H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes

Abstract

We present a measurement of the Hubble constant ($H_0$) and other cosmological parameters from a joint analysis of six gravitationally lensed quasars with measured time delays. All lenses except the first are analyzed blindly with respect to the cosmological parameters. In a flat $\Lambda$CDM cosmology, we find $H_0=73.3_{-1.8}^{+1.7}$, a 2.4% precision measurement, in agreement with local measurements of $H_0$ from type Ia supernovae calibrated by the distance ladder, but in $3.1\sigma$ tension with $Planck$ observations of the cosmic microwave background (CMB). This method is completely independent of both the supernovae and CMB analyses. A combination of time-delay cosmography and the distance ladder results is in $5.3\sigma$ tension with $Planck$ CMB determinations of $H_0$ in flat $\Lambda$CDM. We compute Bayes factors to verify that all lenses give statistically consistent results, showing that we are not underestimating our uncertainties and are able to control our systematics. We explore extensions to flat $\Lambda$CDM using constraints from time-delay cosmography alone, as well as combinations with other cosmological probes, including CMB observations from $Planck$, baryon acoustic oscillations, and type Ia supernovae. Time-delay cosmography improves the precision of the other probes, demonstrating the strong complementarity. Allowing for spatial curvature does not resolve the tension with $Planck$. Using the distance constraints from time-delay cosmography to anchor the type Ia supernova distance scale, we reduce the sensitivity of our $H_0$ inference to cosmological model assumptions. For six different cosmological models, our combined inference on $H_0$ ranges from $\sim 73$-$78\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, which is consistent with the local distance ladder constraints.

arXiv commentAccepted for publication in MNRAS; 23 pages, 13 figures, 8 tables

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• Strong gravitational lensing and microlensing of supernovae
• Modeling the Extragalactic Background Light and the Cosmic Star Formation History
• Automated galaxy-galaxy strong lens modelling: no lens left behind
• Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
• Cosmography by orthogonalized logarithmic polynomials
• Time Delay Lens Modelling Challenge
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Hierarchical Inference With Bayesian Neural Networks: An Application to Strong Gravitational Lensing
• Modelling and testing the equation of state for (Early) dark energy
• Intimate Relationship Between Sterile Neutrino Dark Matter and $\Delta N_{\mathrm{eff}}$
• $S_8$ increases with effective redshift in $\Lambda$CDM cosmology
• Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
• Revealing the late-time transition of $H_0$: relieve the Hubble crisis
• Inference of the cosmic rest-frame from supernovae Ia
• Multi-interacting dark energy and its cosmological implications
• Strong detection of the CMB lensingxgalaxy weak lensingcross-correlation from ACT-DR4,PlanckLegacy and KiDS-1000
• Exploring Early Dark Energy solution to the Hubble tension with Planck and SPTPol data
• Bounds on neutrino-scalar nonstandard interactions from big bang nucleosynthesis
• Gravity in the infrared and effective nonlocal models
• Improved time-delay lens modelling and $H_0$ inference with transient sources
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Line-of-sight effects in strong gravitational lensing
• The Hubble constant from strongly lensed supernovae with standardizable magnifications
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• TDCOSMO. IX. Systematic comparison between lens modelling software programs: time delay prediction for WGD 2038-4008
• Precision cosmology and the stiff-amplified gravitational-wave background from inflation: NANOGrav, Advanced LIGO-Virgo and the Hubble tension
• Cosmology with gravitationally lensed repeating Fast Radio Bursts
• Strong lensing as a giant telescope to localize the host galaxy of gravitational wave event
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• Strengthening the bound on the mass of the lightest neutrino with terrestrial and cosmological experiments
• Exploring the evidence for a large local void with supernovae Ia data
• TDCOSMO. VII. Boxyness/discyness in lensing galaxies : Detectability and impact on $H_0$
• The Cosmic Expansion History from Line-Intensity Mapping
• Towards a model-independent reconstruction approach for late-time Hubble data
• Project Dinos I: A joint lensing-dynamics constraint on the deviation from the power law in the mass profile of massive ellipticals
• Accuracy of environmental tracers and consequence for determining the Type Ia Supernovae magnitude step
• TDCOSMO III: Dark matter substructure meets dark energy -- the effects of (sub)halos on strong-lensing measurements of $H_0$
• A simultaneous solution to the Hubble tension and observed bulk flow within 250 $h^{-1}$ Mpc
• Late time acceleration due to generic modification of gravity and Hubble tension
• The minimally extended Varying Speed of Light (meVSL)
• Exact Spherically Symmetric Solutions in Modified Teleparallel gravity
• A Bayesian interpretation of inconsistency measures in cosmology
• Scalar field dark energy models: Current and forecast constraints
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• A data-driven Reconstruction of Horndeski gravity via the Gaussian processes
• Hubble parameter estimation via dark sirens with the LISA-Taiji network
• Reconciling Hubble Constant Discrepancy from Holographic Dark Energy
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• Over-constrained Models of Time Delay Lenses Redux: How the Angular Tail Wags the Radial Dog
• HOLISMOKES -- IV. Efficient mass modeling of strong lenses through deep learning
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements
• The first simultaneous measurement of Hubble constant and post-Newtonian parameter from Time-Delay Strong Lensing
• Model selection applied to reconstructions of the Dark Energy
