• A General Analysis of Non-Gaussianity from Isocurvature Perturbations
• Complete super-sample lensing covariance in the response approach
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Demonstration of cosmic microwave background delensing using the cosmic infrared background
• Alleviating the Tension in the Cosmic Microwave Background using Planck-Scale Physics
• Results from the Wilkinson Microwave Anisotropy Probe
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• Hydrodynamic Response of the Intergalactic Medium to Reionization
• Detecting patchy reionization in the CMB
• Nuw CDM cosmology from the weak lensing convergence PDF
• Cosmological constraints on the neutrino mass including systematic uncertainties
• Sterile neutrinos as subdominant warm dark matter
• Observational constraints on braneworld inflation: the effect of a Gauss-Bonnet term
• Improved limits on short-wavelength gravitational waves from the cosmic microwave background
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Weighing neutrinos with cosmic neutral hydrogen
• 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
• Fast and accurate CMB computations in non-flat FLRW universes
• The CAMELS project: public data release
• N-body simulations with generic non-Gaussian initial conditions II: Halo bias
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• Oscillations in the inflaton potential: Complete numerical treatment and comparison with the recent and forthcoming CMB datasets
• Resummed propagators in multi-component cosmic fluids with the eikonal approximation
• Observational Evidence for Cosmological-Scale Extra Dimensions
• Model-independent constraints on the cosmological anisotropic stress
• Revealing the effects of curvature on the cosmological models
• Constraints on Primordial Magnetic Fields from Planck combined with the South Pole Telescope CMB B-mode polarization measurements
• B polarization of cosmic microwave background as a tracer of strings
• WMAP5 constraints on the unified model of dark energy and dark matter
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• Dark Energy in Practice
• Higher-order initial conditions for mixed baryon-CDM simulations
• KiDS-1000: cosmic shear with enhanced redshift calibration
• On the impact of galaxy bias uncertainties on primordial non-Gaussianity constraints
• Neutrino mass limits from SDSS, 2dFGRS and WMAP
• A Stringent Limit on the Warm Dark Matter Particle Masses from the Abundance of z=6 Galaxies in the Hubble Frontier Fields
• Correlated adiabatic and isocurvature CMB fluctuations in the wake of the WMAP
• Baryonic Acoustic Oscillations via the Renormalization Group
• On the joint analysis of CMB temperature and lensing-reconstruction power spectra
• Testing coupled dark energy with next-generation large-scale observations
• The exact numerical treatment of inflationary models
• Constraints on massive neutrinos from the pairwise kinematic Sunyaev-Zel'dovich effect
• The galaxy power spectrum: precision cosmology from large scale structure?
• Tomography of the Fermi-LAT gamma-ray diffuse extragalactic signal via cross-correlations with galaxy catalogs
• Combining power spectrum and bispectrum measurements to detect oscillatory features
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Non-Gaussian structure of the lensed CMB power spectra covariance matrix
• Confronting General Relativity with Further Cosmological Data
• HI and cosmological constraints from intensity mapping, optical, and CMB surveys
• Cosmological constraints from the CFHTLenS shear measurements using a new, accurate and flexible way of predicting nonlinear mass clustering
• CMB photons shedding light on dark matter
• Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae
• Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
• On the Cosmological Constant Problems and the Astronomical Evidence for a Homogeneous Energy Density with Negative Pressure
• Constraining massive neutrinos using cosmological 21 cm observations
• The stacked ISW signal of rare superstructures in ΛCDM
• Reconstruction of the Dark Energy equation of state
• N-body Simulations for Extended Quintessence Models
• Large-scale clustering of Lyman-alpha emission intensity from SDSS/BOSS
• Primordial Features from Linear to Nonlinear Scales
• The halo model in a massive neutrino cosmology
• Cosmological Measurements from Angular Power Spectra Analysis of BOSS DR12 Tomography
• Cosmological parameter inference with Bayesian statistics
• Constraining Warm Inflation with CMB data
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• Spherical collapse in $\nu \Lambda CDM$
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Degree-Scale CMB Polarization Measurements from Three Years of BICEP1 Data
• Simulating Structure Formation of the Local Universe
• Cosmology with Doppler Lensing
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• A low CMB variance in the WMAP data
• Unique Signatures of Population III Stars in the Global 21-cm Signal
• Statistical and Systematic Errors in Measurement of Weak-Lensing Minkowski Functionals: Application to Canada-France-Hawaii Lensing Survey
• Do current cosmological observations rule out all Covariant Galileons?
• Full-sky lensing reconstruction of gradient and curl modes from CMB maps
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Generating Log-normal Mock Catalog of Galaxies in Redshift Space
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Constraining neutrino mass with tomographic weak lensing peak counts
• Universal at last? The splashback mass function of dark matter halos
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• WMAP constraints on inflationary models with global defects
• iCosmo: an Interactive Cosmology Package
• A comparison of Einstein-Boltzmann solvers for testing General Relativity
• The Impact of Foregrounds on Redshift Space Distortion Measurements With the Highly-Redshifted 21 cm Line
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements
• The intrinsic bispectrum of the Cosmic Microwave Background [PhD thesis]
• Sloan Digital Sky Survey III Photometric Quasar Clustering: Probing the Initial Conditions of the Universe using the Largest Volume
• Primordial non-Gaussianity in the large scale structure of the Universe
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• Optimal limits on primordial magnetic fields from CMB temperature bispectrum of passive modes
• The Birth and Growth of Neutralino Haloes
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• Light sterile neutrinos after BICEP-2
• Reconciling the local void with the CMB
• Coupled dark energy with perturbed Hubble expansion rate
• Modelling Void Abundance in Modified Gravity
• Principal Power of the CMB
• First results from the Very Small Array -- IV. Cosmological parameter estimation
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection
• Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• Statistics of extreme objects in the Juropa Hubble Volume simulation
• Dark matter annihilation and its effect on CMB and Hydrogen 21 cm observations
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Dark Energy and Modified Gravity in the Effective Field Theory of Large-Scale Structure
• Cosmic Shear Covariance Matrix in $w$CDM: Cosmology Matters
• Non-isotropy in the CMB power spectrum in single field inflation
• {\sc CosmoNet}: fast cosmological parameter estimation in non-flat models using neural networks
• Determining the Neutrino Mass Hierarchy with Cosmology
• An evaluation of cosmological models from expansion and growth of structure measurements
• Constraining the dark energy equation of state with double source plane strong lenses
• Constraints on neutrino and dark radiation interactions using cosmological observations
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
• Cosmological constraints on an exponential interaction in the dark sector
• Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
• Using correlations between CMB lensing and large-scale structure to measure primordial non-Gaussianity
• Joint Measurement of Lensing-Galaxy Correlations Using SPT and DES SV Data
• B-modes and the Nature of Inflation
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample
• Inverted initial conditions: exploring the growth of cosmic structure and voids
• CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
• On the contribution of fluorescence to Ly$\alpha$ halos (LAHs) around star forming galaxies
• CMB spectral distortions revisited: a new take on $\mu$ distortions and primordial non-Gaussianities from FIRAS data
• The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation function
• Imprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scales
• Connecting early and late epochs by f(z)CDM cosmography
• Model independent inference of the expansion history and implications for the growth of structure
• GASP XXIX -- Unwinding the arms of spiral galaxies via ram-pressure stripping
• Fuzzy Dark Matter and the Dark Energy Survey Year 1 Data
• On the insufficiency of arbitrarily precise covariance matrices: non-Gaussian weak lensing likelihoods
• Mocking the Weak Lensing universe: the LensTools python computing package
• Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
• Properties of Resonantly Produced Sterile Neutrino Dark Matter Subhalos
• CMB Temperature and Polarization Anisotropy Fundamentals
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos
• Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space
• ISW measurements with photometric redshift surveys: 2MASS results and future prospects
• 21-cm signal from cosmic dawn - II: Imprints of the light-cone effects
• Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• Galaxy redshift surveys selected by neutral hydrogen using FAST
• A search for sterile neutrinos with the latest cosmological observations
• Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
• Measuring the primordial power spectrum: Principal component analysis of the cosmic microwave background
• The Benefits of CMB Delensing
• Impact of Baryonic Processes on Weak Lensing Cosmology: Power Spectrum, Non-Local Statistics, and Parameter Bias
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment
• Early massive clusters and the bouncing coupled dark energy
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• Primordial Black Holes, Eternal Inflation, and the Inflationary Parameter Space after WMAP5
• Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
• On the connection between the intergalactic medium and galaxies: The HI-galaxy cross-correlation at z < 1
• Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
• Observable primordial vector modes
• The Large-Scale Observational Signatures of Low-Mass Galaxies During Reionization
• Modeling the large-scale redshift-space 3-point correlation function of galaxies
• Constraints on secret neutrino interactions after Planck
• Euclid: Cosmological forecasts from the void size function
• Toward an accurate mass function for precision cosmology
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• Detecting Bispectral Acoustic Oscillations from Inflation Using a New Flexible Estimator
• Warm dark matter signatures on the 21cm power spectrum: Intensity mapping forecasts for SKA
• Introducing SPHINX-MHD: The Impact of Primordial Magnetic Fields on the First Galaxies, Reionization, and the Global 21cm Signal
• Measuring our peculiar velocity on the CMB with high-multipole off-diagonal correlations
• CosmoSpec: Fast and detailed computation of the cosmological recombination radiation from hydrogen and helium
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
• Testing Standard and Degenerate Big Bang Nucleosynthesis with BOOMERanG and MAXIMA-1
• Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
• Anisotropies of gravitational-wave standard sirens as a new cosmological probe without redshift information
• 3D simulations with boosted primordial power spectra and ultracompact minihalos
• Separate Universe Consistency Relation and Calibration of Halo Bias
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Anisotropic dark energy and CMB anomalies
• The High Redshift Integrated Sachs-Wolfe Effect
• Dynamics of Linear Perturbations in the hybrid metric-Palatini gravity
• How Well Can Future CMB Missions Constrain Cosmic Inflation?
• Baryon impact on weak lensing peaks and power spectrum: low-bias statistics and self-calibration in future surveys
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Galaxy and Mass Assembly (GAMA): Redshift Space Distortions from the Clipped Galaxy Field
• Quantifying concordance of correlated cosmological data sets
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Inflationary Steps in the Planck Data
• Empirical constraints on the formation of early-type galaxies
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
• Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering
• The extended Northern ROSAT Galaxy Cluster Survey (NORAS II) I. Survey Construction and First Results
• Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
• Observational constraints on Gauss-Bonnet cosmology
• Probing elastic interactions in the dark sector and the role of $S_8$
• Cosmic Microwave Background constraints for global strings and global monopoles
• Responses in Large-Scale Structure
• From Cavendish to PLANCK: Constraining Newton's Gravitational Constant with CMB Temperature and Polarization Anisotropy
• A look to the inside of haloes: a characterisation of the halo shape as a function of overdensity in the Planck cosmology
• Cosmological constraints on slow-roll inflation: an update
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Non-linear hydrodynamics of axion dark matter: relative velocity effects and "quantum forces"
• Signatures of a Graviton Mass in the Cosmic Microwave Background
• New cosmological bounds on hot relics: Axions $\&$ Neutrinos
• Fitting the nonlinear matter bispectrum by the Halofit approach
• Testing dark energy paradigms with weak gravitational lensing
• Prospects for constraining the shape of non-Gaussianity with the scale-dependent bias
• A combined analysis of 3D Weak Lensing, Lyman-alpha forest and WMAP year three data
• Constraints on the distance duality relation with standard sirens
• Efficient Evaluation of Cosmological Angular Statistics
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• Precision reconstruction of the dark matter-neutrino relative velocity from N-body simulations
• Cosmic bulk flows on 50 {h}^{-1}Mpc scales: A Bayesian hyper-parameter method and multishells likelihood analysis
• Improving constraints on the growth rate of structure by modelling the density-velocity cross-correlation in the 6dF Galaxy Survey
• On the road to percent accuracy II: calibration of the non-linear matter power spectrum for arbitrary cosmologies
• Compatibility of Planck and BICEP2 in the Light of Inflation
• Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• The BACCO simulation project: biased tracers in real space
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 LRG sample: structure growth rate measurement from the anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0
• Non-detection of a statistically anisotropic power spectrum in large-scale structure
• HYREC-2: a highly accurate sub-millisecond recombination code
• A fresh look into the interacting dark matter scenario
• Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
• Planck 2015 constraints on the non-flat XCDM inflation model
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• Inflation in a closed universe
• Spatial curvature and cosmological tests of general relativity
• Dark Radiation and interacting scenarios
• Maximal compression of the redshift space galaxy power spectrum and bispectrum
• 2MTF IV. A bulk flow measurement of the local Universe
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• Polyspectra searches for sharp oscillatory features in cosmic microwave sky data
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• A fake Interacting Dark Energy detection?
• Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
• Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
• Streaming velocities and the baryon-acoustic oscillation scale
• Constraints on early dark energy from CMB lensing and weak lensing tomography
• Large-Scale Structure Formation with Massive Neutrinos and Dynamical Dark Energy
• Constraints on dark-matter properties from large-scale structure
• Complete Reionization Constraints from Planck 2015 Polarization
• WMAP, neutrino degeneracy and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation
• Multi-wavelength constraints on the inflationary consistency relation
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties
• Emergent Dark Energy, neutrinos and cosmological tensions
• Limits on Defects Formation and Hybrid Inflationary Models with Three-Year WMAP Observations
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Structure Formation by the Fifth Force III: Segregation of Baryons and Dark Matter
• Dark matter and halo bispectrum in redshift space: theory and applications
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Predictions for local PNG bias in the galaxy power spectrum and bispectrum and the consequences for $f_{\mathrm{NL}}$ constraints
• Imprints of the Early Universe on Axion Dark Matter Substructure
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• Scale Dependence of Halo Bispectrum from Non-Gaussian Initial Conditions in Cosmological N-body Simulations
• Information Gain on Reheating: the One Bit Milestone
• Updating constraints on inflationary features in the primordial power spectrum with the Planck data
• 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
• Cosmic microwave background constraints on secret interactions among sterile neutrinos
• Search for Compensated Isocurvature Perturbations with Planck Power Spectra
• 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
• Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\alpha$ and Planck full-survey data
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Reconstruction of the Primordial Power Spectrum by Direct Inversion
• Cosmic Bubble Collisions
• PkANN - II. A non-linear matter power spectrum interpolator developed using artificial neural networks
• New limits on Early Dark Energy from the South Pole Telescope
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• CARPool: fast, accurate computation of large-scale structure statistics by pairing costly and cheap cosmological simulations
• TheHaloMod: An online calculator for the halo model
• Lensing Reconstruction in Post-Born Cosmic Microwave Background Weak Lensing
• Probing the neutrino mass hierarchy with CMB weak lensing
• Future CMB cosmological constraints in a dark coupled universe
• COLA with massive neutrinos
• Probing cosmology with weak lensing selected clusters I: Halo approach and all-sky simulations
• $\nu \mathrm{CO}N\mathrm{CEPT}$: Cosmological neutrino simulations from the non-linear Boltzmann hierarchy
• Cosmological parameter estimation and Bayesian model comparison using VSA data
• Light Axinos from Freeze-in: production processes, phase space distributions, and Ly-$\alpha$ forest constraints
• New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood
• Rapid Calculation of Theoretical CMB Angular Power Spectra
• Nonlinear Power Spectrum from Resummed Perturbation Theory: a Leap Beyond the BAO Scale
• Robust covariance estimation of galaxy-galaxy weak lensing: validation and limitation of jackknife covariance
• Testing Hu-Sawicki f(R) gravity with the Effective Field Theory approach
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies
• Horava Gravity in the Effective Field Theory formalism: from cosmology to observational constraints
• Probing the diffuse baryon distribution with the lensing-tSZ cross-correlation
• Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the ${\Omega }_m$-${\sigma }_8$ plane
• Multitracer CMB delensing maps from Planck and WISE data
• Observational constraints on the LLTB model
• Constraining anisotropic models of the early Universe with WMAP9 data
• Cosmological constraints on a light non-thermal sterile neutrino
• CMB-lensing beyond the Born approximation
• Constraining inflation with future galaxy redshift surveys
• Response function of the large-scale structure of the universe to the small scale inhomogeneities
• Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• Rico: An Accurate Cosmological Recombination Code
• Bispectrum of the Sunyaev-Zel'dovich Effect
• The full squeezed CMB bispectrum from inflation
• Features in the primordial power spectrum? A frequentist analysis
• Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
• Cosmological Parameters from Velocities, CMB and Supernovae
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Cosmic Microwave Background Constraints in Light of Priors Over Reionization Histories
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• Enhancing BOSS bispectrum cosmological constraints with maximal compression
• EFTCAMB/EFTCosmoMC: massive neutrinos in dark cosmologies
• Does Chaplygin gas have salvation?
• Galactic Winds in Cosmological Simulations of the Circumgalactic Medium
• Is cosmology compatible with sterile neutrinos?
• Tests of the CMB temperature-redshift relation, CMB spectral distortions and why adiabatic photon production is hard
• How Cold is Cold Dark Matter?
• Probing small-scale cosmological fluctuations with the 21 cm forest: effects of neutrino mass, running spectral index and warm dark matter
• 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
• Dynamical Dark Energy simulations: high accuracy Power Spectra at high redshift
• Cosmological constraints on non-standard inflationary quantum collapse models
• Predictions of just-enough inflation
• On CMB B-Mode Non-Gaussianity
• How to add massive neutrinos to your $\Lambda$CDM simulation -- extending cosmology rescaling algorithms
• The Mira-Titan Universe IV. High Precision Power Spectrum Emulation
• Measuring dark matter spikes around primordial black holes with Einstein Telescope and Cosmic Explorer
• A Measurement of CMB Cluster Lensing with SPT and DES Year 1 Data
• Constraints on primordial isocurvature perturbations and spatial curvature by Bayesian model selection
• Information Gains from Cosmic Microwave Background Experiments
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• Intrinsic alignments in the cross-correlation of cosmic shear and CMB weak lensing
• Constraining Fundamental Physics with Future CMB Experiments
• How well do we know the Halo Mass Function?
• Prospects for Constraining Neutrino Mass Using Planck and Lyman-Alpha Forest Data
• Suppressing the impact of a high tensor-to-scalar ratio on the temperature anisotropies
• Impact of baryons on the cluster mass function and cosmological parameter determination
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• The Dark Energy Survey Year 3 and eBOSS: constraining galaxy intrinsic alignments across luminosity and colour space
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• The VLT LBG Redshift Survey I: Clustering and Dynamics of ~1000 Galaxies at z~3
• Simulating the Impact of X-ray Heating during the Cosmic Dawn
• The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing
• The Effective Field Theory of Large-Scale Structure in the presence of Massive Neutrinos
• Inhomogeneous Reionization Models in Cosmological Hydrodynamical Simulations
• Canny Algorithm, Cosmic Strings and the Cosmic Microwave Background
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
• Is the $H_0$ tension suggesting a 4th neutrino's generation?
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Galaxy imaging surveys as spin-sensitive detector for cosmological colliders
• nestcheck: diagnostic tests for nested sampling calculations
• A Lagrangian Perturbation Theory in the presence of massive neutrinos
• Improving the modelling of redshift-space distortions: I. A bivariate Gaussian description for the galaxy pairwise velocity distributions
• Observational Constraints on Theories with a Blue Spectrum of Tensor Modes
• MultiModeCode: An efficient numerical solver for multifield inflation
• 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
• Non-linear Redshift-Space Power Spectra
• Gauging the cosmic microwave background
• Observing the Big Bounce with Tensor Modes in the Cosmic Microwave Background: Phenomenology and Fundamental LQC Parameters
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Is the Harrison-Zel'dovich spectrum coming back? ACT preference for $n_s\sim 1$ and its discordance with Planck
• Propagating Speed of Primordial Gravitational Waves
• Inference of the cosmic rest-frame from supernovae Ia
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• Does Current Data Prefer a Non-minimally Coupled Inflaton?
• Observational Constraint in $f(R,T)$ gravity from the cosmic chronometers and some standard distance measurement parameters
• Constraining Reionization with the $z\sim 5-6$ Lyman-$\alpha$ Forest Power Spectrum: the Outlook after Planck
• Probing Dark Matter with Future CMB Measurements
• Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
• What is the best way to measure baryonic acoustic oscillations?
