Table 1
Measured and computed parameters for the five stars.
| KIC004914923 | KIC005184732 | KIC006116048 | KIC006933899 | KIC010963065 | |
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| Mass [M⊙] | 1.118 ± 0.020 | 1.205 ± 0.025 | 1.023 ± 0.021 | 1.096 ± 0.026 | 1.062 ± 0.021 |
| Radius [R⊙] | 1.378 ± 0.009 | 1.342 ± 0.010 | 1.225 ± 0.008 | 1.574 ± 0.025 | 1.220 ± 0.009 |
| Xc | 0.000 | 0.216 | 0.036 | 0.000 | 0.108 |
| τ [days] | 16.94 | 23.30 | 34.34 | 28.25 | 33.03 |
| Teff[K] | 5880 ± 70 | 5865 ± 70 | 5990 ± 70 | 5870 ± 70 | 6090 ± 70 |
| PS [days] | 19.49 ± 3.12 | 20.69 ± 0.50 | 17.96 ± 2.11 | 31.63 ± 1.43 | 12.27 ± 0.32 |
| PA [days] |
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| PN [days] | 22.17 ± 3.14 | 18.00 ± 1.76 | 16.34 ± 0.89 | 28.65 ± 5.53 | 14.45 ± 1.43 |
| Seismic age [Gyr] | 6.23 ± 0.36 | 4.39 ± 0.13 | 5.70 ± 0.21 | 6.57 ± 0.30 | 4.18 ± 0.19 |
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| Gyrochronology ages [Gyr] | |||||
| Barnes (2010) |
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| Mamajek & Hillenbrand (2008) |
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| García et al. (2014) |
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Notes. The stellar masses and radii, core hydrogen fraction Xc, and convective turnover time τ, as well as the seismic ages are computed from the best-fit models as described in Sect. 4. The effective temperatures are adapted from Bruntt et al. (2012). The measured surface variability rotation periods PS and asteroseismic rotation periods PA are also listed. These periods are compared to the averaged asteroseismic rotation periods PN from Nielsen et al. (2014). The PN values are averages over several sets of oscillation modes. The gyrochronology ages are calculated from Barnes (2010), Mamajek & Hillenbrand (2008), and García et al. (2014).
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