Fig. A.1.
Chemical abundances of [X/Fe] against [Fe/H] for Mg I, Al I, Si I, Ca I, Ti II, Ni I, and Y II for the K2@Gaia-ESO stars derived based on the final stellar parameters. First column: node (EP,LM) and instrument (U, G) results as specified in the legend. The [Fe/H] overlap is bounded by dashed red lines. The errorbars are the line-by-line values per star per node uncertainties. Second column: homogenised abundances without per node corrections. Third column: node values with corrections applied. Fourth column: final homogenised values.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.