\begin{table}%t2
%%\centering

\par
\caption{Projected rotational velocities for the binary sdB systems from
Table~\ref{tab:atm}.} 
\label{tab:vrotRV}
\begin{tabular}{lllllllll}
\hline \hline 
\noalign{\smallskip}
 System & $T_{\rm eff}$ & $m_{B}$ & $S/N$ & Seeing &  $N_{\rm lines}$ &  ${v_{\rm rot}~\sin~i}$ & Instrument & Reference\\ 
& [K] & [mag] &  & [arcsec] &  & [${\rm km~s^{-1}}$] & \\
\hline\\[-3mm]
PG~1627$+$017$^{l}$ & 23~500 & 11.3 & 64 & & 11 & $<$7.0 & HRS &\\
GD~687 &         24~300 &      &     &     &     & 21.2 $\pm$ 2.0 & & Geier et~al. (\cite{geier4})\\
JL~82$^{l}$ & 25~000 & 12.2 & 55 & & 57 & 10.4 $\pm$ 1.0 & FEROS & \\
PB~7352 & 25~000 & 12.0 & 61 & & 39 & 7.4 $\pm$ 1.0 & FEROS &\\
HE~0532$-$4503 & 25~400 & 16.1 &  83 & 0.8 &  18 &  11.1 $\pm$ 1.0 & UVES & \\
PG~0001$+$275$^{l}$ & 25~400 & 12.8 & 129 & & 24 & 12.6 $\pm$ 1.0 & FOCES &\\
PG~1248$+$164 & 26~600 & 14.4 & 47 & & 13 & 8.9 $\pm$ 1.3 & HRS &\\
PG~1232$-$136 & 26~900 & 13.1 & 167 & & 64 & $<$5.0 & UVES &\\
PG~1432$+$159 & 26~900 & 13.6 & 50 & & 22 & 9.5 $\pm$ 1.0 & HRS &\\
PG~1716$+$426$^{l}$ & 27~400 & 13.7 & 61 & & 24 & 10.9 $\pm$ 1.0 & HRS &\\
PG~0101$+$039$^{l}$ & 27~500 &      &    & &   & 10.9 $\pm$ 1.1 & & Geier et~al. (\cite{geier2})\\
CPD~$-$64~481 & 27~500 & 11.0 & 152 & & 38 & 4.1 $\pm$ 1.0 & FEROS &\\
PG~2345$+$318 & 27~500 & 14.4 & 92 & & 21 & 12.9 $\pm$ 1.0 & HRS &\\
PG~1043$+$760$^{l}$ & 27~600 & 13.4 & 15 & & H/He & $<$88 & Palomar&\\
PG~1743$+$477 & 27~600 & 13.6 & 57 & & 27 & $<$7.0 & HRS &\\
TON~S~183 & 27~600 & 12.4 & 55 & & 57 & 6.7 $\pm$ 1.0 & FEROS &\\
HD~171858 & 27~700 & 9.6 & 90 & & 55 & 6.7 $\pm$ 1.0 & FEROS &\\
HW~Vir & 28~500 & 10.3 & 130 & & H/He & 78.3 $\pm$ 1.0 & FEROS &\\
HS~0705$+$6700 & 28~800 & 14.2 & 28 & & H/He & $<$170 & HRS &\\
 &         &      &    & & H/He &  110 $\pm$ 14 & & Drechsel et~al. (\cite{drechsel})\\
PG~1329$+$159 & 29~100 & 13.3 & 52 & & 26 & 10.7 $\pm$ 1.0 & HRS &\\
Feige~48$^{s}$ & 29~500 & 13.1 & 37 & & 36 & 8.5 $\pm$ 1.0 & HIRES &\\
HE~0929$-$0424 & 29~500 & 15.4 &  25 & 0.6 &   9 &   7.1 $\pm$ 1.0 & UVES &\\
HE~1421$-$1206 & 29~600 & 15.1 &  21 & 0.5 &  18 &   6.7 $\pm$ 1.1 & UVES &\\
PG~0133$+$114 & 29~600 & 10.7 & 194 & & 17 & $<$8.0 & FOCES &\\
PG~1101$+$249 & 29~700 & 12.5 & 66 & & 24 & 8.1 $\pm$ 1.0 & HIRES &\\
PG~1512$+$244 & 29~900 & 13.0 & 87 & & 17 & $<$8.0 & HRS &\\
HE~2135$-$3749 & 30~000 & 13.7 &  84 & 1.0 &  53 &  6.9 $\pm$ 1.0 & UVES &\\
PHL~861 & 30~000 & 15.1 &  24 & 0.6 &  16 &   7.2 $\pm$ 1.3 & UVES &\\
HE~1047$-$0436 & 30~200 & 14.7 &  37 & 0.6 &  37 &   6.2 $\pm$ 1.0 & UVES &\\
HE~2150$-$0238 & 30~200 & 15.8 &  27 & 0.8 &  16 &   8.3 $\pm$ 1.5 & UVES &\\
PG~1017$+$086 & 30~300  &      &     &     &  H/He & 118 $\pm$ 5  & & Maxted et~al. (\cite{maxted3})\\
HE~0230$-$4323$^{s}$ & 31~100 & 13.8 &  59 & 0.9 &  40 &  12.7 $\pm$ 1.0 & UVES &\\
PG~1336$-$018$^{s}$ & 31~300 & 14.0 & 40 & & H/He & $<$79.0 & FEROS &\\
PG~1116$+$301 & 32~500 & 14.3 & 42 & & 8 & 9.0 $\pm$ 1.7 & HRS &\\
KPD~1946$+$4340 & 34~200 & 14.1 & 55 & & H/He & 26.0 $\pm$ 1.0 & HRS &\\
HE~1448$-$0510 & 34~700 & 15.0 &  27 & 0.6 &   8 &   7.2 $\pm$ 1.7 & UVES &\\
KPD~1930$+$2752$^{s}$ & 35~200 &      &     &     &     & 92.3 $\pm$ 1.5 & & Geier et~al. (\cite{geier})\\
CD~$-$24~731 & 35~400 & 11.6 & 42 & &   8 & 12.1 $\pm$ 1.7  & FEROS &\\
$[$CW83$]$~1735$+$22 & 38~000 & 11.5 & 230 & & H/He & 44.0 $\pm$ 1.0 & FOCES &\\ 
BPS~CS~22169$-$0001 & 39~300 & 12.6 & 109 & & 5 & 8.5 $\pm$ 1.5 & FEROS &\\
\hline
\end{tabular}
\tablefoot{For binaries with high ${v_{\rm rot}~\sin~i}$ 
helium lines and Balmer line cores (H/He) are used instead of metal lines. 
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. $^{c}$~Companion visible in the spectrum. 
$^{s}$ Pulsating subdwarf of V~361~Hya type. $^{l}$ Pulsating subdwarf of
 V~1093~Her type.}
\vspace*{-3mm}
\end{table}