Table D.1.
Extracted stellar parameters of HD 139614 when applying the six-dimensional model grid.
| Murphy et al. (2021) | χ2 | χ2 |  |
|
|---|---|---|---|---|
| modelling | 3σ | 1σ | ≤22.36 | |
| same mode identification as in Murphy et al. (2021) | ||||
| M⋆ (M⊙) | 1.520(18) | 1.71(11) | 1.67(9) | 1.66(10) |
| Teff (K) | 7615(64) | 7840(260) | 7670(120) | 7660(130) |
| log g | - | 4.289(9) | 4.286(8) | 4.283(9) |
| R (R⊙) | - | 1.55(3) | 1.54(3) | 1.54(4) |
| L (L⊙) | 6.7(3) | 8.2(1.3) | 7.4(6) | 7.4(7) |
| age (Myr) | 10.75(77) | 12(3) | 13(3) | 12(3) |
| Z | 0.010(1) | 0.018(5) | 0.016(4) | 0.014(5) |
Notes. The expectation value of the extracted parameter adopted as the mean of all chosen models. Only for the metallicity, Z, did we adopt the median as the expectation value since the grid is evenly spaced. Values in parentheses give the uncertainty on the extracted parameter adopted from the standard deviation of all models. We note that this model grid consists of about a factor of three fewer model calculations than than the ten-dimensional model grid.
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