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Fig. 6.


Mass residuals (MSP − MGCS11) between the mean mass value (MSP) delivered by SPInS and the expected (i.e. also mean) mass (MGCS11) given in the GCS11 (Casagrande et al. 2011) for the 12 704 stars with good masses as defined in the text, with no filtering on the parallax error. For ten stars, the masses determined by SPInS and by Casagrande et al. differ by more than 10 per cent. The horizontal grey line shows the locus of equal masses and the dashed lines are for masses differing by ±10 per cent. The colours distinguish stars according to their metallicity.

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