gravito-inertial modes and using the $f_{rot}$ and $\Delta\Pi_{l}$ values obtained from the analysis of the marked prograde series. The white diamonds indicate the model computed for Rossby waves using the same $f_{rot}$ and $\Delta\Pi_{l}$ values, assuming $m=-1$ and $k=-2$ in the k-based indexing scheme by @Lee1997. *Bottom:* The residuals of the fit to the prograde period spacing series.](KIC12066947_wresid2.pdf){width="88mm"}

Sample study {#subsec:sample}
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Subsequently, we also applied our methodology to the other stars in our sample. This led to the mode identification and the determination of the rotation rate $f_{\rm rot}$ for the period spacing series of 40 stars in our sample. Six additional sample stars only exhibit retrograde modes and fast rotation, and cannot be quantitatively analysed with our current methodology. In the case of the remaining four stars, the difference of the best $\chi^2$-value for different ($l$,$m$) combinations is too small, so no unique solution could be determined.

For the 40 stars which were successfully analysed, the results are listed in the appendix in Table \[tab:param\]. The vast majority of the studied stars were found to exhibit prograde dipole modes. For fourteen targets in the sample we had detected multiple series. In principle, these are prime targets to look 