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Fig. 16.
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Difference between Teff (top), R (middle), and M (bottom) from Gaia for the FGKM sample and the PICv1.1 catalogue values normalised to their combined uncertainties for stars in common. We overlay the ±3σ lines. On each panel we also give the median difference (MD) and the MAD in K, R⊙, and M⊙, respectively.
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