activity
20182026
collaborators

12 papers

astro-ph.CO2026

Closing the Observational Gap in Cosmic Dynamics: AI-Enabled Reconstruction of the Universe's Vorticity and Rotational Flow Morphology

Ziyong Wu, Xu Xiao, Fuyu Dong +7

The cosmic vorticity field, an essential tracer of nonlinear structure formation, has remained observationally inaccessible because transverse galaxy motions are difficult to measu…

astro-ph.CO2025

The Most Probable Behaviour of the Dark Energy Equation of State Indicates a Thawing Quintessence Field: Tomographic Alcock-Paczyński Test with Redshift-Space Correlation Function II

Fuyu Dong, Changbom Park

We apply an extended Alcock-Paczyński (AP) test to the Sloan Digital Sky Survey data to constrain the dark energy models with the Chevallier-Polarski-Linder (CPL) parametrization o…

astro-ph.CO2025

Constraining with Lensing Statistics in Low and High Density Regions

Yiqi Huang, Fuyu Dong, Jun Zhang +2

Lensing studies are typically carried out around high density regions, such as groups and clusters, where the lensing signals are significant and indicative of rich density structu…

astro-ph.CO2025

Self-similar decomposition of the hierarchical merger tree of dark matter halos

Wenkang Jiang, Jiaxin Han, Fuyu Dong +1

In the CDM universe, structure formation is generally not a self-similar process, while some self-similarity remains in certain statistics which can greatly simplify our descrip…

astro-ph.CO2024

The direct measurement of gravitational potential decay rate at cosmological scales II -- Improved dark energy constraint from

Fuyu Dong, Pengjie Zhang, Haojie Xu +1

The gravitational potential decay rate (DR) is caused by the cosmic acceleration of the universe, providing a direct probe into the existence of dark energy (DE). We present measur…

astro-ph.GA2021

The clustering of galaxies in the DESI imaging legacy surveys DR8: I. the luminosity and color dependent intrinsic clustering

Zhaoyu Wang, Haojie Xu, Xiaohu Yang +5

In a recent study, we developed a method to model the impact of photometric redshift uncertainty on the two-point correlation function (2PCF). In this method, we can obtain both th…