• Dynamical dark energy in the light of DESI 2024 data
• Axi-Higgs Cosmology
• Intrinsic tension in the supernova sector of the local Hubble constant measurement and its implications
• JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78
• TDCOSMO 2025: Cosmological constraints from strong lensing time delays
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• Cosmological constraints on the Generalized Uncertainty Principle from modified Friedmann equations
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• A measurement of the CMB E-mode angular power spectrum at subdegree scales from 670 square degrees of POLARBEAR data
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Hubble tension vs two flows
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Prospects for Measuring the Hubble Constant with Neutron-Star-Black-Hole Mergers
• Cosmological perturbations in modified teleparallel gravity models: Boundary term extension
• A new way to explore cosmological tensions using gravitational waves and strong gravitational lensing
• Peculiar velocities in the local Universe: comparison of different models and the implications for $H_0$ and dark matter
• Small-scale clumping at recombination and the Hubble tension
• Strong lensing in UNIONS: Toward a pipeline from discovery to modeling
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• Resolving Hubble Tension by Self-Interacting Neutrinos with Dirac Seesaw
• Tensions with the flat $\mathbf{\Lambda }$CDM model from high-redshift cosmography
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Reconstruction of the dark sectors' interaction: A model-independent inference and forecast from GW standard sirens
• Testing dark energy after pre-recombination early dark energy
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
• Minimally Modified Gravity fitting Planck data better than $\Lambda$CDM
• No H_0 Assistance from Assisted Quintessence
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• HOLISMOKES -- III. Achromatic Phase of Strongly Lensed Type Ia Supernovae
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• An updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae
• Hubble tension as a guide for refining the early Universe: Cosmologies with explicit local Lorentz and diffeomorphism violation
• MOG cosmology without dark matter and the cosmological constant
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Effects of Supernova Redshift Uncertainties on the Determination of Cosmological Parameters
• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
• Faint objects in motion: the new frontier of high precision astrometry
• The Impact of Observing Strategy on Cosmological Constraints with LSST
• GIGA-Lens: Fast Bayesian Inference for Strong Gravitational Lens Modeling
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Neutrino Masses and Hubble Tension via a Majoron in MFV
• Hubble Asteroid Hunter: II. Identifying strong gravitational lenses in HST images with crowdsourcing
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• Determination of the Local Hubble Constant from Virgo Infall Using TRGB Distances
• First Constraints on Compact Dark Matter from Fast Radio Burst Microstructure
• TDCOSMO X. Automated Modeling of 9 Strongly Lensed Quasars and Comparison Between Lens Modeling Software
• Sources of $H_0$-tensions in dark energy scenarios
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Magnification, dust and time-delay constraints from the first resolved strongly lensed Type Ia supernova
• LensWatch: I. Resolved HST Observations and Constraints on the Strongly-Lensed Type Ia Supernova 2022qmx ("SN Zwicky")
• Maximally self-interacting dark matter: models and predictions
• Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting
• Testing the violation of the equivalence principle in the electromagnetic sector and its consequences in $f(T)$ gravity
• On the Period--Luminosity--Metallicity relation of Classical Cepheids
• Revising the Hubble constant, spatial curvature and dark energy dynamics with the latest observations of quasars
• Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation
• Detecting gravitational lenses using machine learning: exploring interpretability and sensitivity to rare lensing configurations
• Survey of Gravitationally lensed Objects in HSC Imaging (SuGOHI) -- VII. Discovery and Confirmation of Three Strongly Lensed Quasars
• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
• Do the observational data favor a local void?
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• Possible Hints of Sterile Neutrinos in Recent Measurements of the Hubble Parameter
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Classification of Teleparallel Horndeski Cosmology via Noether Symmetries
• Revisiting the Hubble constant, spatial curvature and cosmography with time-delay and cosmic chronometer observations
• VLT/MUSE observations of SDSS J1029+2623: towards a high-precision strong lensing model
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Inspecting the Cepheid distance ladder: The Hubble Space Telescope distance to the SNIa host galaxy NGC 5584
• Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). VIII. New galaxy-scale lenses from the HSC SSP
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Massive neutrino self-interactions with a light mediator in cosmology
• ${\Lambda }_{\mathrm{s}}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties
• Neural Network Reconstruction of $H^{\prime }(z)$ and its application in Teleparallel Gravity
• Minimal theory of massive gravity in the light of CMB data and the $S_8$ tension
• Measuring accretion disk sizes of lensed quasars with microlensing time delay in multi-band light curves
• Cosmological constraints on Hořava gravity revised in light of GW170817 and GRB170817A and the degeneracy with massive neutrinos
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• Cosmological constraints on dark energy models using DESI BAO 2024
• Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter
• High $H_0$ Values from CMB E-mode Data: A Clue for Resolving the Hubble Tension?
