\begin{table}
\caption{Emission lines in the complete spectrum (ejecta and
circumstellar ring combined corresponding to 281 spaxels) in $K$. The spectral resolution is 67 km~s$^{-1}$ in the $K$~band. Errors for the values listed in the table are given either in the text or in Table~\ref{obsval}.
\label{lineTK}}
%\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
2.00855 & 275 & 239 & 229 & 5  &$\dagger$[\ion{Fe}{ii}] a$^4$P$_{1/2}$--a$^2$P$_{1/2}$ & 2.0067 \\
2.01696 & 272 & 327 & 317 & 8  & * [\ion{Fe}{ii}] a$^2$G$_{9/2}$-a$^2$H$_{9/2}$ & 2.0151 \\
2.04779 & 259 & 293 & 285 & 8  &$\dagger$[\ion{Fe}{ii}] a$^4$P$_{5/2}$--a$^2$P$_{3/2}$ &  2.0460 \\
2.06003 & 275 & 291 & 283 & 108 & $\dagger$\ion{He}{i} 2s$^1$S--2p$^1$P$^0$ & 2.0581\\
2.11412 & 279  & 369 & 363  & 8   & *\ion{He}{i} 1s3p-1s4s  & 2.1121 \\
2.13462 & 258 & 267 & 258 & 3  &  $\dagger$[\ion{Fe}{ii}] a$^4$P$_{3/2}$--a$^2$P$_{3/2}$ & 2.1328 \\
2.16331 &   & 416 & 411  & 4  & * &\\
\multicolumn{7}{l}{Which could be part of a broad component of Br$\gamma$ (not seen on the red side of Br$\gamma$).}\\
\hline
2.16754 & 277 & 291 & 283 & 58   &$\dagger\ion{H}{i}$ Br$\gamma$ & 2.1655 \\
2.19052 &  & 575 & 571 & 3   & * &\\
2.20659 & 255 & 381 & 375 & 2 & *\ion{Na}{i} $2\rm p^65p{-} 2p^69s$ & 2.2047 \\
2.20659 & --58  & 381 & 375 & 2 & or $\dagger$ \ion{Na}{i} $4\rm s^2S{-}4p^2P^o$ & 2.2070 \\
2.22026 &  & 365 & 359 & 4  & * &  \\
2.22593 & 290 & 243 & 234 & 5  & * [\ion{Fe}{ii}] a$^2$G$_{9/2}$--a$^2$H$_{11/2}$ & 2.2238 \\
2.24580 & 286 & 534 & 530 & 4  &  $\dagger$[\ion{Fe}{ii}] a$^4$P$_{1/2}$--a$^2$P$_{3/2}$&2.2436 \\
\multicolumn{7}{l}{Blend? The line transition probability for [\ion{Fe}{ii}] does not support this large flux. Furthermore large $\sigma_{\rm deconv}$.}\\
\hline
2.25525 &  & 452 & 447 & 3  & * & \\
2.31030 & 304 & 403 & 397 & 3  & *\ion{Ni}{ii} $\rm 3p^63d^8(^3F)4s{-}3p^63d^8(^3F)4s$&  2.3079\\
2.32381 & 291 & 284 & 276 & 5  & *\ion{O}{i} $\rm 2s^22p^3(^2D)3s{-}2s^22p^3(^4S)5f$ & 2.3215 \\
\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.}\\
 {The lines 2.24--2.32 $\mu$m were observed in Meikle
et~al. (1993) as a blended unidentified feature.} 
\end{table}