Table 4.
Results of asteroseismic modelling with Y = (Π0) using the full grid of pulsational models, with either a 
or MD merit function.
|
MD | |||||
|---|---|---|---|---|---|---|
| Yobs = (Π0, ℓ = 1) | Yobs = (Π0, ℓ = 2) | Yobs = (Π0, ℓ = 1, Π0, ℓ = 2) | Yobs = (Π0, ℓ = 1) | Yobs = (Π0, ℓ = 2) | Yobs = (Π0, ℓ = 1, Π0, ℓ = 2) | |
| M [M⊙] |
 |
 |
 |
 |
 |
 |
| fov |
 |
 |
 |
 |
 |
 |
| log Dmix |
 |
 |
 |
 |
 |
 |
| Xc |
 |
 |
 |
 |
 |
 |
| R [R⊙] |
 |
 |
 |
 |
 |
 |
| Teff [K] |
 |
 |
 |
 |
 |
 |
| log g [dex] |
 |
 |
 |
 |
 |
 |
| Mcc [M⊙] |
 |
 |
 |
 |
 |
 |
| τ [Gyr] |
 |
 |
 |
 |
 |
 |
 |
2.09 × 10−14 | 8.35 × 10−16 | 7.58 × 10−7 | 1.70 × 10−19 | 4.23 × 10−16 | 7.27 × 10−8 |
Notes. The table is divided into two, with the estimated parameters (M, Xc, fov, and log Dmix) presented in the top four rows and the inferred parameters (R, Teff, log g, Mcc, and τ) in the bottom five rows. The errors quoted are based on 68% HPD intervals of the Monte Carlo parameter distributions. The minimum values of each merit function across all of the Monte Carlo iterations for each parameter setup are quoted in the bottom row of the table.
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