Fig. 31.
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Comparison of the SPSS sample main parameters derived here with the two reference sets by Pancino et al. (2021): the best-fit parameters to the SPSS flux tables are shown in grey, while a collection of literature spectroscopic estimates is coloured according to the interstellar absorption A0 obtained here. Left, middle, and right panels: the cases of Teff, log g, and [Fe/H], respectively. The 1:1 line is shown in green in all panels.
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