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Table 2

Uncertainties of the lead abundances A(Pb) caused by the spectra S/N for different stellar types.

Cool giant Cool dwarf Solar-type
Teff ~4500 K ~5100 K ~5700 K
S/N ~65 ~110 ~65 ~110 ~65 ~110
σMC ±0.05 ±0.04 ±0.05 ±0.03 ±0.05 ±0.04
Ns 28 9 17 21 35 50

Notes. NS is the number of spectra selected to estimate the mean σMC for each stellar type.

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