• Weakening gravity for dark matter in a type-II minimally modified gravity
• Questioning the $H_0$ tension via the look-back time
• Gravitational lensing $H_0$ tension from ultralight axion galactic cores
• A Survey for High-redshift Gravitationally Lensed Quasars and Close Quasars Pairs. I. the Discoveries of an Intermediately-lensed Quasar and a Kpc-scale Quasar Pair at $z\sim 5$
• Observational test for $f(Q)$ gravity with weak gravitational lensing
• Gaussian Process Approach for Model-Independent Reconstruction of $f(Q)$ Gravity with Direct Hubble Measurements
• Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
• Consequences of the lack of azimuthal freedom in the modeling of lensing galaxies
• A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short $\gamma$-ray bursts
• Gaia Data Release 3: The first Gaia catalogue of variable AGN
• The first five years of gravitational-wave astrophysics
• Alleviating $H_0$ tension in Horndeski gravity
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Simulations of multi-field ultralight axion-like dark matter
• A machine learning based approach to gravitational lens identification with the International LOFAR Telescope
• Dynamical systems analysis of tachyon dark energy model from a new perspective
• SLITronomy: towards a fully wavelet-based strong lensing inversion technique
• Growth Rate and Configurational Entropy in Tsallis Holographic Dark Energy
• No-go guide for the Hubble tension: late-time or local-scale new physics
• New Strong Gravitational Lenses from the DESI Legacy Imaging Surveys Data Release 9
• TDCOSMO VI: Distance Measurements in Time-delay Cosmography under the Mass-sheet transformation
• Primordial magnetic field as a common solution of nanohertz gravitational waves and the Hubble tension
• HOLISMOKES -- VII. Time-delay measurement of strongly lensed Type Ia supernovae using machine learning
• Solving the $H_0$ tension in $f(T)$ Gravity through Bayesian Machine Learning
• Constraining interacting dark energy models with the halo concentration-mass relation
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Resolving the Hubble tension in a U(1)${}_{L_{\mu }-L_{\tau }}$ model with Majoron
• Testing f(R) gravity models with quasar X-ray and UV fluxes
• A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
• Hubble constant and sound horizon from the late-time Universe
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• Trans-Planckian Censorship and Inflation in Grand Unified Theories
• Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
• An Efficient Method for Simulating Light Curves of Cosmological Microlensing and Caustic Crossing Events
• STRIDES: Spectroscopic and photometric characterization of the environment and effects of mass along the line of sight to the gravitational lenses DES J0408-5354 and WGD 2038-4008
• Future prospects on testing extensions to $\Lambda$CDM through the weak lensing of gravitational waves
• The role of CMB spectral distortions in the Hubble tension: a proof of principle
• Accretion disks, quasars and cosmology: meandering towards understanding
• The cosmic neutrino background as a collection of fluids in large-scale structure simulations
• hybrid-Lenstool: A self-consistent algorithm to model galaxy clusters with strong- and weak-lensing simultaneously
• Cosmic variance of $H_0$ in light of forthcoming high-redshift surveys
• MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
• TDCOSMO VIII: Cosmological distance measurements in light of the mass-sheet degeneracy -- forecasts from strong lensing and IFU stellar kinematics
• Thermal Dark Energy
• Spontaneous Scalarization of Black Holes in Gauss-Bonnet Teleparallel Gravity
• A common explanation of the Hubble tension and anomalous cold spots in the CMB
• The Unsettled Number: Hubble's Tension
• A framework for the next generation of stationary cosmological models
• GLoW: novel methods for wave-optics phenomena in gravitational lensing
• The impact of line-of-sight structures on measuring $H_0$ with strong lensing time-delays
• Does DESI DR2 challenge $\Lambda$CDM paradigm ?
• Measuring the Hubble function with standard candle clustering
• Euclid: The Early Release Observations Lens Search Experiment
• HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
• Cosmological Perturbation Theory in Metric-Affine Gravity
• Measuring the Hubble constant with kilonovae using the Expanding Photosphere Method
• Neural network reconstruction of cosmology using the Pantheon compilation
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• The impact of human expert visual inspection on the discovery of strong gravitational lenses
• Shedding Light on Dark Matter and Neutrino Interactions from Cosmology
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Galaxy-lens determination of $H_0$: constraining density slope in the context of the mass sheet degeneracy
• J1721$+$8842: a gravitationally lensed binary quasar with a proximate damped Lyman-$\alpha$ absorber
• Barrow and Tsallis entropies after the DESI DR2 BAO data
• Can the Hubble tension be resolved by bulk viscosity?
