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Fig. 6

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Stellar mass estimated from our Gaia catalogue (y-axis) versus the one given in the exoplanet online tables (x-axis). The black dots correspond to the full sample, while the HQ sample is colour-coded by TeffGaia$T_{\rm eff}^\Gaia$. The grey dotted lines show ratios of 2 and 1/2 as visual reference. We refer to Fig. 2 to see the distribution of the MGaia/MLit$M_\star^\Gaia/M_\star^\Lit$ ratio.

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