\begin{table}%t2
\caption{\label{lines}Measurements for the emission lines of the
  LSB~candidate sample. All entries which are marked with $^{a}$ were not used
  for the estimation of the mean redshift $\langle z\rangle $ and therefore also not for
  the estimation of the standard deviation $\sigma_z$. All lines which were
  either influenced by night sky emission lines or which had only upper limits
  were also not used for the determination of the mean redshift. It was not
  possible to resolve the two component of the [S\II]-doublet. Therefore
  [S\II] was not used in order to estimate redshifts. The redshift of
  \object{LSB~J22324-60520} (marked with $^{b}$) was estimated measuring the
  wavelength of the Ca\II-K absorption line.}
\small
%\centering
\par
\begin{tabular}{l l l l l l l l c c}
\hline
\hline 
NAME&[O\II]&H\B&[O\III]&[O\III]&H\A&[N\II]&[S\II]&$z$&$\sigma_z$\\
&\La3727&\La4861&\La4959&\La5007&\La6563&\La6584&\La\La6717,6731&&\\
&[\AA]&[\AA]&[\AA]&[\AA]&[\AA]&[\AA]&[\AA]&&\\
\hline
\object{LSB~J22311-60503}&4172&--&--&-&7351&--&--&0.1198&0.0004\\
\object{LSB~J22325-60155}&3924&5118&5219&5270&6907&--&7077$^{a}$&0.0526&0.0002\\
\object{LSB~J22330-60543}&3936&5133&5236&5287&6929&--&7096$^{a}$&0.0559&0.0001\\
\object{LSB~J22343-60222}&3903&5089&5190&5242&6866&6888$^{a}$&7037$^{a}$&0.0467&0.0005\\
\object{LSB~J22352-60420}&4170&5439&5550$^{a}$&5603$^{a}$&7347&--&--&0.1191&0.0003\\
\object{LSB~J22353-60311}&3946&5146&5250&5297&6943&6968$^{a}$&--&0.0584&0.0004\\
\object{LSB~J22354-60122}&4329&5647&5758&5816&--&--&--&0.1615&0.0002\\
\object{LSB~J22355-60183}&4194&5468&5584$^{a}$&5632&7381&--&--&0.1249&0.0003\\
\hline\noalign{\smallskip}
\object{LSB~J22324-60520}&--&--&--&--&--&--&--&0.1723$^{b}$&--\\
\hline
\end{tabular}
\end{table}