Fig. 7
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Feature importance derived from the XGBoost model. The orbital elements are denoted as follows: The semimajor axis (a), the eccentricity (e), the inclination (i), the argument of pericenter (ω), the longitude of the node (Ω), and the true anomaly ( f ). Planet-specific parameters are indicated with a subscript p. The mass ratio of the system is represented by µ.
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