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20072026
most citedA wide star-black-hole binary system from radial-velocity measurements

200 citations · 1k across the 30 of their papers we have counts for

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astro-ph.SR2024

Minute-Cadence Observations of the LAMOST Fields with the TMTS: IV -- Catalog of Cataclysmic Variables from the First 3-yr Survey

Qichun Liu, Jie Lin, Xiaofeng Wang +24

The Tsinghua University--Ma Huateng Telescopes for Survey (TMTS) started to monitor the LAMOST plates in 2020, leading to the discovery of numerous short-period eclipsing binaries,…

astro-ph.SR2024★ 2 cited

The first low-mass eclipsing binary within the fully convective zone from TMTS

Cheng Liu, Xiaofeng Wang, Xiaobing Zhang +17

We present a comprehensive photometric and spectroscopic analysis of the short-period (5.32 hours) and low-mass eclipsing binary TMTSJ0803 discovered by Tsinghua-Ma Huateng T…

astro-ph.SR2024

Minute-Cadence Observations of the LAMOST Fields with the TMTS V. Machine Learning Classification of TMTS Catalogues of Periodic Variable Stars

Fangzhou Guo, Jie Lin, Xiaofeng Wang +17

Periodic variables are always of great scientific interest in astrophysics. Thanks to the rapid advancement of modern large-scale time-domain surveys, the number of reported variab…

astro-ph.SR2024

Variable white dwarfs in TMTS: Asteroseismological analysis of a ZZ Ceti star, TMTS J17184064+2524314

Jincheng Guo, Yanhui Chen, Yonghui Yang +24

The Tsinghua University-Ma Huateng Telescope for Survey (TMTS) has been constantly monitoring the northern sky since 2020 in search of rapidly variable stars. To find variable whit…

astro-ph.SR2023★ 16 cited

A seven-Earth-radius helium-burning star inside a 20.5-min detached binary

Jie Lin, Chengyuan Wu, Heran Xiong +28

Binary evolution theory predicts that the second common envelope (CE) ejection can produce low-mass (0.32-0.36 Msun) subdwarf B (sdB) stars inside ultrashort-orbital-period binary…

astro-ph.SR2023

LAMOST J2043+3413 -- a Fast Disk Precession SW Sextans Candidate in Period Gap

Xin Li, Xiaofeng Wang, Jiren Liu +5

We present follow-up photometric observations and time-series analysis of a nova-like, SW Sextans-type, cataclysmic variable (CV) candidate, LAMOST J204305.95+341340.6 (here after…