Weak Gravitational Lensing of the CMB

Abstract

Weak gravitational lensing has several important effects on the cosmic microwave background (CMB): it changes the CMB power spectra, induces non-Gaussianities, and generates a B-mode polarization signal that is an important source of confusion for the signal from primordial gravitational waves. The lensing signal can also be used to help constrain cosmological parameters and lensing mass distributions. We review the origin and calculation of these effects. Topics include: lensing in General Relativity, the lensing potential, lensed temperature and polarization power spectra, implications for constraining inflation, non-Gaussian structure, reconstruction of the lensing potential, delensing, sky curvature corrections, simulations, cosmological parameter estimation, cluster mass reconstruction, and moving lenses/dipole lensing.

Accepted by Phys. Rept.; 92 pages, PDF fully hyperlinked

References in corpus (90)

• HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
• Efficient Computation of CMB anisotropies in closed FRW models
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Relativistic gravitation theory for the MOND paradigm
• An All-Sky Analysis of Polarization in the Microwave Background
• Acoustic Signatures in the Primary Microwave Background Bispectrum
• Statistics of Cosmic Microwave Background Polarization
• Signature of Gravity Waves in Polarization of the Microwave Background
• Cosmic Evolution in a Cyclic Universe
• Cosmic Microwave Background Anisotropies
• Mass Reconstruction with CMB Polarization
• Gravitational Lensing Effect on Cosmic Microwave Background Polarization
• CMB Lensing Reconstruction on the Full Sky
• Weak Lensing of the CMB: A Harmonic Approach
• Reconstruction of lensing from the cosmic microwave background polarization
• Ray Tracing Simulations of Weak Lensing by Large-Scale Structure
• A limit on the detectability of the energy scale of inflation
• The Angular Trispectrum of the CMB
• Gravitational lensing as a contaminant of the gravity wave signal in CMB
• Dark Synergy: Gravitational Lensing and the CMB
• Separation of Gravitational-Wave and Cosmic-Shear Contributions to Cosmic Microwave Background Polarization
• Determining Neutrino Mass from the CMB Alone
• Global, Exact Cosmic Microwave Background Data Analysis Using Gibbs Sampling
• A New Method for Determining Cumulative Gravitational Lensing Effects in Inhomogeneous Universes
• Reionization Revisited: Secondary CMB Anisotropies and Polarization
• Reconstructing Projected Matter Density from Cosmic Microwave Background
• The Microwave Background Bispectrum, Paper II: A Probe of the Low Redshift Universe
• Benchmark Parameters for CMB Polarization Experiments
• Lensing Reconstruction with CMB Temperature and Polarization
• The Angular Trispectra of CMB Temperature and Polarization
• Analyzing weak lensing of the cosmic microwave background using the likelihood function
• Analysis of CMB polarization on an incomplete sky
• The Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy
• Lensed CMB power spectra from all-sky correlation functions
• E/B decomposition of finite pixelized CMB maps
• Lensed CMB simulation and parameter estimation
• Observational constraints on the curvaton model of inflation
• Probing neutrino masses with CMB lensing extraction
• Small-scale CMB Temperature and Polarization Anisotropies due to Patchy Reionization
• Primordial Bispectrum Information from CMB Polarization
• Second Order Corrections to Weak Lensing by Large-Scale Structure
• Getting Around Cosmic Variance
• The influence of non-uniform reionization on the CMB
• Peculiar velocity effects in high-resolution microwave background experiments
• Lensing of the CMB: Non Gaussian aspects
• Lensing Induced Cluster Signatures in Cosmic Microwave Background
• Detection of dark matter Skewness in the VIRMOS-DESCART survey: Implications for Ω_0
• A comparison of cosmological Boltzmann codes: are we ready for high precision cosmology?
• Primordial Gravity Waves and Weak Lensing
• Direct Signature of Evolving Gravitational Potential from Cosmic Microwave Background
• Cosmic Shear of the Microwave Background: The Curl Diagnostic
• Cross-correlation of CMB with large-scale structure: weak gravitational lensing
• Rees-Sciama Effect in a CDM Universe
• Non-linear Integrated Sachs-Wolfe Effect
• Bending of Light by Gravity Waves
• Gravitational lensing of cosmic microwave background anisotropies and cosmological parameter estimation
• Aspects of the Cosmic Microwave Background Dipole
• Lensing and caustic effects on cosmological distances
• Non-Gaussian Aspects of Thermal and Kinetic Sunyaev-Zel'dovich Effects
• Microwave background polarization in cosmological models
• Principal Power of the CMB
• Weak lensing in generalized gravity theories
• CMB Temperature and Polarization Anisotropy Fundamentals
• Gravitational Time Delay Effects on CMB Anisotropies
• Geometry of weak lensing of CMB polarization
• Large Scale Structure Effects on the Gravitational Lens Image Positions and Time Delay
• Cosmic 21-cm Delensing of Microwave Background Polarization and the Minimum Detectable Energy Scale of Inflation
• Weak Lensing of the CMB: Sampling Errors on B-Modes
• Harmonic E/B decomposition for CMB polarization maps
• Average magnification effect of clumping of matter
• Weak Lensing Detection in CMB Maps
• What can be learned from the lensed cosmic microwave background B-mode polarization power spectrum?
