\begin{table}%t2.a
%\centering
\par
\tabcolsep=3pt \small
\caption{\label{parameters_bcep}Fundamental parameters of well-studied~$\beta$
Cephei stars (spectral types from SIMBAD), as derived from AnalyseBstar
(values from the closest grid model are listed).}
\begin{tabular}{rlllllcrclrc}
\hline \hline \noalign{\smallskip}
HD  & Alternative & Spectral & \Teff~ & \logg \tablefootmark{a} &
$n$(He)/$n$(H)\tablefootmark{b} & $\logsi$ \tablefootmark{c}
& $\xi$  & \vsini & \vmacro \\ 
number & name & type & (K) & (cgs) & & &(km~s$^{-1}$) & (km~s$^{-1}$) &
(km~s$^{-1}$) \\
\hline
46328 & $\xi^1$ CMa & B0.5-B1IV & 27000 & 3.80 & 0.10 & --4.69 & 6 & 9 $\pm$ 2
&11\\ 
& &   & \textit{27500 }& \textit{3.75} & & \textit{--4.87
$\pm$ 0.21} &\textit{6 $\pm$ 2} & \textit{$10 \pm 2$} & --\\ 
50707 & 15 CMa & B1III & 24000 & 3.40 & 0.10 & --4.79 & 12 & 34 $\pm$ 4
& 38\\ 
& &   & \textit{26000 }& \textit{3.60} & & \textit{--4.69
$\pm$ 0.30} &\textit{7 $\pm$ 3} & \textit{$45 \pm 3$} & -- \\ 
205~021 & $\beta$ Cep & B1IV & 25000 & 3.80 & 0.10 & --4.70 & 6 & 26
$\pm$ 3 & 24\\ 
& &   & \textit{26000} & \textit{3.70} & &\textit{--4.89
$\pm$ 0.23}  &\textit{6 $\pm$ 3 }& \textit{29 $\pm$ 2} & --\\ 
44743 & $\beta$ CMa & B1.5III & 24000 & 3.50 & 0.10 & --4.76 & 15 & 19
$\pm$ 4& 20\\ 
& &   & \textit{24~000} & \textit{3.50 }& & \textit{--4.83
$\pm$ 0.23} &\textit{14 $\pm$3} & \textit{23 $\pm$ 2}& --\\ 
214~993 & 12 Lac & B1.5IV & 23000 & 3.60 & 0.10 & --4.41 & 6 & 44 $\pm$
6 & 37\\
 & & & & & & [--4.83] & [12] & & [0] (forced)\\
& &   & \textit{24500} & \textit{3.65} & & \textit{--4.89
$\pm$ 0.27} &\textit{10 $\pm$ 4 }& \textit{42 $\pm$ 4} & --\\ 
16582 & $\delta$ Ceti & B1.5-B2IV & 23000 & 3.90 & 0.10 & --4.80 & 6 &
14 $\pm$ 2&0\\ 
& &   & \textit{23000} & \textit{3.80} & & \textit{--4.72
$\pm$ 0.29} &\textit{1$^{+3}_{-1}$} &\textit{14~$\pm$~1} & -- \\ 
886 & $\gamma$ Peg & B1.5-B2IV & 23000 & 3.80 & 0.10 & --4.84 & $<$3 &
10 $\pm$ 1&0\\ 
& &   & \textit{22500} & \textit{3.75} & & \textit{--4.81
$\pm$ 0.29} & \textit{1$^{+2}_{-1}$ } & \textit{10 $\pm$ 1} & -- \\ 
29248 & $\nu$ Eri & B1.5-B2IV & 23000 & 3.70 & 0.10 & --4.73 & 10 & 21
$\pm$ 3 &39\\ 
& &   & \textit{23500 }& \textit{3.75} & & \textit{--4.79
$\pm$ 0.26} & \textit{10 $\pm$ 4 }& \textit{36 $\pm$ 3} & --  \\ 
\hline
\end{tabular}
\tablefoot{In italics, we display the results from the DETAIL/SURFACE analysis by \citet{Morel2006,Morel2008}. 
\tablefoottext{a}{Not corrected for centrifugal acceleration due to stellar rotation.} 
\tablefoottext{b}{Solar helium abundance: $n$(He)/$n$(H)~=~0.10.} 
\tablefoottext{c}{Solar silicon abundance: $\logsi = -4.49$. Interpolated values are listed.}}
\end{table}