activity
20112025
most citedCarbon stars identified from LAMOST DR4 using Machine Learning

66 citations · 569 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.GA2025★ 1 cited

Scalable Stellar Parameter Inference Using Python-based LASP: From CPU Optimization to GPU Acceleration

Jun-Chao Liang, Yin-Bi Li, A-Li Luo +13

To enhance the efficiency, scalability, and cross-survey applicability of stellar parameter inference in large spectroscopic datasets, we present a modular, parallelized Python fra…

astro-ph.SR2024

An Empirical Sample of Spectra of M-type Stars with Homogeneous Atmospheric-Parameter Labels

Bing Du, A-Li Luo, Song Wang +6

The discrepancies between theoretical and observed spectra, and the systematic differences between various spectroscopic parameter estimates, complicate the determination of atmosp…

astro-ph.SR2024

Projected rotational velocities for LAMOST stars with effective temperature lower than 9000 K

Fang Zuo, A-Li Luo, Bing Du +5

In Data Release 9 of LAMOST, we present measurements of v sin i for a total of 121,698 stars measured using the Medium Resolution Spectrograph (MRS) and 80,108 stars using the Low…

astro-ph.GA2023

The Stellar Abundances and Galactic Evolution Survey (SAGES) -- -- I. General Description and the First Data Release (DR1)

Zhou Fan, Gang Zhao, Wei Wang +35

The Stellar Abundances and Galactic Evolution Survey (SAGES) of the northern sky is a specifically-designed multi-band photometric survey aiming to provide reliable stellar paramet…

astro-ph.SR2022★ 1 cited

A Spectroscopic Modelling Method for the Detached Eclipsing Binaries to Derive Atmospheric Parameters

Xiang-Lei Chen, A-Li Luo, Jian-Jun Chen +5

Based on luminosity contributions, we develop a spectroscopic modelling method to derive atmospheric parameters of component stars in binary systems. The method is designed for tho…

astro-ph.SR2022★ 3 cited

Identification and parameter determination of F-type Herbig stars from LAMOST DR8

Yun-Jin Zhang, A-Li Luo, Bi-Wei Jiang +5

We identify 20 F-type Herbig stars and provide a list of 22 pre-main-sequence candidates from LAMOST DR8. The effective temperature, distance, extinction, stellar luminosity, mass,…

astro-ph.SR2021★ 31 cited

LAMOST Time-Domain Survey: First Results of four 2 plates

Song Wang, Haotong Zhang, Zhongrui Bai +23

From Oct. 2019 to Apr. 2020, LAMOST performs a time-domain spectroscopic survey of four 2 plates with both low- and med-resolution observations. The low-resolution spectroscopic…

astro-ph.SR2021★ 4 cited

Study on Outliers in the Big Stellar Spectral Dataset of the Fifth Data Release (DR5) of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)

Yan Lu, A-Li Luo, Li-Li Wang +10

To study the quality of stellar spectra of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and the correctness of the corresponding stellar parameters derive…

astro-ph.SR2021★ 6 cited

Rotational Velocities of Am and Non-CP Stars based on Kepler and LAMOST DR5

Li Qin, A-Li Luo, Wen Hou +9

Rotation is a critical physical process operating in the formation of Am stars. There is a strong correlation between low-velocity rotation and chemical peculiarity. However, the e…

astro-ph.SR2020★ 11 cited

M Subdwarf Research. II. Atmospheric Parameters and Kinematics

Shuo Zhang, A-Li Luo, Georges Comte +12

Applying the revised M subdwarf classification criteria discussed in Paper I to LAMOST DR7, combining the M subdwarf sample from Savcheva et al, a new M subdwarf sample was constru…

astro-ph.SR2020★ 45 cited

LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS): Scientific goals and survey plan

Chao Liu, Jianning Fu, Jianrong Shi +38

Since September 2018, LAMOST starts a new 5-year medium-resolution spectroscopic survey (MRS) using bright/gray nights. We present the scientific goals of LAMOST-MRS and propose a…

astro-ph.SR2019★ 40 cited

Properties of Radial Velocities measurement based on LAMOST-II Medium-Resolution Spectroscopic Observations

