\begin{table}%t2a.c
%\centering
\par
\caption{\label{parameters_nonconfirmed}Same as for 
Table~\ref{parameters_bcep}, but now for some well-studied hot B stars.}
\begin{tabular}{rlllllcrclrc}
\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
 93030 & $\theta$ Car & B0Vp & 31000 & 4.20 & 0.15 & --4.38  & 10 & 
108 $\pm$ 3 & 0 \\ 
 & & \hfill \tablefootmark{a}  & \textit{31000}& \textit{4.20} & -- &
\textit{--4.57 $\pm$ 0.23} & \textit{12 $\pm$ 4} & \textit{ 113 $\pm$ 8}
& -- \\
149438 & $\tau$ Sco & B0.2V & 32000 & 4.20 & 0.10 & --4.55 & 6 & 10
$\pm$ 2  & 0 \\ 
 & & \hfill \tablefootmark{a}& \textit{31500} & \textit{4.05}
& -- & \textit{--$4.76 \pm 0.14$} &  \textit{$2 \pm 2$} & \textit{$8 \pm 2$}  & -- \\
& & \hfill \tablefootmark{b}& \textit{31900} & \textit{4.15} & \textit{0.12} &
-- & \textit{10.8} & \textit{5} & -- \\
& & \hfill \tablefootmark{c}& \textit{32000} & \textit{4.30} & \textit{0.10} &
\textit{--4.50} & \textit{5} & \textit{4} & \textit{4} \\
36591 & HR 1861 & B1V & 26000 & 3.90 & 0.10 & --4.73  & 6 & $13
\pm 1$ & 0 \\ 
 & & \hfill \tablefootmark{d} &\textit{27000} & \textit{4.00}
 & -- & \textit{--4.75 $\pm$ 0.29} & \textit{3 $\pm$ 2}  & \textit{16 $\pm$ 2}  &
--\\
 & & \hfill \tablefootmark{c}& \textit{27000} & \textit{4.12} & \textit{0.10} &
\textit{--4.52} & \textit{3 } & \textit{12 } &--\\
52089 & $\epsilon$ CMa & B1.5-B2II/III & 22000 & 3.20 & 0.10 & --4.69 &
15 & 32
$\pm$ 2 & 20 \\ 
 & &  \hfill \tablefootmark{d}& \textit{23000} \tablefootmark{d} & \textit{3.30}
& -- & \textit{--4.77 $\pm$ 0.24} & \textit{16 $\pm$ 4}  & \textit{28 $\pm$ 2}
& -- \\
35468 & $\gamma$ Ori & B2II-III & 22000 & 3.60 & 0.10 & --4.79 & 10 & 46
$\pm$ 8 & 37 \\ 
& & \hfill \tablefootmark{d} & \textit{22000} & \textit{3.50}   & -- &
\textit{--5.00 $\pm$ 0.19}   & \textit{13 $\pm$ 5} & \textit{51 $\pm$ 4}   & -- \\
51309 & $\iota$ CMa & B2.5Ib-II & 17000 & 2.60 & 0.10 & --4.78 & 15 & 27
$\pm$ 4 & 39 \\ 
 & & \hfill \tablefootmark{d}  & \textit{17500}   & \textit{2.75}   &-- &
\textit{--4.82 $\pm$ 0.31}   &
\textit{15 $\pm$ 5}   & \textit{32 $\pm$ 3}   & --\\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Independent results of the DETAIL/SURFACE analysis
by \citet{Hubrig2008}.}
\tablefoottext{b}{Values found by \citet{Mokiem2005} using a genetic algorithm approach.}
\tablefoottext{c}{Results for two objects overlapping with the study of \citet{Przybilla2008}.} 
\tablefoottext{d}{Independent results of the DETAIL/SURFACE analysis
by \citet{Morel2006,Morel2008}.}}
\end{table}