collaborators

5 papers

astro-ph.CO2026

ELUCID-DESI II. Revealing dark matter mass, tidal, and velocity (MTV) fields using galaxy group phase information

Qingyang Li, Xiaohu Yang, Wensheng Hong +24

We introduce a novel method for reconstructing the cosmic mass, tidal, and velocity (MTV) fields over the redshift range using the phase information of galaxy groups.…

astro-ph.IM2026

AstroSkyFlow: an astronomical sky image flow simulator for time domain survey validation and machine learning

Kexin Li, Yicheng Rui, Fabo Feng +5

Modern time-domain optical surveys produce massive data volumes that require robust, high-fidelity simulated datasets for developing and validating automated pipelines and machine-…

astro-ph.GA2026

What can galaxy clustering really tell us about the galaxy-halo connections?

Xiaoju Xu, Xiaohu Yang, Zhongxu Zhai +6

Subhalo abundance matching (SHAM) is a commonly used framework for modeling the galaxy-halo connection. Yet, its standard implementation has difficulty reproducing the observed gal…

astro-ph.CO2026

Filtering Interlopers with Photometry and Diagnostic Features: A Machine Learning Framework Validated with CSST Slitless Spectroscopy

Hui Peng, Yu Yu, Yiyang Guo +13

The slitless spectroscopic method employed by missions such as Euclid and the Chinese Space-station Survey Telescope (CSST) faces a fundamental challenge: spectroscopic redshifts d…

astro-ph.SR2025

Search for Past Stellar Encounters and the Origin of 3I/ATLAS

Yiyang Guo, Luyao Zhang, Fabo Feng +3

3I/ATLAS, the third discovered interstellar object, has a heliocentric speed of 58 km/s and exhibits cometary activity. To constrain the origin of 3I/ATLAS and its past dynamical e…