Fig. 2.
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12 + log O/H computed by NEBULABAYES (12 + log O/HNeb) versus the difference
between 12 + log O/HNeb and the metallicities computed through the (from left to right) SF, COMP (AGN+SF), and AGN calibrators (12 + log O/HCal). These distributions have been smoothed by a 2D Gaussian kernel density estimate (KDE), where the black contours outline density curves and darker shades of pink indicate higher densities. ellow histograms on the top panel showcase the distribution of
along with the 16th and 84th percentiles (purple dotted lines) of the distributions. Values of 12 + log O/HNeb and 12 + log O/HCal are consistent within the errors. Gray arrows point toward the value of the median error on 12 + log O/HNeb (ϵ in top panels), which is outside the range of values shown in the x-axis. This indicates that ϵ is 3× higher than the maximum difference between 12 + log O/HCal and 12 + log O/HNeb.
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