• Resonant neutrino self-interactions and the $H_0$ tension
• Unbiased likelihood-free inference of the Hubble constant from light standard sirens
• Combining cosmological and local bounds on bimetric theory
• Be It Unresolved: Measuring Time Delays from Lensed Supernovae
• Oscillating dark energy in light of the latest observations and its impact on the Hubble tension
• A critical discussion on the $H_0$ tension
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• Structure growth in $f(Q)$ cosmology
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Identification of Galaxy-Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
• Constraining quasar structure using high-frequency microlensing variations and continuum reverberation
• Streamlined Lensed Quasar Identification in Multiband Images via Ensemble Networks
• Running Hubble constant: evolutionary Dark Energy
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• Constraining the anisotropy of the Universe with the X-ray and UV fluxes of quasars
• Revealing the structure of the lensed quasar Q 0957+561: I. Accretion disk size
• Auto-identification of unphysical source reconstructions in strong gravitational lens modelling
• Cosmology-informed neural networks to solve the background dynamics of the Universe
• Noether Symmetry Approach in Scalar-Torsion $f(T,\varphi )$ Gravity
• When tension is just a fluctuation: How noisy data affect model comparison
• TDCOSMO. XVI. Measurement of the Hubble Constant from the Lensed Quasar WGD2038$-$4008
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• Ghost and Laplacian Instabilities in the Teleparallel Horndeski Gravity
• Near infrared and optical continuum emission region size measurements in the gravitationally lensed quasars Q0957+561 and SBS0909+532
• Cosmological models with squared trace in modified gravity
• Theoretical and numerical perspectives on cosmic distance averages
• The cosmological star formation history from the Local Cosmological Volume of galaxies and constraints on the matter homogeneity
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Addressing Cosmological Tensions by Non-Local Gravity
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Neutrino masses from large-scale structures: future sensitivity and theory dependence
• HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
• Constraining $\Lambda$CDM cosmological parameters with Einstein Telescope mock data
• Complex angular structure of three elliptical galaxies from high-resolution ALMA observations of strong gravitational lenses
• Hubble tension as a window on the gravitation of the dark matter sector
• Updating constraints on phantom crossing $f(T)$ gravity
• Toward a simultaneous resolution of the $H_0$ and $S_8$ tensions: early dark energy and an interacting dark sector model
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• HOLISMOKES -- X. Comparison between neural network and semi-automated traditional modeling of strong lenses
• Galaxy-lens determination of $H_0$: the effect of the ellipse+shear modeling assumption
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• Radiative stability and observational constraints on dark energy and modified gravity
• Testing the Cosmic Distance Duality Relation Using Strong Gravitational Lensing Time Delays and Type Ia Supernovae
• Measuring the cosmic expansion rate using 21-cm velocity acoustic oscillations
• The effects of peculiar velocities in SN Ia environments on the local $H_0$ measurement
• Measuring line-of-sight shear with Einstein rings: a proof of concept
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• Euclid: A complete Einstein ring in NGC 6505
• Superhorizon perturbations: A possible explanation of the Hubble--Lemaître Tension and the Large Scale Anisotropy of the Universe
• Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI Response
• Gravitational lenses in arbitrary space-times
• Family dispute: do Type IIP supernova siblings agree on their distance?
• Discovering strongly lensed quasar candidates with catalogue-based methods from DESI Legacy Surveys
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• The DES Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5,000 Sq. Deg. Footprint
• In search of an interaction in the dark sector through Gaussian Process and ANN approaches
• LeMoN: Lens Modelling with Neural networks -- I. Automated modelling of strong gravitational lenses with Bayesian Neural Networks
• Constraining Cosmological and Galaxy Parameters using Strong Gravitational Lensing Systems
• Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals
• Time delay induced by plasma in strong lens systems
• The impact of mass map truncation on strong lensing simulations
• Cosmology of an Axion-Like Majoron
• Noether Symmetries in $f(T,T_G)$ Cosmology
• Discovering Strongly-lensed QSOs From Unresolved Light Curves
• Finding Multiply-Lensed and Binary Quasars in the DESI Legacy Imaging Surveys
• Lensed quasar search via time variability with the HSC transient survey
• DeepZipper: A Novel Deep Learning Architecture for Lensed Supernovae Identification
• Constraints on Dark Energy Models Using Late Universe Probes
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• TDCOSMO VIII: A key test of systematics in the hierarchical method of time-delay cosmography
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Strong-lensing source reconstruction with variationally optimised Gaussian processes
• Quantifying the structure of strong gravitational lens potentials with uncertainty-aware deep neural networks
• Hubble distancing: Focusing on distance measurements in cosmology
• Tracing cosmic evolution through Weyl-Type f(Q,T) gravity model: theoretical analysis and observational validation
• Quasar Sightline and Galaxy Evolution (QSAGE) survey -- II. Galaxy overdensities around UV luminous quasars at z=1-2
• Identifying lensed quasars and measuring their time-delays from unresolved light curves
• Sensitivity reach of gamma-ray measurements for strong cosmological magnetic fields
• Charged Dark Matter and the $H_0$ tension
• A Framework for Obtaining Accurate Posteriors of Strong Gravitational Lensing Parameters with Flexible Priors and Implicit Likelihoods using Density Estimation
• f(R) Gravity in an Ellipsoidal Universe
• TDCOSMO. XI. New lensing galaxy redshift and velocity dispersion measurements from Keck spectroscopy of eight lensed quasar systems
• Strongly lensed SN Refsdal: refining time delays based on the supernova explosion models
• Early dark energy constraints with late-time expansion marginalization
• The cosmic distance duality relation in light of the time-delayed strong gravitational lensing
• Cosmological constraints of Palatini $f(\mathcal{R})$ gravity
• Cosmological study of a symmetric teleparallel gravity model
• Multipole expansion for 21cm Intensity Mapping power spectrum: forecasted cosmological parameters estimation for the SKA Observatory
• Cosmological Parameter Estimation Using Current and Future Observations of Strong Gravitational Lensing
• HOLISMOKES -- XI. Evaluation of supervised neural networks for strong-lens searches in ground-based imaging surveys
• Discovery of Strongly Lensed Quasars in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)
• FRBs Lensed by Point Masses I. Lens Mass Estimation for Doubly Imaged FRBs
• A model for galaxy-galaxy strong lensing statistics in surveys
• J1721+8842: The first Einstein zig-zag lens
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Quantifying effects of inhomogeneities and curvature on gravitational wave standard siren measurements of $H(z)$
• What Moves the Heavens Above?
