activity
20232025
most citedA Differentiable Perturbation-based Weak Lensing Shear Estimator

10 citations · 16 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2025

Mock Observations for the CSST Mission: Multi-Channel Imager--The Cluster Field

Yushan Xie, Xiaokai Chen, Shuai Feng +20

The Multi-Channel Imager (MCI), one of the instruments aboard the China Survey Space Telescope (CSST), is designed to simultaneously observe the sky in three filters, covering wave…

astro-ph.CO2025★ 4 cited

CURLING -- II. Improvement on the Inference from Pixelized Cluster Strong Lens Modeling

Yushan Xie, Huanyuan Shan, Yiping Shu +9

Strongly lensed supernovae (glSNe) provide a powerful, independent method to measure the Hubble constant, , through time delays between their multiple images. The accuracy o…

astro-ph.CO2024

CURLING - I. The Influence of Point-like Image Approximation on the Outcomes of Cluster Strong Lens Modeling

Yushan Xie, Huanyuan Shan, Nan Li +11

Cluster-scale strong lensing is a powerful tool for exploring the properties of dark matter and constraining cosmological models. However, due to the complex parameter space, pixel…

astro-ph.CO2024★ 1 cited

A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing

Alan Junzhe Zhou, Yin Li, Scott Dodelson +4

The analyses of the next generation cosmological surveys demand an accurate, efficient, and differentiable method for simulating the universe and its observables across cosmologica…

astro-ph.CO2023★ 1 cited

Emulating power spectra for pre- and post-reconstructed galaxy samples

Yuting Wang, Ruiyang Zhao, Zhongxu Zhai +10

The small-scale linear information in galaxy samples typically lost during non-linear growth can be restored to a certain level by the density field reconstruction, which has been…

astro-ph.CO2023★ 10 cited

A Differentiable Perturbation-based Weak Lensing Shear Estimator

Xiangchong Li, Rachel Mandelbaum, Mike Jarvis +3

Upcoming imaging surveys will use weak gravitational lensing to study the large-scale structure of the Universe, demanding sub-percent accuracy for precise cosmic shear measurement…