Dependence of [X/Fe] star-to-star scatter for solar analogs with [Fe/H] = 0.0 ± 0.10 dex on the number of lines. Red triangles show the scatter when the individual abundances are calculated as an AM and the blue squares indicate the scatter in [X/Fe] when the WM method was used for the abundance derivation. The black dots show the [X/Fe] scatter for each individual line that was used to derive [X/H]. The error bars indicate the dispersion of possible combinations of the lines.