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Table 5

Average difference and standard deviation (left) between the equivalent width method and the reference values.

Differences Dispersion
ΔTeff Δlog (g) Δ[M/H] ΔTeff Δlog (g) Δ[M/H]
Case μ σ μ σ μ σ

Medium-quality lines 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
High-quality lines 129 311 0.14 0.47 0.09 0.30 39 0.09 0.06

Relaxed EWR limit 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
Strong EWR limit 134 259 0.30 0.50 0.13 0.23 41 0.09 0.02
Unlimited EWR 173 371 0.20 0.53 0.21 0.45 58 0.14 0.06

Outlier filter 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
With outliers 178 374 0.41 0.67 0.13 0.31 80 0.18 0.06

GES 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
VALD 118 313 0.20 0.58 0.19 0.24 57 0.12 0.06
SPECTRUM 1 326 0.06 0.45 0.10 0.29 67 0.12 0.05

MARCS 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
ATLAS 157 221 0.22 0.44 0.13 0.26 37 0.12 0.03

Estimate initial AP 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
Fixed initial AP 152 359 0.23 0.81 0.08 0.26 49 0.18 0.04

R = 70 000 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
R = 16 200 419 598 0.62 0.99 0.53 0.57 118 0.25 0.11
R = 16 200/re-norm 475 520 0.86 0.89 0.21 0.79 62 0.17 0.05

Gaussian profiles 135 241 0.20 0.44 0.12 0.27 38 0.12 0.03
Voigt profiles 131 286 0.30 0.52 0.14 0.24 97 0.19 0.06

Notes. Average dispersion (right) for stars with multiple observed spectra.

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