Fig. 13.
Comparison between our new Te-based MZR Te-based MZR (solid black line, Eq. (14)) and other recent Te-based MZRs from the literature. Fits to the relations from Lee et al. (2006, orange), Andrews & Martini (2013, green), Izotov et al. (2015, light blue), and Ly et al. (2016b, dark blue) are shown. Stellar masses have been corrected for differences in the assumed dimensionless Hubble parameter where possible.
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