activity
20212026
most citedSciences with the 2.5-meter Wide Field Survey Telescope (WFST)

117 citations · 123 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026

The atmospheric extinction curve at Lenghu site

Jin-Sheng Qiu, Xiao-Hui Xu, Qing-Feng Zhu +11

In this study, we use a dedicated spectroscopic telescope to carry out low-resolution measurements of the optical atmospheric extinction curve at Lenghu astronomical site in Qingha…

astro-ph.SR2024

Physical Parameters of 11,100 Short-Period ASAS-SN Eclipsing Contact Binaries

Xu-Zhi Li, Qing-Feng Zhu, Xu Ding +4

Starting from more than 11,200 short-period (less than 0.5 days) EW-type eclipsing binary candidates with the All-Sky Automated Survey for Supernovae (ASAS-SN) V-band light curves,…

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.IM2022★ 3 cited

A New Period Determination Method for Periodic Variable Stars

Xiao-Hui Xu, Qing-Feng Zhu, Xu-Zhi Li +4

Variable stars play a key role in understanding the Milky Way and the universe. The era of astronomical big data presents new challenges for quick identification of interesting and…

astro-ph.SR2022★ 3 cited

Disk dissipation, giant planet formation and star-formation-rate fluctuations in the past three-million-year history of Gould's Belt

Mingchao Liu, Jinhua He, Jixing Ge +3

Although episodic star formation (SF) had been suggested for nearby SF regions, a panoramic view to the latest episodic SF history in the solar neighborhood is still missing. By un…

astro-ph.SR2021

OO Dra: an Algol-type binary formed through an extremely helium-poor mass accretion revealed by asteroseismology

Xinghao Chen, Xiaobin Zhang, Yan Li +4

Based on the two-minutes TESS data, we analyzed intrinsic oscillations of the primary component and identified seven confident independent Scuti frequencies (, , $f_3…