Fig. 27.
Panel a: stellar mass as a function of redshift for our galaxy sample. The galaxies of the primary (“low redshift”) and secondary (“high redshift”) sub-samples of the MaNGA targets (Bundy et al. 2015; Wake et al. 2017) are shown by different symbols. Panel b: stellar mass Tully–Fisher relation for those galaxies. Panels c and d: central oxygen abundance (panel c) and the oxygen abundance at the optical radius (panel d) as a function of stellar mass of the galaxy.
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