Fig. 6
Main panel: modifield Herztsprung-Russell diagram showing the posterior PDF of 
as a function of Teff after interpolating with the Geneva stellar evolution tracks for stars on the main sequence. Masses are indicated and correspond to the bold tracks. The solid, dashed and dotted lines correspond to the 1-σ, 2-σ and 3-σ contours, respectively. Secondary panels: marginalised PDF of and Teff. In both panels, there are three histograms: dotted: input distribution; gray: output distribution; black: output distribution for ages < 12 Gyr.
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