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Table 3

Observed and extinction corrected emission line fluxes for the integrated spectrum of the galaxy.

Integrated
F(λ)/F(Hβ) I(λ)/I(Hβ)

Hγλ4340 46.12 ± 3.88 49.21 ± 7.31
[O iii]λ4363 14.75 ± 0.95 15.69 ± 1.36
He i λ4471 >4.30 ± 0.39 >4.51 ± 0.59
He ii λ4686 >1.20 ± 0.20 >1.22 ± 0.29
He i+[Ar v]λ4711 >3.80 ± 0.53 >3.87 ± 0.76
[Ar v]λ4740 >2.70 ± 0.14 >2.74 ± 0.20
Hβλ4861 100.00 ± 2.71 100.00 ± 3.83
[O iii]λ4959 169.96 ± 5.02 168.61 ± 7.05
[O iii]λ5007 507.75 ± 12.70 499.87 ± 17.68
He i λ5876 11.92 ± 0.68 10.96 ± 0.88
[O i]λ6300 1.03 ± 0.20 0.92 ± 0.25
[S iii]λ6312 1.10 ± 0.12 0.99 ± 0.14
[O i]λ6363 0.32 ± 0.03 0.29 ± 0.04
[N ii]λ6548 0.61 ± 0.10 0.54 ± 0.16
Hαλ6563 317.83 ± 6.25 280.95 ± 7.81
[N ii]λ6584 2.05 ± 0.14 1.81 ± 0.17
He i λ6678 3.43 ± 0.45 3.01 ± 0.56
[S ii]λ6717 4.94 ± 0.30 4.33 ± 0.37
[S ii]λ6731 2.13 ± 0.38 1.86 ± 0.47
F(Hβ)a 5.16 ± 0.07
EW(Hα)b 834
EW(Hβ)b 157
c(Hβ) 0.18

Notes. The fluxes are relative to F(Hβ) = 100. ; .

(a)

In units of ×10-14 erg cm-2 s-1

(b)

in units of Å

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