• Halo clustering and g_{NL}-type primordial non-Gaussianity
• Lagrangian perturbation theory for modified gravity
• Magnification-Temperature Correlation: the Dark Side of ISW Measurements
• Power spectrum of halo intrinsic alignments in simulations
• Weighing obscured and unobscured quasar hosts with the CMB
• Testable dark energy predictions from current data
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• Fourier analysis of multi-tracer cosmological surveys
• Bayesian inflationary reconstructions from Planck 2018 data
• A measurement of the Hubble constant using galaxy redshift surveys
• The Knotted Sky I: Planck constraints on the primordial power spectrum
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Joint analysis of the thermal Sunyaev-Zeldovich effect and 2MASS galaxies: Probing gas physics in the local Universe and beyond
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• Dark Radiation candidates after Planck
• Measuring the neutrino mass from future wide galaxy cluster catalogues
• Joint growth rate measurements from redshift-space distortions and peculiar velocities in the 6dF Galaxy Survey
• New Constraints on variations of the fine structure constant from CMB anisotropies
• Bayesian modelling of clusters of galaxies from multi-frequency pointed Sunyaev--Zel'dovich observations
• A limit on the warm dark matter particle mass from the redshifted 21 cm absorption line
• Including beyond-linear halo bias in halo models
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• The Impact of Magnification and Size Bias on Weak Lensing Power Spectrum and Peak Statistics
• Suite of Hydrodynamical Simulations for the Lyman-Alpha Forest with Massive Neutrinos
• A Multi-Parameter Investigation of Gravitational Slip
• Cosmology with matter diffusion
• Constraining interacting dark energy with CMB and BAO future surveys
• PkANN - I. Non-linear matter power spectrum interpolation through artificial neural networks
• Blinding multi-probe cosmological experiments
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• The growth rate of cosmic structures in the local Universe with the ALFALFA survey
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• On the effect of non-Gaussian lensing deflections on CMB lensing measurements
• Testing Cosmology with Cosmic Sound Waves
• Reconstruction of broad features in the primordial spectrum and inflaton potential from Planck
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• Constraining warm dark matter with cosmic shear power spectra
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• The characteristic halo masses of half-a-million WISE-selected quasars
• Perturbation theory approach for the power spectrum: from dark matter in real space to massive haloes in redshift space
• Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): An unbiased estimate of the growth rate of structure at $⟨\mathbf{z}⟩=0.85$ using the clustering of luminous blue galaxies
• Neutrino mass without cosmic variance
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• CMB Lensing Reconstruction in Real Space
• Cosmological surveys with the Australian Square Kilometre Array Pathfinder
• Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering
• Dynamical Dark sectors and Neutrino masses and abundances
• Early Cosmology Constrained
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Local stochastic non-Gaussianity and N-body simulations
• EFTofPNG: A package for high precision computation with the Effective Field Theory of Post-Newtonian Gravity
• Viscous dark matter growth in (neo-)Newtonian cosmology
• Planck priors for dark energy surveys
• The Power Spectrum of the Lyman-$\alpha$ Forest at z < 0.5
• Reconstructing the primordial power spectrum from the CMB
• Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• The Accuracy of Weak Lensing Simulations
• Closing the window on fuzzy dark matter with the 21cm signal
• Structure Formation in Modified Gravity Scenarios
• Inflation model constraints from data released in 2015
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Ambiguous Tests of General Relativity on Cosmological Scales
• Inflationary Perturbations and Precision Cosmology
• Phenomenology of Large Scale Structure in scalar-tensor theories: joint prior covariance of $w_{\text{DE}}$, $\Sigma$ and $\mu$ in Horndeski
• Imprints of Dark Energy on Cosmic Structure Formation: III. Sparsity of Dark Matter Halo Profiles
• Planck and BICEP/Keck Array 2018 constraints on primordial gravitational waves and perspectives for future B-mode polarization measurements
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence
• Sterile neutrinos with pseudoscalar self-interactions and cosmology
• Primordial power spectrum: a complete analysis with the WMAP nine-year data
• Cosmological Structure Formation and Soliton Phase Transition in Fuzzy Dark Matter with Axion Self-Interactions
• Constraints on Kinetically Modified Inflation from WMAP5
• Structure formation simulations with momentum exchange: alleviating tensions between high-redshift and low-redshift cosmological probes
• An estimation of local bulk flow with the maximum-likelihood method
• 2MTF V. Cosmography, Beta, and the residual bulk flow
• Ruling out the power-law form of the scalar primordial spectrum
• Modeling Dark Photon Oscillations in Our Inhomogeneous Universe
• Time evolution of intrinsic alignments of galaxies
• Light Sterile Neutrinos in Cosmology and Short-Baseline Oscillation Experiments
• Perturbation Theory of the Cosmological Log-Density Field
• Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
• Fast Cosmological Parameter Estimation from Microwave Background Temperature and Polarization Power Spectra
• Spherical collapse in modified gravity with the Birkhoff-theorem
• Unified Dark Matter models with fast transition
• Probing dark energy and neutrino mass from upcoming lensing experiments of CMB and galaxies
• Holographic dark matter and dark energy with second order invariants
• WMAP 7 Constraints on Oscillations in the Primordial Power Spectrum
• Low power on large scales in just enough inflation models
• Probing deviations from General Relativity with the Euclid spectroscopic survey
• Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\mathrm{eff}}$=0.85 from the final dataset
• KiDS-1000: Cosmology with improved cosmic shear measurements
• Dark Energy Survey Year 3 results: Magnification modeling and impact on cosmological constraints from galaxy clustering and galaxy-galaxy lensing
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey
• Constraining Cluster Virialization Mechanism and Cosmology using Thermal-SZ-selected clusters from Future CMB Surveys
• Using dark energy to suppress power at small scales
• CLASH-VLT: a full dynamical reconstruction of the mass profile of Abell S1063 from 1 kpc out to the virial radius
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Precision modelling of the matter power spectrum in a Planck-like Universe
• Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos
• Small-scale Intensity Mapping: Extended Ly$\alpha$, H$\alpha$ and Continuum emission as a Probe of Halo Star Formation in High-redshift Galaxies
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Evidence for CII diffuse line emission at redshift $z\sim 2.6$
• Constraining the Baryon-Dark Matter Relative Velocity with the Large-Scale 3-Point Correlation Function of the SDSS BOSS DR12 CMASS Galaxies
• The Simons Observatory: Constraining inflationary gravitational waves with multi-tracer B-mode delensing
• Massive neutrino self-interactions and inflation
• Imprints of Oscillatory Bispectra on Galaxy Clustering
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Probing Decoupling in Dark Sectors with the Cosmic Microwave Background
• Helium Reionization Simulations. II. Signatures of Quasar Activity on the IGM
• Reconstruction of the neutrino mass as a function of redshift
• Unveiling the Intrinsic Alignment of Galaxies with Self-Calibration and DECaLS DR3 data
• Consistent cosmic shear in the face of systematics: a B-mode analysis of KiDS-450, DES-SV and CFHTLenS
• A new method for the Alcock-Paczynski test
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• Fast Estimation of Gravitational and Primordial Bispectra in Large Scale Structures
• Steps to Reconcile Inflationary Tensor and Scalar Spectra
• Modeling color-dependent galaxy clustering in cosmological simulations
• Lyman-alpha transfer in primordial hydrogen recombination
• The impact of AGN feedback on the 1D power spectra from the Ly$\alpha$ forest using the Horizon-AGN suite of simulations
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Power spectra in the eikonal approximation with adiabatic and non-adiabatic modes
• Scalar field dark energy models: Current and forecast constraints
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Relic Gravitational Waves with Modification due to Neutrino Free-Streaming
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• Warm dark matter and the ionization history of the Universe
• Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational data
• Large Scale Structure Formation in Eddington-inspired Born-Infeld Gravity
• HerMES: detection of cosmic magnification of sub-mm galaxies using angular cross-correlation
• Single-field inflation constraints from CMB and SDSS data
• Accurate Analytic Model for the Weak Lensing Convergence One-Point Probability Distribution Function and its Auto-Covariance
• Cornering the Planck $A_{lens}$ tension with future CMB data
• Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS and 2dFLenS
• Future weak lensing constraints in a dark coupled universe
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Updated measurements of the dark matter halo masses of obscured quasars with improved WISE and Planck data
• An Improved Calculation of the Non-Gaussian Halo Mass Function
• Constraints on the topology of the Universe derived from the 7-year WMAP data
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• CMB constraints on the early universe independent of late time cosmology
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• Hiding neutrino mass in modified gravity cosmologies
• Tilted Physics: A Cosmologically Dipole-Modulated Sky
• Parametrizing modified gravity for cosmological surveys
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Holography and the scale-invariance of density fluctuations
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• A fast particle-mesh simulation of non-linear cosmological structure formation with massive neutrinos
• Cluster-void degeneracy breaking: Neutrino properties and dark energy
• Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing -- validation on cosmological simulations
• CMB Anisotropies in the Presence of Extra Dimensions
• Constraints on dark radiation from cosmological probes
• Inflation in the closed FLRW model and the CMB
• Primordial features and Planck polarization
• An effective description of dark matter and dark energy in the mildly non-linear regime
• Transverse Velocities with the Moving Lens Effect
• Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data
• Small Angular Scale Measurements of the CMB Temperature Power Spectrum from QUaD
• Efficient exploration of cosmology dependence in the EFT of LSS
• Power spectrum multipoles on the curved sky: an application to the 6-degree Field Galaxy Survey
• Quintessence with Yukawa Interaction
• Bias deconstructed: Unravelling the scale dependence of halo bias using real space measurements
• CFHTLenS and RCSLenS Cross-Correlation with Planck Lensing Detected in Fourier and Configuration Space
• Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory
• Reconciling Hubble Constant Discrepancy from Holographic Dark Energy
• Constraining the Mass-Richness Relationship of redMaPPer Clusters with Angular Clustering
• Precise cosmological parameter estimation using CosmoRec
• CMB-lensing beyond the leading order: temperature and polarization anisotropies
• Parametrized modified gravity constraints after Planck
• The dipole of the galaxy bispectrum
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Observational constraints on K-inflation models
• Cosmological Perturbations in Elastic Dark Energy Models
• Biasing and the search for primordial non-Gaussianity beyond the local type
• Cosmic distance inference from purely geometric BAO methods: Linear Point standard ruler and Correlation Function Model Fitting
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Unbiased clustering estimate with VIPERS slit assignment
• How Late can the Dark Matter form in our universe?
• Constraints on primordial magnetic fields from magnetically-induced perturbations: current status and future perspectives with LiteBIRD and future ground based experiments
• Closed Universes from Cosmological Instantons
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• Bispectrum Supersample Covariance
• Implications of Milky Way Substructures for the Nature of Dark Matter
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• Probing gravity at large scales through CMB lensing
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• CMB Lensing Bispectrum from Nonlinear Growth of the Large Scale Structure
• The integrated Sachs-Wolfe effect in the AvERA cosmology
• 2-FAST: Fast and accurate computation of projected two-point functions
• Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
• Accelerating Large-Scale-Structure data analyses by emulating Boltzmann solvers and Lagrangian Perturbation Theory
• COFFE: a code for the full-sky relativistic galaxy correlation function
• Convergence properties of halo merger trees; halo and substructure merger rates across cosmic history
• Fingerprinting Dark Energy II: weak lensing and galaxy clustering tests
• Projected Constraints on Modified Gravity Cosmologies from 21 cm Intensity Mapping
• Signatures of Primordial non-Gaussianities in the Matter Power-Spectrum and Bispectrum: the Time-RG Approach
• Primordial B-mode Diagnostics and Self Calibrating the CMB Polarization
• The Covariance of Squeezed Bispectrum Configurations
• GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part I. Methodology and code description
• (1+3) Covariant Dynamics of Scalar Perturbations in Braneworlds
• New Parametrization for the Scale Dependent Growth Function in General Relativity
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• Neutrino and Dark Radiation properties in light of latest CMB observations
• Impact of theoretical priors in cosmological analyses: the case of single field quintessence
• Noise reduction for weak lensing mass mapping: An application of generative adversarial networks to Subaru Hyper Suprime-Cam first-year data
• Constraints on Light WIMP candidates from the Isotropic Diffuse Gamma-Ray Emission
• Axi-Higgs Cosmology
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• 21-cm constraints on spinning primordial black holes
• Microwave background constraints on inflationary parameters
• Reconstruction of the primordial power spectra with Planck and BICEP2
• Figures of merit and constraints from testing General Relativity using the latest cosmological data sets including refined COSMOS 3D weak lensing
• Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies
• Simulations of the Pairwise Kinematic Sunyaev-Zel'dovich Signal
• Nonlinear Evolution of Cosmic Magnetic Fields and Cosmic Microwave Background Anisotropies
• Constraining Variations in the Fine Structure Constant in the presence of Early Dark Energy
• The halo mass function in interacting Dark Energy models
• Constructing perturbation theory kernels for large-scale structure in generalized cosmologies
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• Lensing reconstruction from line intensity maps: the impact of gravitational nonlinearity
• Testing phenomenological and theoretical models of dark matter density profiles with galaxy clusters
• Relativistic initial conditions for N-body simulations
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• 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
• Gaussian Process Regression for foreground removal in HI intensity mapping experiments
• Early Universe Constraints on Time Variation of Fundamental Constants
• Revisiting CMB constraints on dark matter annihilation
• CMB Beam Systematics: Impact on Lensing Parameter Estimation
• Measuring the scale of cosmic homogeneity with SDSS-IV DR14 quasars
• Measuring primordial non-Gaussianity with weak-lensing surveys
• JWST high-z galaxy constraints on warm and cold dark matter models
• Primordial non-Gaussianity from the 21 cm Power Spectrum during the Epoch of Reionization
• Detecting neutrino mass difference with cosmology
• The HI content of dark matter halos at $z\approx 0$ from ALFALFA
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Constraining the initial conditions of the Universe using large scale structure
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• Mild bounds on bigravity from primordial gravitational waves
• Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
• J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
• Cosmic Magnetism in Centimeter and Meter Wavelength Radio Astronomy
• Constraints on mixed dark matter from anomalous strong lens systems
• Biased Tracers of Two Fluids in the Lagrangian Picture
• BAMBI: blind accelerated multimodal Bayesian inference
• Using the Zeldovich dynamics to test expansion schemes
• First constraints on the running of non-Gaussianity
• Bayesian inference of CMB gravitational lensing
• Constraints on the neutrino parameters by future cosmological 21cm line and precise CMB polarization observations
• Visualizing probabilistic models: Intensive Principal Component Analysis
• Position-Space Description of the Cosmic Microwave Background and Its Temperature Correlation Function
• CMB constraint on non-Gaussianity in isocurvature perturbations
• The Halo Bispectrum Multipoles in Redshift Space
• Cosmic propagators at two-loop order
• Probing spatial homogeneity with LTB models: a detailed discussion
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Response Approach to the Matter Power Spectrum Covariance
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• Reducing sample variance: halo biasing, non-linearity and stochasticity
• Maximum likelihood, parametric component separation and CMB B-mode detection in suborbital experiments
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
• Braneworld Tensor Anisotropies in the CMB
• Constraining Warm Inflation with the Cosmic Microwave Background
• Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data
• Cross-correlation of the thermal Sunyaev-Zel'dovich effect and weak gravitational lensing: Planck and Subaru Hyper Suprime-Cam first-year data
• CMB anisotropies in the presence of a stochastic magnetic field
• Evolution of perturbations and cosmological constraints in decaying dark matter models with arbitrary decay mass products
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• New Limits on Coupled Dark Energy from Planck
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• Statistical Test of Distance--Duality Relation with Type Ia Supernovae and Baryon Acoustic Oscillations
• KiDS-1000: Constraints on the intrinsic alignment of luminous red galaxies
• Enhancing gravitational wave anisotropies with peaked scalar sources
• Spatial curvature endgame: Reaching the limit of curvature determination
• Testing the Cosmic Shear Spatially-Flat Universe Approximation with Generalized Lensing and Shear Spectra
• Intensity mapping with neutral hydrogen and the Hidden Valley simulations
• BeyondPlanck III. Commander3
• Observational constraints on cosmic neutrinos and dark energy revisited
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• The effect of early radiation in N-body simulations of cosmic structure formation
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck II: Cross-correlation measurements and cosmological constraints
• Constraints on the cosmic expansion rate at redshift 2.3 from the Lyman-$\alpha$ forest
• Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
• Searching for axion-like particles through CMB birefringence from string-wall networks
• Constraints on warm dark matter from weak lensing in anomalous quadruple lenses
• Testing the imprint of non-standard cosmologies on void profiles using Monte Carlo random walks
• Connecting the structure of dark matter haloes to the primordial power spectrum
• Figures of merit for present and future dark energy probes
• Dynamical dark energy confronted with multiple CMB missions
• Nonparametric 3D map of the IGM using the Lyman-alpha forest
• Redshift evolution of cosmic birefringence in CMB anisotropies
• CMB Constraint on Dark Matter Annihilation after Planck 2015
• Cosmological ensemble and directional averages of observables
• Magnification effect on the detection of primordial non-Gaussianity from photometric surveys
• Beyond the traditional Line-of-Sight approach of cosmological angular statistics
• Axion Miniclusters Made Easy
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Structure formation in a $\Lambda$ $viscous$ CDM universe
• New Constraints On The Dark Energy Equation of State
• The Cosmological Evolution of the Average Mass Per Baryon
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Fingerprinting Dark Energy III: distinctive marks of viscosity
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Magnification bias in galaxy surveys with complex sample selection functions
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• Extending the generalized Chaplygin gas model by using geometrothermodynamics
• Beware of Fake $\nu$s: The Effect of Massive Neutrinos on the Nonlinear Evolution of Cosmic Structure
• Dark Radiation in extended cosmological scenarios
• ISW Imprint of Superstructures on Linear Scales
• Effects of Dark Energy Perturbations on Cosmological Tests of General Relativity
• No H_0 Assistance from Assisted Quintessence
• Bias-Hardened CMB Lensing with Polarization
• Simulating intergalactic gas for DESI-like small scale Lymanα forest observations
• Determination of miscalibrated polarization angles from observed CMB and foreground $EB$ power spectra: Application to partial-sky observation
• Effects of helical magnetic fields on the cosmic microwave background
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Low-mass suppression of the satellite luminosity function due to the supersonic baryon--cold-dark-matter relative velocity
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• The Dark Side of the Universe after Planck
• Limits on primordial power spectrum resolution: An inflationary flow analysis
• Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model
• The foreground transfer function for HI intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications
• Predictions for the 21cm-galaxy cross-power spectrum observable with LOFAR and Subaru
• Constraints on inflation with LSS surveys: features in the primordial power spectrum
• Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• Characterizing bias on large scale CMB $B$-modes after galactic foregrounds cleaning
• Model marginalized constraints on neutrino properties from cosmology
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II
• Constraints on Brane Inflation and Cosmic Strings
• Impacts of dark energy on weighing neutrinos after DESI BAO
• Optimized Clustering Estimators for BAO Measurements Accounting for Significant Redshift Uncertainty
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• Comparing Planck and WMAP: Maps, Spectra, and Parameters
• CMB Faraday rotation as seen through the Milky Way
• Euclid: Forecasts from the void-lensing cross-correlation
• Direct detection of the kinetic Sunyaev-Zel'dovich effect in galaxy clusters
• MultiDarkLens Simulations: weak lensing light-cones and data base presentation
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Constraints on massive sterile plus active neutrino species in non minimal cosmologies
• Weighing Neutrinos in $f(R)$ gravity
• Constraining Inflation
• Constraining the kinetically dominated Universe
• The Angular Power Spectra of Photometric SDSS LRGs
• Simulations of Galileon modified gravity: Clustering statistics in real and redshift space
• Blue Gravity Waves from BICEP2 ?
• Observing AGN feedback with CO intensity mapping
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys
• Mock Quasar-Lyman-α Forest Data-sets for the SDSS-III Baryon Oscillation Spectroscopic Survey
• A Robust Measure of Cosmic Structure beyond the Power-Spectrum: Cosmic Filaments and the Temperature of Dark Matter
• Cosmological constraints on general, single field inflation
• Microphysics of Early Dark Energy
• Cosmological parameter estimation with free-form primordial power spectrum
• Cosmology with relativistically varying physical constants
• 2MTF - VII. 2MASS Tully-Fisher survey final data release: distances for 2,062 nearby spiral galaxies
• Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest
• 21 cm intensity mapping with the Five hundred metre Aperture Spherical Telescope
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• Searching for primordial localized features with CMB and LSS spectra
• The dark matter transfer function: free streaming, particle statistics and memory of gravitational clustering
• Observational constraints on varying neutrino-mass cosmology
• The dipole anisotropy of AllWISE galaxies
• Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data
• Direct Wavelet Expansion of the Primordial Power Spectrum
• Testing Modified Gravity with Cosmic Shear
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment's Sample-Variance Limited E-Mode Measurement
• Capse.jl: efficient and auto-differentiable CMB power spectra emulation
• Interloper bias in future large-scale structure surveys
• Seeking Inflation Fossils in the Cosmic Microwave Background
• Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg${}^2$ SPT-SZ and Planck Gravitational Lensing Map
• Measuring the reionization optical depth without large-scale CMB polarization
• Cosmic Inflation at the Crossroads
• Formation and Morphology of the First Galaxies in the Cosmic Morning
• Cross-correlating radio continuum surveys and CMB lensing: constraining redshift distributions, galaxy bias and cosmology
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Determination of neutrino mass hierarchy by 21 cm line and CMB B-mode polarization observations
• Origin of Delta N_eff as a Result of an Interaction between Dark Radiation and Dark Matter
• Growth index and statefinder diagnostic of Oscillating Dark Energy
• 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?
