Fig. 8
Relation between different calibrations for obtaining oxygen abundances. In panels a) − d), we compare the methods used for run2 galaxies with the R23 calibration by McGaugh (M91). In panels e) and f), the comparison is for run1 galaxies, between N2 and either O3N2 or SB1. The solid line in each plot shows the agreement between the different methods.
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