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Table C.1.

Fit emission line fluxes. The reported uncertainty is the direct 1σ output of q3dfit.

Line central comp. red comp. blue comp.
f [10−18 erg s−1 cm−2]
[O II]3726,3729 5.8±0.4 2.1±0.4 8.9±1.6
[Ne III]3869 3.3±0.2 0.8±0.2 1.3±0.9
He I3888 + H8* < 0.5
[Ne III]3967 + Hϵ 1.5±0.4 0.4±0.3 0.4±1.4
Hδ 0.7±0.3 0.2±0.2 0.6±0.9
Hγ 1.6±0.2 0.4±0.2 0.4±0.7
He I4472* < 0.4
He II4686 1.4±0.1 < 0.2 1.1±0.8
Hβ 3.9±0.2 0.6±0.2 2.9±0.7
[O III]4959 17.5±0.5 1.8±0.4 8.7±1.5
[O III]5007 53.1±1.0 5.6±1.0 26.3±1.6
He I5876* < 0.6
[Fe VII]6087* < 0.7
[O I]6300 2.4±0.2 0.3±0.2 3.1±0.8
[S III]6312 0.4±0.2 0.2±0.2 0.9±0.9
[O I]6364 0.8±0.3 0.1±0.3 1.0±1.1
[N II]6548 2.0±0.3 0.7±0.3 4.0±1.1
Hα 15.8±0.4 1.2±0.3 14.7±1.1
[N II]6583 6.0±0.4 2.0±0.3 12.0±1.1
[S II]6716 1.6±0.2 0.3±0.2 2.1±0.6
[S II]6731 1.8±0.2 0.6±0.2 4.8±1.1

Notes. *We report 3σ upper limits for lines with low S/N (Sect. 3.3). Though the He II4686 has S/N > 10, the fit reported the flux of its comp. red to be 0. Hence, we report the upper limit here.

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