Online Material

Table 5: List of log gf values for the Si II-IV lines considered in this study (from Atomic Line List v2.05). For the O II lines we refer to Simón-Díaz et al. (2006).

Table 6: Results from the abundance analysis of HD 36512 (B0 V).

Table 7: Results from the abundance analysis of HD 37020 (B0.5 V).

Table 8: Results from the abundance analysis of HD 36960 (B0.5 V).

Table 9: Results from the abundance analysis of HD 37042 (B0.7 V).

Table 10: Results from the abundance analysis of HD 36591 (B1 V).

Table 11: Results from the abundance analysis of HD 36959 (B1 V).

Table 12: Results from the abundance analysis of HD 37744 (B1.5 V).

Table 13: Results from the abundance analysis of HD 35299 (B1.5 V).

Table 14: Results from the abundance analysis of HD 36285 (B2 V).

Table 15: Results from the abundance analysis of HD 35039 (B2 V).

Table 16: Results from the abundance analysis of HD 36629 (B2 V).

Table 17: Results from the abundance analysis of HD 36430 (B2 V).

Table 18: Results from the abundance analysis of HD 35912 (B2 V).

$\begin{figure} \par\includegraphics[angle=180,scale=0.85]{13120f8a.eps} \end{figure}$	Figure 8: The complete atlas of FIES@ NOT spectra (part 1 of 3). The Si II-IV and O II lines used for the abundance analysis are indicated as solid and dashed vertical lines, respectively.
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$\begin{figure} \par\includegraphics[angle=180,scale=0.85]{13120f8b.eps} \end{figure}$	Figure 8: continued.
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$\begin{figure} \par\includegraphics[angle=180,scale=0.85]{13120f8c.eps} \end{figure}$	Figure 8: continued.
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