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Table C.4.
Best fit models according to Mahalanobis distance in the subgrid without CBM.
| Grid | Observables | Pattern construction | Mini [M⊙] | Zini | αCBM | fCBM | log(Denv) | Xc |  |
MD | AICc(MD) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Radiative | ΔP | Longest sequence | 3.3 | 0.019 | (…) | (…) | 1.5 | 0.44 | 1816 | 84 | −380.2 |
| Highest amplitude | 3.3 | 0.019 | (…) | (…) | 1.5 | 0.44 | 1816 | 92 | −373.5 | ||
| Highest frequency | 3.2 | 0.019 | (…) | (…) | 0.0 | 0.50 | 8601 | 83 | −381.8 | ||
| Period | Longest sequence | 3.4 | 0.019 | (…) | (…) | 1.5 | 0.44 | 965 418 | 97 | −376.5 | |
| Highest amplitude | 3.1 | 0.019 | (…) | (…) | 0.5 | 0.40 | 377 038 | 99 | −377.6 | ||
| Highest frequency | 3.3 | 0.023 | (…) | (…) | 0.5 | 0.40 | 792 613 | 107 | −367.9 |
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