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Table 8.
Same as Table 7, but for a grid subset based on the 3σ interval of the ‘pseudo-single-star’ spectroscopic Teff and log g values (see footnote).
|
MD | |||||
|---|---|---|---|---|---|---|
| Y = (ΔPℓ = 1, i) | Y = (ΔPℓ = 2, j) | Y = (ΔPℓ = 1, i, ΔPℓ = 2, j) | Y = (ΔPℓ = 1, i) | Y = (ΔPℓ = 2, j) | Y = (ΔPℓ = 1, i, ΔPℓ = 2, j) | |
| M [M⊙] |
 |
 |
 |
 |
 |
 |
| fov |
 |
 |
 |
 |
 |
 |
| log Dmix |
 |
*0.0+0.5 |
 |
 |
*0.0+0.5 | *0.0+0.5 |
| Xc |
 |
 |
 |
 |
 |
 |
| R [R⊙] |
 |
 |
 |
 |
 |
 |
| Teff [K] |
 |
 |
 |
 |
 |
 |
| log g [dex] |
 |
 |
 |
 |
 |
 |
| Mcc [M⊙] |
 |
 |
 |
 |
 |
 |
| τ [Gyr] |
 |
 |
 |
 |
 |
 |
 |
243 | 399 | 342 | 11 | 17 | 93 |
Notes. Grid subset based on 6965 K ≤ Teff ≤ 7520 K and 3.09 ≤ log g ≤ 4.13.
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