activity
20172024
most citedDistances of Galactic Supernova Remnants Using Red Clump Stars

43 citations · 133 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2024

Transit Timing Variation of K2-237b: Hints Toward Planet Disk Migration

Fan Yang, Richard J. Long, Eamonn Kerins +8

Hot Jupiters should initially form at considerable distances from host stars and subsequently migrate towards inner regions, supported directly by transit timing variation (TTV). W…

astro-ph.GA2023★ 4 cited

Three New Spiral Galaxies with Active Nuclei Producing Double Radio Lobes

Xuyang Gao, Zhongsheng Yuan, Jinlin Han +2

Double radio lobes are generally believed to be produced by active nuclei of elliptical galaxies. However, several double-lobed radio sources have been solidly found to be associat…

astro-ph.EP2022★ 6 cited

Detecting and Monitoring Tidal Dissipation of Hot Jupiters in the Era of SiTian

Fan Yang, Wei Wang, Xing Wei +13

Transit Timing Variation (TTV) of hot Jupiters provides direct observational evidence of planet tidal dissipation. Detecting tidal dissipation through TTV needs high precision tran…

astro-ph.EP2021★ 11 cited

TESS Timings of 31 Hot Jupiters with Ephemeris Uncertainties

Su-Su Shan, Fan Yang, You-Jun Lu +8

A precise transit ephemeris serves as the premise for follow-up exoplanet observations. We compare TESS Objects of Interest (TOI) transit timings of 262 hot Jupiters with the archi…

astro-ph.SR2021★ 7 cited

LTD064402+245919: A Subgiant with a 1-3 M Undetected Companion Identified from LAMOST-TD Data

Fan Yang, Bo Zhang, Richard J. Long +11

Single-line spectroscopic binaries recently contribute to the stellar-mass black hole discovery, independently of the X-ray transient method. We report the identification of a sing…

astro-ph.EP2021★ 9 cited

An Empirical Bayesian Approach to Limb-darkening in Modeling WASP-121b Transit Light Curves

Fan Yang, Richard J. Long, Ji-Feng Liu +6

We present a novel, iterative method using an empirical Bayesian approach for modeling the limb darkened WASP-121b transit from the TESS light curve. Our method is motivated by the…