Fig. 14.
Fit to our Te-based MZR (solid black line, Eq. (14)), plotted alongside the MZR from oxygen recombination lines (yellow/orange points, Esteban et al. 2009, 2014), the MZR from blue supergiant star photospheres (blue points, Kudritzki et al. 2016), and the MZR from the integrated stellar populations of SDSS-DR7 star-forming galaxies (red points, Zahid et al. 2017).
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