\begin{table}%T
  \caption{The emission line fluxes (H$_{\beta}=100$).}\label{tab-7}
  %\centerline
{
  \begin{tabular}{llrrccllrr}
  \hline\hline
   Label & Line & Model flux & Obsd. flux  &&&  Label & Line & Model flux &
  Obsd. flux  \\ &      &            & (dereddened)&&       &      &
    &  (dereddened)\\ 
\hline
TOTL(N 5) &  1240~A  &   17.152 & 25.720 &&& Cl 3 & 5538~A &  0.844 &   0.530\\
REC(C 2)  & 1335~A   & 20.298   & 19.340 &&& Fe 7 & 5722~A &  0.176 &   0.080 \\
TOTL(O 4) & 1402~A   & 33.473   & 87.610 &&& N  2 & 5755~A &  0.222 &   0.220 \\
TOTL(N 4) & 1486~A   & 26.800   & 29.260 &&& He 1 & 5876~A &  3.524 &   4.060 \\
TOTL(C 4) & 1549~A  &1193.302  & 1187.000 &&& Ca 5 & 6087~A & 0.804 & 0.150 \\
Ne 5~,~C 3 & 1575, 77~A  & 0.6~,~5.4   & 10.090 &&&   O  1 & 6300~A & 0.037 & 1.620 \\
Ne 4 & 1602~A  &  3.159   &  16.510 &&&  S  3 & 6312~A & 1.505 & 1.550 \\ 
He 2 & 1640~A  & 590.967  & 585.850 &&&  O  1 & 6363~A & 0.011 & 0.560 \\
TOTL(O 3) & 1665~A  & 42.890   &  45.800 &&&  Ar 5 & 6435~A & 1.129 & 0.990 \\
TOTL(N 3) & 1750~A  & 17.816   &  19.700 &&&  N  2 & 6548~A & 3.086 & 3.420 \\
TOTL(Si 3) & 1888~A  & 28.517   &  30.660 &&&  H  1 & 6563~A & 282.183 & 321.430 \\
TOTL(C 3) & 1909~A  &839.670   & 821.960 &&&  N  2 & 6584~A & 9.108   & 9.860\\ 
C  3 & 2297~A  &5.522     & 14.570  &&&  He 1 & 6678~A & 0.910   & 1.720\\ 
TOTL(C 2) & 2326~A  &38.553    & 33.980  &&&  S II & 6716~A & 2.022   & 1.800\\ 
Ne 4 & 2424~A  & 84.589   & 191.110 &&&  S II & 6731~A & 2.867   & 2.460 \\
He 2 & 2511~A  & 11.882   & 12.750  &&&  Ar 5 & 7005~A & 2.421   & 1.900 \\
He 2 & 2733~A  & 19.474   & 19.430  &&& He 1  & 7065~A & 1.159   & 1.300 \\
He 2 &3203~A   & 36.679   & 36.130 &&& Ar 3 & 7135~A &  10.538  & 9.160 \\
O  3 & 3265~A  & 0.948  &   1.830 &&&  He 2 &7178~A  &  1.429 &  0.850 \\
He 1 &3355~A   & 0.019  &  4.460 &&& Ar 4 &7237~A &  0.124 &  0.350 \\
Ne 5 &3426~A & 58.361 &  138.190 &&& Ar 4 &7263~A &  0.139 &  0.250 \\
O II &3726~A &  23.150&  23.120  &&& Cl 4 &7532~A &  0.479 &  0.290 \\
O II &3729~A &  12.050&  18.690 &&&  Ar 3 & 7751~A  & 2.543 & 2.300 \\
H  1 & 3734~A &  3.870 &  2.950 &&& Cl 4 & 8047~A & 0.960 &  1.190 \\
H  1 & 3750~A &  4.804 &  3.200 &&& H  1 &8598~A  &  1.056&  0.530 \\
H  1 &3771~A  &   6.035&  4.330 &&&H  1 &8665~A   & 1.310 &     0.940\\ 
H  1 &3798~A  &  7.758 &  4.770 &&&H  1 &8750~A   &  1.624&       0.940\\ 
He 1 & 3820~A & 0.290  &  0.490 &&&H  1 &8863~A   & 2.040 &     1.240 \\
H  1 &3835~A  &  8.037 &  7.010 &&&H  1 &9015~A   & 2.619 &     1.360 \\