R. Wang, A. -L. Luo, J. -J. Chen +28

The radial velocity (RV) is a basic physical quantity which can be determined through Doppler shift of the spectrum of a star. The precision of RV measurement depends on the resolu…

astro-ph.GA2019★ 27 cited

Bivariate Luminosity Function of Galaxy Pairs

Shuai Feng, Shi-Yin Shen, Fang-Ting Yuan +8

We measure the bivariate luminosity function (BLF) of galaxy pairs and use it to probe and characterize the galaxy-galaxy interaction between pair members. The galaxy pair sample i…

astro-ph.IM2019★ 16 cited

Recognition of M-type stars in the unclassified spectra of LAMOST DR5 using a hash learning method

Y. -X. Guo, A. -L. Luo, S. Zhang +6

Our study aims to recognize M-type stars which are classified as "UNKNOWN" due to bad quality in Large sky Area Multi-Object fibre Spectroscopic Telescope (LAMOST) DR5 V1. A binary…

astro-ph.SR2019★ 40 cited

Radial velocity measurements from LAMOST medium-resolution spectroscopic observations: A pointing towards the Kepler field

Nian Liu, Jian-Ning Fu, Weikai Zong +20

Radial velocity is one of key measurements in understanding the fundamental properties of stars, stellar clusters and the Galaxy. A plate of stars in the Kepler field were observed…

astro-ph.SR2018★ 17 cited

An Empirical Template Library for FGK and Late--type A Stars Using LAMOST Observed Spectra

Bing Du, A-Li Luo, F. Zuo +16

We present an empirical stellar spectra library created using spectra from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) DR5. This library represents a uni…

astro-ph.SR2018★ 7 cited

LEMONY--a Library of Empirical Medium-resolution spectra by Observations with the NAOC Xinglong 2.16\,m and YNAO Gaomeigu 2.4\,m telescopes

Chun Wang, Xiaowei Liu, Yang Huang +15

This study expands the coverage and improves the homogeneity of the distribution of MILES template stars in the parameter space, as well as extends the wavelength coverage of the t…

astro-ph.SR2018★ 26 cited

A new Hyper-Runaway star discovered from LAMOST and GAIA: ejected almost in the galactic rotation direction

Yin-Bi Li, A-Li Luo, Gang Zhao +11

In this paper, we report the discovery of a new late-B type unbound hyper-runaway star (LAMOST-HVS4) from the LAMOST spectroscopic surveys. According to its atmospheric parameters,…

astro-ph.GA2018★ 15 cited

Testing Area of the SAGE Survey

Jie Zheng, Gang Zhao, Wei Wang +4

Sky survey is one of the most important motivations to improve the astrophysics development, especially when using new photometric bands. We are performing the SAGE (Stellar Abunda…

astro-ph.IM2018★ 32 cited

The SAGE Photometric Sky Survey: Technical Description

Jie Zheng, Gang Zhao, Wei Wang +4

To investigate in more details of Stellar Abundance and Galactic Evolution (SAGE) and in a huge sample, we are performing a northern sky photometric survey named SAGES with the SAG…

astro-ph.GA2018★ 40 cited

The Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release Two and Three

X. Y. Dong, Xue-Bing Wu, Y. L. Ai +19

This is the second installment for the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) Quasar Survey, which includes quasars observed from September 2013 to June…

astro-ph.SR2018★ 66 cited

Carbon stars identified from LAMOST DR4 using Machine Learning

Yin-Bi Li, A-Li Luo, Chang-De Du +27

In this work, we present a catalog of 2651 carbon stars from the fourth Data Release (DR4) of the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST). Using an effici…

astro-ph.IM2016★ 27 cited

LAMOST Spectrograph Response Curves: Stability and Application to flux calibration

Bing Du, A-Li Luo, Zhong-Rui Bai +14

The task of flux calibration for LAMOST (Large sky Area Multi-Object Spectroscopic Telescope) spectra is difficult due to many factors. For example, the lack of standard stars, fla…

astro-ph.SR2015★ 21 cited

SDSS/SEGUE Spectral Feature Analysis For Stellar Atmospheric Parameter Estimation

Xiangru Li, Q. M. Jonathan Wu, Ali Luo +5

Large-scale and deep sky survey missions are rapidly collecting a large amount of stellar spectra, which necessitate the estimation of atmospheric parameters directly from spectra…