activity
20072021
most citedSystematic non-LTE study of the [Fe/H] F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu

169 citations · 517 across the 10 of their papers we have counts for

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5 papers · 1 filter

astro-ph.SR2020★ 44 cited

Detailed chemical compositions of planet hosting stars: I. Exploration of possible planet signatures

F. Liu, D. Yong, M. Asplund +5

We present a line-by-line differential analysis of a sample of 16 planet hosting stars and 68 comparison stars using high resolution, high signal-to-noise ratio spectra gathered us…

astro-ph.SR2016★ 169 cited

Systematic non-LTE study of the [Fe/H] F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu

G. Zhao, L. Mashonkina, H. L. Yan +14

For the first time, we present an extensive study of stars with individual non-local thermodynamic equilibrium (NLTE) abundances for 17 chemical elements from Li to Eu in a sample…

astro-ph.SR2016★ 86 cited

The chemical compositions of solar twins in the open cluster M67

F. Liu, M. Asplund, D. Yong +5

Stars in open clusters are expected to share an identical abundance pattern. Establishing the level of chemical homogeneity in a given open cluster deserves further study as it is…

astro-ph.SR2015★ 21 cited

The detailed chemical composition of the terrestrial planet host Kepler-10

F. Liu, D. Yong, M. Asplund +7

Chemical abundance studies of the Sun and solar twins have demonstrated that the solar composition of refractory elements is depleted when compared to volatile elements, which coul…

astro-ph.SR2015★ 89 cited

Systematic NLTE study of the -2.6 < [Fe/H] < 0.2 F and G dwarfs in the solar neighbourhood. I. Stellar atmosphere parameters

T. Sitnova, G. Zhao, L. Mashonkina +9

We present atmospheric parameters for 51 nearby FG dwarfs uniformly distributed over the -2.60 < [Fe/H] < +0.20 metallicity range that is suitable for the Galactic chemical evoluti…