Fig. 8.

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Relation between g−r color and stellar mass for the selected sample of galaxies. The data is based on stellar luminosities from the IllustrisTNG simulations, with g and r magnitudes calculated in the AB system (see details in Stoughton et al. 2002). The red line (g−r = 0.05log10(M★/M⊙)+0.1 mag) serves as the division between early-type and late-type galaxies.
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