All Tables

Table 1: Investigated stars.
Table 2: Measured equivalent widths given in mÅ.
Table 3: Line parameters.
Table 4: Effects on logarithmic abundances derived when changing the fundamental parameters of the model atmospheres. Two stars of different parameters are presented. The parameters ( ${T_{\rm eff}/ \log g/{\rm [Fe/H]}/\xi_{\rm micro}}$ ) are, respectively: ( ${\rm 4190/1.0/{-}1.75/1.3}$ ) and ( ${\rm 6300/3.97/{-}2.06/1.1}$ ).
Table 5: Abundances of Fe II and S I, the latter based on the $\lambda \lambda 9213{-}38$ lines.
Table 6: Sulfur abundances compared to those from the literature which are based on the $\lambda \lambda 8694{-}95$ lines.
Table 7: The iron and sulfur abundance ratios ([Fe/H], [S/H], and [S/Fe]) from our work and from the literature for the $\lambda \lambda 8694{-}95$ lines.