collaborators

11 papers

stat.ME2026

OASIS: Observation-Aware Simulation-Based Inference via Distributional Matching

Arya Farahi, Conghao Zhou, Ritwik Vashistha

We introduce OASIS, a simulation-based inference framework for scientific settings where observations are distorted by measurement error, selection effects, and other survey-specif…

astro-ph.CO2026

Accurate Galaxy Cluster Shear and Mass Calibration for LSST with AnaCal

Conghao Zhou, Xiangchong Li, Hao-Yi Wu +12

The observed abundance of galaxy clusters as a function of mass and redshift provides a powerful route to precision cosmology; a key challenge for cluster cosmology is to establish…

astro-ph.IM2026

The Vera C. Rubin Observatory Data Preview 1

Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325

We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…

astro-ph.CO2026

Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters

Titus Nyarko Nde, Hao-Yi Wu, Shulei Cao +4

Weak gravitational lensing signals of optically identified clusters are impacted by a selection bias -- halo triaxiality and large-scale structure along the line of sight simultane…

astro-ph.GA2025

Reaching for the Edge II: Stellar Halos out to Large Radii as a Tracer of Dark Matter Halo Mass

Katya Leidig, Benedikt Diemer, Song Huang +3

The diffuse outskirts of brightest cluster galaxies (BCGs) encode valuable information about the assembly history and mass of their host dark matter halos. However, the low surface…

astro-ph.CO2025

Cosmological Constraints from Dark Energy Survey Year 1 Cluster Lensing and Abundances with Simulation-based Forward-Modeling

Andrés N. Salcedo, Eduardo Rozo, Hao-Yi Wu +7

We present a simulation-based forward-modeling framework for cosmological inference from optical galaxy-cluster samples, and apply it to the abundance and weak-lensing signals of D…