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Table 4.

Results of the emission line fitting.

Galaxy name AV EW (Hα) log([OIII]/Hβ) log([NII]/Hα) log([SII]/Hα) log([OI]/Hα])
NGC 2110 2.2 75.3 0.71 0.11 0.05 −0.4
NGC 2992 4.51 62.6 1.05 −0.03 −0.31 −0.96
MCG-05-23-016 1.72 24.4 1.08 −0.1 −0.46 −0.9
NGC 3081 0.88 94.0 1.14 −0.04 −0.3 −0.99
ESO 021-G004 2.35 2.5 0.77 0.3 0.17 −0.47
NGC 5728 1.63 53.1 1.09 0.12 −0.16 −0.91
ESO 137-G034 2.24 116.9 1.09 0.04 −0.13 −0.83
NGC 7172 1.89 7.1 0.57 0.04 −0.34 −1.02
NGC 7582 2.44 65.5 0.39 −0.17 −0.54 −1.64
NGC 718 0.41 0.9 0.44 0.4 0.2 −0.63
NGC 1079 1.08 19.2 −0.13 −0.33 −0.51 −1.91
NGC 1947 4.37 4.8 0.35 −0.06 0.12 −0.52
ESO 208−G021 1.35 2.3 0.1 0.18 0.14 −0.67
NGC 3175 3.26 26.4 −0.76 −0.4 −0.64 −1.74
NGC 3351 0.85 6.6 −0.33 −0.2 −0.59 −1.46
ESO 093−G003 4.96 17.6 −0.2 −0.34 −0.42 −1.46
NGC 3717 2.76 8.3 −0.4 −0.26 −0.51 −1.38
NGC 3749 1.76 2.4 −0.04 −0.05 −0.3 −0.77
NGC 4224 3.25 1.9 0.45 0.16 0.02 −0.34
NGC 4254 1.35 6.3 0.59 −0.12 −0.61 −1.18
NGC 5037 2.95 3.0 0.57 0.32 0.06 −1.0
NGC 5921 2.01 6.2 −0.0 −0.02 −0.17 −0.86
IC 4653 1.16 62.7 −0.01 −0.56 −0.47 −1.66
NGC 7727 0.07 1.5 0.16 0.2 0.06 −0.73

Notes. AV in magnitudes from the Balmer decrement, following the prescription in Domínguez et al. (2013), equivalent to the width of Hα in Å; logarithmic flux ratios for the BPT and VO87 diagnostic diagrams.

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