• Detectability of tensor modes in the presence of foregrounds
• CMB-Cluster Lensing
• Lensing effect on polarization in microwave background: extracting convergence power spectrum
• CMB lensing extraction and primordial non-Gaussianity
• CMB Polarization towards Clusters as a Probe of the Integrated Sachs-Wolfe Effect
• CMB B-polarization to map the Large-scale Structures of the Universe
• Second Order Geodesic Corrections to Cosmic Shear
• Cosmic microwave background constraints on dark energy dynamics: analysis beyond the power spectrum
• Weak Lensing of the CMB: Cumulants of the Probability Distribution Function
• Constraining the dark energy dynamics with the cosmic microwave background bispectrum
• SZ polarisation as a probe of the intracluster medium
• Sunyaev Zel'dovich polarization simulation
• Lens distortion effects on CMB maps
• On the absence of gravitational lensing of the cosmic microwave background
• CMB Anisotropies in the Weak Coupling Limit
• Limits of dark energy measurements from CMB lensing-ISW-galaxy count correlations
• A Lensing Reconstruction of Primordial Cosmic Microwave Background Polarization

Cited by in corpus (761)

• Planck 2015 results. XIII. Cosmological parameters
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Planck 2013 results. XVI. Cosmological parameters
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Planck 2018 results. X. Constraints on inflation
• Weak Gravitational Lensing
• Planck 2018 results. I. Overview and the cosmological legacy of Planck
• Beyond the Cosmological Standard Model
• Revising the Halofit Model for the Nonlinear Matter Power Spectrum
• Planck 2013 results. XXII. Constraints on inflation
• Cosmology and Fundamental Physics with the Euclid Satellite
• Challenges for $\Lambda$CDM: An update
• Cosmology and fundamental physics with the Euclid satellite
• Dark Energy
• Planck 2018 results. VIII. Gravitational lensing
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
• Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
• Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Euclid. I. Overview of the Euclid mission
• CMB power spectrum parameter degeneracies in the era of precision cosmology
• The linear power spectrum of observed source number counts
• A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope
• Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
• Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity
• Testing General Relativity in Cosmology
• Gravitational Lensing
• Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy
• Planck 2013 results. XVII. Gravitational lensing by large-scale structure
• The Quest for B Modes from Inflationary Gravitational Waves
• Detection of Gravitational Lensing in the Cosmic Microwave Background
• Planck 2015 results. XIV. Dark energy and modified gravity
• The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
• Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope
• Stochastic Gravitational Wave Backgrounds
• The dark matter of gravitational lensing
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Planck 2015 results. XV. Gravitational lensing
• The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth
• Detection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope
• CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
• A measurement of gravitational lensing of the microwave background using South Pole Telescope data
• Likelihood Analysis of CMB Temperature and Polarization Power Spectra
• Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
• Probing cosmological parameters with the CMB: Forecasts from full Monte Carlo simulations
• Effective Field Theory of Cosmic Acceleration: an implementation in CAMB
• Estimators for CMB Statistical Anisotropy
• Cosmic Microwave Weak lensing data as a test for the dark universe
• Features and New Physical Scales in Primordial Observables: Theory and Observation
• Revisiting constraints on asteroid-mass primordial black holes as dark matter candidates
• Towards a cosmological neutrino mass detection
• PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White Paper
• Planck 2018 results. VI. Cosmological parameters
• Non-linear perturbation theory extension of the Boltzmann code CLASS
• Simulations of the Microwave Sky
• Weak lensing in a plasma medium and gravitational deflection of massive particles using the Gauss-Bonnet theorem. A unified treatment
• Signatures of $f(Q)$-gravity in cosmology
• The shape of the CMB lensing bispectrum
• Constraints on Large-Scale Dark Acoustic Oscillations from Cosmology
• Bulk Viscous Cosmology
• Planck 2015 results. XXI. The integrated Sachs-Wolfe effect
• On the improvement of cosmological neutrino mass bounds
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectrum at 148 and 218 GHz from the 2008 Southern Survey
• Testing General Relativity with 21 cm intensity mapping
• Phases of New Physics in the CMB
• Planck 2013 results. XVIII. Gravitational lensing-infrared background correlation
• Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter
• Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements
• The 21cm angular-power spectrum from the dark ages
• Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments
• The Kinematic Sunyaev-Zel'dovich Effect with Projected Fields: A Novel Probe of the Baryon Distribution with Planck, WMAP, and WISE Data
• Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Bias-Hardened CMB Lensing
• Limits of Quasi-Static Approximation in Modified-Gravity Cosmologies
• Exploring Cosmic Origins with CORE: Inflation
• CMB temperature lensing power reconstruction
• New constraints on $f(R)$ gravity from clusters of galaxies
• Neutrino mass in cosmology: status and prospects
• A Measurement of the Cosmic Microwave Background Gravitational Lensing Potential from 100 Square Degrees of SPTpol Data
• The Atacama Cosmology Telescope: Two-Season ACTPol Lensing Power Spectrum
• Exploring Cosmic Origins with CORE: Cosmological Parameters
• KiDS-1000 Cosmology: constraints beyond flat $\Lambda$CDM
• The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy
• The nature of the Diffuse Gamma-Ray Background
• Observable Spectra of Induced Gravitational Waves from Inflation
• Probing polarization states of primordial gravitational waves with CMB anisotropies
• The Observational Future of Cosmological Scalar-Tensor Theories
• COrE (Cosmic Origins Explorer) A White Paper
• Exploring Cosmic Origins with CORE: Survey requirements and mission design
• Detection of Thermal SZ -- CMB Lensing Cross-Correlation in Planck Nominal Mission Data
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
• Constraints on Supersymmetric Models of Hybrid Inflation
• CMB lensing tomography with the DES Science Verification galaxies
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Cosmic Rulers
• Impact of post-Born lensing on the CMB
• Delensing the CMB with the Cosmic Infrared Background
• Linear perturbations in Galileon gravity models
• Reconstructing Patchy Reionization from the Cosmic Microwave Background
• Maximum Likelihood algorithm for parametric component separation in CMB experiments
• The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies
• Asymmetric Beams and CMB Statistical Anisotropy
• Planck 2013 results. VII. HFI time response and beams
• Parameterized Post-Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity
• How to De-Rotate the Cosmic Microwave Background Polarization
• Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
• How early is early dark energy?
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• Selected topics in scalar-tensor theories and beyond
• The Atacama Cosmology Telescope: Cross-Correlation of CMB Lensing and Quasars
• BICEP2 / Keck Array VIII: Measurement of gravitational lensing from large-scale B-mode polarization
• Weak lensing of the CMB
• Maximum a posteriori CMB lensing reconstruction
• Cosmological Information from Lensed CMB Power Spectra
• Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
• A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg${}^2$ of SPTpol Temperature and Polarization Data
• The POLARBEAR Experiment
• Physical effects involved in the measurements of neutrino masses with future cosmological data
• Systematic errors in cosmic microwave background polarization measurements
• Mitigating Foreground Biases in CMB Lensing Reconstruction Using Cleaned Gradients
• Line-Intensity Mapping: Theory Review
• Reconstructing Gravity on Cosmological Scales
• Constraints on Cosmological Parameters from the 500 deg${}^2$ SPTpol Lensing Power Spectrum
• Secondary anisotropies of the CMB
• Primordial Gravitational Waves and Cosmology
• Detection of warm and diffuse baryons in large scale structure from the cross-correlation of gravitational lensing and the thermal Sunyaev-Zeldovich effect
• The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data
• Cross-correlation between the CMB lensing potential measured by Planck and high-z sub-mm galaxies detected by the Herschel-ATLAS survey
• Full-sky lensing shear at second order
• Future CMB tests of dark matter: ultra-light axions and massive neutrinos
• De-Rotation of the Cosmic Microwave Background Polarization: Full-Sky Formalism
• Future CMB Constraints on Early, Cold, or Stressed Dark Energy
• The Kinematic Sunyaev-Zel'dovich Effect with Projected Fields II: prospects, challenges, and comparison with simulations
• Imprints of Relic Gravitational Waves in Cosmic Microwave Background Radiation
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• The parameter space in Galileon gravity models
• Constraints on coupled dark energy using CMB data from WMAP and SPT
• The cosmic microwave background bispectrum from the non-linear evolution of the cosmological perturbations
• First Measurement of the Cross-Correlation of CMB Lensing and Galaxy Lensing
• Consistency test of general relativity from large scale structure of the Universe
• Foreground-immune CMB lensing with shear-only reconstruction
• An exact Jacobi map in the geodesic light-cone gauge
• Full covariance of CMB and lensing reconstruction power spectra
• CMB lensing and primordial non-Gaussianity
• $Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis
• unWISE tomography of Planck CMB lensing
• H0 tension or T0 tension?
