Table 4
Summary of our results.
| Name | [Fe/H]i | Y i | Age | ov | Diff | Other |
|
|
||||||
| Kepler-16 | −0.04 | 0.28 | 1.25 ± 0.91 Gyr | − | fe = 0.008 | |
| M55 V54 | −1.86∗ | 0.25 | >13.2 Gyr | ⋆ | ||
| V565 Lyr | 0.40 | 0.32 | 7.08 ± 0.15 Gyr | ⋆ | ||
| V636 Cen | −0.20 | 0.27 | 1.36 ± 0.27 Gyr | ° | fe = 0.33 | |
| V568 Lyr | 0.40 | 0.32 | 6.57 ± 0.14 Gyr | ⋆ | ||
| UX Men | 0.20 | 0.29 | 2.1 ± 0.2 Gyr | ° | • | |
| KOI-3571 | 0.13 | 0.29 | 2.3 ± 0.7 Gyr | ° | • | |
| BG Ind | −0.20 | 0.27 | 3.3 ± 0.1 Gyr | ⋆ | ||
| KIC 9777062 | 0.04 | 0.28 | 1.09 ± 0.07 Gyr | • | • | |
| V906 Sco | 0.05 | 0.28 | 236 ± 13 Myr | • | ||
| MU Cas | 0.02 | 0.30 | 72 ± 2 Myr | ° | ||
| V380 Cyg | −0.25∗ | 0.27 | 16.2 ± 0.3 Myr | ° | ||
| V453 Cyg | −0.04 | 0.27 | 10.8 ± 0.1 Myr | • | − | |
| V578 Mon | − | − | − | × | − | |
| AI Phe | −0.04 | 0.27 | 4.681 ± 0.005 Gyr | × | • | |
| V501 Her | 0.4 | 0.32 | 5.47 ± 0.06 Gyr | • | ° | |
| α Aur | −0.04 | 0.28 | 634 ± 6 Myr | • | fov = 0.025 | |
| V2291 Oph | 0.23 | 0.33 | 188 ± 18 Myr | • | αml = 2.0 | |
| Cep0227 | −0.38 | 0.26 | 157.8 ± 0.6 Myr | ⋆ | ||
Notes. Shown are the initial composition and resulting age of our preferred models. [Fe/H] values marked with an asterisk are α-enhanced. In the “diff” and “ov” column we indicate if diffusion and overshooting, respectively, give improved (•) or similar quality (°) models. The ⋆ indicates that an effect is necessary for the fit, while × shows the opposite. If there is no entry, the physical effect does not apply. The last column gives a possible non-standard value for fov and αml, or the effective spot coverage fe in cases in which the spot model has been used.
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