activity
20242026
most citedYOLO-CL cluster detection in the Rubin/LSST DC2 simulation

4 citations · 5 across the 6 of their papers we have counts for

collaborators

7 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.GA2026

Impact of LSST systematics on stellar-stream density fluctuations for dark matter

Matthieu Pélissier, Peter S. Ferguson, Alex Drlica-Wagner +6

The Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) is expected to significantly advance the study of Milky Way stellar streams. In particular, the deep, precise…

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.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.GA2025★ 1 cited

Forecasting Dark Matter Subhalo Constraints from Stellar Streams using Implicit Likelihood Inference

Tri Nguyen, Rutong Pei, Zhuofu Li +9

The evidence for dark matter (DM) remains compelling, although attempts to understand its particle nature remain inconclusive. One promising method to study DM is detecting DM subh…

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…