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Fig. 14


Two-dimensional posterior probability distribution of νrot and i for KIC 10273246 (the colorbar decodes the probability density level). The prior on i is uniform over the plotted range, whereas the prior on νrot is uniform over the interval 0–2μHz with a decaying Gaussian wing for higher values of the splitting. The dot-dashed line marks the estimate of the stellar rotational period given in Sect. 4.2. Furthermore, the Prot(i) relation (solid curve) of Creevey et al. (in preparation) is shown together with the corresponding confidence interval (dotted curves).

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