\begin{table}%T1
\caption{\label{lines}Properties of the observed emission lines.}
%\centerline
$${
\begin{tabular}{r c c l c r r @{\p}l r @{\p}l r @{\p}l r @{\p}l r @{\p}l r}
\hline \hline 
ID & $S$ & RA and Dec (J2000) & Line & Fit &
\multicolumn{1}{c}{$z$} & \multicolumn{2}{c}{\it FWHM} &
\multicolumn{2}{c}{Flux} & \multicolumn{2}{c}{{\it EW}$_0$} & 
\multicolumn{4}{c}{$_{\rm H\alpha}$~{\it SFR}~$_{\rm UV}$} & O/H \\
(1) & (2) & (3) & \multicolumn{1}{c}{(4)} & (5,6) & 
\multicolumn{1}{c}{(7)} & \multicolumn{2}{c}{(8)} & \multicolumn{2}{c}{(9)} & 
\multicolumn{2}{c}{(10)} & \multicolumn{2}{c}{(11)} & \multicolumn{2}{c}{(12)} & (13) \\ \hline
 79 & 4 & 11:40:52.62 $-$26:30:01.0 & \ha & 1,2 & 2.1558 & 160 &  80 &  3.6 
& 1.9 &  90 &  50 & 11 & 6 & 33 & 1       \\
131 & 2 & 11:40:51.28 $-$26:29:38.7 & \ha & 3,1 & 2.1518 & 320 &  50 & 12.3 
& 2.2 &  65 &  15 & 39 & 7 & 19 & 1 & 8.8 \\
    &   &                         & \nii&     &        & 270 & 100 &  4.4 
& 2.0 &  25 &  10 & \multicolumn{2}{c}{} & \multicolumn{2}{c}{}   &\p0.2\\
131 & 4 & 11:40:51.28 $-$26:29:38.7 & \ha & 3,1 & 2.1537 & 360 &  80 &  8.2 
& 2.4 &  45 &  15 & 26 & 8 & 19 & 1 & 8.8 \\
    &   &                         & \nii&     &        & 420 & 250 &  3.4 
& 2.5 &  20 &  15 & \multicolumn{2}{c}{} & \multicolumn{2}{c}{}   &\p0.2\\
144 & 3 & 11:40:43.45 $-$26:29:37.5 & \ha & 1,3 & 2.1463 &  40 &  20 &  6.7 
& 1.3 & 330 &  70 & 21 & 4 & 15 & 1       \\
183 & 2 & 11:40:46.15 $-$26:29:24.9 & \ha & 3,1 & 2.1546 & 170 &  20 & 13.8 
& 1.7 & 230 &  35 & 44 & 5 & 40 & 1 & 8.6 \\
    &   &                         & \nii&     &        & 200 & 120 &  2.5 
& 1.7 &  40 &  30 & \multicolumn{2}{c}{} & \multicolumn{2}{c}{}   &\p0.4\\
207 & 4 & 11:40:50.20 $-$26:29:21.0 & \ha & 1,2 & 2.1540 & 
                               \multicolumn{2}{l}{\hspace{4mm}$<$100}
& 1.9 & 0.9 & 50 &  25 &  6 & 3  & 12 & 1 \\
215 & 1 & 11:40:46.01 $-$26:29:16.9 & \ha & 3,1 & 2.1568 & 5300 & 800 & 46.2
& 8.8 & 150 &  30 & \multicolumn{2}{c}{$^\dagger$}\\
229 & 1 & 11:40:46.10 $-$26:29:11.5 & \ha & 3,1 & 2.1489 &  290 &  60 &  7.1 
& 1.9 &  30 &  10 & 23 & 6 & 26 & 1 & 8.8 \\
    &   &                         & \nii&     &        &  130 &  90 &  2.4 
& 1.7 &  11 &   8 & \multicolumn{2}{c}{} & \multicolumn{2}{c}{}   &\p0.3\\
284 & 3 & 11:40:45.58 $-$26:29:02.4 & \ha & 1,2 & 2.1523 &   90 &  50 &  3.0
& 1.4 & 300 & 140 & 10 & 4 & 6 & 1        \\
329 & 3 & 11:40:46.88 $-$26:28:41.4 & \ha & 2,3 & 2.1609 &   60 &  40 &  2.7
& 1.3 &1350 & 700 &  9 & 4 & 7 & 1 \\
    &   &                         & \ha & 2,3 & 2.1636 &  110 &  30 &  2.0
& 1.1 &1000 & 550 &  6 & 4 \\
\hline 
\end{tabular}}
$$
\smallskip
Notes: (1) Candidate number; (2) slit number;
(3) coordinates; (4) line identification; (5) type of fit: 1) one
Gaussian curve; 2) two Gaussian curves; 3) two Gaussians for \ha~and
\nii; (6) identification is~1) certain, detection of~\nii; 2)~consistent, expected non detection of~\nii; 3)~possible;~(7) redshift
with random error~0.0002, except for candidate~215, for which it is~0.002;~(8) {\it FWHM} in~km~s$^{-1}$; (9)~flux in~10$^{-17}$~\ecs; (10) {\it EW}$_0$
in~\AA;
(11) {\it SFR}$_{\rm H\alpha}$ in~$M_\odot$~yr$^{-1}$; (12)~{\it SFR}$_{\rm UV}$ in~$M_\odot$~yr$^{-1}$; (13)~metallicity in~$12 +
\log~[$O/H]~($^\dagger$) \ha~unrelated to~{\it SFR}.
\end{table}