• Faraday Rotation Limits on a Primordial Magnetic Field from WMAP Five-Year Data
• DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos
• Model-independent cosmological constraints from the CMB
• CMB Delensing Beyond the B Modes
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• DeepCMB: Lensing Reconstruction of the Cosmic Microwave Background with Deep Neural Networks
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• Effect of Peculiar Motion in Weak Lensing
• The Cosmic Microwave Background and the Ionization History of the Universe
• Exploring redshift-space distortions in large-scale structure
• A 2500 square-degree CMB lensing map from combined South Pole Telescope and Planck data
• Effects of modified gravity on B-mode polarization
• Internal delensing of Planck CMB temperature and polarization
• Lower bias, lower noise CMB lensing with foreground-hardened estimators
• CMB weak-lensing beyond the Born approximation: a numerical approach
• Quadratic estimators for CMB weak lensing
• Massive neutrinos and cosmic composition
• A WISE measurement of the ISW effect
• Demonstration of cosmic microwave background delensing using the cosmic infrared background
• Reconstruction of the remote dipole and quadrupole fields from the kinetic Sunyaev Zel'dovich and polarized Sunyaev Zel'dovich effects
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• CMB Lensing Constraints on Neutrinos and Dark Energy
• Finite distance corrections to the light deflection in a gravitational field with a plasma medium
• On the joint analysis of CMB temperature and lensing-reconstruction power spectra
• Sachs-Wolfe at second order: the CMB bispectrum on large angular scales
• A bias to CMB lensing measurements from the bispectrum of large-scale structure
• Non-Gaussian structure of the lensed CMB power spectra covariance matrix
• Exploring cosmic origins with CORE: gravitational lensing of the CMB
• The Signature of Proper Motion in the Microwave Sky
• Prospects for Delensing the Cosmic Microwave Background for Studying Inflation
• Gravitational lensing of massive particles in Schwarzschild gravity
• The intrinsic bispectrum of the Cosmic Microwave Background [PhD thesis]
• Measuring cluster masses with CMB lensing: a statistical approach
• Lensing of 21-cm Fluctuations by Primordial Gravitational Waves
• Compensated Isocurvature Perturbations and the Cosmic Microwave Background
• The real shape of non-Gaussianities
• Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
• Using correlations between CMB lensing and large-scale structure to measure primordial non-Gaussianity
• The Benefits of CMB Delensing
• Cross-correlation of gravitational lensing from DES Science Verification data with SPT and Planck lensing
• The history of star formation from the cosmic infrared background anisotropies
• Density and temperature of cosmic-web filaments on scales of tens of megaparsecs
• Measuring our peculiar velocity on the CMB with high-multipole off-diagonal correlations
• Measuring the tensor to scalar ratio from CMB B-modes in presence of foregrounds
• Fitting the nonlinear matter bispectrum by the Halofit approach
• Optimal CMB Lensing Reconstruction and Parameter Estimation with SPTpol Data
• Bias to CMB Lensing Reconstruction from Temperature Anisotropies due to Large-Scale Galaxy Motions
• Efficient Evaluation of Cosmological Angular Statistics
• Galaxy-CMB and galaxy-galaxy lensing on large scales: sensitivity to primordial non-Gaussianity
• Constraints on early dark energy from CMB lensing and weak lensing tomography
• Full-sky CMB lensing reconstruction in presence of sky-cuts
• Constraints on dark-matter properties from large-scale structure
• Warm Intermediate Inflation in $F(T)$ Gravity
• Constraining the Baryon Abundance with the Kinematic Sunyaev-Zel'dovich Effect: Projected-Field Detection Using Planck, WMAP, and unWISE
• The Kinetic Sunyaev-Zel'dovich Effect from Reionization: Simulated Full Sky Maps at Arcminute Resolution
• A Large Sky Simulation of the Gravitational Lensing of the Cosmic Microwave Background
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• Full-sky maps for gravitational lensing of the CMB
• Lensing Reconstruction in Post-Born Cosmic Microwave Background Weak Lensing
• Search for Compensated Isocurvature Perturbations with Planck Power Spectra
• Probing the neutrino mass hierarchy with CMB weak lensing
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• CMB-lensing beyond the Born approximation
• Multitracer CMB delensing maps from Planck and WISE data
• The full squeezed CMB bispectrum from inflation
• Planck confronts large scale structure: methods to quantify discordance
• CMB Lensing Beyond the Power Spectrum: Cosmological Constraints from the One-Point PDF and Peak Counts
• Intrinsic alignments in the cross-correlation of cosmic shear and CMB weak lensing
• Constraining Fundamental Physics with Future CMB Experiments
• Baryons do trace dark matter 380,000 years after the big bang: Search for compensated isocurvature perturbations with WMAP 9-year data
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• A 3-D model of polarised dust emission in the Milky Way
• Modeling CMB Lensing Cross Correlations with {\sc CLEFT}
• Boltzmann hierarchy for the cosmic microwave background at second order including photon polarization
• New Optimised Estimators for the Primordial Trispectrum
• Cosmology with dropout selection: Straw-man surveys and CMB lensing
• Evidence of cross-correlation between the CMB lensing and the gamma-ray sky
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Dark energy records in lensed cosmic microwave background
• Do we care about the distance to the CMB? Clarifying the impact of second-order lensing
• Constraints on neutrino mass from Cosmic Microwave Background and Large Scale Structure
• Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
• A Demonstration of Improved Constraints on Primordial Gravitational Waves with Delensing
• Reducing distance errors for standard candles and standard sirens with weak-lensing shear and flexion maps
• An extensive investigation of the Generalised Dark Matter model
• Odd-Parity Bipolar Spherical Harmonics
• Tensions between direct measurements of the lens power spectrum from Planck data
• Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time
• Constraining warm dark matter with cosmic shear power spectra
• On the effect of non-Gaussian lensing deflections on CMB lensing measurements
• Integrated Sachs Wolfe Effect and Rees Sciama Effect
• CMB Lensing Reconstruction in Real Space
• Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing
• Cosmic shear bispectrum from second-order perturbations in General Relativity
• Search for features in the spectrum of primordial perturbations using Planck and other datasets
• Probing dark energy and neutrino mass from upcoming lensing experiments of CMB and galaxies
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• A new approach to the propagation of light-like signals in perturbed cosmological backgrounds
• Internal delensing of Cosmic Microwave Background polarization B-modes with the POLARBEAR experiment
• Separating E and B types of polarization on an incomplete sky
• The Simons Observatory: Constraining inflationary gravitational waves with multi-tracer B-mode delensing
• Aberrating the CMB sky: fast and accurate computation of the aberration kernel
• Reconstruction of the neutrino mass as a function of redshift
• Gravitational lensing of a Schwarzschild-like black hole in Kalb-Ramond gravity
• The Atacama Cosmology Telescope: A Measurement of the Thermal Sunyaev-Zel'dovich Effect Using the Skewness of the CMB Temperature Distribution
• The inner mass power spectrum of galaxies using strong gravitational lensing: beyond linear approximation
• Weak-lensing observables in relativistic N-body simulations
• B-Pol: Detecting Primordial Gravitational Waves Generated During Inflation
• Cornering the Planck $A_{lens}$ tension with future CMB data
• Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Design and development of an ambient-temperature continuously-rotating achromatic half-wave plate for CMB polarization modulation on the POLARBEAR-2 experiment
• CMB-lensing beyond the leading order: temperature and polarization anisotropies
• Charged black-bounce spacetimes: Photon rings, shadows and observational appearances
• Transverse Velocities with the Moving Lens Effect
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• CMB-S4: Iterative Internal Delensing and $r$ Constraints
• Improved cosmic microwave background (de-)lensing using general spherical harmonic transforms
• 2-FAST: Fast and accurate computation of projected two-point functions
• Lensing reconstruction from PLANCK sky maps: inhomogeneous noise
• Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies
• CMB Lensing Bispectrum from Nonlinear Growth of the Large Scale Structure
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• What can CMB observations tell us about the neutrino distribution function?