• Relieving tensions related to the lensing of CMB temperature power spectra
• Measuring our Peculiar Velocity by "Pre-deboosting" the CMB
• Impact of anisotropic stress of free-streaming particles on gravitational waves induced by cosmological density perturbations
• Exploring degeneracies in modified gravity with weak lensing
• The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
• What is the price of abandoning dark matter? Cosmological constraints on alternative gravity theories
• Bispectrum-window convolution via Hankel transform
• Dancing in the dark: detecting a population of distant primordial black holes
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• Perceiving the equation of state of Dark Energy while living in a Cold Spot
• Rejuvenating the Matter Power Spectrum III: The Cosmology Sensitivity of Gaussianized Power Spectra
• Measuring the Tidal Response of Structure Formation: Anisotropic Separate Universe Simulations using TreePM
• Acoustic signatures in the Cosmic Microwave Background bispectrum from primordial magnetic fields
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• A local measurement of the growth rate from peculiar velocities and galaxy clustering correlations in the 6dF Galaxy Survey
• Reionisation in sterile neutrino cosmologies
• On the stability conditions for theories of modified gravity in presence of matter fields
• Simulated forecasts for primordial B-mode searches in ground-based experiments
• On the road to discovery of relic gravitational waves: The TE and BB Correlations in the cosmic microwave background radiation
• Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
• On cosmological signatures of baryons-dark energy elastic couplings
• Moving around the cosmological parameter space: a nonlinear power spectrum reconstruction based on high-resolution cosmic responses
• An exploration of an early gravity transition in light of cosmological tensions
• Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations
• Cosmological searches for a non-cold dark matter component
• Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
• Cosmological parameter estimation using Particle Swarm Optimization (PSO)
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Can modified gravity models reconcile the tension between CMB anisotropy and lensing maps in Planck-like observations?
• Impacts of the physical data model on the forward inference of initial conditions from biased tracers
• Cosmic birefringence tomography and calibration-independence with reionization signals in the CMB
• The degeneracy between primordial non-Gaussianity and foregrounds in 21cm intensity mapping experiments
• Learning to Concentrate: Multi-tracer Forecasts on Local Primordial Non-Gaussianity with Machine-Learned Bias
• Forecast Constraints on Inflation from Combined CMB and Gravitational Wave Direct Detection Experiments
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM
• Redshift-space distortions in massive neutrino and evolving dark energy cosmologies
• Neutrino mass and dark energy constraints from redshift-space distortions
• Foreground-Induced Biases in CMB Polarimeter Self-Calibration
• Dark Radiation and Inflationary Freedom after Planck 2015
• KiDS-Legacy: Consistency of cosmic shear measurements and joint cosmological constraints with external probes
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• The large scale CMB cut-off and the tensor-to-scalar ratio
• Zero-point quantum fluctuations in cosmology
• Impact of next-to-leading order contributions to CMB lensing
• Polarized Sunyaev Zel'dovich tomography
• Information Gains from Cosmological Probes
• Constraints on hidden photons from current and future observations of CMB spectral distortions
• Beating the Lyth bound by parametric resonance during inflation
• Intrinsic alignment contamination to CMB lensing-galaxy weak lensing correlations from tidal torquing
• Varying couplings in the early universe: correlated variations of $\alpha$ and $G$
• Intrinsic galaxy alignment from angular dependent primordial non-Gaussianity
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• Intrinsic alignment statistics of density and velocity fields at large scales: Formulation, modeling, and baryon acoustic oscillation features
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• Probing Primordial Magnetism with Off-Diagonal Correlators of CMB Polarization
• Next-to-leading resummations in cosmological perturbation theory
• Euclid: The reduced shear approximation and magnification bias for Stage IV cosmic shear experiments
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• Characterisation of the non-Gaussianity of radio and IR point-sources at CMB frequencies
• Forecasting Polarized Radio Sources for CMB observations
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• The KBC Void: Consistency with Supernovae Type Ia and the Kinematic SZ Effect in a $\Lambda$LTB Model
• Annealing a Follow-up Program: Improvement of the Dark Energy Figure of Merit for Optical Galaxy Cluster Surveys
• Weak lensing induced by second-order vector mode
• Constraints on holographic multi-field inflation and models based on the Hamilton-Jacobi formalism
• What is the distance to the CMB?
• The squeezed matter bispectrum covariance with responses
• Testing gravity with $E_G$: mapping theory onto observations
• Optimal constraint on g_NL from CMB
• Cosmic Microwave Background Acoustic Peak Locations
• Is there evidence for additional neutrino species from cosmology?
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• Testing standard and non-standard neutrino physics with cosmological data
• New Constraints on the Early Expansion History
• Comparing multi-field primordial feature models with the Planck data
• Dark Matter Interactions, Helium, and the CMB
• Hidden Treasures: sterile neutrinos as dark matter with miraculous abundance, structure formation for different production mechanisms, and a solution to the sigma-8 problem
• Encircling the dark: constraining dark energy via cosmic density in spheres
• Non-linear contributions to angular power spectra
• Cosmology with the moving lens effect
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• Dynamics of neutrino lumps in growing neutrino quintessence
• CMB Lensing Constraints on Dark Energy and Modified Gravity Scenarios
• Extending the Coyote emulator to dark energy models with standard $w_0$-$w_a$ parametrization of the equation of state
• Constraining the time variation of the coupling constants from cosmic microwave background: effect of Λ_{QCD}
• Current and Future Constraints on Primordial Magnetic Fields
• Linear Point and Sound Horizon as Purely Geometric standard rulers
• Post-Planck Dark Energy Constraints
• The angular scale of homogeneity in the Local Universe with the SDSS blue galaxies
• Cosmic Structure Formation with Kinetic Field Theory
• Non-Gaussianity of the Cosmic Infrared Background anisotropies I : Diagrammatic formalism and application to the angular bispectrum
• Search for anomalous alignments of structures in Planck data using Minkowski Tensors
• Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
• Propagating sample variance uncertainties in redshift calibration: simulations, theory and application to the COSMOS2015 data
• Observational Constraints on Constant Roll Inflation
• Proper-Time Hypersurface of Non-Relativistic Matter Flows: Galaxy Bias in General Relativity
• Testing non-minimally coupled inflation with CMB data: a Bayesian analysis
• Tensor Minkowski Functionals: first application to the CMB
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Forecasting sensitivity on tilt of power spectrum of primordial gravitational waves after Planck satellite
• Cosmological $N$-body simulations including radiation perturbations
• Evidence for inhomogeneous reionization in the local Universe from metal-poor globular cluster systems
• Modeling Extragalactic Foregrounds and Secondaries for Unbiased Estimation of Cosmological Parameters From Primary CMB Anisotropy
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum
• Approximate Analytic Spectra of Reionized CMB Anisotropies and Polarization generated by Relic Gravitational Waves
• New MGCAMB tests of gravity with CosmoMC and Cobaya
• J-PAS: Forecasts for dark matter - dark energy elastic couplings
• Disentangling dark sector models using weak lensing statistics
• Strong Bounds on Sum of Neutrino Masses in a 12 Parameter Extended Scenario with Non-Phantom Dynamical Dark Energy ($w(z)\ge -1$)
• Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra
• The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• Power Spectra to 1% Accuracy between Dynamical Dark Energy Cosmologies
• The Topology and Size of the Universe from CMB Temperature and Polarization Data
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
• Precision cosmology in muddy waters: Cosmological constraints and N-body codes
• A coarse grained perturbation theory for the Large Scale Structure, with cosmology and time independence in the UV
• The present and future of the most favoured inflationary models after $Planck$ 2015
• Perturbations in electromagnetic dark energy
• Dark matter velocity dispersion effects on CMB and matter power spectra
• CMB lensing power spectrum estimation without instrument noise bias
• Constraining warm dark matter with 21 cm line fluctuations due to minihalos
• Detectability of CMB tensor B modes via delensing with weak lensing galaxy surveys
• Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
• Map-making in small field modulated CMB polarisation experiments: approximating the maximum-likelihood method
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• Distinguishing standard reionization from dark matter models
• Rayleigh scattering: blue sky thinking for future CMB observations
• CMB internal delensing with general optimal estimator for higher-order correlations
• Likelihood methods for CMB experiments
• CMB Constraints on the Stochastic Gravitational-Wave Background at Mpc scales
• Inflationary Freedom and Cosmological Neutrino Constraints
• Wavelet Band Powers of the Primordial Power Spectrum from CMB Data
• Domain walls coupled to matter: the symmetron example
• On the current status of Modified Gravity
• 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
• The Simons Observatory: Galactic Science Goals and Forecasts
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• A Combined View of Sterile-Neutrino Constraints from CMB and Neutrino Oscillation Measurements
• A new parameterization of the reionisation history
• Globular cluster numbers in dark matter haloes in a dual formation scenario: an empirical model within EMERGE
• Fast Weak Lensing Simulations with Halo Model
• Bayesian analysis of anisotropic cosmologies: Bianchi VII_h and WMAP
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• First observational constraints on tensor non-Gaussianity sourced by primordial magnetic fields from cosmic microwave background
• Uncertainty on w from large-scale structure
• Kinetic Sunyaev-Zeldovich effect in modified gravity
• Observing the Multiverse with Cosmic Wakes
• Hybrid Cosmological Simulations with Stream Velocities
• The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access
• The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering
• Investigating the degeneracy between modified gravity and massive neutrinos with redshift-space distortions
• The Topology and Size of the Universe from the Cosmic Microwave Background
• Lensing reconstruction from a patchwork of polarization maps
• The Simons Observatory: pipeline comparison and validation for large-scale B-modes
• The effect of inhomogeneities on the distance to the last scattering surface and the accuracy of the CMB analysis
• An improved model of HII bubbles during the epoch of reionization
• Discordances in cosmology and the violation of slow-roll inflationary dynamics
• Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
• Modeling the clustering of dark-matter haloes in resummed perturbation theories
• Testing tidal alignment models for anisotropic correlations of halo ellipticities with N-body simulations
• A dynamics-based density profile for dark haloes -- II. Fitting function
• CMB constraints on $\beta$-exponential inflationary models
• Probing features in inflaton potential and reionization history with future CMB space observations
• Probing Modified Gravity Theories with ISW and CMB Lensing
• Understanding parameter differences between analyses employing nested data subsets
• On the information content of the matter power spectrum
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
• Constraints on neutrino masses from the study of the nearby large-scale structure and galaxy cluster counts
• Probing cosmic birefringence with polarized Sunyaev-Zel'dovich tomography
• Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: Statistical and systematic error budgets for future experiments
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Cross-Correlating Probes of Primordial Gravitational Waves
• Lensing power spectrum of the Cosmic Microwave Background with deep polarization experiments
• Robust Simulation-Based Inference in Cosmology with Bayesian Neural Networks
• Halo assembly bias from Separate Universe simulations
• Beating non-linearities: improving the Baryon Acoustic Oscillations with the linear point
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• Correcting correlation functions for redshift-dependent interloper contamination
• The look-elsewhere effect from a unified Bayesian and frequentist perspective
• The Polarization of the Cosmic Microwave Background Due to Primordial Gravitational Waves
• Constraining Cut-off Physics in the Cosmic Microwave Background
• Implications of an extended dark energy model with massive neutrinos
• Complementing the ground-based CMB Stage-4 experiment on large scales with the PIXIE satellite
• Constraints on variation in $\alpha$ and $m_e$ from WMAP 7-year data
• Does Quartessence Ease Tensions?
• CosmicNet I: Physics-driven implementation of neural networks within Boltzmann-Einstein solvers
• New universal property of cosmological gravitational wave anisotropies
• $\text{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum
• N-body simulations with a cosmic vector for dark energy
• Nonlinear cosmological consistency relations and effective matter stresses
• Improved upper limit on degree-scale CMB B-mode polarization power from the 670 square-degree POLARBEAR survey
• Clipping the Cosmos II: Cosmological information from non-linear scales
• Power spectrum modelling of galaxy and radio intensity maps including observational effects
• Coupling between cold dark matter and dark energy from neutrino mass experiments
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• Deep spectroscopy in nearby galaxy clusters: III Orbital structure of galaxies in Abell 85
• Detecting the radiative decay of the cosmic neutrino background with line-intensity mapping
• Mask Effects on Cosmological Studies with Weak Lensing Peak Statistics
• Searching for features of a string-inspired inflationary model with cosmological observations
• Reionization and dark matter decay
• Non-minimal Derivative Coupling Scalar Field and Bulk Viscous Dark Energy
• Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS
• Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements
• Nonlinear evolution of initially biased tracers in modified gravity
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• Cosmology-marginalized approaches in Bayesian model comparison: the neutrino mass as a case study
• Assessing the impact of bulk and shear viscosities on large scale structure formation
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Stacked Weak Lensing Mass Calibration: Estimators, Systematics, and Impact on Cosmological Parameter Constraints
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Fundamental limits on constraining primordial non-Gaussianity
• Constraining viscous dark energy models with the latest cosmological data
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- I. The importance of redshift-space distortions for galaxy number counts
• Constraining neutrino properties with a Euclid-like galaxy cluster survey
• DEMNUni: disentangling dark energy from massive neutrinos with the void size function
• Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• Scale-Dependent Bias of Galaxies from Baryonic Acoustic Oscillations
• CMB anisotropies generated by a stochastic background of primordial magnetic fields with non-zero helicity
• Probing Lorentz-violating electrodynamics with CMB polarization
• The N5K Challenge: Non-Limber Integration for LSST Cosmology
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VII The Mass Function of Galaxy Clusters
• A new measure of tension between experiments
• Measuring nonlocal Lagrangian peak bias
• The Linear Point: A cleaner cosmological standard ruler
• Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
• Hunting down systematics in baryon acoustic oscillations after cosmic high noon
• GLASS: Generator for Large Scale Structure
• Probing features in the primordial perturbation spectrum with large-scale structure data
• A New Method to Constrain the Appearance and Disappearance of Observed Jellyfish Galaxy Tails
• Galaxy bias from the Dark Energy Survey Science Verification data: combining galaxy density maps and weak lensing maps
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
• J-PAS: forecasts on dark energy and modified gravity theories
• Scaling Transformations and the Origins of Light Relics Constraints from Cosmic Microwave Background Observations
• Can dark energy viscosity be detected with the Euclid survey?
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Fast Bayesian inference for slow-roll inflation
• Producing a BOSS-CMASS sample with DES imaging
• Planck ISW-lensing likelihood and the CMB temperature
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Evolution and Statistics of Non-Sphericity of Dark Matter Halos from Cosmological N-Body Simulation
• Assessing the Importance of Noise from Thermal Sunyaev-Zel{'}dovich Signals for CMB Cluster Surveys and Cluster Cosmology
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel'dovich approximation
• Constraints on decaying dark matter from weak lensing and cluster counts
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• Cosmological Imprints of Pre-Inflationary Particles
• Spectral distortion anisotropies from single-field inflation
• How Density Environment Changes the Influence of the Dark Matter-Baryon Streaming Velocity on the Cosmological Structure Formation
• KiDS-450: Enhancing cosmic shear with clipping transformations
• Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors
• Inflationary Features and Shifts in Cosmological Parameters from Planck 2015 Data
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• Wavelet-Bayesian inference of cosmic strings embedded in the cosmic microwave background
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Never mind the gaps: comparing techniques to restore homogeneous sky coverage
• Cosmology with the pairwise kinematic SZ effect: Calibration and validation using hydrodynamical simulations
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• Large-scale clustering as a probe of the origin and the host environment of fast radio bursts
• Axion cold dark matter: status after Planck and BICEP2
• Measuring the cosmic homogeneity scale with SDSS-IV DR16 Quasars
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• Cosmological parameters estimation in the Quintessence Paradigm
• Boundary Inflation and the WMAP Data
• Constraint on the primordial vector mode and its magnetic field generation from seven-year Wilkinson Microwave Anisotropy Probe Observations
• On Minkowski Functionals of CMB polarization
• On dark matter - dark radiation interaction and cosmic reionization
• Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
• The Effects of Rayleigh Scattering on the CMB and Cosmic Structure
• Testing gravity theories using tensor perturbations
• The velocity field in MOND cosmology
• WMAP 5-year constraints on time variation of $\alpha$ and $m_e$ in a detailed recombination scenario
• Thermodynamics of massless particles in curved spacetime
• Constraints on the solid dark universe model
• Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
• Efficient decomposition of cosmic microwave background polarization maps into pure E, pure B, and ambiguous components
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• Probing patchy reionization through tau-21cm correlation statistics
• candl: Cosmic Microwave Background Analysis with a Differentiable Likelihood
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• Euclid: Modelling massive neutrinos in cosmology -- a code comparison
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• Measuring the geometry of the Universe in the presence of isocurvature modes
• Comparison of different approaches to the quasi-static approximation in Horndeski models
• Clustering analysis of high-redshift Luminous Red Galaxies in Stripe 82
• Broadband distortion modeling in Lyman-$\alpha$ forest BAO fitting
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• Computing model independent perturbations in dark energy and modified gravity
• Recovering the CMB Signal with Machine Learning
• Constraints on time variation of fine structure constant from WMAP-3yr data
• Efficient optimal non-Gaussian CMB estimators with polarisation
• Cosmological evidence for leptonic asymmetry after Planck
• Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• Searching for Primordial Magnetic Fields with CMB B-modes
• Probing the first galaxies with the SKA
• Intelligent Design: On the Emulation of Cosmological Simulations
• Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination
• Non-linear dark energy clustering
• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• The Effects of Lyman-Limit Systems on the Evolution and Observability of the Epoch of Reionization
• Impact of reionization on CMB polarization tests of slow-roll inflation
• Super-CMB fluctuations and the Hubble tension
• Equivalence of cosmological observables in conformally related scalar tensor theories
• Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
• Impact of internal-delensing biases on searches for primordial B-modes of CMB polarisation
• Accurate effective fluid approximation for ultralight axions
• Helmholtz Decomposition of the Lagrangian Displacement
• Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
• Confronting the concordance model of cosmology with Planck data
• PT challenge: Validation of ShapeFit on large-volume, high-resolution mocks
• Cosmological signatures of tilted isocurvature perturbations: reionization and 21cm fluctuations
• Three-point phase correlations: A new measure of non-linear large-scale structure
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Phantom braneworld and the Hubble tension
• Efficiency of pseudo-spectrum methods for estimation of Cosmic Microwave Background B-mode power spectrum
• Slow-roll inflation and CMB anisotropy data
• The impact of inhomogeneous subgrid clumping on cosmic reionization II: modelling stochasticity
• First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations
• Observational constraints on conformal time symmetry, missing matter and double dark energy
• Limitations of CMB B-mode template delensing
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Future constraints on neutrino isocurvature perturbations in the curvaton scenario
• Radiative transfer effects during primordial helium recombination
• Disentangling dark energy and cosmic tests of gravity from weak lensing systematics
• Dispu$\tau$able: the high cost of a low optical depth
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• A Bayesian study of the primordial power spectrum from a novel closed universe model
• Consistency check of ΛCDM phenomenology
• Optimal parameterizations for observational constraints on thawing dark energy
• Observational hints on the Big Bounce
• Parametrising non-linear dark energy perturbations
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• The information content of cosmic microwave background anisotropies
• Higher-Curvature Corrections and Tensor Modes
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz
• Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam
• Halo Abundance and Assembly History with Extreme-Axion Wave Dark Matter at $z\ge 4$
• Tomographic imaging of the Fermi-LAT gamma-ray sky through cross-correlations: A wider and deeper look
• Impact of modulation on CMB B-mode polarization experiments
• Cosmic Shear as a Probe of Galaxy Formation Physics
• Bulk flow and shear in the local Universe: 2MTF and COSMICFLOWS-3
• Simulating cosmologies beyond $\Lambda$CDM with PINOCCHIO
• Probing correlations of early magnetic fields using mu-distortion
• Sound speed of scalar field dark energy: weak effects and large uncertainties
• Accuracy of cosmological parameters using the baryon acoustic scale
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Joint Planck and WMAP Assessment of Low CMB Multipoles
• CMB power spectra induced by primordial cross-bispectra between metric perturbations and vector fields
• CMBfit: Rapid WMAP likelihood calculations with normal parameters
• Determining neutrino properties using future galaxy redshift surveys
• Model independent constraints on mass-varying neutrino scenarios
• A Bayesian analysis of inflationary primordial spectrum models using Planck data
• Constraining the Nature of Dark Energy using the SKA
• CMB Temperature Polarization Correlation and Primordial Gravitational Waves
• Constraints on nature of ultra light dark matter particles with 21cm forest
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• CMB EB and TB cross-spectrum estimation via pseudo-spectrum techniques
• One line to run them all: SuperEasy massive neutrino linear response in $N$-body simulations
• Using the Topology of Large Scale Structure to constrain Dark Energy
• Cluster counts: calibration issue or new physics?
