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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.

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