Notes. For all stars except for KIC 3733735 and KIC 9226926, T_eff was taken from Lund et al. (2017), and M_⋆ and R_⋆ from the ASTFIT results from Silva Aguirre et al. (2017). For KIC 3733735, T_eff was taken from Mathur et al. (2017), while M_⋆ and R_⋆ were taken from Breton et al. (2023). For KIC 9226926, all three parameters come from Mathur et al. (2017). P_rot and S​_ph were taken from Santos et al. (2021), except for KIC 9226926, for which the reference P_rot we used is close to the 2.17 days measured by Mathur et al. (2014a). For KIC 3733735, KIC 9226926, we used the stellar inclinations from Mathur et al. (2014a), which were derived by combining spectroscopic measurement of v sin i, and photometric P_rot, and R_⋆ obtained from stellar modelling. The inclination origin specified in the last column is therefore A for asteroseismic and S for spectroscopic measurements. The remaining values were taken from Hall et al. (2021) and were directly obtained from the p-mode parameter extraction performed in the periodogram. Ro was computed using Eqs. (1) and (5) from Corsaro et al. (2021). The identifiers provided in the second columns are used to easily identify the targets in the summary figures of this work.