• Foreground Biases on Primordial Non-Gaussianity Measurements from the CMB Temperature Bispectrum: Implications for Planck and Beyond
• 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
• Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
• QuickPol: Fast calculation of effective beam matrices for CMB polarization
• MUSE: Marginal Unbiased Score Expansion and Application to CMB Lensing
• Bayesian inference of CMB gravitational lensing
• Information Content of Higher-Order Galaxy Correlation Functions
• Detecting relic gravitational waves in the CMB: Optimal parameters and their constraints
• Cosmological ensemble and directional averages of observables
• Foreground-immune CMB lensing reconstruction with polarization
• Weak Lensing of Intensity Mapping: the Cosmic Infrared Background
• Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background
• Transport equations for the inflationary trispectrum
• Bias-Hardened CMB Lensing with Polarization
• Weak Lensing of the Cosmic Microwave Background by Foreground Gravitational Waves
• Weighing Neutrinos in $f(R)$ gravity
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg${}^2$ SPT-SZ and Planck Gravitational Lensing Map
• Effect of lensing non-Gaussianity on the CMB power spectra
• Dependence of the Cosmic Microwave Background Lensing Power Spectrum on the Matter Density
• CoLoRe: fast cosmological realisations over large volumes with multiple tracers
• Cosmological Constraint on the Light Gravitino Mass from CMB Lensing and Cosmic Shear
• Relieving tensions related to the lensing of CMB temperature power spectra
• On the road to discovery of relic gravitational waves: The TE and BB Correlations in the cosmic microwave background radiation
• Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
• Mapping the Integrated Sachs-Wolfe Effect
• Fast and easy super-sample covariance of large scale structure observables
• Polarized Sunyaev Zel'dovich tomography
• Weak-lensing by the large scale structure in a spatially anisotropic universe: theory and predictions
• Intrinsic alignment contamination to CMB lensing-galaxy weak lensing correlations from tidal torquing
• Light propagation in inhomogeneous and anisotropic cosmologies
• Impact of next-to-leading order contributions to CMB lensing
• Consistency relations for large-scale structure in modified gravity and the matter bispectrum
• Can modified gravity models reconcile the tension between CMB anisotropy and lensing maps in Planck-like observations?
• Cosmic Shear from Scalar-Induced Gravitational Waves
• Unified Treatment of the Luminosity Distance in Cosmology
• The intrinsic B-mode polarisation of the Cosmic Microwave Background
• Towards testing CMB anomalies using the kinetic and polarized Sunyaev Zel'dovich effects
• Supernovae, Lensed CMB and Dark Energy
• Cosmic Microwave Background Acoustic Peak Locations
• Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing
• Weak lensing induced by second-order vector mode
• CMB Lensing Constraints on Dark Energy and Modified Gravity Scenarios
• Disentangling Dark Physics with Cosmic Microwave Background Experiments
• On the current status of Modified Gravity
• The Intrinsic Matter Bispectrum in $\Lambda$CDM
• CMB internal delensing with general optimal estimator for higher-order correlations
• CMB Constraints on the Stochastic Gravitational-Wave Background at Mpc scales
• Rayleigh scattering: blue sky thinking for future CMB observations
• Stacked CMB lensing and ISW signals around superstructures in the DESI Legacy Survey
• Detectability of CMB tensor B modes via delensing with weak lensing galaxy surveys
• Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum from Two Years of POLARBEAR Data
• Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra
• Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
• Likelihood methods for CMB experiments
• Do baryons trace dark matter in the early universe?
