Fig. 10.

Three projections of the FMR of Mannucci et al. (2010) compared with the properties of the ancestors of the galaxies that at z = 0.1 follow the MSR and MZRs. The big solid circles are the model galaxies illustrated in Sect. 5.1.1, and for which the SFR, stellar mass and metallicity values reported in the plots are computed at z = 0.1, 0.4, 0.8, 1.5 and 2.2, colour-coded as a function of their SFR values. The small black dots are a second-order fit of the SDSS data as presented in Mannucci et al. (2010).
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