activity
20222026
most citedThe Blending ToolKit: A simulation framework for evaluation of galaxy detection and deblending

2 citations · 5 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2026

Probabilistic characterization of blending with LSST and application to cluster lensing cosmology

Manon Ramel, Cyrille Doux, Marine Kuna +9

Next-generation galaxy surveys, like the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST), will deliver unprecedented depth and sky coverage, enabling precise mea…

astro-ph.IM2026

Neural Posterior Estimation for Tomographic Weak Lensing Mass Mapping

Tim White, Shreyas Chandrashekaran, Camille Avestruz +2

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…

astro-ph.IM2026

Neural Posterior Estimation for Inferring Weak Lensing Shear

Tim White, Dingrui Tao, Camille Avestruz +2

The prevailing approach to inferring weak gravitational lensing shear from images involves detecting galaxies, estimating their ellipticities, and calibrating these estimates to co…

astro-ph.CO2026

Constraining Galaxy Cluster Triaxiality via Weak Lensing --- I. Preparation for the Rubin Data Beyond Leading Order

Shenming Fu, Radhakrishnan Srinivasan, Tae-hyeon Shin +13

The 3D mass distributions of galaxy clusters are generally triaxial, a geometry that is difficult to constrain from projected observations. In this work, we measure the projected h…

astro-ph.IM2026

Differentiable Forward Modeling for Efficient and Accurate Shear Inference

Ismael Mendoza, Axel Guinot, Matthew R. Becker +6

Forthcoming Stage-IV dark energy optical surveys, such as LSST, have the ambitious goal of measuring cosmological parameters at sub-percent precision. Realizing their full scientif…

astro-ph.IM2026

Simulation-Based Inference for Probabilistic Galaxy Detection and Deblending

Ismael Mendoza, Derek Hansen, Runjing Liu +6

Stage-IV dark energy wide-field surveys, such as the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), will observe an unprecedented number density of galaxies. As…

astro-ph.IM2025

Neural Posterior Estimation for Cataloging Astronomical Images from the Legacy Survey of Space and Time

Yicun Duan, Xinyue Li, Camille Avestruz +2

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will commence full-scale operations in 2026, yielding an unprecedented volume of astronomical images. Construct…

astro-ph.IM2025★ 2 cited

Neural Posterior Estimation for Cataloging Astronomical Images with Spatially Varying Backgrounds and Point Spread Functions

Aakash Patel, Tianqing Zhang, Camille Avestruz +2

Neural posterior estimation (NPE), a type of amortized variational inference, is a computationally efficient means of constructing probabilistic catalogs of light sources from astr…

astro-ph.CO2025

Weak lensing mass-richness relation of redMaPPer clusters in the LSST DESC DC2 simulations

Constantin Payerne, Zhuowen Zhang, Michel Aguena +13

Cluster scaling relations are key ingredients in cluster abundance-based cosmological studies. In optical cluster cosmology, where clusters are detected through their richness, clu…

astro-ph.IM2024★ 2 cited

The Blending ToolKit: A simulation framework for evaluation of galaxy detection and deblending

Ismael Mendoza, Andrii Torchylo, Thomas Sainrat +18

We present an open source Python library for simulating overlapping (i.e., blended) images of galaxies and performing self-consistent comparisons of detection and deblending algori…

astro-ph.IM2022

Statistical Inference for Coadded Astronomical Images

Mallory Wang, Ismael Mendoza, Cheng Wang +2

Coadded astronomical images are created by stacking multiple single-exposure images. Because coadded images are smaller in terms of data size than the single-exposure images they s…

astro-ph.IM2022★ 1 cited

Scalable Bayesian Inference for Detection and Deblending in Astronomical Images

Derek Hansen, Ismael Mendoza, Runjing Liu +4

We present a new probabilistic method for detecting, deblending, and cataloging astronomical sources called the Bayesian Light Source Separator (BLISS). BLISS is based on deep gene…