• Detecting relics of a thermal gravitational wave background in the early Universe
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Circular Polarization of the Astrophysical Gravitational Wave Background
• The Simons Observatory: pipeline comparison and validation for large-scale B-modes
• Lensing power spectrum of the Cosmic Microwave Background with deep polarization experiments
• Impact of polarisation on the intrinsic CMB bispectrum
• Measuring Distance Ratios with CMB-Galaxy Lensing Cross-correlations
• The effect of inhomogeneities on the distance to the last scattering surface and the accuracy of the CMB analysis
• Reconstructing Small Scale Lenses from the Cosmic Microwave Background Temperature Fluctuations
• Lensed CMB temperature and polarization maps from the Millennium Simulation
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Constraints on standard and non-standard early Universe models from CMB B-mode polarization
• How to make a clean separation between CMB E and B modes with proper foreground masking
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Baryons still trace dark matter: probing CMB lensing maps for hidden isocurvature
• Foreground Separation and Constraints on Primordial Gravitational Waves with the PICO Space Mission
• Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
• Contamination of early-type galaxy alignments to galaxy lensing-CMB lensing cross-correlation
• Weak lensing generated by vector perturbations and detectability of cosmic strings
• Full-sky formulae for weak lensing power spectra from total angular momentum method
• Scaling Transformations and the Origins of Light Relics Constraints from Cosmic Microwave Background Observations
• CMB anisotropy science: a review
• Isotropy analyses of the Planck convergence map
• Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors
• Gravitational lens effect of a holonomy corrected Schwarzschild black hole
• The perturbative approach for the weak deflection angle
• CMB lensing and primordial squeezed non-Gaussianity
• Calibrating Cluster Number Counts with CMB lensing
• 3D Weak Gravitational Lensing of the CMB and Galaxies
• Improving Small-Scale CMB Lensing Reconstruction
• Multiple Lensing of the Cosmic Microwave Background anisotropies
• Lensing anomaly and oscillations in the primordial power spectrum
• The information content of cosmic microwave background anisotropies
• Impact of modulation on CMB B-mode polarization experiments
• Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam
• Improved estimation of cluster mass profiles from the cosmic microwave background
• Non-linear general relativistic effects in the observed redshift
• Limitations of CMB B-mode template delensing
• Observational test for $f(Q)$ gravity with weak gravitational lensing
• Galaxy shear estimation from stacked images
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• High precision simulations of weak lensing effect on Cosmic Microwave Background polarization
• Optimal multifrequency weighting for CMB lensing
• Expected dipole asymmetry in CMB polarization
• Physics of the cosmic microwave background anisotropy
• Pairwise Transverse Velocity Measurement with the Rees-Sciama Effect
• Perturbative deflection angle for signal with finite distance and general velocities
• Weak lensing B-modes on all scales as a probe of local isotropy
• Do cosmological data rule out $f(\mathcal{R})$ with $w\ne -1$?
• A cryogenic continuously rotating half-wave plate for the POLARBEAR-2b cosmic microwave background receiver
• CMB B-mode non-Gaussianity: optimal bispectrum estimator and Fisher forecasts
• Probing for the Cosmological Parameters with PLANCK Measurement
• Cosmological parameter constraints from CMB lensing with cosmic voids
• Weak Lensing of the Primary CMB Bispectrum
• General and consistent statistics for cosmological observations
• Optimal filters for the moving lens effect
• Interpreting the CMB aberration and Doppler measurements: boost or intrinsic dipole?
• A Semi-analytic Ray-tracing Algorithm for Weak Lensing
• Oscillating modulation to B-mode polarization from varying propagating speed of primordial gravitational waves
• New operator approach to the CMB aberration kernels in harmonic space
• Rotation of the cosmic microwave background polarization from weak gravitational lensing
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Comparison of delensing methodologies and assessment of the delensing capabilities of future experiments
• Lensing in the Geodesic Light-Cone coordinates and its (exact) illustration to an off-center observer in Lemaître-Tolman-Bondi models
• A Constraint On the Integrated Mass Power Spectrum out to z = 1100 from Lensing of the Cosmic Microwave Background
• Measuring Planck beams with planets
• Synergies between radio, optical and microwave observations at high redshift
• Non-Gaussian Covariance of CMB B-modes of Polarization and Parameter Degradation
• Precision of diffuse 21-cm lensing
• Non-Gaussian Structure of B-mode Polarization after Delensing
• Clustering dark energy imprints on cosmological observables of the gravitational field
• Statistical diagnostics to identify Galactic foregrounds in B-mode maps
• Baryonic effects on CMB lensing and neutrino mass constraints
• Optimal filtering for CMB lensing reconstruction
• Testing CPT Symmetry with Current and Future CMB Measurements
• LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
• Probing the statistical properties of CMB $B$-mode polarization through Minkowski Functionals
• Optimal constraints on primordial gravitational waves from the lensed CMB
• Weak gravitational lensing of intrinsically aligned galaxies
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• A hybrid approach to CMB lensing reconstruction on all-sky intensity maps
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• Optimization Study for the Experimental Configuration of CMB-S4
• Constraining cosmology with the cosmic microwave and infrared backgrounds correlation
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Probing spatial variation of the fine-structure constant using the CMB
• New Constraints on Anisotropic Rotation of CMB Polarization
• Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure
• The Cold Spot as a Large Void: Lensing Effect on CMB Two and Three Point Correlation Functions
• Litmus Test for Cosmic Hemispherical Asymmetry in the Cosmic Microwave Background B-mode polarization
• BoloCalc: a sensitivity calculator for the design of Simons Observatory
• Mass Estimation of Galaxy Clusters with Deep Learning II: CMB Cluster Lensing
• Gauge-Invariant Formalism of Cosmological Weak Lensing
• Weak Lensing of Baryon Acoustic Oscillations
• Linear perturbations in K-mouflage cosmologies with massive neutrinos
• The relativistic galaxy number counts in the weak field approximation
• Improving models of the cosmic infrared background using CMB lensing mass maps
• Reconstructing Patchy Reionization with Deep Learning
• Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
• The Cosmic Neutrino Background Anisotropy - Linear Theory
• Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
• Second-order gauge-invariant formalism for the cosmological observables: Complete verification of their gauge-invariance
• Lensing signals from Spin-2 perturbations
• Expressions for optical scalars and deflection angle at second order in terms of curvature scalars
• Reconstructing the Primary CMB Dipole
• Lensing reconstruction of cluster-mass cross-correlation with cosmic microwave background polarization
• Late time sky as a probe of steps and oscillations in primordial Universe
• Born-corrections to weak lensing of the cosmic microwave background temperature and polarisation anisotropies
• Detecting relic gravitational waves in the CMB: Comparison of different methods
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• Robust Evidence for Dynamical Dark Energy from DESI Galaxy-CMB Lensing Cross-Correlation and Geometric Probes
• Planck intermediate results. XLI. A map of lensing-induced B-modes
• New constraints on cosmic polarization rotation from the ACTPol cosmic microwave background B-Mode polarization observation and the BICEP2 constraint update
• Testing physical models for dipolar asymmetry: from temperature to k space to lensing
• The impact of extragalactic foregrounds on internal delensing of CMB B-mode polarization
• Discrimination between Lambda-CDM, quintessence, and modified gravity models using wide area surveys
• Lenses in the forest: cross-correlation of the Lyman-alpha flux with CMB lensing
• 3D Weak Lensing: Modified Theories of Gravity
• Geodesic "curve"-of-sight formulae for the cosmic microwave background: a unified treatment of redshift, time delay, and lensing
• Foreground model recognition through Neural Networks for CMB B-mode observations
• 21cmFirstCLASS I. Cosmological tool for $\Lambda$CDM and beyond
• Probing cosmic strings by reconstructing polarization rotation of the cosmic microwave background
• Neutrinos and dark energy constraints from future galaxy surveys and CMB lensing information
• Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
• The correlation of extragalactic $\gamma$-rays with cosmic matter density distributions from weak-gravitational lensing
