activity
20232026
most citedA Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey

10 citations · 16 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Surface brightness-color relations for red giant branch stars: Observational constraints on metallicity effects using the ARD method

Jianping Xiong, Xiaodian Chen, Jiao Li +5

Aims: We aim to quantify the metallicity dependence of the SBCR for red giant branch (RGB) stars and to test the robustness of the relation using asteroseismic radii, Gaia distance…

astro-ph.SR2025

Fundamental Parameters for Totally Eclipsing Contact Binaries Observed by TESS

Xu Ding, KaiFan Ji, ZhiMing Song +5

Totally eclipsing contact binaries provide a unique opportunity to accurately determine mass ratios through photometric methods alone, eliminating the need for spectroscopic data.…

astro-ph.SR2025

Detection of Semidetached Eclipsing Binaries from TESS

Xu Ding, KaiFan Ji, QiYuan Cheng +4

Semidetached binaries, distinguished by their mass transfer phase, play a crucial role in elucidating the physics of mass transfer within interacting binary systems. To identify th…

astro-ph.SR2025★ 1 cited

Surface brightness-color relations for red giant branch stars using asteroseismic radii and Gaia distances (the ARD method)

Jianping Xiong, Qiyuan Cheng, Xiaodian Chen +4

Aims. Asteroseismic radius and Gaia distance (ARD) method has been proposed to establish the SBCRs for late-type stars. Methods. We select Kepler RGB stars with high-precision aste…

astro-ph.SR2024★ 5 cited

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

Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST

Tongyu He, Jiao Li, Jiangdan Li +8

Triple star systems are critical for understanding stellar dynamics and compact objects in astrophysics, yet confirmed hierarchical triples identified via spectroscopy remain limit…

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 Teles…

astro-ph.IM2024★ 10 cited

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…

astro-ph.SR2023

The Distribution of Semi-Detached Binaries. I.An Efficient Pipeline

JianPing Xiong, Xu Ding, Jiadong Li +5

Semi-detached binaries are in the stage of mass transfer and play a crucial role in studying mass transfer physics between interacting binaries. Large-scale time-domain surveys pro…