Table 2.
Fundamental stellar parameters from asteroseismic modelling.
| KIC ID | M(M⊙) | R(R⊙) | L(L⊙) | Teff(K) | [Fe/H] | Age(Gyr) | Agegyro(GYR) | Xc | Rbc/R | Mce/M |
|---|---|---|---|---|---|---|---|---|---|---|
| KIC2837475 | 1.421 ± 0.040 | 1.625 ± 0.015 | 4.612 ± 0.139 | 6635 ± 35 | −0.44 ± 0.07 | 1.74 ± 0.37 | 1.12 ± 0.34 | 0.45 | 0.92 | 2.6 × 10−5 |
| KIC6508366 | 1.559 ± 0.040 | 2.208 ± 0.018 | 6.727 ± 0.189 | 6255 ± 41 | −0.05 ± 0.08 | 2.71 ± 0.21 | 0.89 ± 0.27 | 0.21 | 0.84 | 6.86 × 10−4 |
| KIC7103006 | 1.520 ± 0.046 | 1.973 ± 0.020 | 5.750 ± 0.173 | 6363 ± 43 | 0.05 ± 0.07 | 2.06 ± 0.15 | 0.37 ± 0.11 | 0.27 | 0.87 | 2.95 × 10−4 |
| KIC7206837 | 1.394 ± 0.045 | 1.586 ± 0.017 | 3.823 ± 0.092 | 6409 ± 30 | 0.11 ± 0.05 | 1.93 ± 0.18 | 0.80 ± 0.24 | 0.43 | 0.87 | 3.80 × 10−4 |
| KIC7940546 | 1.340 ± 0.026 | 1.925 ± 0.014 | 4.958 ± 0.061 | 6207 ± 27 | −0.19 ± 0.05 | 3.55 ± 0.12 | 3.04 ± 0.91 | 0.44 | 0.81 | 1.767 × 10−3 |
| KIC8006161 | 1.006 ± 0.019 | 0.936 ± 0.006 | 0.599 ± 0.016 | 5248 ± 52 | 0.34 ± 0.05 | 5.50 ± 0.23 | 3.28 ± 0.99 | 0.43 | 0.68 | 5.18 × 10−2 |
| KIC8379927 | 1.194 ± 0.027 | 1.146 ± 0.010 | 1.652 ± 0.028 | 6111 ± 50 | 0.05 ± 0.06 | 1.55 ± 0.08 | 3.33 ± 1.00 | 0.56 | 0.78 | 5.91 × 10−3 |
| KIC9139163 | 1.423 ± 0.039 | 1.574 ± 0.015 | 3.663 ± 0.091 | 6364 ± 45 | 0.12 ± 0.05 | 2.01 ± 0.15 | 1.14 ± 0.34 | 0.42 | 0.86 | 5.60 × 10−4 |
| KIC9812850 | 1.359 ± 0.042 | 1.796 ± 0.019 | 4.499 ± 0.159 | 6273 ± 52 | −0.12 ± 0.08 | 3.31 ± 0.24 | 1.42 ± 0.42 | 0.27 | 0.83 | 1 × 10−3 |
| KIC10454113 | 1.290 ± 0.025 | 1.286 ± 0.010 | 2.296 ± 0.033 | 6265 ± 38 | 0.06 ± 0.06 | 1.67 ± 0.12 | 3.68 ± 1.10 | 0.51 | 0.83 | 2.013 × 10−3 |
| KIC10644253 | 1.222 ± 0.029 | 1.137 ± 0.010 | 1.566 ± 0.032 | 6054 ± 54 | 0.14 ± 0.06 | 1.05 ± 0.12 | 1.17 ± 0.35 | 0.61 | 0.78 | 6.93 × 10−3 |
| KIC11081729 | 1.259 ± 0.049 | 1.405 ± 0.018 | 3.173 ± 0.087 | 6502 ± 36 | −0.17 ± 0.08 | 2.03 ± 0.30 | – | 0.45 | 0.88 | 2.80 × 10−4 |
| KIC11253226 | 1.426 ± 0.034 | 1.615 ± 0.013 | 4.628 ± 0.091 | 6662 ± 24 | −0.49 ± 0.10 | 1.85 ± 0.31 | – | 0.52 | 0.93 | 1.8 × 10−5 |
Notes. The last four columns indicate the age estimate through Prot − (B − V)0 gyrochronology relationship (Barnes 2007) for which we assumed a 30% uncertainty, the central abundance of hydrogen, the radius of the base of the convective envelope normalised to the total radius, and the mass contained in the convective envelope, normalised to the total mass.
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