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Table 4

Standard deviation of the differences, residual mean square, mean squared error, and coefficient of determination between the PCA-derived abundances of the training stars and those provided in previous works.

[X/H] nstars σ RMS RMSE R2
MSDL Fe 196 0.22 0.23 0.05 –2.04
RA12 Fe 38 0.19 0.19 0.04 0.42
ON12 Fe 10 0.14 0.14 0.02 0.07
NE13 Fe 100 0.19 0.24 0.06 –0.16
GA14 Fe 81 0.19 0.19 0.03 0.10
NE14 Fe 21 0.22 0.22 0.05 –0.12
WW20 Fe 14 0.25 0.28 0.08 –0.72
SO20 Fe 9 0.14 0.15 0.02 0.72
PA19-N Fe 84 0.28 0.36 0.13 –1.17
PA19-V Fe 85 0.23 0.24 0.06 –1.31

WW20 Ti 14 0.15 0.31 0.10 –1.90
SO20 C 9 0.14 0.19 0.04 –0.15

SO18 6 0.13 0.15 0.02 –3.40

Notes. We note that for SO18 we compare the abundances of six different species for one single star.

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