activity
20242026
most citedLAMA: LAMOST Medium-Resolution Spectral Analysis Pipeline

11 citations · 33 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2026

Carbon in J0815+4729: Casting A Shadow of Doubt on the Interpretation of CH Absorption in the Most Primitive Stars

Junbo Zhang, Carlos Allende Prieto, Yeisson Osorio +7

We revisit the carbon abundance in the primitive iron-poor star J0815+4729 ([Fe/H] 5.49). J0815+4729 is so carbon-enhanced and oxygen-rich that, in addition to CH and C$_{2}…

astro-ph.GA20261 cited

PhDLspec: physical-prior embedded deep learning method for spectroscopic determination of stellar labels in high-dimensional parameter space

Tianmin Wu, Maosheng Xiang, Jianrong Shi +4

Unlocking the full physical information encoded in low-resolution spectra poses a significant challenge for astronomical survey analysis. Such a task demands modeling spectra and o…

astro-ph.SR2026

Lithium in Wide Binaries: Effective Temperature Governs Depletion while Rotation Plays a Minor Role

Cheng-Cheng Xie, Hai-Jun Tian, Jian-Rong Shi +1

Using a sample of 116 wide binary systems as coeval and chemically homogeneous stellar pairs, we investigate the factors governing lithium depletion in main-sequence stars. We reco…

astro-ph.SR2026

Identify ~20,000 Li-rich Giants in the LAMOST Low-Resolution Survey

Ming-Yi Ding, Liang Wang, Jian-Rong Shi +8

Li-rich giants serve as valuable tracers of stellar evolution and surface enrichment processes, for which a statistically large and homogeneous sample is crucial. Using the massive…

astro-ph.SR2026

Discovery of an Extremely Luminous Type II Cepheid in the Andromeda Giant Stellar Stream: Evidence for a Hierarchical Triple with an Inner Binary Merger

Pinjian Chen, Bingqiu Chen, Xiaodian Chen +7

We report the discovery of LAMOST J0041+3948, the most luminous post-AGB Type II Cepheid (TIIC) known, located in the Andromeda Giant Stellar Stream. Its spectral energy distributi…

astro-ph.GA2025

Chemical abundances of seven stars in the GD-1 stream

Jing-Kun Zhao, Guang-Wei Li, Wako Aoki +13

We present the first detailed chemical abundances for seven GD-1 stream stars from Subaru/HDS spectroscopy. Atmospheric parameters were derived via color calibrations (