activity
20132023
most citedM dwarf catalog of LAMOST pilot survey

49 citations · 151 across the 11 of their papers we have counts for

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Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2023

Estimating Stellar Parameters and Identifying Very Metal-poor Stars Using Convolutional Neural Networks for Low-resolution Spectra (R~200)

Tianmin Wu, Yude Bu, Jianhang Xie +5

Very metal-poor (VMP, [Fe/H]<-2.0) stars offer a wealth of information on the nature and evolution of elemental production in the early galaxy and universe. The upcoming China Spac…

astro-ph.SR2022

Identifying hot subdwarf stars from photometric data using Gaussian mixture model and graph neural network

Wei Liu, Yude Bu, Xiaoming Kong +2

Hot subdwarf stars are very important for understanding stellar evolution, stellar astrophysics, and binary star systems. Identifying more such stars can help us better understand…

astro-ph.SR2022★ 4 cited

Searching for Barium Stars from the LAMOST Spectra Using the Machine Learning Method: I

Fengyue Guo, Zhongding Cheng, Xiaoming Kong +5

Barium stars are chemically peculiar stars that exhibit enhancement of s-process elements. Chemical abundance analysis of barium stars can provide crucial clues for the study of th…

astro-ph.SR2018★ 21 cited

M subdwarf research. I. Identification, modified classification system, and sample construction

Shuo Zhang, A-Li Luo, Georges Comte +7

We propose a revision of the system developed by L'epine et al. (2007) for spectroscopic M subdwarf classification. Based on an analysis of subdwarf spectra and templates from Savc…

astro-ph.SR2017★ 2 cited

Low-resolution near-infrared spectroscopic signatures of unresolved ultracool companions to M dwarfs

N. J. Cook, D. J. Pinfield, F. Marocco +14

We develop a method to identify the spectroscopic signature of unresolved L-dwarf ultracool companions, which compares the spectra of candidates and their associated control stars…

astro-ph.SR2016★ 15 cited

A Method for Selecting M dwarfs with an Increased Likelihood of Unresolved Ultra-cool Companionship

N. J. Cook, D. J. Pinfield, F. Marocco +15

Locating ultra-cool companions to M dwarfs is important for constraining low-mass formation models, the measurement of sub-stellar dynamical masses and radii, and for testing ultra…

astro-ph.SR2013★ 49 cited

M dwarf catalog of LAMOST pilot survey

Z. P. Yi, A. L. Luo, Y. H. Song +17

We present a spectroscopic catalog of 67082 M dwarfs from the LAMOST pilot survey. For each spectrum of the catalog, spectral subtype, radial velocity, equivalent width of H, a…