Notes. The first three columns give the target name, spectroscopic dataset, and modified Julian date at which each spectrum was collected. Columns (4)–(6) list the effective temperature and its standard deviation, the surface gravity, and the microturbulent velocity, respectively. The uncertainties in log g and v_t were assumed to be 0.3 dex and 0.5 km s⁻¹ (see the discussion in Genovali et al. 2014). Columns (7)–(10) list the Fe I and Fe II abundances derived from individual lines, together with the standard deviations and the number of lines used (given the small number of Fe II lines, a typical value of 0.11 dex was adopted as a minimum uncertainty for the abundances from this species). The last two columns list the O I and the S I abundances with their uncertainties, estimated as described in Sect. 3. The complete table is available at the CDS.