\begin{table}%t3 \caption{\label{table3}Final results of the HSi~analysis: stellar parameters and Si abundances.} %\centering \small \begin{tabular}{ccccccccccccc} \hline\hline \noalign{\smallskip} & & { ($EW_{\rm 4}$/$EW_{\rm 3}$)$^a$} & { ($EW_{\rm 2A}$/$EW_{\rm 3}$)} & { ($EW_{\rm 2B}$/$EW_{\rm 3}$)} & & \multicolumn{2}{c}{Adopted} & & & \Teff$\pm$500~K\\ \cline{7-8} Target & SpT & \Teff\ -- \ioni{Si}{iv-iii} & \Teff\ -- \ioni{Si}{ii-iii} & \Teff\ -- \ioni{Si}{ii-iii} & \Teff\ -- \ioni{He}{i-ii} & \Teff\ & \grav\ & \micro(Si) & \abun{Si}$\pm$$\Delta$\abun{Si}[$\sigma$, \micro] & $\Delta$\abun{Si} %%@ (\ion{Si}{iii}) \\ \hline \noalign{\smallskip} & & { ($1.42 \pm 0.06$)} & & & & & & \\ \hd{36512} & B0~V & $33~700 \pm 200$ & ... & ... & $34~000 \pm 500$ & {\bf 33~700} & {\bf 4.2} & $4.3 \pm 0.7$ & {\bf %%@ 7.49}$\pm$~[0.07, 0.05] & $\pm$0.12 \\ & & { ($0.69 \pm 0.09$)} & & & & & & \\ \hd{37020} & B0.5~V & $30~500 \pm 600$ & ... & ... & $30~000 \pm 500$ & {\bf 30~500} & {\bf 4.2} & $0.5 \pm 0.5$ & {\bf %%@ 7.47}$\pm$~[0.10, 0.04] & $\pm$0.06 \\ & & { ($0.60 \pm 0.04$)} & & & & & & \\ \hd{36960} & B0.5~V & $28~900\pm300$ & ... & ... & $29~000\pm500$ & {\bf 28~900} & {\bf 3.9} & $5.4 \pm 0.6$ & {\bf %%@ 7.53}$\pm$~[0.02, 0.06] & $\pm$0.06 \\ & & { ($0.64 \pm 0.07$)} & & & & & & \\ \hd{37042} & B0.7~V & $29~700\pm 400$ & ... & ... & $29~500 \pm 500$ & {\bf 29~700} & {\bf 4.2} & $1.4 \pm 0.3$ & {\bf %%@ 7.55}$\pm$~[0.03, 0.04] & $\pm$0.05 \\ & & { ($0.39 \pm 0.01$)} & & & & & & \\ \hd{36591} & B1~V & $27~200 \pm 100$ & ... & ... & ... & {\bf 27200} & {\bf 4.1} & $1.3 \pm 0.3$ & {\bf 7.53}$\pm$~[0.06, 0.03] %%@ & $\pm$0.01 \\ & & { ($0.25 \pm 0.02$)} & { ($0.12 \pm 0.02$)} & & & & & \\ \hd{36959} & B1~V & $25~900 \pm 300$ & $25~900 \pm 100$ & ... & ... & {\bf 25~900} & {\bf 4.2} & $0.0 \pm 1.0$ & {\bf %%@ 7.50}$\pm$~[0.05, 0.07] & $\mp$0.02 \\ & & { ($0.16 \pm 0.03$)} & { ($0.12 \pm 0.01$)} & { ($0.12 \pm 0.04$)} & & & & \\ \hd{37744} & B1.5~V & $23~900 \pm 600$ & $25~700 \pm 100$ & $23~600 \pm 600$ & ... & {\bf 23~800} & {\bf 4.1} & $0.5 \pm 0.5$ & {\bf %%@ 7.54}$\pm$~[0.06, 0.04] & $\mp$0.05 \\ & & { ($0.14 \pm 0.02$)} & { ($0.20 \pm 0.01$)} & { ($0.17 \pm 0.03$)} & & & & \\ \hd{35299} & B1.5~V & $23~900 \pm 300$ & $24~900 \pm 300$ & $23~700 \pm 300$ & ... & {\bf 23~700} & {\bf 4.2} & $0.5 \pm 0.5$ & {\bf %%@ 7.50}$\pm$~[0.08, 0.02] & $\mp$0.06 \\ & & & { ($0.26 \pm 0.01$)} & { ($0.41 \pm 0.03$)} & & & & \\ \hd{36285} & B2~V & ... & $23~900 \pm 200$ & $20~600 \pm 200$ & ... & {\bf 20~600} & {\bf 4.0} & $1.7 \pm 0.5$ & {\bf %%@ 7.49}$\pm$~[0.06, 0.05] & $\mp$0.11 \\ & & & { ($0.36 \pm 0.02$)} & { ($0.44 \pm 0.04$)} & & & & \\ \hd{35039} & B2~V & ... & $22~200 \pm 200$ & $19~900 \pm 200$ & ... & {\bf 19~800} & {\bf 3.7} & $3.3 \pm 1.0$ & {\bf %%@ 7.52}$\pm$~[0.06, 0.08] & $\mp$0.14 \\ & & & { ($0.39 \pm 0.02$)} & { ($0.53 \pm 0.02$)} & & & & \\ \hd{36629} & B2~V & ... & $22~800 \pm 300$ & $20~000 \pm 100$ & ... & {\bf 20~000} & {\bf 4.1} & $1.0 \pm 0.5$ & {\bf %%@ 7.54}$\pm$~[0.04, 0.05] & $\mp$0.13 \\ & & & { ($0.65 \pm 0.06$)} & { ($0.96 \pm 0.09$)} & & & & \\ \hd{36430} & B2~V & ... & $21~000 \pm 300$ & $18~600 \pm 200$ & ... & {\bf 18~600} & {\bf 4.1} & $3.5 \pm 1.0$ & {\bf %%@ 7.47}$\pm$~[0.08, 0.07] & $\mp$0.13 \\ & & & { ($0.73 \pm 0.05$)} & { ($0.92 \pm 0.05$)} & & & & \\ \hd{35912} & B2~V & ... & $20~400 \pm 300$ & $18~500 \pm 150$ & ... & {\bf 18~500} & {\bf 4.0} & $3.2 \pm 0.5$ & {\bf %%@ 7.48}$\pm$~[0.07, 0.04] & $\mp$0.13 \\ \hline \end{tabular} \tablefoot{Detailed results (line-by-line) of the Si~abundance analysis are presented in Tables~\ref{res1} to~\ref{res13}. %in the electronic version of the paper. All \Teff\ values correspond to the \grav\ indicated in the 8th column.\\ \tablefoottext{a}{$EW_{\rm 4}$: \ioni{Si}{iv}~4116; $EW_{\rm 3}$: \ioni{Si}{iii}~4552; $EW_{\rm 2A}$: \ioni{Si}{ii}~4130; $EW_{\rm 2B}$: \ioni{Si}{ii}~6371.}} \end{table}