Fig. D.2
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Iron abundance versus V absolute magnitude, using a subset of set B(see Table 3 and text forthe selection ofthis subset). Lines are the resulting linear regressions. For better visibility, the set using Fourier-based abundances (FEH31) has been shifted downward by 2 mag with respect of the set using the mixture of gravity and source ZP-corrected HDS and LDS metallicities.
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