DiRIM uses a diffusion model with recurrent score refinement to sample pixel-space joint posteriors of the lensed source and foreground mass map, reproducing mock strong-lens observations to the noise level.
Monthly Notices of the Royal Astronomical Society , author=
8 Pith papers cite this work, alongside 236 external citations. Polarity classification is still indexing.
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Dynamical systematics in eight time-delay lenses can shift H0 by more than the 2% target, so velocity dispersions must be controlled to about 1% accuracy.
A new compilation of over 30,000 strong-lensing candidates with multi-survey images yields an independent ground-based constraint γ_PPN = 1.023 ± 0.028 and a combined constraint γ_PPN = 1.034 ± 0.025.
A Vision Transformer trained with interactive multi-class feedback and checked by citizen scientists finds 1,328 strong lens candidates in DES Year 6 data, including 147 new systems.
The KBC void and local expansion rate measurements are jointly very unlikely in Lambda CDM, and a Milgromian dynamics model with 11 eV sterile neutrinos matches them at about 2.5 sigma tension.
A convLSTM classifier identifies lensed SNe Ia in simulated LSST-like time series, reaching ~60% true-positive rate at O(10^{-4}) false-positive rate by the seventh epoch even after adding realistic PSF variations and foreground SN contaminants.
A review of late-universe models concludes that DESI BAO plus uncalibrated supernovae data indicate the Hubble tension originates in new low-redshift physics.
This paper is a review of published gravitational wave standard siren measurements of the Hubble constant; it contributes a compilation table and no new measurement.
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A Review on Resolving the Hubble Tension via Late-Universe Physics
A review of late-universe models concludes that DESI BAO plus uncalibrated supernovae data indicate the Hubble tension originates in new low-redshift physics.