\begin{table}%t4
\par
%\centering
\par
\caption{Spectral analysis. The error in the redshift is $\approx$$  \pm $$ 0.002$. The codes for the last two columns
are: 0-absorption emission line galaxy; 1-narrow emission line galaxy; 2-star; 
3-contamination by the filament; 4-spectra
very noisy.\label{spectra_table}}
\begin{tabular}{llllll}
\hline\hline
Slit Pos. & Object  & Spectral features ($>$$3\sigma $) & Redshift  & Type & Notes\\
\hline
1,~3 & NGC~7603B & CaH\&K, MgI, NaI, etc. & 0.056 & 0 \\
1 &  \#1     & OII, H$\beta$, OIII, OI, H$\alpha$ & 0.394 & 1 \\
1 &  \#2     & OII, NeIII, H$\beta$, OIII, H$\alpha$ & 0.245  & 1 \\
1 & Filament & H$\beta $, MgI, NaI & 0.030 &  Abs. & 4, Paper I \\
2 & \#17     & H$\alpha$, H$\beta$  & 0 & 2 & 3 \\
2 & 3.6\arcsec-WNW of \#17   &  --  & -- & --  & 4 \\
2 & \#19   &  --  & -- & --  & 4 \\
2,~3 & \#21  & OIII$_{5007}$, H$\alpha$, NII, SII & 0.117 & 1 \\
2,~3 & \#22 &  OII, H$\beta $, H$\alpha $ & 0.401  & 1 &  \\
3 & \#23 & H$\alpha $ & 0.246  & 1 \\
\hline
\end{tabular}
\end{table}