Table 2: IRS spectrum of NGC 6369. The measured line intensity is given in Col. 3. The last column gives the ratio of the line intensity to H$\beta $(=100).
Identification $\lambda $($\mu $m) Intensity $^{\dagger}$ I/H$\beta $
[S IV] 10.505 2110 $\pm$ 66 65.2
H I(9-7) 11.301 14.2 $\pm$ 0.6  
  11.755 9.95 $\pm$ 0.7 0.308
H I (7-6+11-8) 12.365 31.3 $\pm$ 1.3  
  12.806 147 $\pm$ 6.0 4.14
  13.10 $\leq$0.90 $\leq$0.026
  13.52 $\leq$1.27 $\leq$0.035
  14.356 2.13 $\pm$ 0.41 0.060
  15.546 4971 $\pm$ 147 139.0
H I (10-8) 16.198 4.29 $\pm$ 0.24  
H2 17.036 2.63 $\pm$ 0.15  
  17.882 28.5 $\pm$ 0.9 0.814
  18.703 870 $\pm$ 24 24.8
H I (8-7) 19.056 11.1 $\pm$ 0.27  
$^{\dagger}$ Intensities measured in units of 10-14 erg cm-2 s-1 and are as measured through the SH diaphragm.
: Indicates an uncertain value.

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