Notes.The effective temperature T_eff, surface gravity log g, and frequency intervals considered for each star are also listed, where each interval is divided into segments of length approximately equal to the large frequency separation. The variance weighted mean splittings ⟨ δν ⟩ are shown as dashed lines in Fig. 2, where the listed errors are the standard deviations of the weighted mean values. We note that the posterior distributions for the δν are only approximately Gaussian. The posterior distributions of inclination measurements cannot be approximated as a Gaussian and so we only show the unweighted mean of the inclinations where typical errors are ~20°. The reader should not use the mean values and associated errors reported here, but should refer to the online material for more accurate values for each mode set. For comparison, the final column shows the stellar rotation rate relative to the solar value (we used Ω_⊙ = 0.424 μHz).