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Table C.3.
Best fit models according to Mahalanobis distance where fCBM = 0 was fixed.
| Grid | Observables | Pattern construction | Mini [M⊙] | Zini | αCBM | fCBM | log(Denv) | Xc |  |
MD | AICc(MD) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Radiative | ΔP | Longest sequence | 3.4 | 0.023 | 0.05 | (…) | 0.5 | 0.40 | 2227 | 112 | −355.7 |
| Highest amplitude | 3.4 | 0.019 | 0.2 | (…) | 0.5 | 0.46 | 1783 | 121 | −347.6 | ||
| Highest frequency | 3.3 | 0.023 | 0.0 | (…) | 0.5 | 0.40 | 2369 | 116 | −351.7 | ||
| Period | Longest sequence | 3.4 | 0.023 | 0.05 | (…) | 0.5 | 0.40 | 758 935 | 105 | −370.5 | |
| Highest amplitude | 3.4 | 0.019 | 0.2 | (…) | 0.5 | 0.46 | 92 393 | 108 | −369.7 | ||
| Highest frequency | 3.4 | 0.019 | 0.2 | (…) | 0.5 | 0.46 | 92 393 | 110 | −367.0 | ||
| Péclet | ΔP | Longest sequence | 3.4 | 0.023 | 0.05 | (…) | 0.5 | 0.40 | 2318 | 130 | −344.1 |
| Highest amplitude | 3.2 | 0.023 | 0.15 | (…) | 0.5 | 0.40 | 1299 | 138 | −337.2 | ||
| Highest frequency | 3.2 | 0.015 | 0.2 | (…) | 0.0 | 0.42 | 2630 | 132 | −343.3 | ||
| Period | Longest sequence | 3.2 | 0.023 | 0.25 | (…) | 0.0 | 0.40 | 363 903 | 130 | −352.4 | |
| Highest amplitude | 3.2 | 0.023 | 0.25 | (…) | 0.0 | 0.40 | 363 903 | 134 | −351.1 | ||
| Highest frequency | 3.2 | 0.023 | 0.25 | (…) | 0.0 | 0.40 | 363 903 | 140 | −345.2 | ||
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