Top: marginalised posterior probability distribution (PPD) for the stellar inclination i_⋆. Here we have folded the full distribution (−90 to 180°) onto the the range from 0 to 90°. Bottom right: PPD for the rotational splitting. Bottom left: correlation map between the inclination and the rotational splitting. The 68% credible regions (highest posterior density credible regions) are indicated by the dark-grey parts, while light-grey indicates the additional parts covered in a 95% credible region. Included are also lines of constant v sin i_⋆, computed using the radius estimate from our analysis and with v sin i_⋆ values from the literature (see Table 3), arranged in the legend in order of increasing v sin i_⋆ value (top to bottom). The dashed black horizontal line indicates the value of ν_s = 5 μHz above which walkers were excluded from the PPDs. The grey dash-dotted lines give lines of constant v sin i_⋆ from 8 to 48 km s^-1 in steps of 8 km s^-1.