collaborators

6 papers

astro-ph.SR2025

Identify Main-sequence Binaries from the Chinese Space Station Telescope Survey with Machine Learning. II. Based on Gaia and GALEX

Jia-jia Li, Jian-ping Xiong, Zhi-jia Tian +3

The statistical characteristics of double main-sequence (MS) binaries are essential for investigating star formation, binary evolution, and population synthesis. Our previous study…

astro-ph.SR2024

The Red Supergiant Progenitor of the Type II Supernova 2024abfl

Jingxiao Luo, Lifu Zhang, Bing-Qiu Chen +9

Linkage between core-collapse supernovae (SNe) and their progenitors is not fully understood and ongoing effort of searching and identifying the progenitors is needed. $\mathrm{SN\…

astro-ph.SR2024

Fundamental Parameters of a Binary System Consisting of a Red Dwarf and a Compact Star

Xu Ding, KaiFan Ji, ZhiMing Song +7

TIC 157365951 has been classified as a Scuti type by the International Variable Star Index (VSX). Through the spectra from Large Sky Area Multi-Object Fiber Spectroscopic Tele…

astro-ph.SR2024

Estimating the Atmospheric Parameters of Early-type Stars from the Chinese Space Station Telescope (CSST) Slitless Spectra Survey

JiaRui Rao, HaiLiang Chen, JianPing Xiong +6

The measurement of atmospheric parameters is fundamental for scientific research using stellar spectra. The Chinese Space Station Telescope (CSST), scheduled to be launched in 2024…

astro-ph.IM2024

A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey

JinLiang Wang, Xu Ding, JiaJia Li +3

With the continuous development of large optical surveys, a large number of light curves of late-type contact binary systems (CBs) have been released. Deriving parameters for CBs u…

astro-ph.SR2024

The First Photometric Analysis of Two Low Mass Ratio Contact Binary Systems In TESS Survey

Qiyuan Cheng, Jianping XIong, Xu Ding +8

Low mass-ratio (q) contact binary systems are progenitors of stellar mergers such as blue straggles (BS) or fast-rotating FK Com stars. In this study, we present the first light cu…