\begin{table}%t9
\caption[]{\label{tab:nsv5783_feros}FEROS spectra of NSV5783. $S/N$ is the signal to noise ratio
at approximately 5000~{\AA}. The exposure time is 30~min
for all spectra, and the Heliocentric Julian Dates correspond
to mid-exposure. 
The radial velocities given in brackets are strongly affected
by blending and have not been used to estimate the spectroscopic
elements. See text for details.}
\begin{tabular}{llrrrr}
\hline\hline\noalign{\smallskip}
\multicolumn{1}{c}{HJD}               & ID & $S/N$  & \multicolumn{1}{c}{Phase} &\multicolumn{1}{c}{$\mathrm{RV_p}$}      &\multicolumn{1}{c}{$\mathrm{RV_s}$}  \\
\multicolumn{1}{c}{$-$2\,400\,000}&    &    &                                  &\multicolumn{1}{c}{$\mathrm{(km\,s^{-1})}$}&\multicolumn{1}{c}{($\mathrm{km\,s^{-1})}$}  \\
\hline\noalign{\smallskip}
51\,208.76908   & s1  & 190 &0.8097               & 86.2   & $-$152.5  \\         % f3601  1
51\,209.83220   & s2  & 190 &0.9056               &(58.5)  & ($-$88.7) \\         % f3644  2
51\,211.79340   & s3  & 160 &0.0827               &$(-$61.1)&  (36.0)\\         % f3730  3
51\,212.87435   & s4  & 125 &0.1803               &($-$124.7)&   (4.9)\\          % f3773  4
51\,374.59662   & s5  &  75 &0.7795               &  83.2  &  $-$160.6 \\          % f3773  5
\hline\noalign{\smallskip}
\end{tabular}
\end{table}