Sign inGet started
Paper · arXiv

Neural Posterior Estimation for Tomographic Weak Lensing Mass Mapping

Weak gravitational lensing shear and convergence trace the distribution of baryonic and dark matter across space, making them a powerful probe of cosmic structure. Inferring shear and convergence from images is a challenging inverse problem. The prevailing approach to this task estimates shear from weighted averages of galaxy ellipticities, calibrates these estimates to account for systematic biases, and transforms them to reconstruct convergence, a multistage procedure that requires substantial computational resources and meticulous handling of statistical uncertainties. As an alternative, we propose a probabilistic approach to field-level weak lensing inference in which we train a deep ...

AuthorsTim White, Shreyas Chandrashekaran, Camille Avestruz et al.
Primary categoryastro-ph.IM
Published7 September 2026
Last updated at source7 September 2026
astro-ph.IMastro-ph.COcs.CVstat.AP
Embed this entry
<iframe src="https://silytics.si/embed/item/e7c6fbab-23cc-4fe6-9885-572c7bb2e173" width="420" height="190" style="border:0" loading="lazy" title="Silytics entry"></iframe>

Free, no tracking. More about feeds and embeds.

Silytics shows public metadata from arXiv and links to the original. Information may be incomplete or out of date. Last refreshed 17 October 2026. Licenses and terms of the original apply to the work itself. Not financial, legal or professional advice.