\begin{table}
\caption{Emission lines in the integrated spectrum (ejecta and
circumstellar ring combined corresponding to 281 spaxels) in~$H$. The spectral resolution is 
150~km~s$^{-1}$ in the $H$~band. Errors for the values listed in the table are given either in the text or in Table~\ref{obsval}.
\label{lineTH}}
%\centerline
 {
\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
1.49825 & 301  & 320 & 283 & 2   & *$\ion{H}{i}$ Br25& 1.4967\\
1.50986 &295  & 278 & 234 & 5  & $\dagger\ion{He}{i}$ 3s$^1$S--4p$^1$P$^0$ & 1.5084\\
1.51461 &  253  & 257 & 209 & 3 & * $\ion{H}{i}$ Br21  &   1.5133      \\
1.52037 & 232    & 276 & 232 & 3  & * $\ion{H}{i}$ Br20   & 1.5192   \\
1.52705 &  197   & 334 & 298  & 4  & *  $\ion{H}{i}$ Br19  &    1.5261   \\
1.53494 & 285 & 254 & 205 & 19& $\dagger[\ion{Fe}{ii}]$ a$^4$F$_{9/2}$--a$^4$D$_{5/2}$ & 1.5335\\
1.54512 & 237 & 272 & 227 & 5  & * $\ion{H}{i}$ Br17     & 1.5439 \\
1.55707 &273 & 270 & 224  & 5  &  * $\ion{H}{i}$ Br16 & 1.5556 \\
1.57142 &  257 & 305 & 266 & 7  & $\dagger\ion{H}{i}$ Br15 & 1.5701 \\
1.58947 & 273  & 283 & 240 & 10  &  $\dagger\ion{Si}{i}$ 4s$^1$P$^0$--4p$^1$P & 1.5880\\
& 267  & &&  &  $\dagger\ion{H}{i}$ Br14& 1.5881\\
\multicolumn{7}{l}{The transition probability for Br14 alone fits with the flux. \ion{Si}{i} identification tentative.}\\
\hline
1.60098 & 281  & 225 & 168 & 11   & $\dagger$[\ion{Fe}{ii}] a$^4$F$_{7/2}$--a$^4$D$_{3/2}$& 1.5995 \\
1.61232 & 257  & 279 & 235 & 12  & $\dagger\ion{H}{i}$ Br13 & 1.6109\\
1.64236 & 298  & 219 & 160 & 12   & $\dagger\ion{H}{i}$ Br12   &  1.6407 \\
1.64438 & 150 & 3393 & 3390 & 47   & $\dagger$[\ion{Fe}{ii}] a$^4$F$_{9/2}$--a$^4$D$_{7/2}$ &1.6435 \\
\multicolumn{7}{l}{Broad component. See text for comments. }\\
\hline
1.64518 & 296  & 171 & 82 & 51   &  $\dagger$[\ion{Fe}{ii}] a$^4$F$_{9/2}$--a$^4$D$_{7/2}$& 1.6435\\
\multicolumn{7}{l}{This component sits on top of the broad component (previous line).}\\
\hline
1.66534 & 282   & 234 & 180 & 6  &$\dagger$[\ion{Fe}{ii}] a$^4$F$_{5/2}$--a$^4$D$_{1/2}$& 1.6638\\
1.67851 & 290   & 233 & 178 & 12   &$\dagger$[\ion{Fe}{ii}] a$^4$F$_{7/2}$--a$^4$D$_{5/2}$ & 1.6769\\
1.68227 & 286   & 268 & 222 & 15   &  $\dagger\ion{H}{i}$ Br11  & 1.6807\\
1.70171 &  259  & 247 & 196 & 15   & $\dagger$\ion{He}{i} 3p$^3$P$^0$--4d$^3$D&1.7002\\
1.71289 & 307   &263 & 216  & 3  &$\dagger$[\ion{Fe}{ii}] a$^4$F$_{5/2}$--a$^4$D$_{3/2}$ & 1.7111\\
1.73769 & 254  & 311 & 272 & 21   & $\dagger\ion{H}{i}$ Br10& 1.7362\\
1.74661 & 286   & 327 & 291 & 6  & $\dagger$[\ion{Fe}{ii}] a$^4$F$_{3/2}$--a$^4$D$_{1/2}$& 1.7449\\
\hline
\end{tabular}}
\par
\smallskip
 {The lines marked with $\dagger$ have been observed previously for this object.}\\
 {The lines marked with * are new for this object or have a new identification.} 
\end{table}