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Table C.2.
Best fit models according to Mahalanobis distance where αCBM = 0 was fixed.
| Grid | Observables | Pattern construction | Mini [M⊙] | Zini | αCBM | fCBM | log(Denv) | Xc |  |
MD | AICc(MD) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Radiative | ΔP | Longest sequence | 3.3 | 0.019 | (…) | 0.01 | 0.5 | 0.42 | 1335 | 171 | −307.5 |
| Highest amplitude | 3.3 | 0.019 | (…) | 0.01 | 0.5 | 0.42 | 1335 | 171 | −308.1 | ||
| Highest frequency | 3.3 | 0.023 | (…) | 0.0 | 0.5 | 0.40 | 2369 | 150 | −329.1 | ||
| Period | Longest sequence | 3.4 | 0.023 | (…) | 0.02 | 1.0 | 0.46 | 464 512 | 152 | −334.9 | |
| Highest amplitude | 3.5 | 0.023 | (…) | 0.02 | 1.0 | 0.46 | 209 399 | 155 | −334.1 | ||
| Highest frequency | 3.3 | 0.023 | (…) | 0.0 | 0.5 | 0.40 | 818 181 | 147 | −340.9 | ||
| Péclet | ΔP | Longest sequence | 3.0 | 0.019 | (…) | 0.025 | 0.0 | 0.44 | 1714 | 170 | −310.6 |
| Highest amplitude | 3.2 | 0.015 | (…) | 0.015 | 0.0 | 0.44 | 1934 | 178 | −303.7 | ||
| Highest frequency | 3.3 | 0.023 | (…) | 0.0 | 0.5 | 0.40 | 2369 | 164 | −317.9 | ||
| Period | Longest sequence | 3.3 | 0.023 | (…) | 0.03 | 0.5 | 0.46 | 450 592 | 163 | −326.5 | |
| Highest amplitude | 3.3 | 0.023 | (…) | 0.03 | 0.5 | 0.46 | 450 592 | 168 | −323.8 | ||
| Highest frequency | 3.4 | 0.023 | (…) | 0.03 | 0.0 | 0.46 | 265 614 | 171 | −319.6 | ||
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