log g vs. T_eff diagrams of Milky Way field stars in the metallicity range −0.2 < [Fe/H] < +0.2, available in iDR6. In the large panel we show the recommended stellar parameters from WG11 (in orange), while in the small panels we plot the results of the seven individual nodes contributing to the final parameters. Parsec isochrones (Bressan et al. 2012) at solar metallicity, and at three different ages are shown: 2 Gyr (in red), 5 Gyr (in black), 7 Gyr (in blue).