• Delensing the CMB with the cosmic infrared background: the impact of foregrounds
• Jacobi Mapping Approach for a Precise Cosmological Weak Lensing Formalism
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Magnification Bias Estimators for Realistic Surveys: an Application to the BOSS Survey
• An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators
• New Constraints on Cosmic Polarization Rotation from B-Mode Polarization in Cosmic Microwave Background
• CMB spectra and bispectra calculations: making the flat-sky approximation rigorous
• Formulating Weak Lensing from the Boltzmann Equation and Application to Lens-lens Couplings
• Clustering of Local Extrema in Planck CMB maps
• Spectral distortions in the cosmic microwave background polarization
• Simulated reconstruction of the remote dipole field using the kinetic Sunyaev Zel'dovich effect
• CMB Mode Coupling with Isotropic Polarization Rotation
• B polarization of cosmic background radiation from second-order scattering sources
• An accurate analytic mass model for lensing galaxies
• Reconstruction of primordial tensor power spectra from B-mode polarization of the cosmic microwave background
• CMB probes on the correlated axion isocurvature perturbation
• Revised estimates of CMB $B$-mode polarization induced by patchy reionization
• The cross-correlation between 3d cosmic shear and the integrated Sachs-Wolfe effect
• Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimation
• Intensity mapping of the 21cm emission: lensing
• Patchy Screening of the CMB from Dark Photons
• CMB seen through random Swiss Cheese
• Lensing simulations by Taylor expansion -- not so inefficient after all
• Cosmological Probes of Structure Growth and Tests of Gravity
• Weak Deflection Angle, Greybody Bound and Shadow for Charged Massive BTZ Black Hole
• Cubic Derivative Interactions and Asymptotic Dynamics of the Galileon Vacuum
• Real-world CMB lensing quadratic estimator power spectrum response
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• Cosmologically probing ultra-light particle dark matter using 21 cm signals
• Robust and efficient CMB lensing power spectrum from polarization surveys
• Lensing as a Probe of Early Universe: from CMB to Galaxies
• Neutrino mass tension or suppressed growth rate of matter perturbations?
• Constraining Light Gravitino Mass from Cosmic Microwave Background
• Detecting Relic Gravitational Waves in the CMB: Comparison of Planck and Ground-based Experiments
• Universal Weak Lensing Distortion of Cosmological Correlation Functions
• From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI
• Cosmology before noon with multiple galaxy populations
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Observing relativistic features in large-scale structure surveys -- II: Doppler magnification in an ensemble of relativistic simulations
• Target Neutrino Mass Precision for Determining the Neutrino Hierarchy
• A new line-of-sight approach to the non-linear Cosmic Microwave Background
• Cosmology from the kinetic polarized Sunyaev Zel'dovich effect
• Real space lensing reconstruction using cosmic microwave background polarization
• CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations
• CMB Lens Sample Covariance and Consistency Relations
• Real space estimator for the weak lensing convergence from the CMB
• Flat Universe with Hyperbolic Voids
• CMB lensing reconstruction using cut sky polarization maps and pure-$B$ modes
• Parameter constraints from weak lensing tomography of galaxy shapes and cosmic microwave background fluctuations
• Rotation of the CMB polarisation by foreground lensing
• A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing
• Constraining f(R) gravity with cross-correlation of galaxies and cosmic microwave background lensing
• Cosmic Microwave Background Bispectrum from the Lensing--Rees-Sciama Correlation Reexamined: Effects of Non-linear Matter Clustering
• CMB lensing with shear-only reconstruction on the full sky
• On a possible nonequilibrium imprint in the cosmic background at low frequencies
• Lensing covariance on cut sky and SPT-Planck lensing tensions
• Lensed Cosmic Microwave Background Constraints on Post-General Relativity Parameters
• Evolution of Primordial Neutrino Helicities in Cosmic Gravitational Inhomogeneities
• Cosmology using numerical relativity
• Cross-Correlation of Far-Infrared Background Anisotropies and CMB Lensing from Herschel and Planck satellites
• Dynamical systems analysis of the cubic galileon beyond the exponential potential and the cosmological analogue of the vDVZ discontinuity
• Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen
• On the asymptotic connection between full- and flat-sky angular correlators
• Application of cross correlations between CMB and large scale structure to constraints on the primordial non-Gaussianity
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• Inference of gravitational lensing and patchy reionization with future CMB data
• Excess of lensing amplitude in the Planck CMB power spectrum
• Effects of Destriping Errors on CMB Polarisation Power Spectra and and Pixel Noise Covariances
• Is patchy reionization an obstacle in detecting the primordial gravitational wave signal?
• $\alpha$-attractor dark energy in view of next-generation cosmological surveys
• Reconstructing Cosmic Polarization Rotation with ResUNet-CMB
• Tetrad formalism for exact cosmological observables
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Detecting relic gravitational waves in the CMB: The contamination caused by the cosmological birefringence
• Lensing-induced morphology changes in CMB temperature maps in modified gravity theories
• Weak lensing of the Lyman-alpha forest
• LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB
• Impact of Instrumental Systematic Contamination on the Lensing Mass Reconstruction using the CMB Polarization
• CMBR Weak Lensing and HI 21-cm Cross-correlation Angular Power Spectrum
• Delensing Degree-Scale $B$-Mode Polarization with High-Redshift Line Intensity Mapping
• Cross-correlations of the Lyman-alpha forest with weak lensing convergence I: Analytical Estimates of S/N and Implications for Neutrino Mass and Dark Energy
• Lensing smoothing of BAO wiggles
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• Probing early structure and model-independent neutrino mass with high-redshift CMB lensing mass maps
• Weak lensing of CMB by cosmic (super-)strings
• Noise Estimates for Measurements of Weak Lensing from the Lyman-alpha Forest
• Testing for spectral index variations in polarised CMB foregrounds
• A New Window into Stochastic Gravitational Wave Background
• Evidence of dark energy in different cosmological observations
• Free-Streaming Neutrinos and Their Phase Shift in Current and Future CMB Power Spectra
• The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
• Deflection angle with electromagnetic interaction and gravitational-electromagnetic dual lensing
• Joint analyses of 2D CMB lensing and 3D galaxy clustering in the spherical Fourier-Bessel basis
• Testing inflationary consistency relations by the potential CMB observations
• Impact of Anisotropic Birefringence on Measuring Cosmic Microwave Background Lensing
• A Clipping Method to Mitigate the Impact of Catastrophic Photometric Redshift Errors on Weak Lensing Tomography
• The Integrated Sachs-Wolfe Effect in the Bulk Viscous Dark Energy Model
• Morphology of CMB fields -- effect of weak gravitational lensing
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Simulations for 21 cm radiation lensing at EoR redshifts
• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
• Understanding the neutrino mass constraints achievable by combining CMB lensing and spectroscopic galaxy surveys
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• The redshifted HI 21 cm signal from the post-reionization epoch: Cross-correlations with other cosmological probes
• A cross-correlation analysis of CMB lensing and radio galaxy maps
• High resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations
• The role of $T_0$ in CMB anisotropy measurements
• Local patch analysis for testing statistical isotropy of the Planck convergence map
• Gravitational lensing of the cosmic microwave background by nonlinear structures
• Planck intermediate results. LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect
• Delensing of Cosmic Microwave Background Polarization with machine learning
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• Impact of SZ cluster residuals in CMB maps and CMB-LSS cross-correlations
• The Jacobi map for gravitational lensing: the role of the exponential map
• Probing Neutrinos from Planck and Forthcoming Galaxy Redshift Surveys
• The Impact of Secondary non-Gaussianities in the CMB on Cosmological Parameter Estimation
• Detecting the Cold Spot as a Void with the Non-Diagonal Two-Point Function
• Skewing the CMB$\times$LSS: a Fast Method for Bispectrum Analysis
• Detection of relic gravitational waves in the CMB: Prospects for CMBPol mission
• Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
• Impact of nonlinear growth of the large-scale structure on CMB B-mode delensing
• Signatures of the Baryon Acoustic Oscillations on the Convergence Power Spectrum of Weak lensing by Large Scale Structure
• How Sensitive is the CMB to a Single Lens?
