most citedSpectroscopic analysis of metal-poor stars from LAMOST: early results

80 citations · 197 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201511 cited

Palladium and silver abundances in stars with [Fe/H] > -2.6

Xiaoshu Wu, Liang Wang, Jianrong Shi +2

Palladium (Pd) and silver (Ag) are the key elements for probing the weak component in the rapid neutron-capture process (r-process) of stellar nucleosynthesis. We performed a detai…

astro-ph.SR201513 cited

Calibrating the α parameter of convective efficiency using observed stellar properties

X. S. Wu, S. Alexeeva, L. Mashonkina +3

Context. Synthetic model atmosphere calculations are still the most commonly used tool when determining precise stellar parameters and stellar chemical compositions. Besides three-…

astro-ph.IM201550 cited

Comb-calibrated solar spectroscopy through a multiplexed single-mode fiber channel

R A Probst, L Wang, H-P Doerr +7

We investigate a new scheme for astronomical spectrograph calibration using the laser frequency comb at the Solar Vacuum Tower Telescope on Tenerife. Our concept is based upon a si…

astro-ph.SR201580 cited

Spectroscopic analysis of metal-poor stars from LAMOST: early results

Hai-Ning Li, Gang Zhao, Norbert Christlieb +5

We report on early results from a pilot program searching for metal-poor stars with LAMOST and follow-up high-resolution observation acquired with the MIKE spectrograph attached to…

astro-ph.EP201443 cited

The Pan-Pacific Planet Search. II. Confirmation of a two-planet system around HD 121056

Robert A. Wittenmyer, Liang Wang, Fan Liu +5

Precise radial velocities from the Anglo-Australian Telescope confirm the presence of a rare short-period planet around the K0 giant HD 121056. An independent two-planet solution u…

astro-ph.IM2014

Asteroseismic based estimation of the surface gravity for the LAMOST giant stars

Chao Liu, Min Fang, Yue Wu +7

Asteroseismology is one of the most accurate approaches to estimate the surface gravity of a star. However, most of the data from the current spectroscopic surveys do not have aste…