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

5 citations · 9 across the 5 of their papers we have counts for

collaborators

5 papers

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.CO2025

Tomographic Alcock-Paczynski Test with Marked Correlation Functions

Liang Xiao, Limin Lai, Zhujun Jiang +2

The tomographic Alcock-Paczynski(AP) method, developed over the past decade, exploits redshift evolution for cosmological determination, aiming to mitigate contamination from redsh…

astro-ph.CO2024

AI-Powered Reconstruction of Dark Matter Velocity Fields from Redshift-Space Halo Distribution

Xu Xiao, Jiacheng Ding, XiaoLin Luo +6

We propose a UNet-based deep learning model to reconstruct the real-space dark matter (DM) velocity field from the redshift-space distribution of sparse DM halos. Using various sta…

astro-ph.CO2024★ 5 cited

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…

astro-ph.CO2024★ 4 cited

Improving SDSS cosmological constraints through -skeleton weighted correlation functions

Fenfen Yin, Jiacheng Ding, Limin Lai +6

The -skeleton approach can be conveniently utilized to construct the cosmic web based on the spatial geometry distribution of galaxies, particularly in sparse samples. This meth…