\begin{table}%t3
\caption{Line identifications and redshifts.}
\label{Lines}
\small%\centerline
{
\begin{tabular}{ccccccccc}
\hline
\hline
% & & & & & & & & \\[-8pt]
Name & ID  & Line & Wavelength (\AA) & Redshift & Mean  &Flux & {\it FWHM} & Log Power 5 GHz\\
\hline 
\object{B0008--421}  & G  &     [\ion{Ne}{v}] 3425? & 7294 & 1.130 & 1.130* & 0.3&29&26.7\\
                  &   &       [\ion{O}{ii}] 3727? & 7940 & 1.130& &0.7&39 \\
\hline
\object{B0316+161}   &  G   & [\ion{O}{ii}] 3727 & 7102 & 0.906 &  0.907 &5.4&21&27.6\\
                    &   &   [\ion{Ne}{iii}] 3869 & 7381& 0.908 & &1.8&32\\
                  &   &     H$_\beta$ 4861 & 9277 & 0.908 & &4.7 & 49\\
                  &   &     [\ion{O}{iii}] 4959 & 9464& 0.908& &8.3 & 35\\
                  &   &       [\ion{O}{iii}] 5007 & 9544& 0.906&&33 &51\\
\hline
\object{B0407--658}  & G  & [\ion{Ne}{v}] 3425 & 6721 & 0.962 & 0.962 & 11&25 &27.7\\ 
                  &   & [\ion{O}{ii}] 3727 & 7314 & 0.962  &   &6.9&29\\
                    &   &   [\ion{Ne}{iii}] 3869 & 7595& 0.963 & &2.0&44\\
                  &   &   [\ion{Ne}{iii}] 3967 & 7787& 0.963 & &0.7&29\\
                  &   &     H$_\gamma$ 4102 & 8048 & 0.962 && 0.3& 18\\
                  &   &     H$_\beta$ 4861 & 9538 & 0.962 && 4.4&52\\
                  &   &     [\ion{O}{iii}] 4959 & 9731& 0.962& &43&51\\
                  &   &       [\ion{O}{iii}] 5007 & 9823& 0.962& &16&54\\
\hline
\object{B0904+039}   & G & [\ion{O}{ii}] 3727 & 6822 & 0.830 & 0.830&  1.9&17& 24.9\\
                  &   &       [\ion{O}{iii}] 4959 & 9078& 0.831&& 1.8&26\\
                  &   &      [\ion{O}{iii}] 5007 & 9162& 0.830&& 4.4&26\\
\hline
\object{B0914+114} & G & Break 4000 & 4711 & 0.178 & 0.178 &  --&--& --\\
                   &  &  H$\beta$ 4861 & 5690?  & 0.171? & $\pm$0.005&  --&--\\
                   &  &  Mg{\it b} 5200 & 6115 & 0.183& &  --&--\\
                   &  &  [\ion{N}{ii}] 6548 & 7667 & 0.171& &  --&--\\
                &  & H$\alpha$ 6563 & 7772 & 0.184 &  &--&--\\
                   &  &  [\ion{S}{ii}] 6716 & 7952 & 0.184& &  --&--\\
\hline            
\object{B1045+019}  &  &  [\ion{O}{ii}] 3727 & 6297 & 0.689 &  0.689*&0.4&12&26.6 \\
                  &   &      H$_\gamma$ 4102 & 7327 & 0.688 &&   0.3&12\\
                  &   &      [\ion{He}{ii}] 4686 & 7918& 0.689&& 0.3&29\\
\hline
\object{PMN J1300--1059}   &Q?   &  \ion{Mg}{ii} 2799  & 6385 & 1.283 & 1.283*&10&125&--  \\
\hline
\object{B1433--040}   & Q &  [\ion{O}{ii}] 3727 & 6694 & 0.796 &  0.795& 17&19&26.3\\
                    &   &     [\ion{Ne}{iii}] 3869 & 6949& 0.796 && 32 & 54\\
                  &   &     [\ion{Ne}{iii}] 3967 & 7122& 0.795 && 10&21\\
                  &   &      H$_\delta$ 4102 & 7355  & 0.794  &&  23&84\\
                  &   &      H$_\gamma$ 4341 & 7790 & 0.795 &&  76&113 \\
                  &   &      H$_\beta$ 4861 & 8724 & 0.795 && 347&192\\
                  &   &      [\ion{O}{iii}] 4959 & 8900& 0.795&& 63&30\\
                  &   &      [\ion{O}{iii}] 5007 & 8987& 0.795&& 121&27\\
\hline
\end{tabular}}
\medskip
For \object{B1433--040}, the redshift is measured with the narrow emission profiles. The *~means the redshift estimation is uncertain for that source, see text for details. The {\it FWHM} listed is the observed {\it FWHM} corrected for the {\it FWHM} of the instrumental spectrum. Fluxes in 10$^{-16}$~erg/cm$^2$/s. A~conservative error for~{\it z} is $\pm$0.001. The \object{B0914+114} results correspond to the unrelated galaxy. It shows emission and absorption lines mixed so the centers are more uncertain than in the other sources (the 1$\sigma$~error in~{\it z} is listed below the mean value) and line properties will depend on the stellar population model. The last column lists the radio power in~W/Hz of the source for the redshifts listed. The 5~GHz fluxes are from \citet{O'Dea98} and \citet{Wright90}.
\end{table}