Youth analysis of near-infrared spectra of young low-mass stars and brown dwarfs

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Table D.1.

Hyper-parameters selected for each of the models in the four case scenarios inspected.

	SVM		PCA+SVM			RF
	γ	C	γ	C	n_ca	n_treesb	max_fc
2-JHK	0.3	40	0.012	50	9	200	14
2-HK	-	-	0.012	45	12	200	40
3-JHK	0.05	30	0.012	30	10	200	70
3-HK	-	-	0.012	45	12	200	70

^(a)

Number of principal components.

^(b)

Number of trees.

^(c)

Maximum number of features included in each tree.

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