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Fig. 7


Marginalised posterior distribution of radii given flux, , plotted for different planet masses; see Eq. (12). The shaded region is the central 68% interval within which 68% of planet true radii should lie for a given incident flux and planet mass. It represents the 1σ points of ; the central dashed line is the median and the dotted lines are the 95% interval. The red points represent the posterior true values of the planet parameters of our sample with posterior uncertainty error bars.

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