activity
20102025
most citedRed Supergiant Stars in the Large Magellanic Cloud: I. The Period-Luminosity Relation

59 citations · 487 across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2025

Metallicity Distribution in M31 and M33 Based on the Tip-RGB Near-infrared Color

Ying Li, Biwei Jiang, Yi Ren

This study investigates the metallicity distribution in M31 and M33 by using the near-infrared color index of tip-red-giant-branch (TRGB) of the member stars from \cite{2021A…

astro-ph.GA2025

Extinction Distributions in Nearby Star-resolved Galaxies. I. M31

Yuxi Wang, Jian Gao, Yi Ren +1

An extinction distribution of the Andromeda Galaxy (M31) is constructed with member stars as tracers by fitting multiband photometric data from UKIRT/WFCAM, PS1, and Gaia DR3. The…

astro-ph.GA2025

New Red Supergiant Stars in the other side of our Galaxy

Lin Zhang, Bingqiu Chen, Yi Ren +3

Red supergiant stars (RSGs) are massive stars in a late stage of evolution, crucial for understanding stellar life cycles and Galactic structure. However, RSGs on the far side of o…

astro-ph.SR2024★ 3 cited

Searching for Galactic Red Supergiants with Gaia RVS Spectra

Zehao Zhang, Biwei Jiang, Yi Ren +2

Red supergiants (RSGs) are essential to understanding the evolution and the contribution to the interstellar medium of massive stars. However, the number of identified RSGs within…

astro-ph.SR2024

Data-driven stellar intrinsic colors and dust reddenings for spectro-photometric data: From the blue-edge method to a machine-learning approach

He Zhao, Shu Wang, Biwei Jiang +4

Intrinsic colors (ICs) of stars are essential for the studies on both stellar physics and dust reddening. In this work, we developed an XGBoost model to predict the ICs with the at…

astro-ph.SR2024★ 1 cited

Modeling of Granulation in Red Supergiants in the Magellanic Clouds with the Gaussian Process Regressions

Zehao Zhang, Yi Ren, Biwei Jiang +2

The granulation of red supergiants (RSGs) in the Magellanic Clouds are systematically investigated by combining the latest RSGs samples and light curves from the Optical Gravitatio…