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Table A.4.

Chemical abundances estimated from optical emission lines.

Name 12 + log(O/H) log(N/O) log(U) 12 + log(O/H)FM+20 12 + log(O/H)Ca+20
(1) (2) (3) (4) (5) (6)
IRAS00198-7926 8.28±0.24 -0.51±0.26 -1.87±0.10 7.65±0.20 8.45±0.13
NGC185 8.55±0.2 -0.97±0.25 -1.47±0.1 7.78±0.18 8.51±0.12
MCG-01-24-012 8.82±0.07 -0.98±0.14 -1.73±0.01 8.36±0.01 8.52±0.1
NGC4593 8.04±0.53 - -1.97±0.06 - -
NGC5506 8.59±0.16 -1.11±0.32 -1.71±0.06 8.17±0.16 8.54±0.12
IRAS08572+3915 8.17±0.33 -0.85±0.14 -3.58±0.08 - 8.36±0.09
Arp299A 8.00±0.26 -0.63±0.13 -3.26±0.06 - 8.33±0.06
NGC6240 8.25±0.34 -1.28±0.20 -3.89±0.02 7.96±0.20 8.72±0.11

Notes. Column (1): name of the galaxy. Columns (2)-(4): chemical abundances and ionization parameters with their corresponding uncertainties derived from HCM using the grid of AGN models for αOX = 0.8 and the stopping criteria of 2% of free electrons. Column (5): oxygen abundances and their uncertainties derived with the calibration proposed by Flury & Moran (2020) (Eq. 12). Column (6): oxygen abundances and their uncertainties derived with the calibration proposed by Carvalho et al. (2020) (Eq. 13). The complete version of this table is available at the CDS.

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