Table 1: Properties of the observed emission lines.
\begin{displaymath}{ \begin{tabular}{r c c l c r r @{$~\pm~$}l r @{$~\pm~$}l r @... ... 30 & 2.0 & 1.1 &1000 & 550 & 6 & 4 \\ \hline \end{tabular}} \end{displaymath}
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 H$\alpha $ and [N II]; (6) identification is 1) certain, detection of [N II]; 2) consistent, expected non detection of [N II]; 3) possible; (7) redshift with random error 0.0002, except for candidate 215, for which it is 0.002; (8) FWHM in km s-1; (9) flux in 10-17 erg cm-2 s-1; (10) EW0in Å; (11) SFR $_{\rm H\alpha}$ in $M_\odot$ yr-1; (12) SFR$_{\rm UV}$ in $M_\odot$ yr-1; (13) metallicity in  $12 + \log~[$O/H] ($^\dagger$) H$\alpha $ unrelated to SFR.

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