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Table A.1
Details of the best fit models for the various solar calibrations performed with mesa.
| Abundances | Observables used for χ2 |
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χ 2 | [Fe/H] | Y | α |
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| GS98 | {L, Teff} | 5777 | 5.12(−10) | 2.302(−2) | 0.2454 | − | 1.565(−3) | 1.66(−11) | 5.535(−2) | 0.2714 | 1.877 |
| GS98 | {L, Teff, Z/X} | 5777 | −3.73(−7) | 2.303(−2) | 0.2454 | − | 1.563(−3) | 4.23(−4) | 5.5371(−2) | 0.2714 | 1.877 |
| GS98 | {L, Teff, Rcz} | 5782 | 9.35(−5) | 2.311(−2) | 0.2456 | 7.140(−1) | 4.159(−3) | 6.48(−1) | 5.680(−2) | 0.2716 | 1.893 |
| GS98 | {L, Teff, Rcz, Z/X, He} | 5781 | −7.409(−5) | 2.320(−2) | 0.2459 | 7.141(−1) | 3.652(−3) | 5.16(−1) | 5.842(−2) | 0.2719 | 1.892 |
| GS98 | {L, Teff, Rcz, Z/X, He, cs} | 5776 | 5.723(−5) | 2.536(−2) | 0.2526 | 7.133(−1) | 6.257(−4) | 7.01 | 9.694(−2) | 0.2788 | 1.907 |
| A09 | {L, Teff} | 5777 | −3.481(−9) | 1.848(−2) | 0.2403 | − | 3.737(−3) | 7.78(−11) | −3.512(−2) | 0.2672 | 1.790 |
| A09 | {L, Teff, Z/X} | 5777 | −1.924(−6) | 1.812(−2) | 0.2389 | − | 3.995(−3) | 4.35(−5) | −4.313(−2) | 0.2658 | 1.783 |
| A09 | {L, Teff, Rcz} | 5796 | −4.033(−4) | 1.860(−2) | 0.2407 | 7.167(−1) | 1.469(−2) | 9.94 | −3.439(−2) | 0.2670 | 1.848 |
| A09 | {L, Teff, Rcz, Z/X, He} | 5797 | −9.791(−4) | 1.846(−2) | 0.2401 | 7.164(−1) | 1.600(−2) | 7.75 | −3.747(−2) | 0.2663 | 1.847 |
| A09 | {L, Teff, Rcz, Z/X, He, cs} | 5776 | 1.171(−4) | 2.4573(−2) | 0.2610 | 7.150(−1) | 8.914(−4) | 17.91 | 8.475(−2) | 0.2883 | 1.886 |
Notes. Numbers are given in the format n(m) = n × 10m for concision.
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