• Quantum origin of dark energy and the Hubble tension
• $f(T,B)$ Gravity in the late Universe in the context of local measurements
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• LADUMA: Discovery of a luminous OH megamaser at $z>0.5$
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Rotating Kerr-Newman space-times in Metric-Affine Gravity
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• A More Accurate Parameterization based on cosmic Age (MAPAge)
• Direct tests of General Relativity under screening effect with galaxy-scale strong lensing systems
• Towards a Solution to the H0 Tension: the Price to Pay
• AI-driven spatio-temporal engine for finding gravitationally lensed type Ia supernovae
• Strong lensing systems and galaxy cluster observations as probe to the cosmic distance duality relation
• Comprehensive Constraints on Dark Radiation Injection After BBN
• Dissecting kinetically coupled quintessence: phenomenology and observational tests
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• Possible Resolution of the Hubble Tension with Weyl Invariant Gravity
• Gravitational Microlensing Time Delays at High Optical Depth: Image Parities and the Temporal Properties of Fast Radio Bursts
• Viewing angle observations and effects of evolution with redshift, black hole mass, and Eddington ratio in quasar based cosmology
• Mathematical Underpinnings of the Multi-Wavelength Structure of the TRGB
• Fractional Einstein-Gauss-Bonnet scalar field cosmology
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• Shan--Chen interacting vacuum cosmology
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Cosmological Distances And Hubble Tension In Einstein-Cartan Theory
• Interacting dark sector: a dynamical system perspective
• Probing compact dark matter objects with microlensing in gravitationally lensed quasars
• Measuring time delays: I. Using a flux time series that is a linear combination of time-shifted light curves
• Light Dark Matter: A Common Solution to the Lithium and $H_0$ Problems
• Late-time and Big Bang nucleosynthesis constraints for generic modify gravity surveys
• Optical Observations of the Nearby Type Ia Supernova 2021hpr
• Exploiting the diversity of modeling methods to probe systematic biases in strong lensing analyses
• Constraints on sterile neutrinos and the cosmological tensions
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Revealing the structure of the lensed quasar Q 0957+561 III. Constraints on the size of the broad-line region
• The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey Galaxy Cluster Catalogue
• Retrospective Search for Strongly Lensed Supernovae in the DESI Legacy Imaging Surveys
• Investigating the Hubble Tension: Effect of Cepheid Calibration
• Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020
• Imprint of Early Dark Energy in Stochastic Gravitational Wave Background
• Simulating time-varying strong lenses
• The effect of screening mechanisms on black hole binary inspiral waveforms
• Relic Neutrino Degeneracies and Their Impact on Cosmological Parameters
• Observational constraints in Delta Gravity: CMB and supernovas
• Lessons from the first multiply imaged supernova II: A parametric strong-lensing model for the galaxy cluster MACS J1149.5+2223
• Model-Independent Perspectives on Coupled Dark Energy and the Swampland
• Constraining VLBI-optical offsets in high redshift galaxies using strong gravitational lensing
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• Towards a 1% Measurement of the Hubble Constant: Accounting for Time Dilation in Variable Star Light Curves
• Improving Constraints on Models Addressing the Hubble Tension with CMB Delensing
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Interplay of CMB Temperature, Space Curvature, and Expansion Rate Parameters
• Galaxy-galaxy lensing data: $f(T)$ gravity challenges General Relativity
• Improved model of the Supernova Refsdal cluster MACS J1149.5+2223 thanks to VLT/MUSE
• Is there a dynamical tendency in H0 with late time measurements?
• 21 cm power spectrum in interacting cubic Galileon model
• Machine learning unveils the linear matter power spectrum of modified gravity
• Measuring Cosmological Distances Using Cluster Edges as a Standard Ruler
• The Carousel Lens: A Well-Modeled Strong Lens with Multiple Lensed Sources
• Constraints on Equivalence Principle Violation from Gamma Ray Bursts
• Galaxy mass profiles from strong lensing III: The two-dimensional broken power-law model
• Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
• HOLISMOKES XIII: Strong-lens candidates at all mass scales and their environments from the Hyper-Suprime Cam and deep learning
• Tests of Standard Cosmology in Horava Gravity and Bayesian Evidence for a Closed Universe, and the Hubble Tension
• Combining strong and weak lensing estimates in the Cosmos field
• Developing a Victorious Strategy to the Second Strong Gravitational Lensing Data Challenge
• Eliminating the Hubble Tension in the Presence of the Interconnection between Dark Energy and Matter in the Modern Universe
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Impact of Microlensing on Observational Strategies for Gravitational Time Delay Measurements
• Fundamental Physics and Cosmology with TianQin
• Determining Cosmological-model-independent $H_0$ with Gravitationally Lensed Supernova Refsdal
• TDCOSMO XVII. New time delays in 22 lensed quasars from optical monitoring with the ESO-VST 2.6m and MPG 2.2m telescopes
• Consistency of Cubic Galileon Cosmology: Model-Independent Bounds from Background Expansion and Perturbative Analyses
• Plasma lensing in comparison to gravitational lensing -- Formalism and degeneracies
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• Fireball baryogenesis from early structure formation due to Yukawa forces
• An approach to cold dark matter deviation and the $H_0$ tension problem by using machine learning
