\begin{table}%T5
\caption{Sine fits to the \Ha\ radial velocities of
HS~1016, HS,1340, and HS~1857. For HS~2214 a combination of \Ha\
and \Hb\ radial velocities were fitted, as the September 2000 Calar
Alto spectra did not cover \Ha. For HS~1857 and HS~2214, the periods
were fixed to their values determined from the photometry. \label{t-rvfits}}
%
%\centering
\small
\begin{tabular}{ccccc}
\hline\hline\noalign{\smallskip} Object & \T\ & Period
(days) & $K$ (\kms) & $\gamma$ (\kms)\\ \hline\noalign{\smallskip}
%
HS~1016+3412 & $2452737.4039\pm0.0012$ & $0.0794\pm0.0019$ &
$93.0\pm5.3$ & $35.6\pm3.9$ \\ 
HS~1340+1524 & $2452737.4438\pm0.0018$ & $0.06435\pm0.00012$ & 
$57.5\pm6.2$  & $-31.1\pm4.1$ \\ 
HS~1857+7127 & $2452368.53243\pm0.00098$ & $0.189109\pm0.000001$ & 
$128.0\pm9.6$ & $-17.9\pm7.4$ \\ 
HS~2214+2845 & $2451812.3309\pm0.0028$ & $0.17918\pm0.00039$ & 
$73.5\pm6.5$  & $29.8\pm5.0$ \\
%
\noalign{\smallskip}\hline
\end{tabular}
\end{table}