• Cosmic Reionization May Still Have Started Early and Ended Late: Confronting Early Onset with CMB Anisotropy and 21 cm Global Signals
• Bulk flow of halos in ΛCDM simulation
• Constraining Scale-Dependent Non-Gaussianity with Future Large-Scale Structure and the CMB
• Prospects of Future CMB Anisotropy Probes for Primordial Black Holes
• Current constraints on deviations from General Relativity using binning in redshift and scale
• Changes in the halo formation rates due to features in the primordial spectrum
• Perturbations in a scalar field model with virtues of $\Lambda$CDM
• A short review on clustering dark energy
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Compressing the cosmological information in one-dimensional correlations of the Lyman-$\alpha$ forest
• Pairwise Transverse Velocity Measurement with the Rees-Sciama Effect
• Bayesian analysis of inflationary features in Planck and SDSS data
• CMB and matter power spectra with non-linear dark-sector interactions
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• New fitting formula for cosmic non-linear density distribution
• Cosmological Parameters from the QUaD CMB polarization experiment
• The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite
• New constraints on primordial features from the galaxy two-point correlation function
• Effects of electrically charged dark matter on cosmic microwave background anisotropies
• Viable Gauge Choices in Cosmologies with Non-Linear Structures
• Dark Before Light: Testing the Cosmic Expansion History through the Cosmic Microwave Background
• How to constrain inflationary parameter space with minimal priors
• Measurement of the integrated Sachs-Wolfe effect using the AllWISE data release
• Modified Gravity: the CMB, Weak Lensing and General Parameterisations
• Coupling parsec and gigaparsec scales: primordial non-Gaussianity with multi-tracer intensity mapping
• Anisotropic separate universe simulations
• A model-independent fit to Planck and BICEP2 data
• A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol
• Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear dark matter density field
• Euclid: Cosmology forecasts from the void-galaxy cross-correlation function with reconstruction
• Measuring the transition to homogeneity with photometric redshift surveys
• Testing gravity at large scales with HI intensity mapping
• Peculiar Velocities into the Next Generation: Cosmological Parameters From Large Surveys without Bias from Nonlinear Structure
• A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear Surveys
• Constraining primordial magnetic fields with CMB polarization experiments
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Turning noise into signal: learning from the scatter in the Hubble diagram
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos
• Isocurvature perturbations in extra radiation
• Dipole Modulation of Cosmic Microwave Background Temperature and Polarization
• Probing neutrino physics with a self-consistent treatment of the weak decoupling, nucleosynthesis, and photon decoupling epochs
• Gravitational Lensing of Cosmological 21cm Emission
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• Physics of the cosmic microwave background anisotropy
• Bayesian Inference of Initial Conditions from Non-Linear Cosmic Structures using Field-Level Emulators
• Extracting cosmological parameters from N-body simulations using machine learning techniques
• An interacting New Holographic Dark Energy in the framework of fractal cosmology
• CMB B-mode non-Gaussianity: optimal bispectrum estimator and Fisher forecasts
• Peculiar velocities into the next generation: cosmological parameters from the SFI++ survey
• What sets the splashback radius of dark matter haloes: accretion history or other properties?
• Hint of a truncated primordial spectrum from the CMB large-scale anomalies
• Analytical and EZmock covariance validation for the DESI 2024 results
• Probing for the Cosmological Parameters with PLANCK Measurement
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Light Fields during Inflation from BOSS and Future Galaxy Surveys
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• Cosmological consequences of classical flavor-space locked gauge field radiation
• Is Dynamical Dark Energy Necessary? DESI BAO and Modified Recombination
• A search for sterile neutrinos in interacting dark energy models using DESI baryon acoustic oscillations and DES supernovae data
• Inflationary Tensor Perturbations After BICEP
• Consistency of cosmic shear analyses in harmonic and real space
• Using Cross-Correlations to Calibrate Lensing Source Redshift Distributions: Improving Cosmological Constraints from Upcoming Weak Lensing Surveys
• Fast simulations of cosmic large-scale structure with massive neutrinos
• CMB constraints on a physical model of reionization
• Constraining holographic inflation with WMAP
• KaRMMa -- Kappa Reconstruction for Mass Mapping
• Radiative transfer effects in primordial hydrogen recombination
• RELIKE: Reionization Effective Likelihood from Planck 2018 Data
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck I: Construction of CMB Lensing Maps and Modeling Choices
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• Observational Constraints on Warm Inflation in Loop Quantum Cosmology
• The two and three-loop matter bispectrum in perturbation theories
• Large-scale 3D mapping of the intergalactic medium using the Lyman Alpha Forest
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• The triply-ionized carbon forest from eBOSS: cosmological correlations with quasars in SDSS-IV DR14
• Constraints on perturbations to the recombination history from measurements of the CMB damping tail
• The Impact of Nonlinear Structure Formation on the Power Spectrum of Transverse Momentum Fluctuations and the Kinetic Sunyaev-Zel'dovich Effect
• Cosmological constraints on the Multi Scalar Field Dark Matter model
• Data-constrained reionization and its effects on cosmological parameters
• Revisiting a pre-inflationary radiation era and its effect on the CMB power spectrum
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• The galaxy-galaxy lensing contribution to the cosmic shear two point function
• Phenomenological models for Unified Dark Matter with fast transition
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• Cosmological Tests of Everpresent $\Lambda$
• Scrutinizing Various Phenomenological Interactions In The Context Of Holographic Ricci Dark Energy Models
• The HI intensity mapping bispectrum including observational effects
• The FLAMINGO project: Baryon effects on the matter power spectrum
• On the running of the spectral index to all orders: a new model dependent approach to constrain inflationary models
• Weak lensing with 21cm intensity mapping at $z\sim 2-3$
• Relic gravitational waves: latest revisions and preparations for new data
• Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies
• Constraints on CDM cosmology from galaxy power spectrum, CMB and SNIa evolution
• CMB distortion anisotropies due to the decay of primordial magnetic fields
• Cosmological parameter constraints from CMB lensing with cosmic voids
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• The cosmic neutrino background as a collection of fluids in large-scale structure simulations
• The WIRCam Deep Survey II: Mass Selected Clustering
• A Bayesian method for combining theoretical and simulated covariance matrices for large-scale structure surveys
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• Confronting DGP Braneworld Gravity with Cosmic Observations after Planck Data
• A Dark Energy model from Generalized Proca Theory
• Neural networks as optimal estimators to marginalize over baryonic effects
• On the growth of perturbations in interacting dark energy and dark matter fluids
• Beyond CMB cosmic variance limits on reionization with the polarized SZ effect
• Phase-space structure of cold dark matter halos inside splashback: multi-stream flows and self-similar solution
• Constraining Sterile Neutrino Cosmology with Terrestrial Oscillation Experiments
• Dark energy perturbations in $N$-body simulations
• Fitting and forecasting non-linear coupled dark energy
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Characterizing fast radio bursts through statistical cross-correlations
• Impacts of Dark Stars on Reionization and Signatures in the Cosmic Microwave Background
• Inflationary generalized Chaplygin gas and dark energy in the light of the Planck and BICEP2 experiments
• Should we doubt the cosmological constant?
• Generation of Curvature Perturbations with Extra Anisotropic Stress
• Constraints on Superconducting Cosmic Strings from Early Reionization
• Constraining holographic cosmology using Planck data
• On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
• General relativistic effects on non-linear power spectra
• Chiral Imprint of a Cosmic Gauge Field on Primordial Gravitational Waves
• Constraints on Primordial Power Spectrum from Galaxy Luminosity Functions
• Velocity reconstruction with the cosmic microwave background and galaxy surveys
• Studying cosmic reionization with observations of the global 21-cm signal
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• Model Independent Early Expansion History and Dark Energy
• Pre-inflationary genesis with CMB B-mode polarization
• Magnetic field generation from primordial black hole distributions
• Efficient calculation of cosmological neutrino clustering with both linear and non-linear gravity
• Smallest Remnants of Early Matter Domination
• Back to the features: assessing the discriminating power of future CMB missions on inflationary models
• Shot noise and scatter in the star formation efficiency as a source of 21-cm fluctuations
• A Constraint On the Integrated Mass Power Spectrum out to z = 1100 from Lensing of the Cosmic Microwave Background
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Modified recombination and the Hubble tension
• Observational constraints on $\alpha$-attractor inflationary models with a Higgs-like potential
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• Cumulative Neutrino and Gamma-Ray Backgrounds from Halo and Galaxy Mergers
• Weak lensing of large scale structure in the presence of screening
• The e-MANTIS emulator: fast predictions of the non-linear matter power spectrum in $f(R)$CDM cosmology
• Dwarf Spheroidal Satellite Formation in a Reionized Local Group
• Observational signatures of a non-singular bouncing cosmology
• Does Planck 2015 polarization favor high redshift reionization?
• Scaling defect decay and the reionization history of the Universe
• BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn
• Constraining f(R) Gravity with Planck Sunyaev-Zel'dovich Clusters
• Cosmological Vlasov-Poisson Simulations of Structure Formation with Relic Neutrinos: Nonlinear Clustering and the Neutrino Mass
• Wiener filter reloaded: fast signal reconstruction without preconditioning
• Perturbation theory with dispersion and higher cumulants: non-linear regime
• Optimal filtering for CMB lensing reconstruction
• Can primordial parity violation explain the observed cosmic birefringence?
• Baryonic effects on CMB lensing and neutrino mass constraints
• Likelihood-free Inference with Mixture Density Network
• Host Dark Matter Halos of WISE-selected Obscured & Unobscured Quasars: Evidence for Evolution
• 50 Years of Horndeski Gravity: Past, Present and Future
• Probing the primordial universe with gravitational waves detectors
• Small-scale primordial fluctuations in the 21cm Dark Ages signal
• Probing dynamics of dark energy with latest observations
• Update constraints on neutrino mass and mass hierarchy in light of dark energy models
• Constraints on ionising photon production from the large-scale Lyman-alpha forest
• Improved constraints on reionisation from CMB observations: A parameterisation of the kSZ effect
• Optimal constraints on primordial gravitational waves from the lensed CMB
• Cosmographic Footprints of Dynamical Dark Energy
• Inevitable imprints of patchy reionization on the cosmic microwave background anisotropy
• Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure
• Improving Fisher matrix forecasts for galaxy surveys: window function, bin cross-correlation, and bin redshift uncertainty
• COWS: A filament finder for Hessian cosmic web identifiers
• Non-Gaussian Error in Galaxy Survey (Part 1)
• Expansion-history preferences of DESI DR2 and external data
• Analyzing clustering of astrophysical gravitational-wave sources: Luminosity-distance space distortions
• Bulk flow in the combined 2MTF and 6dFGSv surveys
• Non-Gaussian isocurvature perturbations in dark radiation
• Probing the statistical properties of CMB $B$-mode polarization through Minkowski Functionals
• Primordial polymer perturbations
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• Precise Measurement of the Radial Baryon Acoustic Oscillation Scales in Galaxy Redshift Surveys
• CosmoFlow: Python Package for Cosmological Correlators
• LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
• Tensor perturbations during inflation in a spatially closed Universe
• Inflationary vs. Reionization Features from Planck 2015 Data
• Resurrecting the Power-law, Intermediate, and Logamediate Inflations in the DBI Scenario with Constant Sound Speed
• PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass
• Forecasts on the contamination induced by unresolved point sources in primordial non-Gaussianity beyond Planck
• Effect of Measurement Errors on Predicted Cosmological Constraints from Shear Peak Statistics with LSST
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• Cosmic birefringence tomography with polarized Sunyaev Zel'dovich effect
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• A new pressure-parametrization unified dark fluid model
• Non-Gaussian Structure of B-mode Polarization after Delensing
• Multi-tracer power spectra and bispectra: Formalism
• Effects of CMB temperature uncertainties on cosmological parameter estimation
• Cosmological Information in the Gravitational Lensing of Pregalactic HI
• Non-Gaussianity of secondary anisotropies from ACTPol and Planck
• Planck Satellite Constraints on Pseudo-Nambu--Goldstone Boson Quintessence
• Optimal ISW detection and joint likelihood for cosmological parameter estimation
• Detecting Primordial $B$-Modes after Planck
• Early dark energy and its interaction with dark matter
• KiDS-1000 Cosmology: machine learning -- accelerated constraints on Interacting Dark Energy with COSMOPOWER
• Multi-Scale Pipeline for the Search of String-Induced CMB Anisotropies
• Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
• Living with Neighbors. II. Statistical Analysis of Flybys and Mergers of Dark Matter Halos in Cosmological Simulations
• On the peculiar momentum of baryons after Reionization
• Principal component analysis of the primordial tensor power spectrum
• A framework for testing isotropy with the cosmic microwave background
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• Cross-correlating 2D and 3D galaxy surveys
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• $\alpha$-attractor inflation: Models and predictions
• Effect of Template Uncertainties on the WMAP and Planck Measures of the Optical Depth Due To Reionization
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Cosmological Constraints on Dissipative Models of Inflation
• Group-galaxy correlations in redshift space as a probe of the growth of structure
• Modelling the matter bispectrum at small scales in modified gravity
• Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
• Probing spatial variation of the fine-structure constant using the CMB
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Statistical Properties of Radio Halos in Galaxy Clusters and Origin of Seed Electrons for Reacceleration
• A precise symbolic emulator of the linear matter power spectrum
• Measuring the Hubble function with standard candle clustering
• Black hole formation and growth with non-Gaussian primordial density perturbations
• Signatures of Cosmic Ray Heating in 21-cm Observables
• Photometric Selection of Emission Line Galaxies, Clustering Analysis and a Search for the ISW effect
• Amending the halo model to satisfy cosmological conservation laws
• The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2\le z<1$ by PDF analysis
• Hydrodynamical structure formation in Milgromian cosmology
• Massive neutrinos and degeneracies in Lyman-alpha forest simulations
• Non-Gaussianity in WMAP Data Due to the Correlation of CMB Lensing Potential with Secondary Anisotropies
• The traces of anisotropic dark energy in light of Planck
• Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
• Unified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing
• Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics
• Redshift-space distortions from the cross-correlation of photometric populations
• Hybrid Natural Inflation
• Single frequency CMB B-mode inference with realistic foregrounds from a single training image
• Expectation of primordial gravity waves generated during inflation
• Removing BAO-peak Shifts with Local Density Transforms
• Blind Observers of the Sky
• Constraints on general primordial non-Gaussianity using wavelets for the Wilkinson Microwave anisotropy probe 7-year data
• Quintessential Scale Dependence from Separate Universe Simulations
• Cosmological parameter inference from galaxy clustering: The effect of the posterior distribution of the power spectrum
• Fast Analytic Computation of Cosmic String Power Spectra
• Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• Neutrinos in Non-linear Structure Formation - a Simple SPH Approach
• Harrison-Z'eldovich primordial spectrum is consistent with observations
• EDGE: A new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation
• Large scale CMB anomalies from thawing cosmic strings
• Mass Estimation of Galaxy Clusters with Deep Learning II: CMB Cluster Lensing
• Modelling non-dust fluids in cosmology
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• Prospects for 21cm-Galaxy Cross-Correlations with HERA and the Roman High-Latitude Survey
• Constraining gravity at large scales with the 2MASS Photometric Redshift catalogue and Planck lensing
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• Detectability of large-scale power suppression in the galaxy distribution
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• A hybrid approach to CMB lensing reconstruction on all-sky intensity maps
• Linear effects of perturbed recombination
• Properties and uncertainties of scalar field models of dark energy with barotropic equation of state
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• Modified theory of gravity and the history of cosmic evolution
• Constraints on Modified Gravity from Sunyaev-Zeldovich Cluster Surveys
• Time variation of the fine structure constant in the early universe and the Bekenstein model
• Constraints on neutrino density and velocity isocurvature modes from WMAP-9 data
• Measurement of Redshift Space Power Spectrum for BOSS galaxies and the Growth Rate at redshift 0.57
• Phenomenological approaches of inflation and their equivalence
• Impact of general reionization scenarios on extraction of inflationary parameters
• Testing parity-violating physics from cosmic rotation power reconstruction
• Cosmic microwave background anisotropies in the timescape cosmology
• Systematic uncertainties in models of the cosmic dawn
• Weak Lensing Effects on the Galaxy Three-Point Correlation Function
• Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
• Reconstructing Patchy Reionization with Deep Learning
• Blind component separation for polarized observations of the CMB
• Perturbed Recombination from Dark Matter Annihilation
• Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2
• Light Sterile Neutrinos and Inflationary Freedom
• Cosmology from weak lensing alone and implications for the Hubble tension
• Cold dark energy constraints from the abundance of galaxy clusters
• Matter Distribution around Galaxies
• The Impact of Non-Gaussianity upon Cosmological Forecasts
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Dynamical Background
• Screening in perturbative approaches to LSS
• A Simple Proposal for Radial 3D Needlets
• Inflationary Potential from 21 cm Tomography and Planck
• Phase decoherence of gravitational wave backgrounds
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Cosmological measurements from void-galaxy and galaxy-galaxy clustering in the Sloan Digital Sky Survey
• Growth-rate measurement with type-Ia supernovae using ZTF survey simulations
• The very wide-field $gzK$ galaxy survey -- I. Details of the clustering properties of star-forming galaxies at $z\sim 2$
• Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
• Parameter Estimation from Improved Measurements of the CMB from QUaD
• Estimating the bispectrum of the Very Small Array data
• Constraints on features in the inflationary potential from future Euclid data
• Photons and Baryons before Atoms: Improving the Tight-Coupling Approximation
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Imprints of Reionization in Galaxy Clustering
• Constraining Reionization in Progress at z=5.7 with Lyman-$\alpha$ Emitters: Voids, Peaks, and Cosmic Variance
• Characterizing unknown systematics in large scale structure surveys
• No evidence for dynamical dark energy in two models
• Wiener filtering and pure E/B decomposition of CMB maps with anisotropic correlated noise
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Constraints on decaying early modified gravity from cosmological observations
• Neutrino mass effects on vector and tensor CMB anisotropies in the presence of a primordial magnetic field
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• Extreme data compression for the CMB
• Born-corrections to weak lensing of the cosmic microwave background temperature and polarisation anisotropies
• Multipoles of the relativistic galaxy bispectrum
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Evidence for horizon-scale power from CMB polarization
• Parity violation in pre-inflationary bounce
• Breaking Be: a sterile neutrino solution to the cosmological lithium problem
• Compatibility of JWST results with exotic halos
• Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum
• Beyond $\Lambda$CDM with HI intensity mapping: robustness of cosmological constraints in the presence of astrophysics
• Signatures of Modified Gravity on the 21-cm Power Spectrum at Reionisation
• What is the amplitude of the Gravitational Waves background expected in the Starobinsky model ?
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Can $f(R)$ gravity relieve $H_0$ and ${\sigma }_8$ tensions?
• Measuring gravitational lensing of the cosmic microwave background using cross correlation with large scale structure
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• The Evolution of the Cosmic Microwave Background
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• Improved model-independent constraints on the recombination era and development of a direct projection method
• Time variation of the electron mass in the early universe and the Barrow-Magueijo model
• Conservative Estimates of the Mass of the Neutrino from Cosmology
• Spatial and temporal tuning in void models for acceleration
• Raytracing simulations of coupled dark energy models
• On the impact of large angle CMB polarization data on cosmological parameters
• An Accurate Analytic Model for the Thermal Sunyaev-Zel'dovich One-Point PDF
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys
• Constraining the primordial curvature perturbation using dark matter substructure
• Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach
• CoLFI: Cosmological Likelihood-free Inference with Neural Density Estimators
• A simulation-based inference pipeline for cosmic shear with the Kilo-Degree Survey
• Constraints on ultra-slow-roll inflation from the third LIGO-Virgo observing run
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• DeepSZ: Identification of Sunyaev-Zel'dovich Galaxy Clusters using Deep Learning
• Delensing the CMB with the cosmic infrared background: the impact of foregrounds
• Reconstructing Quintessence
• Theoretical and numerical perspectives on cosmic distance averages
• Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
• Informing dark matter direct detection limits with the ARTEMIS simulations
• Matter Power Spectrum of Light Freeze-in Dark Matter: With or without Self-Interaction
• Joining bits and pieces of reionization history
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
• Modeling the large-scale power deficit with smooth and discontinuous primordial spectra
• The Cross-correlation of KSZ Effect and 21 cm Intensity Mapping with Tidal Reconstruction
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Stability and the Gauge Problem in Non-Perturbative Cosmology
• A Hint of a Blue Axion Isocurvature Spectrum?
