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20152026
most citedH0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model

469 citations · 1k across the 31 of their papers we have counts for

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19 papers · 1 filter

astro-ph.CO2025

Precision Measurement of Large Shear Signals

Jiarui Sun, Jun Zhang, Li Cui +2

So far, estimators of galaxy shape distortions are only carefully studied perturbatively in the case of small shear signals, mainly for weak lensing science. However, in the neighb…

astro-ph.CO2025★ 38 cited

TDCOSMO 2025: Cosmological constraints from strong lensing time delays

TDCOSMO Collaboration, Simon Birrer, Elizabeth J. Buckley-Geer +30

We present cosmological constraints from 8 strongly lensed quasars (hereafter, the TDCOSMO-2025 sample). Building on previous work, our analysis incorporated new deflector stellar…

astro-ph.CO2024

Caustic area biases and how to deal with them

Alessandro Sonnenfeld

Quadruply-imaged strongly lensed quasars (quads) are routinely used for measurements of the expansion rate of the Universe with time delays. It has recently been suggested that any…

astro-ph.CO2024★ 3 cited

Constraining galaxy properties with complete samples of lenses

Qing Zhou, Alessandro Sonnenfeld, Henk Hoekstra

The statistics of Einstein radii for a sample of strong lenses can provide valuable constraints on the underlying mass distribution. The correct interpretation, however, relies cri…

astro-ph.CO2024

Neural network prediction of model parameters for strong lensing samples from Hyper Suprime-Cam Survey

Priyanka Gawade, Anupreeta More, Surhud More +4

Strong lensing of background galaxies provides important information about the matter distribution around lens galaxies. Traditional modelling of such strong lenses is both time an…

astro-ph.CO2022★ 6 cited

Photometric redshift estimation of strongly lensed galaxies

Danial Langeroodi, Alessandro Sonnenfeld, Henk Hoekstra +1

Around strongly lensed galaxies are expected to be discovered with Euclid and the LSST. Utilising these large samples to study the inner structure of lens galaxies requires…