Equivalent widths measured in the UVES spectra in 2014 (EW(2014)) vs. equivalent widths measured in the GIRAFFE spectra in 2009 (EW(2009)), and residuals between the two. For each star the upper panel gives EW(2014) vs. EW(2009), and the lower panel gives the residuals. For star B-108, also the measurements with IRAF on the UVES spectra are compared with EW(2009).
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