Summary of our results.
|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||•||−|
|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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