Fig. B.2.
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Comparison of the photometric metallicities derived by the SOS Cep&RRL pipeline and the metal abundances from high-resolution spectra of 16 RR Lyrae stars in Pancino et al. (2015) (left panel) and the metal abundances listed in Column 10 of Table A.3 of 19 RR Lyrae stars used to validate the RV curves from the RVS (right panel).
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