Table 3
Fundamental properties of the stellar targets.
| Name | M | R |
|
log (g) | t | rBCZ | τTot. | τBCZ | αMLT | αov | Diff. | Mix. | Atm. | B.C. |
| (M⊙) | (R⊙) | (g cm-3) | (dex) | (Gyr) | (R) | (s) | (s) | |||||||
|
|
||||||||||||||
| Coco | 0.78 | 0.815 | 2.029 | 4.508 | 9.616 | 0.746 | 2999 | 1293 | 1.6708 | – | No | GN93 | Edd. | δP = 0 |
| Aardvark | 1.00 | 0.959 | 1.596 | 4.474 | 3.058 | 0.731 | 3371 | 1405 | 1.6708 | – | No | GN93 | Edd. | δP = 0 |
| Elvis | 1.00 | 1.087 | 1.097 | 4.365 | 6.841 | 0.727 | 4045 | 1656 | 1.6708 | – | No | GN93 | Edd. | Isoth. |
| Henry | 1.10 | 1.138 | 1.051 | 4.367 | 2.055 | 0.839 | 4199 | 2280 | 1.8045 | – | Yes | GN93 | Edd. | δP = 0 |
| Izzy | 1.10 | 1.141 | 1.041 | 4.364 | 2.113 | 0.849 | 4219 | 2353 | 1.6708 | – | No | GN93 | Edd. | δP = 0 |
| Blofeld | 1.22 | 1.359 | 0.684 | 4.257 | 2.595 | 0.838 | 5107 | 2811 | 1.6738 | 0.10 | Yes | AGS05 | Trun. | Isoth. |
| Diva | 1.22 | 1.353 | 0.693 | 4.261 | 4.622 | 0.767 | 5082 | 2288 | 1.6708 | 0.10 | No | GN93 | Edd. | δP = 0 |
| Felix | 1.33 | 1.719 | 0.369 | 4.091 | 2.921 | 0.842 | 7014 | 3830 | 1.6708 | 0.05 | No | GN93 | Edd. | δP = 0 |
| George | 1.33 | 1.697 | 0.383 | 4.102 | 2.944 | 0.875 | 6930 | 4156 | 1.6708 | 0.25 | No | GN93 | Edd. | δP = 0 |
| Jam | 1.33 | 1.468 | 0.592 | 4.228 | 1.681 | 0.905 | 5666 | 3718 | 1.6708 | 0.05 | No | GN93 | Edd. | δP = 0 |
Notes. M is the mass, R the radius, the mean density, g the surface gravity, t the stellar age, rBCZ the radius at the base of the convection zone, τTot. the acoustic radius, τBCZ the acoustic radius at the base of the convection zone, and αov the overshooting parameter. “Diff.” represents atomic diffusion, “Mix.” the abundances mixture, “Atm.” the atmosphere, “Edd.” a radiative grey Eddington atmosphere, “Trun.” a truncated atmosphere, and “B.C.” boundary condition on the pulsation modes. The abundances mixtures were GN93 (Grevesse & Noels 1993) and AGS05 (Asplund et al. 2005). Reference values are given in Table 4.
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