Table 1
Details of the parameters for the solar calibrations of the various codes included in this study.
| Code | Solar | Z0 | X0 | αMLT | Diffusion |
| abundance | |||||
|
|
|||||
| stars | GN93 | 0.0184 | 0.7012 | 2.090 | yes |
| A09 | 0.0142 | 0.7293 | 2.025 | yes | |
| mesa | GS98 | 0.0185 | 0.7101 | 1.877 | yes |
| A09 | 0.0149 | 0.7193 | 1.783 | yes | |
| Y2 | GNS96 | 0.0181 | 0.7149 | 1.7432 | He only |
| BASTI | GN93 | 0.198 | 0.7068 | 1.913 | yes |
| Padova | GS98 | 0.017 | 0.723 | 1.68 | no |
| Dartmouth | GS98 | 0.0188 | 0.7063 | 1.938 | yes |
| Geneva | A05 | 0.014 | 0.7200 | 1.6467 | yes |
| PARSEC | GS98+C11 | 0.0177 | 0.7027 | 1.74 | yes |
| Victoria- | A09 | 0.0133 | 0.7367 | 2.007 | He only |
| Regina | |||||
Notes. The abbreviations for the choice of solar abundances are: GN93, Grevesse & Noels (1993); GNS96, Grevesse et al. (1996); GS98, Grevesse & Sauval (1998); A05, Asplund et al. (2005); A09, Asplund et al. (2009); C11, Caffau et al. (2011). Note that the quoted values for mesa are based on the calibration with L,Teff and Z/X alone.
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