• Constraints on running vacuum model with $H(z)$ and $f{\sigma }_8$
• Probing the Neutrino Mass Hierarchy beyond $\Lambda$CDM Model
• Increasing Fisher Information by Moving-Mesh Reconstruction
• Robust predictions for an oscillatory bispectrum in Planck 2015 data from transient reductions in the speed of sound of the inflaton
• Consistency of the Planck CMB data and $\Lambda$CDM cosmology
• New observational limits on dark radiation in brane-world cosmology
• Testing physical models for dipolar asymmetry: from temperature to k space to lensing
• The dark matter dispersion tensor in perturbation theory
• Imprint of Inhomogeneous and Anisotropic Primordial Power Spectrum on CMB Polarization
• Small scale clustering of late forming dark matter
• The Komatsu Spergel Wandelt estimator for oscillations in the cosmic microwave background bispectrum
• Cosmological parameter estimation from CMB and X-ray clusters after Planck
• Neutrinos and dark energy constraints from future galaxy surveys and CMB lensing information
• Quintessence versus phantom dark energy: the arbitrating power of current and future observations
• Cosmic microwave background constraints on light dark matter candidates
• Observational constraints on scalar field models of dark energy with barotropic equation of state
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• Relic gravitational waves in the light of 7-year Wilkinson Microwave Anisotropy Probe data and improved prospects for the Planck mission
• Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters
• Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot
• Evolution of skewness and kurtosis of cosmic density fields
• A null test to probe the scale-dependence of the growth of structure as a test of General Relativity
• Future CMB ISW-Lensing bispectrum constraints on modified gravity in the Parameterized Post-Friedmann formalism
• Cosmological forecasts on thermal axions, relic neutrinos and light elements
• Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
• Revisiting the matter power spectra in $f(R)$ gravity
• Current constraints on early and stressed dark energy models and future 21 cm perspectives
• A novel model-marginalized cosmological bound on the QCD axion mass
• Forecasting neutrino masses from galaxy clustering in the Dark Energy Survey combined with the Planck Measurements
• Lensing Bias to CMB Measurements of Compensated Isocurvature Perturbations
• Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis
• An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators
• Probing the Seesaw Mechanism with Cosmological Data
• B polarization of cosmic background radiation from second-order scattering sources
• Ballistic Dark Matter oscillates above $\Lambda$CDM
• Computation approach for CMB bispectrum from primordial magnetic fields
• The 6x2pt method: supernova velocities meet multiple tracers
• The abundance of dark matter haloes down to Earth mass
• An HI intensity mapping survey with a Phased Array Feed
• Structure formation in a mixed dark matter model with decaying sterile neutrino: the 3.5 keV X-ray line and the Galactic substructure
• A cosmic glitch in gravity
• Constraints on a scale-dependent bias from galaxy clustering
• ELG Spectroscopic Systematics Analysis of the DESI Data Release 1
• Galaxy clustering with photometric surveys using PDF redshift information
• Constraining the topology of the Universe using the polarised CMB maps
• Galilean invariant resummation schemes of cosmological perturbations
• Differentiating dark interactions with perturbation
• CMB Mode Coupling with Isotropic Polarization Rotation
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Covariance of the redshift-space matter power spectrum after reconstruction
• Nonlinear matter spectra in growing neutrino quintessence
• Constraining cosmology with pairwise velocity estimator
• Adiabatic regularization of power spectrum and stress tensor of relic gravitational wave without low-frequency distortion
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• Combined constraints on deviations of dark energy from an ideal fluid from Euclid and Planck
• Estimating Cosmological Parameters from the Dark Matter Distribution
• Optimal bispectrum estimator and simulations of the the CMB Lensing-ISW non-Gaussian signal
• Large-scale structure in mimetic Horndeski gravity
• Virial halo mass function in the $Planck$ cosmology
• Constraining Cosmic Expansion and Gravity with Galaxy Redshift Surveys
• General CMB bispectrum analysis using wavelets and separable modes
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• General quadrupolar statistical anisotropy: Planck limits
• Dark Energy Constraints in light of Pantheon SNe Ia, BAO, Cosmic Chronometers and CMB Polarization and Lensing Data
• Weak lensing probe of cubic Galileon model
• Maximum Entropy deconvolution of Primordial Power Spectrum
• Probing Primordial Non-Gaussianity with Weak Lensing Minkowski Functionals
• Large Scale Structure Forecast Constraints on Particle Production During Inflation
• Spectral distortions in the cosmic microwave background polarization
• The PAU survey: Ly$\alpha$ intensity mapping forecast
• KiDS-1000: cross-correlation with Planck cosmic microwave background lensing and intrinsic alignment removal with self-calibration
• On general features of warm dark matter with reduced relativistic gas
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• Reconstruction of primordial tensor power spectra from B-mode polarization of the cosmic microwave background
• The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
• Constraining quantum collapse inflationary models with CMB data
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Euclid: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Neutrino mass tension or suppressed growth rate of matter perturbations?
• Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimation
• Baryon Physics and Tight Coupling Approximation in Boltzmann Codes
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• Cosmologically probing ultra-light particle dark matter using 21 cm signals
• Bubble mapping with the Square Kilometer Array -- I. Detecting galaxies with Euclid, JWST, WFIRST and ELT within ionized bubbles in the intergalactic medium at z>6
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Direct cosmological inference from three-dimensional correlations of the Lyman-$\alpha$ forest
• On the amount of peculiar velocity field information in supernovae from LSST and beyond
• Searching for Signatures of Cosmic Superstrings in the CMB
• Combining gravitational lensing and gravitational redshift to measure the anisotropic stress with future galaxy surveys
• Cosmological Constraints on the Higgs Boson Mass
• Level Crossing Analysis of Cosmic Microwave Background Radiation: A method for detecting cosmic strings
• Probing higher-spin fields from inflation with higher-order statistics of the CMB
• Probing Large-Angle Correlations with the Microwave Background Temperature and Lensing Cross Correlation
• Dark Matter Annihilation into Four-Body Final States and Implications for the AMS Antiproton Excess
• Probing Reionization and Early Cosmic Enrichment with the MgII Forest
• Validating the Fisher approach for stage IV spectroscopic surveys
• Confronting Kähler moduli inflation with CMB data
• The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ~0.7
• Patchy Screening of the CMB from Dark Photons
• Thawing Versus. Tracker Behaviour: Observational Evidence
• Internal dark matter structure of the most massive galaxy clusters
• CMB probes on the correlated axion isocurvature perturbation
• Cosmic Flow Measurement and Mock Sampling Algorithm of Cosmicflows-4 Tully-Fisher Catalogue
• Testing Alternative Theories of Dark Matter with the CMB
• Bispectrum as Baryon Acoustic Oscillation Interferometer
• Cubic Derivative Interactions and Asymptotic Dynamics of the Galileon Vacuum
• Consistent Cosmic Microwave Background Spectra from Quantum Depletion
• Weak Lensing Science, Surveys, and Systematics
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• Simultaneous Constraints on Cosmology and Photometric Redshift Bias from Weak Lensing and Galaxy Clustering
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Implications of bias evolution on measurements of the integrated Sachs-Wolfe effect: errors and biases in parameter estimation
• Testing distance duality with CMB anisotropies
• Probing for Dynamics of Dark-Energy in Mass Varying Neutrinos: Cosmic Microwave Background Radiation and Large Scale Structure
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Sunyaev-Zel'dovich Cluster Survey Simulations for Planck
• CMB anomalies and the effects of local features of the inflaton potential
• Constraining quantum collapse inflationary models with current data: The semiclassical approach
• Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae
• Observational constraints of an anisotropic boost due to the projection effects using redMaPPer clusters
• Cosmology with Peculiar Velocities: Observational Effects
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• Linking the BICEP2 result and the hemispherical power asymmetry through spatial variation of $r$
• Effects of local features of the inflaton potential on the spectrum and bispectrum of primordial perturbations
• Effect of supersonic relative motion between baryons and dark matter on collapsed objects
• A minimal empirical model for the cosmic far-infrared background anisotropies
• CMB with the background primordial magnetic field
• Cosmological Constraints on 4-Dimensional Einstein-Gauss-Bonnet Gravity
• 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
• Generalized Uncertainty Principle mimicking dynamical Dark Energy: matter perturbations and gravitational wave data analysis
• Bayesian angular power spectrum analysis of interferometric data
• Supersonic baryon-CDM velocities and CMB B-mode polarization
• Delayed Recombination and Standard Rulers
• High-resolution CMB bispectrum estimator with flexible modal basis
• Universal Weak Lensing Distortion of Cosmological Correlation Functions
• Uncorrelated estimates of the primordial power spectrum
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
• Impact of the damping tail on neutrino mass constraints
• Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
• Imprint of spatial curvature on inflation power spectrum
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• Primordial power spectrum features in phenomenological descriptions of inflation
• Test of consistency between Planck and WMAP
• Constraining cosmic string parameters with curl mode of CMB lensing
• Testing model independent modified gravity with future large scale surveys
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• Linear and non-linear perturbations in dark energy models
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Aspects of Dark Matter Annihilation in Cosmology
• Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Neutrino footprint in Large Scale Structure
• Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
• Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables
• Transitioning from Stage-III to Stage-IV: Cosmology from galaxy$\times$CMB lensing and shear$\times$CMB lensing
• The RayGalGroupSims cosmological simulation suite for the study of relativistic effects: an application to lensing-matter clustering statistics
• Cosmic microwave background polarization analysis
• Speeding Up Cosmological Boltzmann Codes
• Distinguishing between $\Lambda$CDM and $f(R)$ gravity models using halo ellipticity correlations in simulations
• Prospects for kSZ${}^2$-Galaxy Cross-Correlations during Reionization
• Cosmic microwave background with Brans-Dicke Gravity: I. Covariant Formulation
• Limits on Brane-World and Particle Dark Radiation from Big Bang Nucleosynthesis and the CMB
• Semi-blind Bayesian inference of CMB map and power spectrum
• New model of axion monodromy inflation and its cosmological implications
• Decomposing CMB lensing power with simulation
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Theoretical and observational constraints on Tachyon Inflation
• On the total cosmological information in galaxy clustering: an analytical approach
• Initial conditions for cosmological N-body simulations of the scalar sector of theories of Newtonian, Relativistic and Modified Gravity
• Lensing covariance on cut sky and SPT-Planck lensing tensions
• The Impact of Anisotropic Redshift Distributions on Angular Clustering
• 3D cosmic shear: numerical challenges, 3D lensing random fields generation and Minkowski Functionals for cosmological inference
• Cluster Probes of Dark Energy Clustering
• An analytic approach to baryon acoustic oscillations
• Testing Gaussianity on Archeops Data
• Constraining Dark Energy With Stacked Concave Lenses
• Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
• First comprehensive constraints on the Finslerian models using cosmological observations
• Characterising the Structure of Halo Merger Trees Using a Single Parameter: The Tree Entropy
• Model independent approaches to reionization in the analysis of upcoming CMB data
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Fibre inflation and precision CMB data
• Structural properties of artificial halos in non-standard dark matter simulations
• Real space estimator for the weak lensing convergence from the CMB
• A generalized method of constraining Warm Inflation with CMB data
• Growth of non-linear structures and spherical collapse in the Galileon Ghost Condensate model
• Role of ionizing background on the statistics of metal absorbers in hydrodynamical simulations
• Anisotropic CMB distortions from non-Gaussian isocurvature perturbations
• Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
• Planck and reionization history: a model selection view
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• Chasing cosmic inflation: constraints for inflationary models and reheating insights
• Lorentz invariance violation in the neutrino sector: a joint analysis from big bang nucleosynthesis and the cosmic microwave background
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• The effects on CMB power spectra and bispectra from the polarization rotation and its correlations with temperature and E-polarization
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• Rotation of the CMB polarisation by foreground lensing
• Quantifying the CMB Degeneracy Between the Matter Density and Hubble Constant in Current Experiments
• Brane inflation and the robustness of the Starobinsky inflationary model
• Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
• Observing trans-Planckian ripples in the primordial power spectrum with future large scale structure probes
• Weighing neutrinos in the presence of a running primordial spectral index
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Generalized Brans-Dicke theories in light of evolving dark energy
• A numerical study of observational systematic errors in lensing analysis of CMB polarization
• Non-minimally coupled gravity constraints from DESI DR2 data
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• CMB lensing reconstruction using cut sky polarization maps and pure-$B$ modes
• Peak-peak correlations in the cosmic background radiation from cosmic strings
• CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations
• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• Edges and Endpoints in 21-cm Observations from Resonant Photon Production
• Generation of magnetic fields in Einstein-Aether gravity
• Cosmology from the kinetic polarized Sunyaev Zel'dovich effect
• Role of the Hubble Scale in the Weak Lensing vs. CMB Tension
• Constraining the WMAP9 bispectrum and trispectrum with needlets
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Using machine learning to compress the matter transfer function $T(k)$
• Real space lensing reconstruction using cosmic microwave background polarization
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs
• An empirical approach to model selection: weak lensing and intrinsic alignments
• Investigating clustering dark energy with 3d weak cosmic shear
• GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part II. Initial conditions
• Estimating the tensor-to-scalar ratio and the effect of residual foreground contamination
• Hints of Primordial Magnetic Fields at Recombination and Implications for the Hubble Tension
• A dark energy view of inflation
• Cosmological constraints on sterile neutrino oscillations from Planck
• Linear Systematics Mitigation in Galaxy Clustering in the Dark Energy Survey Year 1 Data
• Bayesian evidence of non-standard inflation: isocurvature perturbations and running spectral index
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• Combined cosmological tests of a bivalent tachyonic dark energy scalar field model
• Small scale contributions to CMB: A coherent analysis
• The ISW effect and the lack of large-angle CMB temperature correlations
• Optimal Weights For Measuring Redshift Space Distortions in Multi-tracer Galaxy Catalogues
• Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
• Biases on cosmological parameter estimators from galaxy cluster number counts
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• Enhanced n-body annihilation of dark matter and its indirect signatures
• Accurate field-level weak lensing inference for precision cosmology
• Was there an early reionization component in our universe?
• Is gravity getting weaker at low z? Observational evidence and theoretical implications
• Dynamics of minimally coupled dark energy in spherical halos of dark matter
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• Predicted Constraints on Cosmic String Tension from Planck and Future CMB Polarization Measurements
• Beyond optical depth: Future determination of ionization history from the CMB
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Mimetic DBI Inflation in Confrontation with Planck2018 data
• Probing gaseous galactic halos through the rotational kSZ effect
• Galactic Faraday rotation effect on polarization of 21 cm lines from the epoch of reionization
• Hierarchical Bayesian CMB Component Separation with the No-U-Turn Sampler
• Predictions for the 21cm-galaxy cross-power spectrum observable with SKA and future galaxy surveys
• Separating the Intrinsic Alignment Signal and the Lensing Signal using Self-Calibration in Photo-z Surveys with KiDS450 and KV450 Data
• A galaxy-free phenomenological model for the 21-cm power spectrum during reionization
• Is patchy reionization an obstacle in detecting the primordial gravitational wave signal?
• Impact of Massive Neutrinos and Dark Radiation on the High-redshift Cosmic Web. I. Lyman-Alpha Forest Observables
• Application of cross correlations between CMB and large scale structure to constraints on the primordial non-Gaussianity
• Vector modes in $\Lambda$CDM: the gravitomagnetic potential in dark matter haloes from relativistic $N$-body simulations
• Constraints on Cubic and $f(P)$ Gravity from the Cosmic Chronometers, BAO & CMB datasets : Use of Machine Learning Algorithms
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Boltzmann hierarchies for self-interacting warm dark matter scenarios
• What initial condition of inflation would suppress the large-scale CMB spectrum?
• Constraining dynamical neutrino mass generation with cosmological data
• Correlations between 21 cm Radiation and the CMB from Active Sources
• Lensing impact on cosmic relics and tensions
• Third-order corrections to the slow-roll expansion: calculation and constraints with Planck, ACT, SPT, and BICEP/Keck
• Reconstructing Cosmic Polarization Rotation with ResUNet-CMB
• Constraints on single-field inflation with WMAP, SPT and ACT data -- A last-minute stand before Planck
• Expected constraints on the Galactic magnetic field using PLANCK data
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Baryonic feedback measurement from KV450 cosmic shear analysis
• The Music of the Aetherwave - B-mode Polarization in Einstein-Aether Theory
• A revised density split statistic model for general filters
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Material models of dark energy
• Testing the conditional mass function of dark matter halos against numerical N-body simulations
• Fingers-of-God effect of infalling satellite galaxies
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• CMB-S4 forecast on the primordial non-Gaussianity parameter of feature models
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Joint Bayesian analysis of large angular scale CMB temperature anomalies
• Inpainting CMB maps using Partial Convolutional Neural Networks
• BAO Modulation as a Probe of Compensated Isocurvature Perturbations
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• The impact of spurious shear on cosmological parameter estimates from weak lensing observables
• Dark sector evolution in Horndeski models
• Host Dark Matter Halos of SDSS Red and Blue Quasars: No Significant Difference in Large-scale Environment
• Constraints on Generalized Dark Energy from Recent Observations
• Reconstruction of Gravitational Lensing Using WMAP 7-Year Data
• Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
• Structure Formation in Various Dynamical Dark Energy Scenarios
• The Impact of the Spectral Response of an Achromatic Half-Wave Plate on the Measurement of the Cosmic Microwave Background Polarization
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• Mass-varying neutrino in light of cosmic microwave background and weak lensing
• Low-$\ell$ power suppression in punctuated inflation
• Detection and Removal of B-mode Dust Foregrounds with Signatures of Statistical Anisotropy
• Reionization in the dark and the light from Cosmic Microwave Background
• Interpreting the cosmic far-infrared background anisotropies using a gas regulator model
• Constraining cluster masses from the stacked phase space distribution at large radii
• Primordial gravitational wave phenomenology with polarized Sunyaev Zel'dovich tomography
• Measuring the Expansion of the Universe Through Changes in the CMB Photosphere
• Integrated Sachs-Wolfe map reconstruction in the presence of systematic errors
• Observational constraints on the energy scale of inflation
• Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
• Imprint of a Steep Equation of State in the growth of structure
• Lensing-induced morphology changes in CMB temperature maps in modified gravity theories
• From heaviness to lightness during inflation
• Exact joint likelihood of pseudo-$C_{\ell }$ estimates from correlated Gaussian cosmological fields
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• Gamma-rays From Warm WIMP Dark Matter Annihilation
• CMB polarization as a tool to constrain the optical properties of the Universe
• Weighing neutrinos in $f(R)$ gravity in light of BICEP2
• Revisiting constraints on (pseudo)conformal Universe with Planck data
• Primordial power spectrum of tensor perturbations in Finsler spacetime
• The ALHAMBRA survey : Estimation of the clustering signal encoded in the cosmic variance
• Probing Oscillons of Ultra-Light Axion-like Particle by 21cm Forest
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• Clustering of CODEX clusters
• Confronting Dark Energy Anisotropic Stress
• Uneven flows: On cosmic bulk flows, local observers, and gravity
• Mixed three-point correlation functions of the nonlinear integrated Sachs-Wolfe effect and their detectability
• How CMB and large-scale structure constrain chameleon interacting dark energy
• Lensing smoothing of BAO wiggles
• Towards a Solution to the H0 Tension: the Price to Pay
• Sensitivity tests of cosmic velocity fields to massive neutrinos
• Combining spectroscopic and photometric surveys using angular cross-correlations I: Algorithm and modelling
• The Physical Origin of Dark Energy Constraints from Rubin Observatory and CMB-S4 Lensing Tomography
• Constraining the neutrino mass using a multi-tracer combination of two galaxy surveys and CMB lensing
• Cosmological Constraints from Weak Lensing Peaks: Can Halo Models Accurately Predict Peak Counts?
