activity
20212025
most citedSciences with the 2.5-meter Wide Field Survey Telescope (WFST)

117 citations · 135 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco

Chao Yang, Zhizheng Pan, Min Fang +34

We carry out deep imaging of the Milky Way satellite galaxies, Bootes III and Draco, with WFST as one pilot observing program to demonstrate the capability of WFST. Combining catal…

astro-ph.GA2025

ViT-based Local Volume dwarf galaxy Identificationin (VIDA) in the CSST survey

Han Qu, Zhen Yuan, Chengliang Wei +11

Identifying dwarf galaxies within the Local Volume is crucial for constraining the luminosity function of satellite galaxies in the nearby universe. We report the detection capabil…

astro-ph.IM2024★ 1 cited

How to coadd images: II. Anti-aliasing and PSF deconvolution

Lei Wang, Huanyuan Shan, Lin Nie +8

We have developed a novel method for co-adding multiple under-sampled images that combines the iteratively reweighted least squares and divide-and-conquer algorithms. Our approach…

astro-ph.IM2023★ 117 cited

Sciences with the 2.5-meter Wide Field Survey Telescope (WFST)

WFST Collaboration, Tinggui Wang, Guilin Liu +60

The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility being built jointly by the University of Science and Technology of China and the Purple Mountai…

astro-ph.GA2022★ 15 cited

Local Group Dwarf Galaxy Detection Limit in the CSST survey

Han Qu, Zhen Yuan, Amandine Doliva-Dolinsky +9

We predict the dwarf galaxy detection limits for the upcoming Chinese Space Station Telescope (CSST) survey that will cover 17,500 deg of the sky with a wide field of view of…

astro-ph.GA2021★ 2 cited

The Formation of M101-alike Galaxies in the Cold Dark Matter Model

Dali Zhang, Yu Luo, Xi Kang +1

The population of satellite galaxies in a host galaxy is a combination of the cumulative accretion of subhaloes and their associated star formation efficiencies, therefore, the lum…