Table 1
Parameters found in the literature of the stars used in this study.
| KIC | ν max | M | R | P rot | Age | Ref. |
| [μHz] | [M⊙] | [R⊙] | [days] | [Gyr] | ||
|
|
||||||
| 3241581⋆ | 2969±17 | 1.04±0.02 | 1.08±0.10 | 26.3±2.0 | 3.8±0.6 | 1 |
| 3656476⋆ | 1947±78 | 1.10±0.03 | 1.32±0.01 | 31.7±3.5 | 8.9±0.4 | 2 |
| 4914923⋆ | 1844±73 | 1.04±0.03 | 1.34±0.02 | 20.5±2.8 | 7.0±0.5 | 2 |
| 5084157 | 1788±14 | 1.06±0.13 | 1.36±0.08 | 22.2±2.8 | 7.8±3.4 | 3 |
| 5774694 | 3671±20 | 1.06±0.05 | 1.00±0.03 | 12.1±1.0 | 1.9±1.8 | 3 |
| 6116048⋆ | 2098±84 | 1.05±0.03 | 1.23±0.01 | 17.3±2.0 | 6.1±0.5 | 2 |
| 6593461 | 2001±18 | 0.94±0.16 | 1.29±0.07 | 25.7±3.0 | 10.7±4.4 | 3 |
| 7296438⋆ | 1846±73 | 1.10±0.02 | 1.37±0.01 | 25.2±2.8 | 6.4±0.6 | 2 |
| 7680114⋆ | 1709±58 | 1.09±0.03 | 1.40±0.01 | 26.3±1.9 | 6.9±0.5 | 2 |
| 7700968 | 2010±25 | 1.00±0.12 | 1.21±0.06 | 36.2±4.2 | 7.5±3.1 | 3 |
| 9049593 | 1983±13 | 1.13±0.14 | 1.40±0.06 | 12.4±2.5 | 6.4±3.4 | 3 |
| 9098294⋆ | 2347±84 | 0.98±0.02 | 1.15±0.01 | 19.8±1.3 | 8.2±0.5 | 2 |
| 10130724 | 2555±27 | 0.85±0.12 | 1.08±0.05 | 32.6±3.0 | 13.8±5.0 | 3 |
| 10215584 | 2172±28 | 0.99±0.13 | 1.12±0.05 | 22.2±2.9 | 6.8±3.5 | 3 |
| 10644253⋆ | 2892±157 | 1.09±0.09 | 1.09±0.02 | 10.9±0.9 | 0.9±0.3 | 2 |
| 10971974 | 2231±6 | 1.04±0.12 | 1.09±0.03 | 26.9±4.0 | 5.8±3.0 | 3 |
| 11127479 | 1983±7 | 1.14±0.12 | 1.36±0.06 | 17.6±1.8 | 5.1±2.2 | 3 |
| 11971746 | 1967±23 | 1.11±0.14 | 1.35±0.06 | 19.5±2.1 | 6.0±2.8 | 3 |
Notes.Kepler input catalogue (KIC) number, central frequency of the oscillation power excess νmax by Chaplin et al. (2014), stellar mass and radius in solar units from seismology, surface rotation period Prot from García et al. (2014), stellar age from seismic modelling, and reference to the published seismic studies: [1] Garcia et al. (in prep., see also Beck et al. 2016); [2] Creevey et al. (2017) and [3] Chaplin et al. (2014). Stars whose parameters were obtained through the detailed modelling approach as described in Sect. 2 are flagged with an asterisk.
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