activity
20052026
most citedGaia FGK Benchmark Stars - Metallicity

314 citations · 936 across the 18 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2026★ 1 cited

Solar twins in Gaia DR3 GSP-Spec II. Age distribution and its implications for the Sun's migration

Takuji Tsujimoto, Daisuke Taniguchi, Alejandra Recio-Blanco +2

Solar twins are among the most powerful tracers of Galactic disk evolution owing to their unique property of sharing nearly solar metallicities ([Fe/H] ~ 0) while spanning a wide r…

astro-ph.GA2025★ 1 cited

Caveats about measuring carbon abundances in stars using the CH band

Pablo Santos-Peral, Patricia Sánchez-Blázquez, Alejandro Vazdekis +4

Deriving accurate carbon abundance estimates for a wide variety of stars is still complex due to the difficulties in properly measuring it from atomic and molecular lines. The aim…

astro-ph.GA2019★ 49 cited

The bimodal [Mg/Fe] versus [Fe/H] bulge sequence as revealed by APOGEE DR14

A. Rojas-Arriagada, M. Zoccali, M. Schultheis +5

The Galactic bulge has a bimodal metallicity distribution function: different kinematic, spatial, and, potentially, age distributions characterize the metal-poor and metal-rich com…

astro-ph.GA2018★ 35 cited

The AMBRE Project: r-process elements in the Milky Way thin and thick discs

G. Guiglion, P. de Laverny, A. Recio-Blanco +1

The chemical evolution of neutron capture elements in the Milky Way disc is still a matter of debate. We aim to understand the chemical evolution of r-process elements in Milky Way…

astro-ph.GA2018★ 20 cited

The metal-rich halo component extended in z: a characterization with Gaia DR2 and APOGEE

Emma Fernández-Alvar, J. G. Fernández-Trincado, Edmundo Moreno +12

We report an analysis of the metal-rich tail ([Fe/H] ) of halo stars located at distances from the Galactic plane up to kpc, observed by the Apache Point…

astro-ph.GA2013★ 314 cited

Gaia FGK Benchmark Stars - Metallicity

Paula Jofre, U. Heiter, C. Soubiran +22

To calibrate automatic pipelines that determine atmospheric parameters of stars, one needs a sample of stars -- ``benchmark stars'' -- with well defined parameters to be used as a…