activity
20212026
most citedLAMA: LAMOST Medium-Resolution Spectral Analysis Pipeline

11 citations · 37 across the 15 of their papers we have counts for

collaborators

15 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

Aims. 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 C2 m…

astro-ph.GA2026★ 1 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 (…

astro-ph.SR2025★ 11 cited

Homogeneous Stellar Atmospheric Parameters and 22 Elemental Abundances for FGK Stars Derived From LAMOST Low-resolution Spectra with DD-Payne

Meng Zhang, Maosheng Xiang, Yuan-Sen Ting +11

A deep understanding of our Galaxy desires detailed decomposition of its stellar populations via their chemical fingerprints. This requires precise stellar abundances of many eleme…

astro-ph.SR2025

Revisiting the Li abundances of Stars with and without Detected Planets from the High Resolution Spectroscopy

Jinxiao Qin, Hong-Liang Yan, Wenyuan Cui +12

Whether the presence of planets affects the lithium (Li) abundance of their host stars is still an open question. To investigate the difference of the Li abundance between planet-h…

astro-ph.SR2025★ 2 cited

LAMOST YSOs. I. Spectroscopically identifying and characterizing M-type young stellar objects

Xiang-Song Fang, Jian-Rong Shi, Ming-Yi Ding +1

This study utilized LAMOST low-resolution spectra to identify M-type YSOs and characterize their accretion signatures. We measured characteristic features, including hydrogen Balme…

astro-ph.IM2024

Mining double-line spectroscopic candidates in the LAMOST medium-resolution spectroscopic survey using human-AI hybrid method

Shan-shan Li, Chun-qian Li, Chang-hua Li +5

We utilize a hybrid approach that integrates the traditional cross-correlation function (CCF) and machine learning to detect spectroscopic multi-systems, specifically focusing on d…

astro-ph.SR2024★ 11 cited

LAMA: LAMOST Medium-Resolution Spectral Analysis Pipeline

Chun-qian Li, Jian-rong Shi, Hong-liang Yan +3

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) has obtained more than 23 million spectra, opening an unprecedented opportunity to study stellar physics, as…

astro-ph.SR2024★ 8 cited

Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78

Xiao-Jin Xie, Jianrong Shi, Hong-Liang Yan +9

Highly r-process-enhanced stars are rare and usually metal-poor ([Fe/H] < - 1.0), and mainly populate the Milky Way halo and dwarf galaxies. This study presents the discovery of a…

astro-ph.SR2024

Reconstructing Intrinsic Stellar Noise with Stellar Atmospheric Parameters and Chromospheric Activity

Jinghua Zhang, Maosheng Xiang, Jie Yu +9

Accurately characterizing intrinsic stellar photometric noise induced by stellar astrophysics, such as stellar activity, granulation, and oscillations, is of crucial importance for…

astro-ph.SR2024

Lithium Abundances from the LAMOST Med-Resolution Survey Data Release 9

Ming-Yi Ding, Jian-Rong Shi, Hong-liang Yan +9

Lithium is a fragile but crucial chemical element in the universe, exhibits interesting and complex behaviors. Thanks to the massive spectroscopic data from the Large Sky Area Mult…

astro-ph.SR2021★ 4 cited

Chemical abundances of three new Ba stars from the Keck/HIRES spectra

Shuai Liu, Liang Wang, Jian-Rong Shi +4

Based on high resolution, high signal-to-noise (S/N) ratio spectra from Keck/HIRES, we have determined abundances of 20 elements for 18 Ba candidates. The parameter space of these…