Fig. 14
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Comparison of the pairwise differences between the predicted values from the S-PLUS (this work), J-PLUS and spectroscopic values from GALAH for [Fe/H], Teff, and log g, for 186 dwarf stars. The dashed-dotted lines represent mean value of each distribution. The 1σ value of the difference of each pair of surveys are displayed in the legend.
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