activity
20242026
most citedCSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

24 citations · 47 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2026

Improved Cosmological Constraints from Morphology-Based Marked Correlation Functions

Xu Xiao, Zhao Chen, Yu Yu +2

The cosmic web contains morphology-dependent information that is not fully captured by standard two-point statistics. We construct morphology-based marked correlation functions (MC…

astro-ph.CO2026

Cosmological constraints from neighbor-density-weighted marked correlation functions

Xu Xiao, Zhao Chen, Yu Yu +3

We investigate whether neighbor-density-weighted marked correlation functions (MCFs) can extract cosmological information beyond the standard redshift-space two-point correlation f…

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.GA2026

ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations

Wensheng Hong, Xiaohu Yang, Junde Li +10

We present a highly scalable, MPI-parallelized framework for reconstructing the initial cosmic density field, designed to meet the computational demands of next-generation cosmolog…

astro-ph.CO2026

MIU2Net: weak-lensing mass inversion using deep learning with nested U-structures

Han W. G., An Zhao, Xinyue Chen +5

One of the primary goals of next-generation gravitational lensing surveys is to measure the large-scale distribution of dark matter, which requires accurate mass inversion to conve…

astro-ph.CO2025★ 2 cited

Extending CSST Emulator to post-DESI era

Zhao Chen, Yu Yu

The recent DESI BAO measurements have revealed a potential deviation from a cosmological constant, suggesting a dynamic nature of dark energy. To rigorously test this result, compl…

astro-ph.CO2025★ 6 cited

CSST Cosmological Emulator III: Hybrid Lagrangian Bias Expansion Emulation of Galaxy Clustering

Shuren Zhou, Zhao Chen, Yu Yu

Galaxy clustering is an important probe in the upcoming China Space Station Telescope (CSST) survey to understand the structure growth and reveal the nature of the dark sector. How…

astro-ph.CO2025

Validation of Fast Mocks Generation for CSST Photometric Survey

Yiming Hu, Yu Yu

Weak lensing has become a powerful tool for probing the matter distribution in the Universe and constraining cosmological parameters. This paper aims to explore the fast mock gener…

astro-ph.CO2025★ 7 cited

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation

Zhao Chen, Yu Yu

Accurate theoretical prediction for halo mass function across a broad cosmological space is crucial for the forthcoming China Space Station Telescope (CSST) observations, which wil…

astro-ph.CO2025★ 24 cited

CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

Zhao Chen, Yu Yu, Jiaxin Han +1

In the near future, the China Space Station Telescope (CSST) will obtain unprecedented imaging and spectroscopic data. The statistical errors in the cosmological parameter constrai…

astro-ph.GA2024★ 8 cited

PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies

Yun Zheng, Kun Xu, Y. P. Jing +6

The roles that mass and environment play in the galaxy quenching are still under debate. Leveraging the Photometric objects Around Cosmic webs (PAC) method, we analyze the excess s…