collaborators

7 papers

astro-ph.GA2026

A Tale of Two Dust Disks in Our Milky Way

Ruoyi Zhang, Haibo Yuan, Bingqiu Chen +4

Cosmic dust plays a vital role in stellar and galactic formation and evolution, but its three-dimensional structure in the Milky Way has remained unclear due to insufficient precis…

astro-ph.SR2025

Recalibration of the Landolt UBVRI Standard Stars and the Generation of 5.4 Million New UBVRI Standard Stars using LAMOST and Gaia

Bowen Huang, Haibo Yuan, Kai Xiao +1

We present an independent validation and recalibration of the Landolt 2013 (celestial equator and ) and 2016 () standard stars in the Johnson $U…

astro-ph.GA2025

A Comprehensive All-Sky Catalog of 3345 Molecular Clouds from Three-dimensional Dust Extinction

Tao Wang, Haibo Yuan, Bingqiu Chen +4

Understanding the distribution and properties of molecular clouds is crucial for tracing the structure and evolution of the interstellar medium and the large-scale morphology of th…

astro-ph.GA2025

An all-sky 3D dust map Based on Gaia and LAMOST

Tao Wang, Haibo Yuan, Bingqiu Chen +6

We present a comprehensive 3D dust reddening map covering the entire Milky Way, constructed by combining reddening estimates based on LAMOST low-resolution spectra (E(BV)$_{\rm…

astro-ph.GA2025

The Dust Extinction Curve: Beyond R(V)

Gregory M. Green, Xiangyu Zhang, Ruoyi Zhang

The dust extinction curve is typically parameterized by a single variable, R(V), in optical and near-infrared wavelengths. R(V) controls the slope of the extinction-vs.-wavelength…

astro-ph.SR2025

Metallicities of 20 Million Giant Stars Based on Gaia XP spectra

Lin Yang, Haibo Yuan, Bowen Huang +8

We design an uncertainty-aware cost-sensitive neural network (UA-CSNet) to estimate metallicities from dereddened and corrected Gaia BP/RP (XP) spectra for giant stars. This method…