• Unveiling Neutrino Halos with CMB Lensing
• Probing the Cosmological Principle with weak lensing shear
• Exact CMB B-mode power spectrum from anisotropic cosmic birefringence
• Improved Modeling of the Kinematic Sunyaev-Zel'dovich Projected-Fields signal and its Cosmological Dependence
• Improving Constraints on Models Addressing the Hubble Tension with CMB Delensing
• New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• CMB lensing reconstruction with point source masks
• Unified approach to secondary effects on the CMB B-mode polarization
• Constraints on primordial non-Gaussianity from Galaxy-CMB lensing cross-correlation
• The reconstructed CMB lensing bispectrum
• Lens covariance effects on likelihood analyses of CMB power spectra
• Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies
• Optimising Boltzmann codes for the Planck era
• Galaxy-cluster masses via 21st-century measurements of lensing of 21-cm fluctuations
• Normalizing flows for random fields in cosmology
• Reassessing Dust's Role in Forming the CMB
• The CIB-lensing bispectrum: impact on primordial non-Gaussianity and detectability for the Planck mission
• Evolution of intrinsic ellipticity correlations due to peculiar motion
• Single-Field Inflation and the Local Ansatz: Distinguishability and Consistency
• Improving Constraints on Inflation with CMB Delensing
• Beyond scalar, vector and tensor harmonics in maximally symmetric three-dimensional spaces
• Effect of electric interaction on the deflection and gravitational lensing in the strong field limit
• Solar System-scale interferometry on fast radio bursts could measure cosmic distances with sub-percent precision
• Joint Bayesian estimation of tensor and lensing B-modes in the power spectrum of CMB polarization data
• Flat-sky Angular Power Spectra Revisited
• N-body lensed CMB maps: lensing extraction and characterization
• Cosmic topology. Part IIIa. Microwave background parity violation without parity-violating microphysics
• Full-sky weak lensing: a nonlinear post-Friedmann treatment
• Quantifying the statistics of CMB-lensing-derived galaxy cluster mass measurements with simulations
• Cosmology at high redshift -- a probe of fundamental physics
• A comparison of CMB lensing efficiency of gravitational waves and large scale structure
• A framework to mitigate patchy reionization contamination on the primordial gravitational wave signal
• Probing inflation with CMB polarization : weak lensing effect on the covariance of CMB spectra
• The Atacama Cosmology Telescope: Delensed Power Spectra and Parameters
• Improving CMB non-Gaussianity estimators using tracers of local structure
• Astrophysical Searches and Constraints on Ultralight Bosonic Dark Matter
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Controlling systematics in ground-based CMB surveys with partial boresight rotation
• Perturbative deflection angles of timelike rays
• CMB Lensing and Scale Dependent New Physics
• Detecting the tensor-to-scalar ratio with the pure pseudospectrum reconstruction of $B$-mode
• Cluster profiles from beyond-the-QE CMB lensing mass maps
• Delensing Galaxy Surveys
• Probing Quintessence Potential with Future Cosmological Surveys
• CMB lensing power spectrum without noise bias
• Impact of Low ell's on Large Scale Structure Anomalies
• Gravity waves from cosmic bubble collisions
• Impact of thermal SZ effect on cross-correlations between Planck CMB lensing and SDSS galaxy density fields
• Thermal gravitational-wave background in the general pre-inflationary scenario
• Estimating small angular scale CMB anisotropy with high resolution N-body simulations: weak lensing
• Statistical imprints of CMB B-type polarization leakage in an incomplete sky survey analysis
• Higher-Order Gravitational Lensing Reconstruction using Feynman Diagrams
• By Dawn's Early Light: CMB Polarization Impact on Cosmological Constraints
• A measurement of cluster masses using Planck and SPT-SZ CMB lensing
• Design and characterization of a ground-based absolute polarization calibrator for use with polarization sensitive CMB experiments
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• Lensing reconstruction from the cosmic microwave background polarization with machine learning
• The Simons Observatory: Assessing the Impact of Dust Complexity on the Recovery of Primordial $B$-modes
• Blind Map Level Systematics Cleaning: A Quadratic Estimator Approach
• A deconvolution map-making method for experiments with circular scanning strategies
• Conformal invariant cosmological perturbations via the covariant approach
• Gravitational Lensing of the Cosmic Neutrino Background
• The first direct measurement of gravitational potential decay rate at cosmological scales and improved dark energy constraint
• Observable cosmological vector mode in the dark ages
• EBWeyl: a Code to Invariantly Characterize Numerical Spacetimes
• The art of building a smooth cosmic distance ladder in a perturbed universe
• The interplay of CMB temperature lensing power reconstruction with primordial non-Gaussianity of local type
• New probe of inflationary gravitational waves: cross-correlations of lensed primary CMB B-modes with large-scale structure
• The Effect of Lensing on the Large-Scale CMB Anisotropy
• Reconstructing patchy helium reionization using the cosmic microwave background and large-scale structure
• A Pop III generated dust screen at z~16
• Spectral Distortion Signatures of Step-like Inflationary Potential
• Exploring sub-GeV Dark Matter Physics with Cosmic Ray and Future Telescopes
• Cool dark sector, concordance, and a low ${\sigma }_8$
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Cosmic variance mitigation in measurements of the integrated Sachs-Wolfe effect
• On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations
• Optimistic estimation on probing primordial gravitational waves with CMB B-mode polarization
• Matter power spectrum reconstruction with KiDS-Legacy: Improved internal $\Lambda$CDM consistency and preference for strong baryonic feedback
• Impact of a primordial magnetic field on cosmic microwave background $B$ modes with weak lensing
• Reconstructing the Gravitational Lensing Potential from the Lyman-$\alpha$ Forest
• Characterization of Extragalactic Point-Sources on E- and B-mode Maps of the CMB Polarization
• A wide-angle formulation of foreground filters for HI intensity mapping
• The parity-odd Intrinsic Bispectrum
• The imprint of primordial gravitational waves on the CMB intensity profile
• The Atacama Cosmology Telescope: Mitigating the impact of extragalactic foregrounds for the DR6 CMB lensing analysis
• Testing Cotton gravity as dark matter substitute with weak lensing
• Cosmology with Planck T-E correlation coefficient
• A Minkowski Functional Analysis of the Cosmic Microwave Background Weak Lensing Convergence
• The Moving Lens Effect: Simulations, Forecasts and Foreground Mitigation
• Improving Cosmic Birefringence Constraints via Delensing
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey
• Gauss-Bonnet lensing of spinning massive particles in static spherically symmetric spacetimes
• CMB anisotropies from patchy reionisation and diffuse Sunyaev-Zel'dovich effects
• Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements
• A Novel Bispectrum Estimator of the Kinematic Sunyaev-Zel'dovich Effect using Projected Fields
• An Estimator for the lensing potential from galaxy number counts
• Towards reconstruction of unlensed, intrinsic CMB power spectra from lensed map
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Model independent variance cancellation in CMB lensing cross-correlations
• Distortions in the Surface of Last Scattering
• KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies
• Mapping possible non-Gaussianity in the Planck maps
• Is there a need for dark matter in galaxies?
