\begin{table}%t2.b
%\centering
\par
\caption{\label{parameters_SPB}Same as for Table~\ref{parameters_bcep}, but
now for some well-studied SPBs.}
\begin{tabular}{rllccccrccrc}
\hline \hline \noalign{\smallskip}
HD & Alternative & Spectral & \Teff~& \logg~& $n$(He)/$n$(H) & $\logsi$
& $\xi$ & \vsini & \vmacro\\ 
number & name & Type & (K) & (cgs) &  & & (km~s$^{-1}$) &  (km~s$^{-1}$) &
(km~s$^{-1}$) \\
\hline
3360 & $\zeta$ Cas & B2IV & 22000 & 3.80 & 0.10 & --4.76 & $<$3 & 18
$\pm$ 2 & 13\\
     &  &   \hfill \tablefootmark{a}  & \textit{22000} & \textit{3.70} &  &
\textit{--4.72 $\pm$ 0.30} &
\textit{1 $\pm$ 1} & \textit{19 $\pm$ 1} & --  \\ 
85953 & V335 Vel &  B2IV & 20000 & 3.80 & 0.10  & --4.84 & 6 & 30
$\pm$ 1 & 20 \\ 
  & & \hfill \tablefootmark{a}& \textit{21000} & \textit{3.80}  & &
\textit{--4.75 $\pm$ 0.30}&
\textit{1 $\pm$ 1} & \textit{29 $\pm$ 2} & --   \\ 
3379 & 53 Psc & B2.5IV & 20000 & 4.30 & 0.10 & --4.73 & $<$3 & 48 $\pm$
8&43\\
74195 & o Vel & B3IV & 16500 & 3.70 & 0.10 & --4.79 & $<$3 &18 $\pm$ 2
&18\\
160762 & $\iota$ Her & B3IV & 19500 & 4.10 & 0.10 & --4.86 & 3 & 8$\pm$
2 &0\\
25558 & 40 Tau & B3V & 17500 & 4.00 & 0.10  & --4.72 & 6 & 28 $\pm$ 2 &
31 \\
181558 & HR 7339 & B5III & 15000 & 4.00 & 0.10  & --4.79 & 6 & 17 $\pm$
2 & 0 \\
26326 & HR 1288 & B5IV & 15500 & 3.60 & 0.10 & --4.49 & $<$3 & 17 $\pm$
1 &17\\
206540 & HR 8292 & B5IV & 13500 & 3.80 & 0.10 & --4.79 & 3 & 15 $\pm$ 2
& 0 \\
24587 & HR 1213 & B5V & 14500 & 4.00 & 0.10 & -4.79 & $<$3 & 25 $\pm$
4 &21\\
28114 & HR 1397 & B6IV & 14000 & 3.50 & 0.10 & --4.79 & $<$3 & 21 $\pm$
4 &17\\
138764 & HR 5780 & B6IV & 14500 & 3.90 & 0.10 & --4.51 & 3 & 21 $\pm$ 2
&0\\
215573 & HR 8663 & B6IV & 13500 & 3.80 & 0.10 & --4.49 & $<$3 & 8 $\pm$
1 &0 \\
39844 & HR 2064 & B6V & 14500 & 3.70 & 0.10  & --4.39 & $<$3 & 16 $\pm$
1 & 0\\
191295 & V1473 Aql & B7III & 13000 & 3.70 & 0.10 & --4.79 & 3 & 16 $\pm$
1 &15\\
21071 & V576 Per &  B7V & 13500 & 3.70 & 0.10  & --4.79 & 3 & 22 $\pm$ 1
& 0\\
37151 & V1179 Ori & B8V & 12500 & 3.80 & 0.10  & --4.79 & $<$3 & 20
$\pm$ 2 & 0\\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Independent results of the DETAIL/SURFACE analysis by \citet{Briquet2007a}.}}
\end{table}