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Fig. 5.

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Residuals between SAPP parameters and reference parameters versus the signal-to-noise ratio of four stars: β Vir, η Boo, β Hyi, and α Cen A. Open circles show cases where a purely spectroscopic module (without error model) was used; these have an average and 1σ in the legend named ⟨Δ[Fe/H]⟩. Filled circles show cases where a spectroscopic module was used with the error model; these have an average and 1σ in the legend named ⟨Δ[Fe/H]emodel⟩.

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