Table 4: Infrared measured line intensities for NGC 6543. In the last column the dereddened and aperture corrected fluxes (Flux $^{\rm corr}$) are given. The EB-V=0.07, and the aperture correction factor is 1.3 for ions measured with the smallest ISO SWS aperture (<12 $\mu $m).
$\lambda (\mu$m) Ident. Flux $^{\rm obs}$ Flux $^{\rm corr}$
2.625 H I (Br$\beta$) 10.6 13.9
3.038 H I (10-5) 1.56 2.04
3.296 H I (Pf$\delta$) 1.41: 1.85
3.739 H I (Pf$\gamma$) 2.57 3.36
4.051 H I (Br$\alpha$) 17.7 23.2
4.486 Mg IV <1.88 <2.45
4.653 H I (Pf$\beta$) 4.32 5.64
6.984 [Ar II] 3.60: 4.69
7.312 [Na III] 3.28 4.27
7.459 H I (Pf$\alpha$) 5.79 7.54
7.502 H I (8-6) 2.43 3.17
8.990 [Ar III] 68.8 90.3
10.51 [S IV] 385.2 505.6
12.81 [Ne II] 22.2 22.3
15.55 [Ne III] 631.8 634.0
18.70 [S III] 132.0 132.6
19.06 H I (8-7) 1.82 1.83
21.83 [Ar III] 4.41 4.43
22.32 H I, He II 0.41: 0.41
25.89 O IV <0.36 <0.36
33.48 [S III] 51.2 51.3
34.81 [Si II] 1.21: 1.21:
36.01 [Ne III] 52.8 52.9
51.80$^\dagger$ [O III] 504.7 505.2
57.31$^\dagger$ [N III] 120.6 126.7
88.33$^\dagger$ [O III] 144.3 144.3
$^\dagger$From the LWS spectrum.
: Noisy.

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