Fig. 6.
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Relation between the inferred stellar mass and the measured luminosity from Gaia of the stars in the sample. The solid red line indicates the fitted mass-luminosity relation, yielding log(L⋆/L⊙)=4.0623(6)log(M⋆/M⊙)+0.3468(2). The black triangles indicate bin averaged-values. Average uncertainties are indicated by the red data point.
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