\begin{table}%t4
\caption{Radial velocities of the spectral lines of HDE~327083.\label{t4}}
%%\centerline
\par
{\begin{tabular}{lrrcrcc}
\hline\hline\noalign{\smallskip}
Date       & Photosph.   &$N$ &Fe {\sc ii}&$N$ & DIB          & $N$ \\
           & km~s$^{-1}$&  &km~s$^{-1}$& & km~s$^{-1}$ &   \\
\noalign{\smallskip}\hline\noalign{\smallskip}
2000/07/19 & $-5\pm5$  &  9  &	 &  &         &  \\
2000/07/21 & $-1\pm7$  & 12  & $-15\pm1$ &4 &$-3\pm2$ & 3\\
2002/03/03 & $-56\pm9$ & 37  & $+25\pm6$ &9 &$-6\pm3$ & 5\\
2002/05/23 & $+13\pm5$ & 13  & $-82\pm8$ &4 &$-4\pm2$ & 3\\
2002/05/24 & $+13\pm4$ & 24  & $-79\pm6$ &3 &$-5\pm2$ & 3\\
2002/06/23 & $-62\pm5$ & 23  & $+23\pm1$ &2 &$-7\pm2$ & 3\\
2002/06/24 & $-64\pm5$ & 45  & $+21\pm5$ &5 &$-5\pm2$ & 5\\
2002/06/25 & $-67\pm5$ & 48  & $+22\pm4$ &7 &$-6\pm2$ & 4\\
2002/09/25 & $-36\pm5$ & 14  & $-27\pm2$ &3 &$-8\pm3$ & 7\\
\hline
\end{tabular}}
\smallskip
The mean $HRV$ of the photospheric lines are listed in Col.~2,
those of the emission peaks of the Fe~{\sc ii} lines in Col.~4, and
those of the~DIBs in~Col.~6. The number of lines used for the
averaging are listed in Cols.~3, 5, and~7, respectively.
The~DIBs~$HRV$ measurements show the wavelength scale stability.
\end{table}