S II &4070~A  &  0.775 &  1.590 &&&S  3 &9069~A   &13.549 &    12.170 \\
S II &4078~A  &  0.250 &  0.420 &&&H  1 &9229~A   & 2.704 &     2.420 \\
C  3 &4159~A  &  0.015 &  0.260 &&&He 2 &9345~A   & 2.981 &     2.240 \\
C  2 &4267~A  &  0.336 &  0.410 &&&H  1 &1.005~m  & 5.510 &     5.420 \\
H  1 &4340~A  & 47.440 &  48.670 &&& He 2 & 1.012~m  & 22.765&     20.550 \\
TOTL(O 3) &4363~A  & 22.280 &  22.080 &&& Si 7 & 2.483~m  &  0.000& $<$2.650 \\
He 1 &4388~A  & 0.143  &   0.190 &&&H  1 & 4.051~m  & 7.304 &     4.310 \\
He 1 &4471~A  &  1.180 &  1.240 &&&Ca 7&  4.086~m   & 1.543 & $<$12.930 \\
He 2 &4686~A  & 85.612 & 87.730 &&&Mg 4 & 4.485~m   &22.523 &    17.540 \\
Ar 4 &4711~A  &  5.778 &  7.900 &&&Ar 6 & 4.528~m   &11.800 & $<$10.130 \\
Ne 4 &4720~A  &  0.728 &  1.750 &&&Mg 7 & 5.502~m   & 0.000 & $<$18.170 \\
Ar 4 &4740~A  &  5.409 &  5.530 &&&Mg 5 & 5.608~m   & 12.233&    15.190 \\
O  3 &4959~A  &526.738 &   485.760 &&&Si 7&6.491~m  &  0.000& $<$10.640 \\
O  3 &5007~A &1585.481 &  1422.210 &&&Ne 6&7.650~m  &  3.927&     2.960 \\
Fe 6 &5177~A &   0.154 &     0.130 &&&Ne 2&12.81~m  &  0.296& $<$4.740 \\
Fe 3 &5270~A &   0.011 &     0.040 &&&Mg 5&13.52~m  &  1.006& $<$3.150 \\
N  4 &5209~A &   0.000 &     0.130 &&&Ne 5&14.32~m  &171.256&    122.490 \\
Cl 4 &5324~A &   0.030 &     0.060 &&&Ne 3&15.55~m  & 67.821&     61.350 \\
He 2 &5412~A &   6.894 &     6.360 &&&Ne 5&24.31~m  &136.497&    165.360 \\
Cl 3 &5518~A &   0.874 &     0.570&&&O  4&25.88~m  &813.774 &   929.370 \\
\hline
\end{tabular}}
\par
\medskip
\par
  Absolute H$_{\beta}$ flux  model: $8.32\times10^{-12}~\rm erg~cm^{-2}~s^{-1}$
  Obsn: $8.93\times10^{-12}~\rm erg~cm^{-2}~s^{-1}$. \\
  $\bf{Notes}$: "A'' in Col.  "Line'' signifies Angstrom;
  "m'' signifies $\mu$m.  In Col. "Label'', we have
  followed the notation used by Cloudy for atoms and ions; this will
  make identifying a line in Cloudy's huge line list easy.  Neutral
  state is indicated by "1'' and singly ionized state by "2'' etc., "TOTL''
  typically means the sum of all the lines in the doublet/multiplet; or it
  could mean sum of all processes: recombination, collisional excitation,
  and charge transfer.
  "REC'' indicates radiative recombination line;  for such cases, we
  have added the ionic name within parentheses for convenience though
  Cloudy does not.
  Some elements are represented by usual notation as per Cloudy.
  A symbol "$<$'' in the Col. "Obsd. flux'' indicates that these lines have not been
  detected by ISO and the values given are upper limits.
\par
  \end{table}