\begin{table}%t2
\caption{Emission lines of the integrated spectrum (ejecta and
circumstellar ring combined corresponding to the central 281 spaxels)
in the $J$~band. The spectral resolution is 150~km~s$^{-1}$ in the $J$~band. Errors for the values listed in the table are given either in the text or in Table~\ref{obsval}. 
\label{lineTJ}}
%%\centerline{
%\begin{center}
{
\begin{tabular}{ccccccc}
\hline\hline
$\lambda_{\rm obs}$& $v_{\rm obs}$ & $\sigma_{\rm obs}$ & $\sigma_{\rm deconv}$ &  Flux & Identification & $\lambda_{\rm air}$ \\
($\mu$m) & (km~s$^{-1}$) & (km~s$^{-1}$) & (km~s$^{-1}$) &
($10^{-16}~$erg~s$^{-1}$~cm$^{-2}$) & & ($\mu$m) \\
\hline
1.253885 & 408 & 431& 404 & 14 & *[\ion{Fe}{ii}] a$^6$D$_{3/2}$--a$^4$D$_{1/2}$ & 1.2521\\
1.25385 & 261 & 431& 404 & 14 & *He I 1s3s--1s4p(3S-3P) & 1.2528\\
\multicolumn{7}{l}{Blend? The line transition probability for [\ion{Fe}{ii}] does not support this large flux. Furthermore large $\sigma_{\rm deconv}$.}\\
\hline
1.25787 & 277 & 200& 132&69&$\dagger$[\ion{Fe}{ii}] a$^6$D$_{9/2}$--a$^4$D$_{7/2}$& 1.2567 \\
1.27169 & 315 & 236 & 182 & 7 & $\dagger$[\ion{Fe}{ii}] a$^6$D$_{1/2}$--a$^4$D$_{1/2}$& 1.2703 \\
1.27983 & 245 & 305 & 266 & 43 &$\dagger$[\ion{Fe}{ii}] a$^6$D$_{3/2}$--a$^4$D$_{3/2}$&1.2788\\
1.27983 & 310 & 305 & 266 & 43 & * He I 1s3d--1s5f(3D-3F) &  1.2785 \\
\multicolumn{7}{l}{Blend? The line transition probability for [\ion{Fe}{ii}] does not support this large flux. Furthermore large $\sigma_{\rm deconv}$.}\\
\hline
1.28300 & 277  & 281 & 238 &  367 &$\dagger$Pa$\beta$  &1.2818   \\
1.29562 & 311  & 190 & 117 & 18  &$\dagger$[\ion{Fe}{ii}] a$^6$D$_{5/2}$--a$^4$D$_{5/2}$ &1.2943 \\
1.30651 & 302 & 253 & 204&12&  *\ion{N}{i}& 1.3052 \\
1.32178 & 277 & 166 & 71 & 23 & $\dagger$[\ion{Fe}{ii}] a$^6$D$_{7/2}$--a$^4$D$_{7/2}$ &1.3206 \\
1.32901 & 226 & 339 & 304 & 10 & $\dagger$[\ion{Fe}{ii}] a$^6$D$_{3/2}$--a$^4$D$_{5/2}$ & 1.3278\\
\hline
\end{tabular}}
\par
{\smallskip
 {The lines marked with $\dagger$ have been observed previously for this object in Meikle et~al. (1993).}\\
 {The lines marked with * are new for this object or have a new identification.} }
  %\end{center}
\end{table}