\begin{table}%t3
%%\centering

\par
\caption{\label{tab:vrotnosol}Projected rotational velocities of radial velocity variable sdBs, for which orbital parameters are unavailable or uncertain.} 
\begin{tabular}{llllllll}
\hline \hline \noalign{\smallskip}
 System & $T_{\rm eff}$ & $m_{B}$ & $S/N$ & seeing &  $N_{\rm lines}$ &  ${v_{\rm rot}~\sin~i}$ & Instrument\\ 
& [K] & [mag] &  & [arcsec] &  & [${\rm km~s^{-1}}$] & \\
\hline
HE~2208$+$0126 & 24~300 & 15.6 &  24 & 0.8 &  15 & $<$5.0 & UVES\\
TON~S~135 & 25~000 & 13.1 &  47 & &  35 &  6.6 $\pm$ 1.0  & FEROS\\
HE~2322$-$4559$^{c}$ & 25~500 & 15.5 &  23 & 0.7 &  16 &  10.9 $\pm$ 1.1 & UVES\\
HS~2043$+$0615 & 26~200 & 16.0 &  22 & 1.3 &  26 &  12.3 $\pm$ 1.1 & UVES\\
HE~1309$-$1102$^{c}$ & 27~100 & 16.1 &  7 & 0.6 &  7 &  7.6 $\pm$ 2.3 & UVES\\
HS~2357$+$2201 & 27~600 & 13.3 &  29 & 0.7 &  26 & 6.1 $\pm$ 1.1 & UVES\\
HS~2359$+$1942 & 31~400 & 14.4 &  14 & 0.6 &  26 &  $<$ 5.0 & UVES\\
PG~1032$+$406 & 31~600 & 10.8 & 20 & & H/He & $<$34 & Palomar\\
HE~1140$-$0500$^{c}$ & 34~500 & 14.8 &  18 & 0.9 &   5 &   5.2 $\pm$ 2.7 & UVES\\
HS~1536$+$0944$^{c}$ & 35~100 & 15.6 &  19 & 1.1 &  15 &  12.2 $\pm$ 1.6 & UVES\\
HE~1033$-$2353 & 36~200 & 16.0 &  13 & 0.6 &   7 &   9.3 $\pm$ 2.3 & UVES\\
\hline
\end{tabular}
\tablefoot{The average seeing is only given if the spectra were obtained with a wide slit in the course of the SPY survey. In all other cases the seeing should not influence the measurements. Atmospheric parameters are taken from Lisker et~al. (\cite{lisker}) except TON~S~135 (Heber \cite{heber1}) and PG~1032$+$406 (Maxted et~al. \cite{maxted2}). $^{c}$ Companion visible in the spectrum.}
\end{table}