Table D.1
Stellar and physical parameters of the 3D stellar models at solar metallicity used to determine the scaling relation of F8. From left to right: model name, target effective temperature (target Teff, in K) corresponding to the Teff that we aimed to achieve for each model, mean Teff (K) from the time series, surface gravity in logarithm scale (logɡ) (cm/s2), metallicity [Fe/H], vmax (µHz), standard deviation of the brightness fluctuations (σHD) (ppm), and F8HD (ppm).
| Model | Target Teff | Teff | logɡ | [Fe/H] | vmax | σHD | F8hd |
|---|---|---|---|---|---|---|---|
| t50g30m00 | 5000 | 4960 | 3.00 | 0.0 | 121.516 | 219 | 286 |
| t47g32m00 | 4750 | 4727 | 3.25 | 0.0 | 221.351 | 199 | 220 |
| t55g35m00 | 5500 | 5516 | 3.50 | 0.0 | 364.387 | 136 | 145 |
| t50g35m00 | 5000 | 4958 | 3.50 | 0.0 | 384.345 | 142 | 153 |
| t65g40m00 | 6500 | 6413 | 4.00 | 0.0 | 1068.672 | 88 | 83 |
| t60g40m00 | 6000 | 5962 | 4.00 | 0.0 | 1108.355 | 83 | 88 |
| t55g40m00 | 5500 | 5462 | 4.00 | 0.0 | 1157.975 | 81 | 85 |
| t5777g44m00 | 5777 | 5759 | 4.44 | 0.0 | 3106 | 38 | 46 |
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