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Table 7

Machine learning (M.L.) results of Teff and [Fe/H] after injecting uncertainties with Gaussian distributions of 100 K and 0.17 dex in the parameters of the training HARPS datasets, their dispersion (Disp.), the mean absolute errors (M.A.E.) of the models, and the reference values (Ref.) for comparison.

Star Spec. Res. Ref. M.L. M.A.E. Disp. Ref. M.L. M.A.E. Disp.
Teff Teff Teff Teff [Fe/H] [Fe/H] [Fe/H] [Fe/H]
[K] [K] [K] [K] [dex] [dex] [dex] [dex]
Gl643 HARPS 115 000 3102 3126 65 60 −0.26 −0.29 0.10 0.10
Gl846 UVES 110 000 3682 3678 68 109 −0.08 −0.06 0.10 0.18
Gl514 CARMENES 94 600 3574 3545 77 113 −0.13 −0.13 0.12 0.19
Gl908 SOPHIE 75 000 3587 3585 78 120 −0.38 −0.36 0.13 0.21
Gl674 FEROS 48 000 3284 3324 80 138 −0.18 −0.15 0.13 0.22

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