• Geometric Distances of Quasars Measured by Spectroastrometry and Reverberation Mapping:Monte Carlo Simulations
• A structured analysis of Hubble tension
• Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
• Strong Lensing and $H_0$
• On measuring the Hubble constant with X-ray reverberation mapping of active galactic nuclei
• Interacting dark energy axions in light of the Hubble tension
• Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars
• Out of One, Many: Distinguishing Time Delays from Lensed Supernovae
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Inferring Cosmological Parameters with Evidential Physics-Informed Neural Networks
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• A search for gravitationally lensed supernovae within the Zwicky Transient Facility public survey
• A targeted search for strongly lensed supernovae with the Las Cumbres Observatory
• Unveiling the Effects of Coupling Extended Proca-Nuevo Gravity on Cosmic Expansion with Recent Observations
• Constraining cosmological scaling solutions of a Galileon field
• PSJ2107-1611: a new wide-separation, quadruply imaged lensed quasar with flux ratio anomalies
• The impact of 2D and 3D BAO measurements on the Cosmic Distance Duality Relation with HII galaxies
• Toward a more stringent test of gravity with redshift space power spectrum: simultaneous probe of growth and amplitude of large-scale structure
• Strongly Lensed Supernovae in Well-Studied Galaxy Clusters with the Vera C. Rubin Observatory
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• Constraints on dark energy from TDCOSMO & SLACS lenses
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• Peculiar velocity cosmology with type Ia supernovae
• Chromatic Microlensing Time Delays
• Effects of the Hubble Parameter on the Cosmic Growth of the First Quasars
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• Difficulties in reconciling non-negligible differences between the local and cosmological values of the gravitational coupling in extended Brans-Dicke theories
• Unveiling the Universe with Emerging Cosmological Probes
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Evidence for evolving dark energy from DESI DR2 BAO and Pantheon${}^{+}$, DES-Dovekie, and Union3
• Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes
• Climbing out of the shadows: building the distance ladder with black hole images
• Cosmological evolution with negative energy densities
• Cosmological parameters from Planck data in SU(2)${}_{\mathrm{CMB}}$, their local $\Lambda$CDM values, and the modified photon Boltzmann equation
• Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model
• Probing a scale dependent gravitational slip with galaxy strong lensing systems
• Model-independent Gamma-Ray Bursts Constraints on Cosmological Models Using Machine Learning
• HOLISMOKES -- XII. Time-delay Measurements of Strongly Lensed Type Ia Supernovae using a Long Short-Term Memory Network
• Detecting unresolved lensed SNe Ia in LSST using blended light curves
• Dark sector production and baryogenesis from not quite black holes
• A new parametrization of Hubble function and Hubble tension
• Weak lensing of strong lensing: beyond the tidal regime
• Foreground biases in strong gravitational lensing
• High-resolution imaging follow-up of doubly imaged quasars
• Thermodynamic and observational constraints on black holes with primary hair in Beyond Horndeski Gravity: Stability and shadows
• Gravitational lens time-delay as a probe of a possible time variation of the fine-structure constant
• LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia Supernova 2022qmx ("SN Zwicky") with HST Template Observations
• Forecast of strongly lensed supernovae rates in the China Space Station Telescope surveys
• Challenges and Opportunities for time-delay cosmography with multi-messenger gravitational lensing
• Discovery of 19 strongly-lensed quasars, dual and projected quasars in DESI-LS
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• An SU(2) gauge principle for the Cosmic Microwave Background: Perspectives on the Dark Sector of the Cosmological Model
• Subaru Telescope -- History, Active/Adaptive Optics, Instruments, and Scientific Achievements
• Discovery of the lensed quasar eRASS1 J050129.5-073309 with $\text{SRG}/$eROSITA and $Gaia$
• Inverse Seesaw, dark matter and the Hubble tension
• A Hubble Constant Determination Through Quasar Time Delays and Type Ia Supernovae
• Signatures of Very Early Dark Energy in the Matter Power Spectrum
• DESI-253.2534+26.8843: A New Einstein Cross Spectroscopically Confirmed with VLT/MUSE and Modeled with GIGA-Lens
• Quintessence scalar field and cosmological constant: Dynamics of a multi-component dark energy model
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Configurational entropy in $f(T)$ gravity
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Strongly lensed candidates from the HSC transient survey
• Galaxy Spectra neural Networks (GaSNets). I. Searching for strong lens candidates in eBOSS spectra using Deep Learning
• Testing the local supervoid solution to the Hubble tension with direct distance tracers
• Prospects of probing dark energy with eLISA: Standard versus null diagnostics
• Einstein clusters as models of inhomogeneous spacetimes
• Evidence for the dynamical dark energy with evolving Hubble constant
• Teleparallel dark energy in a nonflat universe
• Elliptical multipoles for gravitational lenses
• MNELLS: The MUSE Nearby Early-Type Galaxy Lens Locator Survey
• Measuring the Hubble constant through the galaxy pairwise peculiar velocity
• Impact of weak lensing on bright standard siren analyses
• The powerful lens galaxy cluster PLCK G287.0+32.9 (${\theta }_E\sim 43^{\prime \prime }$)
• GausSN: Bayesian Time-Delay Estimation for Strongly Lensed Supernovae
• What Prevents Resolving the Hubble Tension through Late-Time Expansion Modifications?
