Table B.1.
Parameters of the gravity-mode pulsators covered by the solar metallicity grid.
| Gaia DR3 ID | frot | afrot | bfrot | M⋆ | aM⋆ | bM⋆ | Xc/Xini | aXc/Xini | bXc/Xini | mcc | amcc | bmcc | log(R⋆/R⊙) | alog(R⋆/R⊙) | blog(R⋆/R⊙) | fco − rot | spin | fsurf ⋅ sin i | frot/(fsurf ⋅ sin i) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 164941072177351424 | 0.93767 | 0.16430 | 0.12293 | 3.77256 | 0.07590 | 0.04231 | 0.51880 | 0.06017 | 0.03535 | 0.60150 | 0.04841 | 0.02017 | 0.53383 | 0.01765 | 0.01497 | 0.51010 | 3.67642 | — | — |
| 185403705126528256 | 1.16134 | 0.16431 | 0.12293 | 1.50733 | 0.01523 | 0.01123 | 0.80702 | 0.04583 | 0.03352 | 0.13033 | 0.01222 | 0.00585 | 0.18797 | 0.01018 | 0.00689 | 0.55408 | 4.19196 | — | — |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
| 200619262425969024 | 1.64651 | 0.16497 | 0.12382 | 1.48797 | 0.03052 | 0.01000 | 0.89223 | 0.07543 | 0.04644 | 0.12030 | 0.02328 | 0.00319 | 0.17293 | 0.01266 | 0.01166 | 0.64949 | 5.07016 | 1.42700 | 1.15383 |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
Notes. When available, the error estimates of a quantity X are given as aX and bX in the notation X−aX+bX. Frequencies are given in the unit d−1 while the stellar (core) mass and radius are given in solar units. The quantity fco − rot is the frequency of the dominant gravito-inertial mode in a frame of reference co-rotating with frot, while ‘spin’ stands for the spin parameter of the dominant mode in the region just outside the convective core.
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