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Table 3

Error metric for five pairs of randomly selected planets.

Planets Error metric DNN XG
F1800 R2 0.9971 0.9971
K800 RMSE 48.7536 49.1047

G1800 R2 0.9817 0.9813
K1800 RMSE 117.3391 118.8262

F2000 R2 0.9835 0.9843
G2200 RMSE 121.7374 118.7824

G2000 R2 0.9931 0.9953
K600 RMSE 77.0609 63.4323

F400 R2 0.9975 0.9987
F1600 RMSE 44.6912 32.3724

Notes. R2 and RMSE for Tgas data of the five independent pairs of randomly selected planets removed from training (Fig. 9, Figs. B.5B.8). All of the R2 values are very close to one, showing good agreement between the prediction and the ground truth. Although the RMSE is high due to large absolute deviations, the ML models successfully capture the underlying trends and variability, as evidenced by the high R2 values.

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