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Effects of boosting on extragalactic components: methods and statistical studies
• Lensing anomalies from the epoch of reionisation
• Delensing for Precision Cosmology: Optimizing Future CMB B-mode Surveys to Constrain r
• CMB delensing with deep learning
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone
• Detecting cosmic voids via maps of geometric-optics parameters
• Small Correlated Against Large Estimator (SCALE) for Cosmic Microwave Background Lensing
• 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
• Cosmological Implications of a Neutrino Mass Detection
• Approximate Likelihood Approaches for Detecting the Influence of Primordial Gravitational Waves in Cosmic Microwave Background Polarization
• CMB polarization analysis on circular scans
• Baryonic effects in the Effective Field Theory of Large-Scale Structure and an analytic recipe for lensing in CMB-S4
• Excessive shift of the CMB acoustic peaks of the Cold Spot area
• Needlet estimation of cross-correlation between CMB lensing maps and LSS
• A New Probe of Gaussianity and Isotropy applied to the CMB Maps
• Observable CMB B-modes from Cosmological Phase Transitions
• Weak Gravitational Lensing of CMB - Revisit
• Deflection and gravitational lensing of null and timelike signals in general asymptotically (anti-)de Sitter spacetimes
• Shrinking the Quadratic Estimator
• Weak lensing "post-Born" effects are equivalent to pure lens-lens couplings
• Delensing CMB B-modes using galaxy surveys: the effect of galaxy bias and matter clustering non-linearities
• Extragalactic Background Light: Measurements and Applications
• Weak lensing deflection of three-point correlation functions
• On the absence of shear from perfect Einstein rings and the stability of geometry
• LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
• Forecasting isocurvature models with CMB lensing information: axion and curvaton scenarios
• CMB lensing from early-formed dark matter halos
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Characterizing CMB noise anisotropies from CMB delensing
• Testing for directionality in the Planck polarization and lensing data
• Position-space curved-sky anisotropy quadratic estimation
• Weak lensing from self-ordering scalar fields
• Simulation budgeting for hybrid effective field theories
• Cross-correlating the EMU Pilot Survey 1 with CMB lensing: Constraints on cosmology and galaxy bias with harmonic-space power spectra
• A Small-Scale Modification to the Lensing Kernel
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Large-scale acoustic peak shift in the Planck CMB data
• Lensing contribution to the 21cm intensity bispectrum
• The non-thermal secondary CMB anisotropies from a cosmic distribution of radio galaxy lobes
• Cosmological constraints on viable $f(R)$ models using weak lensing
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Reconstructing spatially-varying multiplicative bias for Stage IV weak lensing galaxy surveys with a quadratic estimator
• CMB lensing tomography with clustering estimation of lens redshift distributions
• Relativistic Angular Redshift Fluctuations embedded in Large Scale Varying Gravitational Potentials
• Fluctuation of the Hubble parameter
• A Demonstration of Spectral Level Reconstruction of Intrinsic $B$-mode Power
• Foreground Mitigation for CMB Lensing with the Global Minimum Variance Quadratic Estimator
• The Atacama Cosmology Telescope: A demonstration of CMB lensing measurement from daytime data
• Neutrino matter with PLANCK
• The Distortion of the Cosmic Microwave Background by the Milky Way
• The Bias to Cosmic Microwave Background Lensing Reconstruction from the Kinematic Sunyaev-Zel'dovich Effect at Reionization
• Time-dependent deflection reconstruction: new technique to search for gravitational waves with the cosmic microwave background
• Weak Lensing the non-Linear Ly-alpha Forest
• Extreme value statistics of CMB lensing deflection angles
• Theoretical and observational aspects of cosmological inflation
• Statical properties of CMB B-mode polarisation in a partial sky analysis
• Origin & evolution of the Universe
• The case for an all-sky millimetre survey at sub-arcminute resolution
• Systematic effects on lensing reconstruction from a patchwork of CMB polarization maps
• Probing CMB Polarization Gaussianity with the Statistics of Unpolarized Points: Non-Gaussianity of Planck Data and Prospects for Future B-Mode Measurements
• Running the small-correlated-against-large estimator at scale: Applications of small-scale CMB lensing estimators on realistic simulations
• Sector-Resolved Bayesian Model Averaging for DESI-Era Cosmology
• Detectability of Galactic Faraday Rotation in Multi-wavelength CMB Observations: A Cross-Correlation Analysis of CMB and Radio Maps
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• Revisiting secondary CMB distortions due to kinetic Sunyaev-Zel'dovich effect from quasar bubbles before reionization
• First constraints on the intrinsic CMB dipole and our velocity with Doppler and aberration
• Les Houches on Dark Universe 2025: Elements of cosmology beyond FLRW
• Weak Lensing Effect on CMB in the Presence of a Dipole Anisotropy
• Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity