activity
20242026
collaborators

6 papers

astro-ph.CO2026

Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys

Zhujun Jiang, Xu Xiao, Zhiwei Min +5

A central challenge in precision cosmology with galaxy surveys is to extract non-Gaussian information from large-scale structure while controlling systematic uncertainties such as…

astro-ph.CO2026

Extracting Cosmological Information from Lightcone Data: A Comparison of CNNs and Summary-Statistic-Based Approaches

Min Zhiwei, Xiao Xu, Jiang Zhujun +9

Lightcone observations are the natural data format of galaxy surveys, but their evolving geometry breaks the translational symmetry assumed by standard convolutional neural network…

astro-ph.CO2026

Enhancing cosmological constraints with nonlinear tanh transformations of Hermite-Gaussian Derivative fields

Zhiwei Min, Ye Ma, Zhujun Jiang +4

A key goal in large-scale structure analysis is to extract multi-scale information to improve cosmological parameter constraints. In particular, higher-order derivative fields are…

astro-ph.CO2025

A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure

Zhujun Jiang, Xiaolin Luo, Wenying Du +6

Large-scale structure (LSS) analysis in galaxy surveys is a powerful cosmological probe but is limited by tracer bias, which can obscure underlying information and weaken parameter…

astro-ph.CO2025

Enhancing Cosmological Constraints by Two-dimensional -cosmic-web Weighted Angular Correlation Functions

Fenfen Yin, Liang Xiao, Wenying Du +6

In this study, we investigate the potential of mark-weighted angular correlation functions (MACFs), which integrate -cosmic-web classification with angular correlation function…

astro-ph.CO2024

Deep learning for cosmological parameter inference from a dark matter halo density field

Zhiwei Min, Xu Xiao, Jiacheng Ding +11

We propose a lightweight deep convolutional neural network (lCNN) to estimate cosmological parameters from simulated three-dimensional dark matter (DM) halo distributions and assoc…