Table 2.
Stellar parameters of the target modes used as hare in the hare and hound exercises.
| Model | M | R | X | Z | αov | Xc | Diff | Solar mixture | Opacities | Atm | Te | log g |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (R⊙) | (K) | (g in cm s−2) | |||||||||
| t1 | 14 | 7.48 | 0.70 | 0.014 | 0.2 | 0.288 | N | AGS05 | OP | Edd | 27 647 | 3.8364 |
| t2 | 11 | 5.98 | 0.70 | 0.016 | 0.2 | 0.351 | N | GN93 | OP | K | 25 293 | 3.9258 |
| t6 | 10 | 4.020 | 0.70 | 0.014 | 0 | 0.388 | Y | AGS05 | OP | Edd | 24 487 | 4.0196 |
Notes. The acronyms GN93 and AGS05 stand for the solar chemical mixtures of Grevesse & Noels (1993) and Asplund et al. (2005), respectively. The “Diff” column indicates whether the model is computed with additional turbulent mixing (Y) or without (N). The Edd and K symbols indicates whether the stellar model atmosphere is computed following Eddington’s law or from Kurucz models.
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