activity
20152020
most citedEstimation of distances to stars with stellar parameters from LAMOST

42 citations · 62 across the 5 of their papers we have counts for

collaborators

12 papers

astro-ph.SR202015 cited

Stellar Spectral Interpolation using Machine Learning

Kaushal Sharma, Harinder P. Singh, Ranjan Gupta +6

Theoretical stellar spectra rely on model stellar atmospheres computed based on our understanding of the physical laws at play in the stellar interiors. These models, coupled with…

astro-ph.GA2018

GD-1: the relic of an old metal-poor globular cluster

Guang-Wei Li, Brian Yanny, Yue Wu

Combining data from Gaia DR2, SDSS DR14 and LAMOST DR6, we update the fit to model of the properties of the stellar stream GD-1 and find that it has an age of Gyr, [Fe/H]…

astro-ph.SR2018

LAMOST observations in the Kepler field. II. Database of the low-resolution spectra from the five-year regular survey

Weikai Zong, Jian-Ning Fu, Peter De Cat +19

The LAMOST-Kepler (LK-) project was initiated to use the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) to make spectroscopic follow-up observations for the tar…

astro-ph.GA2018

Time stamps of vertical phase mixing in the Galactic disk from LAMOST-Gaia stars

Hai-Jun Tian, Chao Liu, Yue Wu +2

The perturbation mechanism of the Galactic disk has puzzled us for a long time. The imprints from perturbations provide important diagnostics on the disk formation and evolution. H…

astro-ph.GA2018

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

Misclassified B stars in the Kepler field

Chunguang Zhang, Chao Liu, Yue Wu +7

Stellar fundamental parameters are important in the asteroseismic study of Kepler light curves. However, the most used estimates in the Kepler Input Catalog (KIC) are not accurate…