Fig. 1.
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Redshift–M⋆ plane of the MaNGA sample utilized in this study. The star-forming galaxies (see Sect. 2.1) chosen for the study of gas-phase metallicity are shown in green and the entire MaNGA DR17 sample in gray. The redshift and stellar mass distributions for the selected and full samples used in this work are shown as green and gray histograms.
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