• Dynamics of Inspiraling Dark Energy
• Relaxing cosmological constraints on current neutrino masses
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• Modified cosmology through generalized mass-to-horizon entropy: observational constraints from DESI DR2 BAO data
• Configurational Entropy in Chaplygin Gas Models
• CURLING -- II. Improvement on the $H_0$ Inference from Pixelized Cluster Strong Lens Modeling
• Black hole and cosmological analysis of BF sequestered gravity
• TDCOSMO: XX. WFI2033--4723, the First Quadruply-Imaged Quasar Modeled with JWST Imaging
• Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset
• Tackling the Problem of Distributional Shifts: Correcting Misspecified, High-Dimensional Data-Driven Priors for Inverse Problems
• Defrosting and Blast Freezing Dark Matter
• Host group degeneracy in gravitational lensing time delay determination of $H_0$
• A Targeted Search for Variable Gravitationally Lensed Quasars
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• Viewing angle effects in quasar application to cosmology
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Pixel-level modelling of group-scale strong lens CASSOWARY 19
• The establishment of the Standard Cosmological Model through observations
• Simulation-guided galaxy evolution inference: A case study with strong lensing galaxies
• Effective field theory of coupled dark energy and dark matter
• A test for the redshift dependence of ${\sigma }_8$ using $f{\sigma }_8$ measurements
• Performance of Non-Parametric Reconstruction Techniques in the Late-Time Universe
• Angular Correlation Function from sample covariance with BOSS and eBOSS LRG
• Can the quasi-molecular mechanism of recombination decrease the Hubble tension?
• Breaking the ${\tau }_{\mathrm{T}}-f$ degeneracy of the kinetic Sunyaev Zel'dovich cosmology in redshift space
• Peculiar velocity effects on the Hubble constant from time-delay cosmography
• Cosmography from accurate mass modeling of the lens group SDSS J0100+1818: five sources at three different redshifts
• Using Neutrino Oscillations to Measure $H_0$
• Probing Cosmology beyond $\Lambda$CDM using the SKA
• Modified propagation of gravitational waves from the early radiation era
• TDCOSMO. XXIII. Measurement of the Hubble constant from the doubly lensed quasar HE1104-1805
• Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood
• The COSMOS-Web Lens Survey (COWLS) III: forecasts versus data
• From inflation to dark energy in scalar-tensor cosmology
• Revisiting the Hubble constant, sound horizon and cosmography from late-time Universe observations
• Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
• The Effect of Superpositions on the Planetary Nebula Luminosity Function
• ParamANN: A Neural Network to Estimate Cosmological Parameters for $\Lambda$CDM Universe Using Hubble Measurements
• Remarks on overestimating the effects of inhomogeneities on the Hubble constant
• Early dark energy and scalarization in a scalar-tensor model
• Exploring thermodynamics inconsistencies in unimodular gravity: a comparative study of two energy diffusion functions
• HOLISMOKES -- XIV. Time-delay and differential dust extinction determination with lensed type II supernova color curves
• Polarizations of CMB and the Hubble tension
• Ultra Long Period Cepheids as standard candles from Gaia to Rubin-LSST
• FIMP Dark Matter in bulk viscous non-standard cosmologies
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Strong gravitational lensing with upcoming wide-field radio surveys
• Determining $H_0$ from distance sum rule combining gamma-ray bursts with observational Hubble data and strong gravitational lensing
• Measuring the gravitomagnetic distortion from rotating halos I: methods
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• HOLISMOKES XVI: Lens search in HSC-PDR3 with a neural network committee and post-processing for false-positive removal
• Searching for strong lensing by late-type galaxies in UNIONS
• Revealing Limitation in the Standard Cosmological Model: A Redshift-Dependent Hubble Constant from Fast Radio Bursts
• Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• The revolution in strong lensing discoveries from Euclid
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• $H_0$ Reconstruction with Type Ia Supernovae, Baryon Acoustic Oscillation and Gravitational Lensing Time-Delay
• FBQ 0951+2635: time delay and structure of the main lensing galaxy
• Accelerating lensed quasar discovery and modeling with physics-informed variational autoencoders
• Common Origin of Warm Dark Matter and Dark Radiation
• Time delay estimation in unresolved lensed quasars
• A Geometric Probe of Cosmology -- II. Gravitational Lensing Time Delays and Quasar Reverberation Mapping Revisited
• Fundamental Physics in 2025: Status, Decisive Targets, and Path Forward
• The Impact of $\text{CLEAN}$ing on Strong Gravitational Lens Modelling
• Reducing false positives in strong lens detection through effective augmentation and ensemble learning
• Large, fast and accurate HI intensity maps with latent overlap diffusion
• A compact group lens modeled with GIGA-Lens: Enhanced inference for complex systems
• Predicting High-magnification Events in Microlensed Quasars in the Era of LSST using Recurrent Neural Networks
• Investigating the Redshift Evolution of Lensing Galaxy Density Slopes via Model-Independent Distance Ratios
• Degrees of Freedom of New General Relativity I: Type 2, Type 3, Type 5, and Type 8
• Dynamical Shortcomings in the Generalized SU(2) Proca Theory: Challenges for Cosmic Acceleration
• H0 tension in Tsallis and Renyi statistics
• Revisiting cosmological diffusion models in Unimodular Gravity and the $H_0$ tension
• M33 Cepheids from CFHT/MegaCAM survey
