Fig. 6
The central panel shows the posterior probability-density distribution for stellar age against stellar mass for WASP-30. The contours show the 1-, 2- and 3-σ confidence regions; the side panels show the marginalised distributions as histograms. The data derive from interpolating using the mean stellar density, Teff and metallicity, into the Geneva stellar evolution tracks (Mowlavi et al. 2012).
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