• Effect of damped oscillations in the inflationary potential
• Spatial curvature sensitivity to local $H_0$ from the Cepheid distance ladder
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Constraints on a special running vacuum model
• Constraining IGM enrichment and metallicity with the C IV forest correlation function
• Optimizing future experiments of cosmic far-infrared background: a principal component approach
• The $n$-point streaming model: how velocities shape correlation functions in redshift space
• Log-transforming the matter power spectrum
• Monopole Fluctuation of the CMB and its Gauge Invariance
• Mock halo catalogs: assigning unresolved halo properties using correlations with local halo environment
• Probing early structure and model-independent neutrino mass with high-redshift CMB lensing mass maps
• Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models
• Constraining the reionization history with CMB and spectroscopic observations
• On the accuracy of N-body simulations at very large scales
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Wide-angle effects in the galaxy bispectrum
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4
• Euclid: Covariance of weak lensing pseudo-$C_{\ell }$ estimates. Calculation, comparison to simulations, and dependence on survey geometry
• Role of spatial curvature in the primordial gravitational wave power spectrum
• ISW effect as probe of features in the expansion history of the Universe
• Cosmic topology. Part IIa. Eigenmodes, correlation matrices, and detectability of orientable Euclidean manifolds
• Nonlinear stochastic biasing of halos: Analysis of cosmological N-body simulations and perturbation theories
• Testing the nature of Dark Energy with Precision Cosmological constraints
• Nested solitons in two-field fuzzy dark matter
• Constraints on the Tensor-to-Scalar ratio for non-power-law models
• Non-Gaussian Shape Recognition
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• Accuracy requirements on intrinsic alignments for Stage-IV cosmic shear
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Measuring neutrino masses with joint JWST and DESI DR2 data
• DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
• Extended analysis of CMB constraints on non-Gaussianity in isocurvature perturbations
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Dimensionless cosmology
• Dark Energy Survey Year 3: Blue Shear
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• Baryon Acoustic Oscillations in the Lyman Alpha Forest
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Projection effects of large-scale structures on weak-lensing peak abundances
• Morphology of CMB fields -- effect of weak gravitational lensing
• The ALHAMBRA survey: evolution of galaxy spectral segregation
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• Joint analyses of 2D CMB lensing and 3D galaxy clustering in the spherical Fourier-Bessel basis
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Lensing corrections on galaxy-lensing cross correlations and galaxy-galaxy auto correlations
• Galaxy blending effects in deep imaging cosmic shear probes of cosmology
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- III. Implementing the multi-tracer technique to constrain neutrino masses
• The kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• The Impact of Primordial Magnetic Fields on Future CMB Bounds on Inflationary Gravitational Waves
• Imprints of primordial magnetic fields on intrinsic alignments of galaxies
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• Revisiting cosmic acceleration with DESI BAO
• Consistency relations for large scale structures with primordial non-Gaussianities
• LINX: A Fast, Differentiable, and Extensible Big Bang Nucleosynthesis Package
• Effects of cosmic strings with delayed scaling on CMB anisotropy
• Fast and effortless computation of profile likelihoods using CONNECT
• Wilkinson Microwave Anisotropy Probe 7-yr constraints on fNL with a fast wavelet estimator
• The tension in the absolute magnitude of Type Ia supernovae
• Dark Energy Perturbations Revisited
• Modeling parity-violating spectra in Galactic dust polarization with filaments and its applications to cosmic birefringence searches
• Cosmological Model Parameter Dependence of the Matter Power Spectrum Covariance from the DEUS-PUR $Cosmo$ Simulations
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• Distribution of Dust around Galaxies: An Analytic Model
• Constraining Hybrid Natural Inflation with recent CMB data
• Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross correlations
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Unbiased contaminant removal for 3D galaxy power spectrum measurements
• Linear Density Perturbations in Multifield Coupled Quintessence
• Observational consequences of the Standard Model Higgs inflation variants
• Running cosmological constant with observational tests
• Shan--Chen interacting vacuum cosmology
• Unexpected dancing partners: Tracing the coherence between the spin and motion of dark matter halos
• 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 contribution of the kinematic Sunyaev-Zel'dovich Effect from the Warm Hot Intergalactic Medium to the Five-Year WMAP Data
• On the question of measuring spatial curvature in an inhomogeneous universe
• The impact of theoretical assumptions in the determination of the neutrino effective number from future CMB measurements
• Real Space Approach to CMB deboosting
• Independent constraints on local non-Gaussianity from the peculiar velocity and density fields
• Constraints on neutrino masses from the lensing dispersion of Type Ia supernovae
• The Hubble tension in the non-flat Super-$\Lambda \mathrm{CDM}$ model
• Testing the Impact of Satellite Anisotropy on Large and Small Scale Intrinsic Alignments using Hydrodynamical Simulations
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Circumventing the challenges in the choice of the non-conformal coupling function in inflationary magnetogenesis
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Constraining the Break of Spatial Diffeomorphism Invariance with Planck Data
• Asymptotic expansions for the Large Scale Structure
• Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations
• Quasi-matter bounce and inflation in the light of the CSL model
• Testing anthropic reasoning for the cosmological constant with a realistic galaxy formation model
• A new probe of magnetic fields in the pre-reionization epoch: II. Detectability
• Cosmological N-body simulations with generic hot dark matter
• Explaining low l anomalies in the CMB power spectrum with resonant superstring excitations during inflation
• PINION: Physics-informed neural network for accelerating radiative transfer simulations for cosmic reionization
• Testing $\alpha$-attractor quintessential inflation against CMB and low-redshift data
• Fast CMB lensing using statistical interpolation on the sphere
• Future detectability of gravitational-wave induced lensing from high-sensitivity CMB experiments
• Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Accelerated expansion of the universe and chasing photons from the CMB to study the late time integrated Sachs-Wolfe effect over different redshift ranges
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• Cosmological Tests of Gravity: A Future Perspective
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• Possible Evidence for Planck-Scale Resonant Particle Production during Inflation from the CMB Power Spectrum
• Observational constraints in Delta Gravity: CMB and supernovas
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Halo Mass-Concentration Relation at High-Mass End
• Brane inflation revisited after WMAP five-year results
• Testing statistical Isotropy in Cosmic Microwave Background Polarization maps
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• The thermal SZ tomography
• Constraining higher-order parameters for primordial non-Gaussianities from power spectra and bispectra of imaging survey
• Mitigating the impact of fiber assignment on clustering measurements from deep galaxy redshift surveys
• Recovering the Tidal Field in the Projected Galaxy Distribution
• Forecasts on neutrino mass constraints from the redshift-space two-point correlation function
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• An Introduction into the Theory of Cosmological Structure Formation
• No evidence for EDE from Planck data in extended scenarios
• Evolution of the cosmic matter density field with a primordial magnetic field
• Cosmological perturbations in extended electromagnetism. General gauge invariant approach
• Generation of inflationary perturbations in the continuous spontaneous localization model: The second order power spectrum
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Bayesian and frequentist perspectives agree on dynamical dark energy
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• Parametric tension between even and odd multipole data of WMAP power spectrum: unaccounted contamination or missing parameters?
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• Subtracting the kinetic Sunyaev-Zeldovich effect from the cosmic microwave background with surveys of large-scale structure
• Constraining $f(R)$ Gravity with a $k$-cut Cosmic Shear Analysis of the Hyper Suprime-Cam First-Year Data
• The causal effect of environment on halo mass and concentration
• Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear halo density field
• Exploring suppressed long-distance correlations as the cause of suppressed large-angle correlations
• The Effective Fluid approach for Modified Gravity and its applications
• Weighing neutrinos using high redshift galaxy luminosity functions
• Cosmology with extragalactic proper motions: harmonic formalism, estimators, and forecasts
• Dynamical friction in the primordial neutrino sea
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Direct reconstruction of spherical harmonics from interferometer observations of the CMB polarization
• Calibrating magnification bias for the $E_G$ statistic to test general relativity
• On the primordial origin of the smoothing excess in the $Planck$ temperature power spectrum in light of LSS data
• Cosmological tests of gravity with latest observations
• Short Distance Physics and Initial State Effects on the CMB Power Spectrum
• Fast likelihood-free inference in the LSS Stage IV era
• Locating the Baryon Acoustic Peak
• Scale Dependence of the Halo Bias in General Local-Type Non-Gaussian Models I: Analytical Predictions and Consistency Relations
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• Cosmological effects of coupled dark matter
• Joint Analysis of Constraints on f(R) Parametrization from Recent Cosmological Observations
• Late Time Modification of Structure Growth and the S8 Tension
• Constraints on Neutrino Mass from Sunyaev--Zeldovich Cluster Surveys
• Cosmic Bose dark matter
• Parameter estimation biases due to contributions from the Rees-Sciama effect to the integrated Sachs-Wolfe spectrum
• Scaling solutions as Early Dark Energy resolutions to the Hubble tension
• Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Constraining ultra slow roll inflation using cosmological datasets
• One-Dimensional Fuzzy Dark Matter Models: Structure Growth and Asymptotic Dynamics
• Local patch analysis for testing statistical isotropy of the Planck convergence map
• Gauge-Invariant Tensor Perturbations Induced from Baryon-CDM Relative Velocity and the B-mode Polarization of the CMB
• Late-time acceleration with steep exponential potentials
• The role of $T_0$ in CMB anisotropy measurements
• The bispectrum of cosmic string temperature fluctuations including recombination effects
• Relic Neutrino Degeneracies and Their Impact on Cosmological Parameters
• Dark matter perturbations and viscosity: a causal approach
• Cosmological nonlinear density and velocity power spectra including nonlinear vector and tensor modes
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• A Generalized Doppler and Aberration Kernel for Frequency-Dependent Cosmological Observables
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Joint Minkowski Functionals and Bispectrum Constraints on Non-Gaussianity in the CMB
• The Impact of Secondary non-Gaussianities in the CMB on Cosmological Parameter Estimation
• Window function convolution with deep neural network models
• Interpreting Internal Consistency of DES Measurements
• Is there another coincidence problem at the reionization epoch?
• Constraining Mixed Dark Matter models with high redshift Lyman-alpha forest data
• Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes
• Parametrizing growth in dark energy and modified gravity models
• Forecasts of cosmological constraints from Type Ia supernovae including the weak-lensing convergence
• Perturbed dark energy: classical scalar field versus tachyon
• The halo bias for number counts on the light cone from relativistic N-body simulations
• Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
• Disentangling modified gravity from a dark force with gravitational redshift
• Impact of nonlinear growth of the large-scale structure on CMB B-mode delensing
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• Effects of a primordial magnetic field with log-normal distribution on the cosmic microwave background
• Iterative map-making with two-level preconditioning for polarized Cosmic Microwave Background data sets
• Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
• Quantum collapse as source of the seeds of cosmic structure during the radiation era
• New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
• Introducing constrained matched filters for improved separation of point sources from galaxy clusters
• Asymmetry of the CMB map: local and global anomalies
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Forecast for growth-rate measurement using peculiar velocities from LSST supernovae
• Tests of Standard Cosmology in Horava Gravity and Bayesian Evidence for a Closed Universe, and the Hubble Tension
• WMAP Constraints On K-Inflation
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Gamma-ray and Synchrotron Radiation from Dark Matter annihilations in Ultra-faint Dwarf Galaxies
• The magnitude of the non-adiabatic pressure in the cosmic fluid
• Machine learning unveils the linear matter power spectrum of modified gravity
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• Improved Modeling of the Kinematic Sunyaev-Zel'dovich Projected-Fields signal and its Cosmological Dependence
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Unveiling Neutrino Halos with CMB Lensing
• Curvature bounce in general relativity: background and primordial spectrum
• Using measurements of the cosmic bulk flow to constrain $f(R)$ Gravity
• Testing the ABS method with the simulated Planck temperature maps
• CMB Neutrino Mass Bounds and Reionization
• Bayesian Inference of Polarized CMB Power Spectra from Interferometric Data
• Large scale distribution of mass versus light from Baryon Acoustic Oscillations: Measurement in the final SDSS-III BOSS Data Release 12
• Skewing the CMB$\times$LSS: a Fast Method for Bispectrum Analysis
• Gravitational waves, CMB polarization, and the Hubble tension
• Constraints on Running of Non-Gaussianity from Large Scale Structure Probes
• Probing helium reionization with kinetic Sunyaev Zel'dovich tomography
• Optimal and fast E/B separation with a dual messenger field
• Fast generation of mock galaxy catalogues with COLA
• Probing the Weak Gravity Conjecture in the Cosmic Microwave Background
• Constraining primordial and gravitational mode coupling with the position-dependent bispectrum of the large-scale structure
• Running vacuum model in non-flat universe
• Remote Dipole Field Reconstruction with Dusty Galaxies
• Cosmological Parameters from CMB Maps without Likelihood Approximation
• Constraints on electromagnetic form factors of sub-GeV dark matter from the Cosmic Microwave Background anisotropy
• Linear anisotropies in dispersion-measure-based cosmological observables
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• Detection of relic gravitational waves in the CMB: Prospects for CMBPol mission
• Probing Neutrinos from Planck and Forthcoming Galaxy Redshift Surveys
• Recovering dark-matter clustering from galaxies with Gaussianization
• External priors for the next generation of CMB experiments
• Structure Formation with Two Periods of Inflation: Beyond PLaIn $\Lambda$CDM
• Constraints on long-lived electrically charged massive particles from anomalous strong lens systems
• Lightcone Averaging and Precision Cosmology
• Dark matter kinetic decoupling with a light particle
• How does pressure gravitate? Cosmological constant problem confronts observational cosmology
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• Simple numerical implementation of general dark energy models
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• Constraining Decaying Dark Matter
• The halo 3-point correlation function: a methodological analysis
• Interacting parametrized post-Friedmann method
• Understanding large scale CMB anomalies with the generalized non-minimal derivative coupling during inflation
• Constraints on primordial non-Gaussianity from Galaxy-CMB lensing cross-correlation
• Constraints on the multi-lognormal magnetic fields from the observations of the cosmic microwave background and the matter power spectrum
• Small-scale clumping of dark matter and the mean free path of ionizing photons at $z=6$
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• Probing dark energy using convergence power spectrum and bi-spectrum
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• Constraints on the cosmological parameters from BICEP2, Planck and WMAP
• The Effective Field Theory and Perturbative Analysis for Log-Density Fields
• Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies
• The density distributions of cosmic structures: impact of the local environment on weak-lensing convergence
• Hybrid multi-fluid-particle simulations of the cosmic neutrino background
• CMB power spectrum in the emergent universe with k-essence
• Interacting dark energy axions in light of the Hubble tension
• Searching for dilaton fields in the Ly$\alpha$ forest
• Mapping gravitational lensing of the CMB using local likelihoods
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• New constraints on red-spiral galaxies from their kinematics in clusters of galaxies
• Unified approach to secondary effects on the CMB B-mode polarization
• Primordial Gravitational Waves Spectrum in the Coupled-Scalar-Tachyon Bounce Universe
• The reconstructed CMB lensing bispectrum
• Cosmology in a certain vector-tensor theory of gravitation
• Inflation and Scale-invariant $R^2$-Gravity
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Stress testing the dark energy equation of state imprint on supernova data
• Limits on Entanglement Effects in the String Landscape from Planck and BICEP/Keck Data
• Dark Energy Survey Year 1: An independent E/B-mode cosmic shear analysis
• The geometrical meaning of statistical isotropy of smooth random fields in two dimensions
• Cross-Correlation Forecast of CSST Spectroscopic Galaxy and MeerKAT Neutral Hydrogen Intensity Mapping Surveys
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• An improved estimator for non-Gaussianity in cosmic microwave background observations
• Planck constraints on neutrino isocurvature density perturbations
• The integrated angular bispectrum
• Optimising Boltzmann codes for the Planck era
• Improving initialization and evolution accuracy of cosmological neutrino simulations
• Evolution of density and velocity profiles of dark matter and dark energy in spherical voids
• Lens covariance effects on likelihood analyses of CMB power spectra
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• Detection of transplanckian effects in the cosmic microwave background
• Freezing Out Early Dark Energy
• Optimal analysis of azimuthal features in the CMB
• Small-scale CMB anisotropies induced by the primordial magnetic fields
• Efficient cosmological parameter sampling using sparse grids
• A method of weak lensing reconstruction through cosmic magnification with multi-band photometry information
• Constraints on Dark Energy state equation with varying pivoting redshift
• Binomial Line Cox Processes: Statistical Characterization and Applications in Wireless Network Analysis
• The influence of the effective number of active and sterile neutrinos on the determination of the values of cosmological parameters
• On the galaxy 3-point correlation function in Modified Gravity
• Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Improving Constraints on Inflation with CMB Delensing
• 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
• Diverse dark matter haloes in Two-field Fuzzy Dark Matter
• Cosmological perturbations without the Boltzmann hierarchy
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Revisiting CPL with sign-switching density: To cross or not to cross the NECB
• Null energy condition violation and beyond Horndeski physics in light of DESI DR2 data
• Cross-correlation analysis of CMB with foregrounds for residuals
• Gaussianization of peculiar velocities and bulk flow measurement
• Metastability in Emergent Dark Energy: A New Framework Confronting Cosmological Observations
• A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
• Simultaneous constraints on bias, normalization and growth index through power spectrum measurements
• Foreground removal with ILC methods for AliCPT-1
• Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
• Particle initialization effects on Lyman-$\alpha$ forest statistics in cosmological SPH simulations
• Symbolic Implementation of Extensions of the $\text{PyCosmo}$ Boltzmann Solver
• Dark Twilight Joined with the Light of Dawn to Unveil the Reionization History
• Selecting samples of galaxies with fewer Fingers-of-God
• Cosmology when living near the Great Attractor
• The primordial "f_NL" non-Gaussianity, and perturbations beyond the present horizon
• Cosmological Constraints on Rapid Roll Inflation
• Cosmological perturbations: non-cold relics without the Boltzmann hierarchy
• Cosmological evolutions in Tsujikawa model of $f(R)$ Gravity
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• CMB lensing reconstruction with point source masks
• Footprints of Doppler and Aberration Effects in CMB Experiments: Statistical and Cosmological Implications
• Computing 3 point correlation function randoms counts without the randoms catalogue
• Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
• Ghostly Stellar Haloes and their Relationship to Ultra-faint Dwarfs
• Cosmological Constraints on the Global Star Formation Law of Galaxies: Insights From Baryon Acoustic Oscillation Intensity Mapping
• Relativistic effects in the large-scale structure with effective dark energy fluids
• Inference of the optical depth to reionization $\tau$ from $\text{Planck}$ CMB maps with convolutional neural networks
• A Systematic Study of Projection Biases in Weak Lensing Analysis
• Beyond the Runge-Kutta-Wentzel-Kramers-Brillouin method
• Perturbative Gaussianizing transforms for cosmological fields
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Optimizing galaxy samples for clustering measurements in photometric surveys
• Improving Constraints on Fundamental Physics Parameters with the Clustering of Sunyaev-Zeldovich Selected Galaxy Clusters
• Bayesian model selection for dark energy using weak lensing forecasts
• Physics of the Cosmic Microwave Background Radiation
• Probing supervoids with weak lensing
• Anisotropies of cosmological gravitational wave backgrounds in non-flat spacetime
• Detectable Data-driven Features in the Primordial Scalar Power Spectrum
• New natural shapes of non-Gaussianity from high-derivative interactions and their optimal limits from WMAP 9-year data
• X-ray cluster cosmology
• The primordial information content of Rayleigh Anisotropies
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• The Einstein-Boltzmann equations revisited
• Modelling the WMAP large-angle anomalies as an effect of a local density inhomogeneity
• Testing consistency of ${\Omega }_b{h}^2$ in the Planck data
• Constraints on dark energy from TDCOSMO & SLACS lenses
• Impact of Instrumental Systematics on the CMB Bispectrum
• Joint Bayesian estimation of tensor and lensing B-modes in the power spectrum of CMB polarization data
• Early dark energy constraints on growing neutrino quintessence cosmologies
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Extended Stellar Components of Galaxies & the Nature of Dark Matter
• Testing primordial non-Gaussianities on galactic scales at high redshift
• On the Hubble expansion in a Big Bang quantum cosmology
• What can be learned about dark energy evolution?