• A Review on Resolving the Hubble Tension via Late-Universe Physics
• Mapping Large-Scale-Structure Evolution over Cosmic Times
• Parameter free Hubble constant from the quadruply lensed quasar SDSS J1004 + 4112
• Cepheid distances based on Gaia and VMC@VISTA observations
• Galaxy cluster count cosmology with simulation-based inference
• Accelerated inference of microlensed gravitational waves with machine learning
• KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
• Inference of matter power spectrum at z=0 using DESI DR1 Full-Shape data
• A new quasar strongly-lensed candidate by the galaxy cluster WHJ0400-27 with a $18^{\prime \prime }$ image-separation
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Revisiting the effect of lens mass models in cosmological applications of strong gravitational lensing
• A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant
• Harnessing Unresolved Lensed Quasars: The Mathematical Foundation of the Fluctuation Curve
• The Quasar Candidates Catalogs of DESI Legacy Imaging Survey Data Release 9
• Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive
• Testing the Distance Duality Relation with Cosmological Observations at high Redshift using Artificial Neural Network
• Time delay measurements with Broken Power Law model
• Ricci cosmology in light of astronomical data
• From Nonparametric Distance Reconstruction to Testing the Etherington Relation and Cosmic Curvature Using 2D and 3D BAO Measurements
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Lenses In VoicE (LIVE): Searching for strong gravitational lenses in the VOICE@VST survey using Convolutional Neural Networks
• HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• Gaia GraL: Gaia gravitational lens systems IX. Using XGBoost to explore the Gaia Focused Product Release GravLens catalogue
• Confirming HSC strong lens candidates with DESI Spectroscopy. I. Project overview and first results
• A semi-cosmographic approach to study cosmological evolution in phase space
• Blois 2019: highlights and outlook
• Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope
• The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles
• Robustness of the Cosmological Constant Damping Mechanism Through Matter Eras
• A robust assessment of the local anisotropy of the Hubble constant
• Precision Cosmology in Modified and Extended Theories of Gravity: an insightful test
• Improving NASA/IPAC Extragalactic Database Redshift Calculations
• Prospects of Gluino searches in multi-lepton channels in the light of ongoing LHC RUN-III
• Late time attractors of some varying Chaplygin gas cosmological models
• Hubble Tension and Gravitational Self-Interaction
• A dynamical dark energy solution to Hubble-Lemaître tension in the light of the multimessenger era
• Lensing in the Darkness: A Bayesian Analysis of 22 Chandra Sources at $z\gtrsim 6$ Shows No Evidence of Lensing
• MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
• Impact of Large-Scale Structure along Line-of-Sight on Time-Delay Cosmography
• Forecasting the FRB Population Observed Through Galaxy Cluster Lenses
• The impact of ultraviolet suppression on the rates and properties of strongly lensed Type IIn supernovae detected by LSST
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• Testing the cosmological principle on gigaparsec scales
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Time Delay Cosmography: Analysis of Quadruply Lensed QSO SDSSJ1433 from Wendelstein Observatory
• New Constraint of the Hubble Constant by Proper Motions of Radio Components Observed in AGN Twin-jets
• Most Strong Lensing Deflectors in the AGEL Survey Are in Group and Cluster Environments
• Probing modified gravitational wave propagation with strongly lensed coalescing binaries
• HOLISMOKES -- XVIII. Cosmology with strongly lensed type II supernovae: Effects of instrumental setups on $H_0$
• Gravitational lensing of fast radio bursts: prospects for probing microlens populations in lensing galaxies
• SHARP VIII: J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging
• NuAncestor: an artificial satellite-borne star for accurate frequency calibration of ground-based EPRV spectrographs
• Cosmology of Cubic Poincaré Gauge gravity
• Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Accelerated expansion as manifestation of gravity: when Dark Energy belongs to the left
• Bayesian and Machine-Learning Analyses of Nonminimal $f(Q)$ Gravity and $H_0$ Tension
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• Analysis of some classical and quantum aspects of black holes
• Phenomenological model explaining Hubble Tension origin
• Effect of primary scalar hair on black hole's strong lensing in Beyond Horndeski Gravity
• FLRW Kinematic-Induced Measurement of the Hubble Constant from Cosmic Chronometer and Redshift Drift Observations
• Constraining beyond $\Lambda$CDM models with 21cm intensity mapping forecast observations combined with latest CMB data
• First Life in the Universe
• SDSS-IV MaNGA: A Catalogue of Spectroscopically Detected Strong Galaxy-Galaxy Lens Candidates
• Testing a nonlinear solution of the Israel-Stewart theory
• Breaking the Mass-sheet Degeneracy in Time-delay Cosmology with Lensed and Unlensed Type Ia Supernovae
• Revisiting the gluino mass limits in the pMSSM in the light of the latest LHC data and Dark Matter constraints
• Confusing dark matter particle properties with modifications to General Relativity
• Probing dark energy using anisotropies in the clustering of post-EoR HI distribution
• Yano-Schrödinger Hyperfluid: Cosmological Implications
• Lessons from the first multiply imaged supernova: A revised Light-Traces-Mass strong lensing model for the galaxy cluster MACS J1149.5+2223