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Table 3:

Visual spectrum of NGC 6210.
$\lambda$ Ion Meas.Intens.$^{\dagger}$) Corr. Intens.
3726 [O II] 23.1 25.0
3729 [O II] 11.6 12.5
3869 [Ne III] 80.9 86.7
4101 H 24.4 25.8
4267 C II 0.327 0.341
4340 H 45.7 47.5
4363 [O III] 5.85 6.08
4481 Mg II 0.19 0.020
4686 He II 1.48 1.50
4711 [Ar IV] 1.16 1.173
4740 [Ar IV] 1.52 1.534
4861 H 100 100
5007 [O III]   1084
5276 [Fe VII] 0.015 0.015
5517 [Cl III] 0.419 0.400
5538 [Cl III] 0.492 0.469
5755 [N II] 0.417 0.393
5876 He I 14.6 13.7
6312 [S III] 1.19 1.093
6563 H 304 276
6584 [N II] 20.6 18.7
6717 [S II] 2.42 2.185
6731 [S II] 4.01 3.618
6794 [K IV] 0.029 0.026
7135 [Ar III] 12.0 10.66
7237 [Ar IV] 0.099 0.088
7530 [Cl IV] 0.256 0.224
9532 [S III] 44.3 49.6
$^{\dagger}$ References: all values are taken from Liu et al. (2004a) except for $\lambda$9532 taken from Hippelein & Munch (1981).
$^{\ast}$ This is a blend of $\lambda$3726 and $\lambda$3729 lines.

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