Open Access

Table A.1.

Emission line fluxes normalized to Hβ = 100.

Line FastSpecFit a Gaussian fit b Case Bc Corrd
[O II]λ3726 22.71±0.70 0.88
[O II]λ3729 33.07±0.85 0.88
Hδ 29.73±0.54 30.47±1.18 26.4 0.88
Hγ 52.41±0.72 50.91±0.99 47.5 0.9
[O III]λ4363 6.96±0.43 0.9
Hβ 100.00±0.65 100.00±1.04 100.0
[O III]λ4959 58.27±0.49
[O III]λ5007 169.25±0.89
[S III]λ6312 0.67±0.10
[N II]λ6548 0.49±0.09
Hα 264.90±0.95 278.02±2.56 274.6
[N II]λ6584 1.44±0.09
[S II]λ6716 3.94±0.11
[S II]λ6731 2.67±0.10
[O II]λ7320e 0.89±0.08
[O II]λ7330f 0.70±0.06
[S III]λ9069 3.07±0.07
[S III]λ9531 9.43±0.13

Notes.

a

Flux from FastSpecFit VAC.

b

Flux from our Gaussian fit without subtraction of stellar continuum.

c

Recombination line flux expected from Case B.

d

Flux correction coefficient.

e

The line corresponds to unresolved doublet [O II]λλ7319,7320.

f

The line corresponds to unresolved doublet [O II]λλ7329,7330.

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