Fig. 5

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Normalised cumulative histograms for [Fe/H], [Mg/Fe], and [Si/Fe] for the stars analysed in this work. The stars have been separated into two populations: stars with known planets (red) and stars without known planets (green). Our statistical analysis reveals that the distributions corresponding to this two populations are not different according to the Kolmogorov-Smirnoff test (see text for details).
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