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Fig. 8


Upper panels: simulated passive and star-forming galaxies that are able to reproduce the MZ relations of Peng et al. (2015) in the 3D plot to test a more general relation between stellar M, average stellar metallicity Z, and the SFR using a Chabrier (2003; left panel) and a Salpeter IMF (right panel). Lower panels: 2D projection in the M- SFR plane.

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