Table 14
Summary of stellar properties for KIC 11395018 (C1), KIC 10273246 (C2), KIC 10920273 (C3), KIC 10339342 (C4), and KIC 11234888 (C5), derived from atmospheric and mean seismic parameters, and stellar models.
| C1 | C2 | C3 | C4 | C5 | ||||||||||||||||||||||||||||||||||||
|
|
||||||||||||||||||||||||||||||||||||||||
| a ⟨ ρ ⟩ ν (kg m-3) | 175 ± 2 | 185 ± 1 | 254 ± 1 | 39 ± 16 | 135 ± 1 | |||||||||||||||||||||||||||||||||||
| b ⟨ ρ ⟩ MR (kg m-3) | 174 ± 4 | 189 ± 2 | 257 ± 5 | 46 ± 4 | 140 ± 2 | |||||||||||||||||||||||||||||||||||
| alog gν (dex) | 3.86 ± 0.03 | 3.88 ± 0.03 | 3.94 ± 0.03 | 3.47 ± 0.03 | 3.79 ± 0.04 | |||||||||||||||||||||||||||||||||||
| blog gMR (dex) | 3.88 ± 0.02 | 3.88 ± 0.02 | 3.97 ± 0.03 | 3.52 ± 0.04 | 3.82 ± 0.03 | |||||||||||||||||||||||||||||||||||
| R (R⊙) | 2.23 ± 0.04 | 2.11 ± 0.05 | 1.90 ± 0.05 | 3.81 ± 0.19 | 2.44 ± 0.14 | |||||||||||||||||||||||||||||||||||
| M (M⊙) | 1.37 ± 0.11 | 1.26 ± 0.10 | 1.25 ± 0.13 | 1.79 ± 0.12 | 1.44 ± 0.26 | |||||||||||||||||||||||||||||||||||
| τ (Gyr) | 3.9 ± 1.4 | 3.7 ± 0.7 | 4.5 ± 1.8 | 1.1 ± 0.2 | 2.6 ± 0.9 | |||||||||||||||||||||||||||||||||||
| cτ⟨δν⟩ (Gyr) | 4.5 ± 0.5 | 3.7 ± 0.6 | 5.0 ± 1.9 | ... | 1.6 ± 0.2 | |||||||||||||||||||||||||||||||||||
| L (L⊙) | 4.2 ± 1.1 | 5.3 ± 1.1 | 3.6 ± 1.2 | 20.0 ± 1.1 | 7.8 ± 1.1 | |||||||||||||||||||||||||||||||||||
| Teffmodel (K) | 5547 | 6047 | 5789 | 6255 | 6180 | |||||||||||||||||||||||||||||||||||
| i (°) |
|
|
|
... | ... | |||||||||||||||||||||||||||||||||||
| PROTmax (days) | 384 | 64 | ... | 168 | ... | |||||||||||||||||||||||||||||||||||
| dPROTest (days) | 36 (6) | 23 | 27 | ... | 19–27 (5) | |||||||||||||||||||||||||||||||||||
| d (pc) | 318 |
366 |
470 |
1212 |
735 |
|||||||||||||||||||||||||||||||||||
Notes.
Subscripts ν and MR indicate that the value was obtained directly from the data and from the models, respectively.
τ ⟨ δν ⟩ is when ⟨ δν02 ⟩ is included as an observational constraint. In this case the uncertainties in log g, R, and M for C5 reduce by a factor of three.
PROTest as reported by Campante et al. (2011) and Mathur et al. (2011), with uncertainties in parenthesis.
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