• Statistical anisotropies in temperature and polarization fluctuations from a scale-dependent trispectrum
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• A theoretical view of the T-web statistical description of the cosmic web
• CMB anisotropies and linear matter power spectrum in models with non-thermal neutrinos and primordial magnetic fields
• Power Spectrum Precision for Redshift Space Distortions
• Smoothing the redshift distributions of random samples for the baryon acoustic oscillations : applications to the SDSS-III BOSS DR12 and QPM mock samples
• Testing modified gravity scenarios with direct peculiar velocities
• A Simulation-Based Method for Correcting Mode Coupling in CMB Angular Power Spectra
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• Cosmological Leverage from the Matter Power Spectrum in the Presence of Baryon and Nonlinear Effects
• Constraints on Non-Gaussianity from Sunyaev--Zeldovich Cluster Surveys
• Constraints on non-thermal Dark Matter from Planck lensing extraction
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• A framework to mitigate patchy reionization contamination on the primordial gravitational wave signal
• Observational constraints on running vacuum model
• Almanac: MCMC-based signal extraction of power spectra and maps on the sphere
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• Screened fifth forces in parity-breaking correlation functions
• Self-Calibrating the Look-Elsewhere Effect: Fast Evaluation of the Statistical Significance Using Peak Heights
• The measurements of matter density perturbations amplitude from cosmological data
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• Tachyonic vs Quintessence dark energy: linear perturbations and CMB data
• Constraining Ultra-light Axions with Galaxy Cluster Number Counts
• How accurately can we measure the hydrogen 2S->1S transition rate from the cosmological data?
• 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
• Evolution of the CMB Power Spectrum Across WMAP Data Releases: A Nonparametric Analysis
• Weighing the Light Gravitino Mass with Weak Lensing Surveys
• Scalar quadratic maximum likelihood estimators for the CMB cross power spectrum
• HI HOD -- I. The Halo Occupation Distribution of HI Galaxies
• Consistency of CMB experiments beyond cosmic variance
• Gauge Issues in Extended Gravity and f(R) Cosmology
• Scalar field descriptions of two dark energy models
• Constraining modified gravity scenarios with the 6dFGS and SDSS galaxy peculiar velocity datasets
• Constraints on the Sunyaev-Zel'dovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
• Bias in Matter Power Spectra ?
• King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z=0.55 using the Subaru Hyper Suprime-Cam
• Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure
• A comparative analysis of dissipation coefficients in warm inflation
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Fast scalar quadratic maximum likelihood estimators for the CMB B-mode power spectrum
• Learn-As-You-Go Acceleration of Cosmological Parameter Estimates
• The impact of the cosmological constant on past and future star formation
• Precise peculiar velocities from gravitational waves accompanied by electromagnetic signals and cosmological applications
• Synchronous coordinates and gauge-invariant observables in cosmological spacetimes
• Ghost Dark Matter
• Anticipating the XRISM search for the decay of resonantly produced sterile neutrino dark matter
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• Flat-sky Angular Power Spectra Revisited
• The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters
• Halos in Dark Ages: formation and chemistry
• Probing the Primordial Power Spectrum with Cluster Number Counts
• An Informational Approach to Cosmological Parameter Estimation
• Relative baryon-dark matter velocities in cosmological zoom simulations
• Reionization and Cosmic Dawn: theory and simulations
• Anisotropic power spectrum and the observed low-l power in PLANCK CMB data
• Detecting Electron Density Fluctuations from Cosmic Microwave Background Polarization using a Bispectrum Approach
• Isocurvature initial conditions for second order Boltzmann solvers
• On Observables in a Dark Matter-Clustering Quintessence System
• Visualizing Invisible Dark Matter Annihilation with the CMB and Matter Power Spectrum
• Effects of Redshift Uncertainty on Cross-Correlations of CMB Lensing and Galaxy Surveys
• Cosmological constraints on $\Lambda (\alpha )$CDM models with time-varying fine structure constant
• Non-parametric Cosmology with Cosmic Shear
• Suitable Initial Conditions for Newtonian Simulations with Massive Neutrinos
• Probing the Neutrino Mass through the Cross Correlation between the Rees-Sciama Effect and Weak Lensing
• Suppressing the thermal SZ-induced variance in CMB-cluster lensing estimators
• Nonlinear structure formation in Bound Dark Energy
• Thermal Loop Effects on Large-Scale Curvature Perturbation in the Higgs Inflation
• Ionization from Cosmic Strings at Cosmic Dawn
• Constraining the Neutrino Mass with the Drifting Coefficient of the Field Cluster Mass Function
• Dark Matter with N-Body Numerical Simulations
• Isocurvature modes: joint analysis of the CMB power spectrum and bispectrum
• Do current observations support transient acceleration of our universe?
• Principal component analysis of the reionization history from Planck 2015 data
• Brane inflation driven by an arctan potential: CMB constraints and Reheating
• Cosmological test of an extended quintessence model
• Primordial Non-Gaussianities of inflationary step-like models
• The effect of finite halo size on the clustering of neutral hydrogen
• CMB Lensing and Scale Dependent New Physics
• A forecast of the sensitivity on the measurement of the optical depth to reionization with the GroundBIRD experiment
• Current and Future constraints on single-field $\alpha$-Attractor model
• Weak Lensing Magnification Reconstruction with the Modified Internal Linear Combination Method
• Astrophysical Searches and Constraints on Ultralight Bosonic Dark Matter
• PhotoNs-GPU:A GPU accelerated cosmological simulation code
• Effects of Neutrino Masses and Asymmetries on Dark Matter Halo Assembly
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Probing Lepton Asymmetry with 21 cm Fluctuations
• Constraints on cosmic birefringence using $E$-mode polarisation
• Probing Quintessence Potential with Future Cosmological Surveys
• Towards Optimal Foreground Mitigation Strategies for Interferometric HI Intensity Mapping in the Low-Redshift Universe
• Interacting photon-baryon fluid, warm dark matter and the first acoustic peak
• Signal of Cosmic Strings in Cross-Correlation of 21-cm Redshift and CMB Polarization Maps
• Cosmological parameters from Planck data in SU(2)${}_{\mathrm{CMB}}$, their local $\Lambda$CDM values, and the modified photon Boltzmann equation
• Measuring cosmic filament spin with the kinetic Sunyaev-Zel'dovich effect
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• Complementary Cosmological Simulations
• Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
• Constraining neutrino mass in dynamical dark energy cosmologies with the logarithm parametrization and the oscillating parametrization
• CMB power spectrum for emergent scenario and slow expansion in scalar-tensor theory of gravity
• Higgs Inflation: constraining the top quark mass and breaking the $H_0$-${\sigma }_8$ correlation
• On validity of the quasi-static approximation in scalar-tensor theories
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Modern Cosmology: Interactive Computer Simulations that use Recent Observational Surveys
• CMB lensing power spectrum without noise bias
• Forecast of CMB TB and EB correlations for AliCPT-1
• Deep learning insights into non-universality in the halo mass function
• A search for concentric rings with unusual variance in the 7-year WMAP temperature maps using a fast convolution approach
• Cosmological Parameters from a re-analysis of the WMAP-7 low resolution maps
• Cosmic Microwave Background constraints of decaying dark matter particle properties
• Can Baby Universe Absorption Explain Dark Energy?
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• Impact of Low ell's on Large Scale Structure Anomalies
• Euclid preparation. Simulations and nonlinearities beyond $\Lambda$CDM. 1. Numerical methods and validation
• An Analytic Formula for the Supercluster Mass Function
• Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
• Weak-lensing tunnel voids in simulated light cones: A new pipeline to investigate modified gravity and massive neutrinos signatures
• Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Reconstruction of inflationary scenarios in non-conservative unimodular gravity
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• Numerical Discreteness Errors in Multi-Species Cosmological N-body Simulations
• Dissociation of dark matter and gas in cosmic large-scale structure
• What does a cosmological experiment really measure? Covariant posterior decomposition with normalizing flows
• Accessing the high-$\ell$ frontier under the Reduced Shear Approximation with $k$-cut Cosmic Shear
• CMB Shadows: The Effect of Interstellar Extinction on Cosmic Microwave Background Polarization and Temperature Anisotropy
• Markov Chain Beam Randomization: a study of the impact of PLANCK beam measurement errors on cosmological parameter estimation
• Full-Sky Lensing Reconstruction of 21 cm Intensity Maps
• Small-scale Effects of Thermal Inflation on Halo Abundance at High-$z$, Galaxy Substructure Abundance and 21-cm Power Spectrum
• Evaluating backreaction with the ellipsoidal collapse model
• Thermal gravitational-wave background in the general pre-inflationary scenario
• Complementarity of Future Dark Energy Probes
• More about a successful vector-tensor theory of gravitation
• Statistical imprints of CMB B-type polarization leakage in an incomplete sky survey analysis
• Precision of future experiments measuring primordial tensor fluctuation
• The Superhorizon Test of Future B-mode Experiments
• On the anisotropic density distribution on large scales
• Limits on Semiclassical Fluctuations in the Primordial Universe
• Constraints on the SZ Power Spectrum on Degree Angular Scales in WMAP Data
• Teleparallel dark energy in a nonflat universe
• Smallest Halos in Thermal Wino Dark Matter
• Constraining equilateral-type primordial non-Gaussianities from imaging surveys
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• Dynamics of pairwise motions in the fully non-linear regime in LCDM and Modified Gravity cosmologies
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• On the viability of a certain vector-tensor theory of gravitation
• Fitting functions on the cheap: the relative nonlinear matter power spectrum
• Enhancing CMB map reconstruction and power spectrum estimation with convolutional neural networks
• Identifying frequency decorrelated dust residuals in B-mode maps by exploiting the spectral capability of bolometric interferometry
• Comparison of results on $N_{\mathrm{eff}}$ from various Planck likelihoods
• Systematic Effects in Interferometric Observations of the CMB Polarization
• Constraining cosmic reionization by combining the kinetic Sunyaev-Zel'dovich and the 21 cm power spectra
• Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes
• Unified dark fluid with null sound speed as an alternative to phantom dark energy
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
• A High Throughput Workflow Environment for Cosmological Simulations
• The T-E correlation coefficient of Planck legacy data
• On (non-)dynamical dark energy
• Physical Models for the Clustering of Obscured and Unobscured Quasars
• A Bayesian estimate of the CMB-large-scale structure cross-correlation
• Observing the Epoch of Reionization with the Cosmic Microwave Background
• Perturbations and Linearization Stability of Closed Friedmann Universes
• Cosmic topology. Part IVa. Classification of manifolds using machine learning: a case study with small toroidal universes
• Probing Long-Range Forces Between Neutrinos with Cosmic Structures
• Impacts of pre-initial conditions on anisotropic separate universe simulations: a boosted tidal response in the epoch of reionization
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Maximum likelihood analysis of systematic errors in interferometric observations of the cosmic microwave background
• BICEP's acceleration
• Mapping the Cosmological Confidence Ball Surface
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• Can Dark Stars account for the star formation efficiency excess at very high redshifts?
• Cosmological signatures of a Rapid Diluted Energy Density
• Principal Components of CMB non-Gaussianity
• Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
• Breaking the Dark Degeneracy with the Drifting Coefficient of the Field Cluster Mass Function
• Extended Fast Action Minimisation method: application to SDSS-DR12 Combined Sample
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis
• What is the optimal way to measure the galaxy power spectrum?
• Blind Map Level Systematics Cleaning: A Quadratic Estimator Approach
• Full sky Integrated Sachs-Wolfe maps for the MICE Grand Challenge lightcone simulation
• The interplay of CMB temperature lensing power reconstruction with primordial non-Gaussianity of local type
• The Diffusion Coefficient of the Splashback Mass Function as a Probe of Cosmology
• Joint constraints on galaxy bias and ${\sigma }_8$ through the N-pdf of the galaxy number density
• Holographic inflation and holographic dark energy from entropy of the anti-de Sitter black hole
• Hydrodynamics of ultralight complex scalar field dark matter and its impact on the growth of structure
• On the $2^{\text{nd}}$ feature of the matter two-point function
• Reconstructing matter profiles of spherically compensated cosmic regions in $\Lambda$CDM cosmology
• The effect of reionization on the COBE normalization
• Using relativistic effects in large-scale structure to constrain astrophysical properties of galaxy populations
• Emergent universe revisited through the CSL theory
• Knot reconstruction of the scalar primordial power spectrum with Planck, ACT, and SPT CMB data
• Nonlinear power spectrum in clustering and smooth dark energy models beyond the BAO scale
• Efficient implementation of the Time Renormalization Group
• Observational constraints on inflection point quintessence with a cubic potential
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• Joint Modelling of Astrophysical Systematics for Cosmology with LSST Cosmic Shear
• Lensing Bias to CMB Polarization Measurements of Compensated Isocurvature Perturbations
• Structure Formation Constraints on Sommerfeld-Enhanced Dark Matter Annihilation
• Novel vacuum conditions in inflationary collapse models
• Masked areas in shear peak statistics: a forward modeling approach
• Pure-mode correlation functions for cosmic shear and application to KiDS-1000
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Can the homogeneity scale be used as a standard ruler?
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• Non-linear matter power spectrum without screening dynamics modelling in $f(R)$ gravity
• Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
• The art of building a smooth cosmic distance ladder in a perturbed universe
• Impact of our local environment on cosmological statistics
• Hawaii Two-0: High-redshift galaxy clustering and bias
• Optimal Boltzmann hierarchies with non-vanishing spatial curvature
• Taller in the saddle: constraining CMB physics using saddle points
• Signature of short distance physics on inflation power spectrum and CMB anisotropy
• Emergent universe: tensor perturbations within the CSL framework
• A Simple Gravitational Lens Model For Cosmic Voids
• Cosmological probes of helium reionization
• Parameters and pitfalls in dark energy models with time varying equation of state
• Fast and precise way to calculate the posterior for the local non-Gaussianity parameter $f_{\text{nl}}$ from cosmic microwave background observations
• Constraints on the primordial gravitational waves with variable sound speed from current CMB data
• On the impact of the galaxy window function on cosmological parameter estimation
• A Maximum Likelihood Approach to Estimating Correlation Functions
• Reconstructing the dark matter and dark energy interaction scenarios from observations
• Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data
• Lensing reconstruction from the cosmic microwave background polarization with machine learning
• Measuring the Hubble constant through the galaxy pairwise peculiar velocity
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• A flexible parameterization to test early physics solutions to the Hubble tension with future CMB data
• Dark Universe inspired by the Kaluza-Klein gravity and impact on Primordial Gravitational Waves
• A glitch in gravity: cosmic Lorentz-violation from fiery Big Bang to glacial heat death
• Sound Horizon Independent Constraints on Early Dark Energy: The Role of Supernova Data
• Comparing the motion of dark matter and standard model particles on cosmological scales
• The Simons Observatory: impact of bandpass, polarization angle and calibration uncertainties on small-scale power spectrum analysis
• Scale and redshift dependent limits on cosmic neutrino properties
• Joint inference of multiplicative and additive systematics in galaxy density fluctuations and clustering measurements
• Reconstructing the epoch of reionisation with Planck PR4
• Measuring neutrino mass and asymmetry with matter pairwise velocities
• The SDSS DR7 Galaxy Angular Power Spectrum: Volume-Limits and Galaxy Morphology
• Reconstructing patchy helium reionization using the cosmic microwave background and large-scale structure
• Cosmic Strings as Dynamical Dark Energy: Novel Constraints
• Reconstructing the Long-wavelength Matter Density Fluctuation Modes from the Scalar-Type Clustering Fossils
• Information Wells and the Emergence of Primordial Black Holes in a Cyclic Quantum Universe
• Cosmological constraints on neutrino masses in light of JWST red and massive candidate galaxies
• High-redshift Galaxies from JWST Observations in More Realistic Dark Matter Halo Models
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• 21 cm Intensity Mapping with the DSA-2000
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Updated observational constraints on $\varphi$CDM dynamical dark energy cosmological models
• Thawing Quintessence: Priors, evidence, and likely trajectories
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• A method to extract the redshift distortions beta parameter in configuration space from minimal cosmological assumptions
• Role of ionizing background on the non-thermal broadening inferred for the aligned absorbers
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Trans-Planckian Effect in $f(R)$ Cosmology
• Examining statistical isotropy of CMB low multipoles from Planck PR4 data
• Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation
• Can the NANOGrav observations constrain the geometry of the universe?
• Infrared divergence of pure Einstein gravity contributions to cosmological density power spectrum
• Dependence on the environment of the abundance function of light-cone simulation dark matter haloes
• Signature of Massive Neutrinos from the Clustering of Critical Points. I. Density-threshold-based Analysis in Configuration Space
• Impact of a primordial magnetic field on cosmic microwave background $B$ modes with weak lensing
• HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions
• Non-linear Matter Spectrum for a Variable Equation of State
• Formation of Compact Clusters from High Resolution Hybrid Cosmological Simulations
• Beyond Fisher Forecasting for Cosmology
• Constraints on the phase transition of Early Dark Energy with the CMB anisotropies
• Study on the filters of atmospheric contamination in ground based CMB observation
• Effect of Dark Energy Perturbation on Cosmic Voids Formation
• Weak lensing forecasts for dark energy, neutrinos and initial conditions
• Constraining primordial tensor features with the anisotropies of the Cosmic Microwave Background
• A note on the initial conditions within the effective field theory approach of cosmic acceleration
• Perturbation in an interacting dark universe
• Planck and WMAP constraints on generalised Hubble flow inflationary trajectories
• Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
• Evolution of the Deterministic Collapse Barrier of the Field Clusters as a Probe of Cosmology
• Structure Formation in Dark Matter Particle Production Cosmology
• Cosmic distance determination from photometric redshift samples using BAO peaks only
• Numerical implementation of the Cubic Galileon model in PINOCCHIO
• Stability of small-scale baryon perturbations during cosmological recombination
• Abundance of peaks and dips in three-dimensional mass and halo density fields: a test for cosmology
• Discerning Dark Energy Models with High-Redshift Standard Candles
• An analytical approach to the CMB anisotropies in a Spatially Closed background
• Cosmological boost factor for dark matter annihilation at redshifts of $z=10$-$100$ using the power spectrum approach
• The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps
• Forecasts for Broadband Intensity Mapping of the Ultraviolet-Optical Background with CASTOR and SPHEREx
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• Evolution of the real-space correlation function from next generation cluster surveys
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• Data Compression and Covariance Matrix Inspection: Cosmic Shear
• The Low Redshift survey at Calar Alto (LoRCA)
• The impact of super-survey modes on cosmological constraints from cosmic shear fields
• Optimistic estimation on probing primordial gravitational waves with CMB B-mode polarization
• Signatures of Spatial Curvature on Growth of Structures
• Reconstructing the Gravitational Lensing Potential from the Lyman-$\alpha$ Forest
• Constraints on primordial magnetic fields from the optical depth of the cosmic microwave background
• Suppression of scalar power on large scales and associated bispectra
• Perturbative interaction approach to cosmological structure formation
• A simple supergravity model of inflation constrained with Planck 2018 data
• Cosmological constraints on Lorentz invariance violation in the neutrino sector
• Lightening the Dark Matter from its Viscosity and Explanation of EDGES Anomaly
• Prospects for cosmic magnification measurements using HI intensity mapping
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• Effect of Priomordial non-Gaussianities on Galaxy Clusters Scaling Relations
• B-mode polarization induced by gravitational waves from kinks on infinite cosmic strings
• Averaged universe confronted with cosmological observations: A fully covariant approach
• Cosmic variance mitigation in measurements of the integrated Sachs-Wolfe effect
• Measuring neutrino mass imprinted on the anisotropic galaxy clustering
• Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
• Calculating Bayesian evidence for inflationary models using CONNECT
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Can MONDian vector theories explain the cosmic speed up ?
• Effects of boosting on extragalactic components: methods and statistical studies
• Self-calibrating BAO measurements in the presence of Small Displacement Interlopers
• Analytical warm dark matter power spectrum on small scales
• Clusternets: A deep learning approach to probe clustering dark energy
• Cosmic Kite: Auto-encoding the Cosmic Microwave Background
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Relic Vector Field and CMB Large Scale Anomalies
• Extended Delta-map: a map-based foreground removal method for CMB polarization observations
• Optimizing interferometer experiments for CMB B mode measurement
• Reconciling cosmic dipolar tensions with a gigaparsec void
• Probing the time variation of the effective Newton's constant with optimal redshift weights
• Can the angular scale of cosmic homogeneity be used as a cosmological test?
• Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
• Improving CMB constraints on early Universe physics with LSS: A multi-probe forecast including cross-covariance
• Cosmology with Planck T-E correlation coefficient
• A Minkowski Functional Analysis of the Cosmic Microwave Background Weak Lensing Convergence
• In search for the Local Universe dynamical homogeneity scale with CF4++ peculiar velocities
• Consequences of CCD imperfections for cosmology determined by weak lensing surveys: From laboratory measurements to cosmological parameter bias
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Neutrino physics from future weak lensing surveys
• The imprint of dark subhaloes on the circumgalactic medium
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Cosmic microwave background constraints on a decaying cosmological term related to the thermal evolution
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Cosmological constraints in Lambda-CDM and Quintessence paradigms with Archeops
• A Brachistochrone Approach to Reconstruct the Inflaton Potential
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Linear Relativistic Corrections in the Spherical Fourier-Bessel Power Spectrum
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Probing the independence within the dark sector in the fluid approximation
• Cosmic microwave background constraints on the tensor-to-scalar ratio
• Dark energy explained by a bias in the measurements
• Lensing Noise in mm-wave Galaxy Cluster Surveys
• Simulations and Observations of the Microwave Universe
• Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs
• Effect of redshift bin mismatch on cross correlation between DESI Legacy Imaging Survey and Planck CMB lensing potential
• Maximum likelihood kinetic Sunyaev Zel'dovich velocity reconstruction
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Nonparametric Forecasts of the CMB Angular Power Spectra for the Planck Mission
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Modelling the environmental dependence of the growth rate
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Dependence of the dynamical properties of light-cone simulation dark matter halos on their environment
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Baryon acoustic oscillations from a joint analysis of the large-scale clustering in Fourier and configuration space
• Cosmological Perturbations in the 5D Holographic Big Bang Model
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• Probing the shape and internal structure of dark matter halos with the halo-shear-shear three-point correlation function
• Non-linear coupling in the dark sector as a running vacuum model
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Power law $\alpha$-Starobinsky inflation
• Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements
• Constraining modified growth patterns with tomographic surveys
• Effect of the field self-interaction of General Relativity on the Cosmic Microwave Background Anisotropies
• Cosmic Microwave Background Polarization
• Prospects for studying the mass and gas in protoclusters with future CMB observations
• Theoretical Estimates of Integrated Sachs-Wolfe Effect Detection through EMU-ASKAP Survey with Confusion, Position Uncertainty, Shot Noise and SNR analysis
• Growing neutrino cosmology
• Doppler bias: impact of peculiar velocities on color selection and the large scale structure of galaxy surveys
• An Estimator for the lensing potential from galaxy number counts
• Future constraints on variations of the fine structure constant from combined CMB and weak lensing measurements
• Superimposed Oscillations in Brane Inflation
• A Novel Bispectrum Estimator of the Kinematic Sunyaev-Zel'dovich Effect using Projected Fields
• Evolution of density and velocity profiles of matter in large voids
• CMB anisotropies from patchy reionisation and diffuse Sunyaev-Zel'dovich effects
• Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples
• CMB Anomalies from Imperfect Dark Energy: Confrontation with the Data
• A Bayesian ILC method for CMB B-mode posterior estimation and reconstruction of primordial gravity wave signal
• Imprints of the post recombination dissipation of helical magnetic field on the Cosmic Microwave Background Radiation
• A convolutional-neural-network estimator of CMB constraints on dark matter energy injection
• Improving Cosmic Birefringence Constraints via Delensing
• Observational constraints on inflationary potentials within the quantum collapse framework
• Do data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Forecasts of effects of beam systematics and deprojection on the third-generation ground-based cosmic microwave background experiment
• Observational effects of the early episodically dominating dark energy
• Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes
• Analytic expressions for the background evolution of massive neutrinos and dark matter particles
• The Effect of Corner Modes in the Initial Conditions of Cosmological Simulations
• Detecting the neutrino mass and mass hierarchy from global data
• Physics of Cosmic Microwave Background anisotropies and primordial fluctuations
• Probing the primordial Universe from the low-multipole CMB data
• Fast Generation of Weak Lensing Maps in Modified Gravity with COLA
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Squeezing information from radio surveys to probe the primordial Universe
• Linear and non-linear Modified Gravity forecasts with future surveys
• Results and forecasts on cosmic inflation from weak lensing
• On the tomographic cluster clustering as a cosmological probe
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Effect of Our Galaxy's Motion on Weak Lensing Measurements of Shear and Convergence
• Cosmology with shear ratios: a joint study of weak lensing and spectroscopic redshift datasets
• Inference of matter power spectrum at z=0 using DESI DR1 Full-Shape data
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• Minimal parameterizations for modified gravity
• Constraining the primordial power spectrum using a differentiable likelihood
• Subdominant Dark Matter sterile neutrino resonant production in the light of Planck
• Galaxies and Cluster of Galaxies as Peak Patches of the Density Field
• The reach of next-to-leading-order perturbation theory for the matter bispectrum
• Higgs mass from cosmological and astrophysical measurements
• Alleviating the Hubble tension with Torsion Condensation (TorC)
• Tensor Tilt from Primordial B-modes
• Anthropic Origin of the Neutrino Mass from Cooling Failure
• Scalar field models of dark energy with barotropic equation of state: properties and observational constraints from different datasets
• Searching for ring-like structures in the Cosmic Microwave Background
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Non-adiabatic instability in coupled dark sectors
• Cosmoglobe: Towards end-to-end CMB cosmological parameter estimation without likelihood approximations
• Cosmology of Single Species Hidden Dark Matter
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
• Evolution of the early universe in Einstein-Cartan theory
• E and B modes of the CMB y-type distortions: polarised kinetic Sunyaev-Zeldovich effect from the reionisation and post-reionisation eras
• Probing Primordial Symmetry Breaking with Cosmic Microwave Background Anisotropy
• The running of featureful primordial power spectra
• A simulation experiment of a pipeline based on machine learning for neutral hydrogen intensity mapping surveys
• CMB delensing with deep learning
• Dark matter search with CMB: a study of foregrounds
• Weighing Neutrinos with Large-Scale Structure
• The BINGO/ABDUS Project: Forecast for cosmological parameters from a mock Fast Radio Bursts survey
• ForestFlow: predicting the Lyman-$\alpha$ forest clustering from linear to nonlinear scales
• Small Correlated Against Large Estimator (SCALE) for Cosmic Microwave Background Lensing
• Observational constraints on the second-order primordial power spectrum: Exploring a Continuous Spontaneous Localization inspired inflationary model
• The AIDA-TNG project: 3D halo shapes
• A Multifrequency approach of the cosmological parameter estimation in presence of extragalactic point sources
• Measuring the cosmological density field twice: A novel test of dark energy using the CMB quadrupole
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• CMB low multipole alignments across WMAP and \emph{Planck} data releases
• On the Outskirts of Dark Matter Haloes
• Lensing anomalies from the epoch of reionisation
• Viable Intermediate Inflation in the Mimetic DBI Model
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• 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
• Quantum Statistical Effects on Warm Dark Matter and the Mass Constraint from the Cosmic Structure at Small Scales
• The Pseudo Evolution of Galaxy-Cluster Masses and Its Connection to Mass Density Profile
• Constraints on Multicomponent Dark Energy from Cosmological Observations
• Cosmological consequences of intrinsic alignments super-sample covariance
• Primordial fluctuations from deformed quantum algebras
• Constraint on the growth factor of the cosmic structure from the damping of the baryon acoustic oscillation signature
• Detailed analysis of the curvature bounce: background dynamics and imprints in the CMB
• Amplitudes of thermal and kinetic Sunyaev-Zel'dovich signals from small-scale CMB anisotropies
• Numerical Analysis of the Primordial Power Spectrum for (Small Field) Inflationary Potentials
• PySCo: A fast Particle-Mesh $N$-body code for modified gravity simulations in Python
• Distinguishing Primordial Magnetic Fields from Inflationary Tensor Perturbations in the Cosmic Microwave Background
• An Optimal and Model-Independent Measurement of the Intracluster Pressure Profile I: Methodology and First Applications
• Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics
• Sunyaev-Zel'dovich contribution in CMB analysis
• Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments
• Needlet estimation of cross-correlation between CMB lensing maps and LSS
• Dark Energy Survey: DESI-Independent Angular BAO Measurement
• A systematic study of projection biases in the Weak Lensing analysis of cosmic shear and the combination of galaxy clustering and galaxy-galaxy lensing
• Cosmological neutrino N-body simulations of dark matter halo
• Prospects for constraining quasar ages with fiber spectrographs: quasar-induced Ly$\alpha$ emission from the intergalactic medium
• Conformal Killing Gravity: New Constraints from DESI DR2 BAO datasets
• The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles
• Power Spectrum Emulators from Neural Networks and Tree-Based Methods
• Layered dark structure with a Structuring Field: A $Z_4$-symmetric Inert Doublet-Singlet realization and implications for the $S_8$ tension
• The pairwise and cross-pairwise y-type polarised kinetic Sunyaev Zeldovich effect from transverse velocity of galaxy clusters
• Dusty Clump Survival in Supernova Ejecta: Dust-Mediated Growth vs. Crushing by the Reverse Shock
• Forecasting Cosmological Bias due to Local Gravitational Redshift
• Emergence of the Galaxy Morphology-Star Formation Activity-Clustercentric Radius Relations in Galaxy Clusters
• Does History Repeat Itself? Periodic Time Cosmology
• Interpreting deviations between AR-VTG and GR
• An approach for the detection of point-sources in very high resolution microwave maps
• Kiloparsec-scale turbulence driven by reionization may grow intergalactic magnetic fields
• Viscous Cold Dark Matter in agreement with observations
• Dipole Distortions in the Intergalactic Medium
• Initial Conditions in the Effective Field Theory of Inflation
• Imprints of fermionic and bosonic mixed dark matter on the 21-cm signal at cosmic dawn
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Revealing the formation histories of the first stars with the cosmic near-infrared background
• Non-linear structure formation in the "Running FLRW" cosmological model
• Search for dark Higgs inflaton with curvature couplings at LHC experiments
• Pico: Parameters for the Impatient Cosmologist
• $f(R)$ gravity with broken Weyl gauge symmetry, cosmological backreaction, and its effects on CMB anisotropy
• A Foreground Model Independent Bayesian CMB Temperature and Polarization Signal Reconstruction and Cosmological Parameter Estimation over Large Angular Scales
• Neutrino masses from CMB B-mode polarization and cosmic growth rate
• A Python compressed low-$\ell$ Planck likelihood for temperature and polarization
• Estimating the Impact of foregrounds on the Future Detection of Rayleigh scattering
• Cosmological constraints on mass-varying dark matter
• Anchors no more: Using peculiar velocities to constrain $H_0$ and the primordial Universe without calibrators
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
• CMB lensing from early-formed dark matter halos
• Non-linear effects in early Universe cosmology
• A neutrino model fit to the CMB power spectrum
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• From WMAP to Planck: Exact reconstruction of 4- and 5-dimensional inflationary potential from high precision CMB measurements
• Constant-roll inflation and primordial black holes within Barrow entropic framework
• Forecasting isocurvature models with CMB lensing information: axion and curvaton scenarios
• The Angular Correlation Function as measured by the GLEAM-X Survey
• Cross bispectra and trispectra of the non-linear integrated Sachs-Wolfe effect and the tracer galaxy density field
• Missing Components in ΛCDM from DESI Y1 BAO Measurements: Insights from Redshift Remapping
• Cosmic topology. Part IIIb. Eigenmodes and correlation matrices of spin-2 perturbations in orientable Euclidean manifolds
• Shrinking the Quadratic Estimator
• Exploring Inflationary Initial State With Large Scale Structure Observations
• Artificial Neural Networks for Galaxy Clustering. Learning from the two-point correlation function of BOSS galaxies
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Inflation Story: slow-roll and beyond
• The comptonization parameter from simulations of single-frequency, single-dish, dual-beam, cm-wave observations of galaxy clusters and mitigating CMB confusion using the Planck sky survey
• Does the Reionization Model Influence the Constraints on Dark Matter Decay or Annihilation?
• Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
• Cosmological Parameter Biases from Doppler-Shifted Weak Lensing in Stage IV Experiments
• AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
• Constraints on the birth of the universe and origin of cosmic dark flow
• Number counts, confusion, mapping issues and sky coverage analysis for radio continuum surveys through EMU Early Science, EMU-ASKAP, and WODAN especially for cosmology science goals
• Neural Networks for cosmological model selection and feature importance using Cosmic Microwave Background data
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Refitting cosmological data with neutrino mass and degeneracy
• Cross-correlating the patchy screening and kinetic Sunyaev-Zel'dovich effects as a new probe of reionization
• Robustness of cosmological axion mass limits
• The effect of massive neutrinos on the BAO peak
• The Odd-Parity Part of the Observed Galaxy Trispectrum
• A gigaparsec-scale local void and the Hubble tension
• Cross-correlating the EMU Pilot Survey 1 with CMB lensing: Constraints on cosmology and galaxy bias with harmonic-space power spectra
• Can dark energy explain a high growth index?
• Selected Topics in Numerical Methods for Cosmology
• On the virialization threshold for halo mass functions
• Measuring CMB non-Gaussianity as a probe of Inflation and Cosmic Strings
• Cosmological Simulations of Satellites around Isolated Dwarf Galaxies
• The Lyman-$\alpha$ Forest from LBGs: First 3D Correlation Measurement with DESI and Prospects for Cosmology
• Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory
• Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmaking
• Cosmic Microwave Background Science at Commercial Airline Altitudes
• Probing the Type 3 interacting dark-energy model using matter pairwise velocity
• Detection likelihood of cluster-induced CMB polarization
• Cosmology in warped massive gravity
• Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA
• Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times 2$pt Photometric Survey
• Cosmological Parameter Estimation: Method
• KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• Limits in late time conversion of cold dark matter into dark radiation
• String-inspired Gauss-Bonnet Gravity Inflation and ACT
• Mock data sets for the Eboss and DESI Lyman-$\alpha$ forest surveys
• Probing the last scattering surface through the recent and future CMB observations
• Origin & evolution of the Universe
• Can Gibbons-Hawking Radiation and Inflation Arise Due to Spacetime Quanta?
• Temperature fluctuations in an inhomogeneous diffusive fluid
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• The Covariance of Photometric and Spectroscopic Two-Point Statistics: Implications for Cosmological Parameter Inference
• Smoothed quantum fluctuations and CMB observations
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Constraining effective neutrino species with bispectrum of large scale structures
• Kolmogorov complexity in the Milky Way and its reduction with warm dark matter
• Primordial non-Gaussianity systematics from redshift mismatch with SPHEREx
• Constraints on polynomial inflation under power-law perturbations
• Baryon Acoustic Oscillations in tomographic Angular Density and Redshift Fluctuations
• Weak Lensing the non-Linear Ly-alpha Forest
• Perturbations In Some Dark Energy Models
• Dipole Modulation in Tensor Modes: Signatures in CMB Polarization
• Non-Gaussianity in Cosmology: from Inflation to the CMB
• Interacting dark energy from redshift-space galaxy clustering
• Kinematic effects of the velocity fluctuations for dark halos population in LCDM model
• On the capability of high redshift kSZ measurement with galaxy surveys
• Measuring peculiar velocity and tomographic redshift dipole with DESI DR1 catalogs
• Primordial magnetic non-Gaussianity with generic vacua and detection prospects in CMB spectral distortions
• Internal dark matter structure of the most massive galaxy clusters since redshift 1
• Cylindrical cosmological simulations with StePS
• The impact of projection effects on cluster observables: stacked lensing and projected clustering
• Neural Network Acceleration of Large-scale Structure Theory Calculations
• The Hydrostatic Mass Bias and the ${\sigma }_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys
• Reionization process dependence of the ratio of CMB polarization power spectra at low-$\ell$
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• APES: Approximate Posterior Ensemble Sampler
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• Hybrid $P_{\ell }(k)$: general, unified, non-linear matter power spectrum in redshift space
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics
• CMB polarization anisotropies from cosmological reionization: extension to B-modes
• Kinetic field theory: effects of modified gravity theories with screening mechanisms on non-linear cosmic density fluctuations
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• Evaluation of multi-parameter likelihoods through iteration of two-dimensional slices
• Bayesian evidence and model selection approach for time-dependent dark energy
• Inflationary study of non-Gaussianity using two-dimensional geometrical measures of CMB temperature maps
• Enhancing Bispectrum Estimators for Galaxy Redshift Surveys with Velocities
• Testing the Anton-Schmidt dark energy model with the DESI DR2 measurements
• Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
• ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum
• Improving Photometric Galaxy Clustering Constraints With Cross-Bin Correlations
• Superhorizon isocurvature fluctuations relax tensions
• Excess of substructure due to primordial black holes
• Classification of Radio Backgrounds at Cosmic Dawn and 21 cm Signal Confirmation Using Neural Networks
• A cross-epoch endpoint-consistency test of a single effective scaling from dark energy to inflation
• Power spectrum multipoles and clustering wedges during the Epoch of Reionization
• Validating dark energy models using polarised Sunyaev-Zel'dovich effect with large-angle CMB temperature and E-mode polarization anisotropies
• A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation
• BICEP/Keck XXI: Constraints on Early-Universe Parity Violation from Multipole-Dependent Birefringence
• Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
• B-mode polarization forecasts for GreenPol
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Systematic effects on lensing reconstruction from a patchwork of CMB polarization maps
• High redshift galaxies in the ALHAMBRA survey: II. strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z <= 4.5 by PDF analysis
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
• The effect of a scanning flat fold mirror on a CMB B-mode experiment
• Constraining Early Dark Energy cosmological models with Big Bang Nucleosynthesis
• Cosmic Dipoles from Large-Scale Structure Surveys
• Revisiting observational constraints on coupled exponential quintessence with energy and momentum transfers: degeneracy with massive neutrinos
• Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB
• Accurate and efficient likelihood modeling for large-scale CMB data
• CMB lensing reconstruction from the WMAP 7-year data
• Integrated Markov Chain Monte Carlo (MCMC) analysis of primordial non-Gaussianity (f_NL) in the recent CMB data
• Late-Transition Interacting Thawer Dark Energy: Model Definition and Benchmark Consistency Tests
• Probing power spectrum enhancement at small scales with the SKA
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Ray-traced weak lensing convergence in screened modified gravity theories
• Forecasts of constraining isotropic cosmic birefringence on AliCPT-1
• J-PAS: forecast on the primordial power spectrum reconstruction
• 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
• Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference
• The Atacama Cosmology Telescope: A demonstration of CMB lensing measurement from daytime data
• Detecting the signature of helium reionization through 3HeII 3.46cm line-intensity mapping
• Probing the warm dark matter mass with [C II] intensity mapping
• Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints
• Constraints on the Modified Emergent Dark Energy Model Using DESI DR2 BAO
• Unified reconstruction of the Lyman-alpha power spectrum with Hamiltonian Monte Carlo
• Measurements of quasar proximity zones with the Ly$\alpha$ forest of DESI Y1 quasars
• Confronting phantom inflation with Planck data
• Living on the Fermi Edge: On Baryon Transport and Fermi Condensation
• Calibrating Bayesian Tension Statistics using Neural Ratio Estimation
• Detectability of Galactic Faraday Rotation in Multi-wavelength CMB Observations: A Cross-Correlation Analysis of CMB and Radio Maps
• Determining Frequentist Confidence Limits Using a Directed Parameter Space Search
• Cosmic voids and BAO with relative baryon-CDM perturbations
• How to embed any likelihood into SBI: Application to Planck + Stage IV galaxy surveys and Dynamical Dark Energy
• Spin-Torsion, Braneworlds and Changing Symmetry in the Universe
• Constraining beyond $\Lambda$CDM models with 21cm intensity mapping forecast observations combined with latest CMB data
• Statical properties of CMB B-mode polarisation in a partial sky analysis
• The Simons Observatory: Quantifying the impact of beam chromaticity on large-scale B-mode science
• Categorizing models using Self-Organizing Maps: an application to modified gravity theories probed by cosmic shear
• The Parameter-Level Performance of Covariance Matrix Conditioning in Cosmic Microwave Background Data Analyses
• Effect of the cosmological transition to metal-enriched star-formation on the hydrogen 21-cm signal
• Cosmological implications from the observed properties of CMB
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• Dark Matter Energy Deposition and Production from the Table-Top to the Cosmos
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• Towards a universal model for the density profiles of dark matter haloes
• No preference for generalized emergent dark energy from current cosmological data
• Extreme value statistics of CMB lensing deflection angles
• Breaking Free from the Swampland of Impossible Universes through the DESI Portal
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• Testing string theory with combined cosmological probes: a case study for dark matter gravitons
• Dark energy model selection with current and future data
• Three-point intrinsic alignments of galaxies and haloes in the FLAMINGO simulations
• Sector-Resolved Bayesian Model Averaging for DESI-Era Cosmology
• Braneworld Baryogenesis and QCD-Era Magnetogenesis: A Predictive Link
• Fluctuations in the Ginzburg-Landau Theory of Dark Energy: internal (in-)consistencies in PLANCK data set
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• Cosmological constraints on viable $f(R)$ models using weak lensing
• Non-Gaussian likelihood of weak lensing power spectra
• The impact of the locally measured Hubble parameter on the mass of Sterile neutrino
• Extragalactic Searches for Dark Matter Annihilation
• Towards simulating a realistic data analysis with an optimised angular power spectrum of spectroscopic galaxy surveys