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Fig. 10

image

Cosmic evolution of the SFR density, ρSFR (upper panels), the sSFR(t) (middle panels), and the stellar mass volume density, ρ (lower panels) as a function of the morphology: early-type (E, S0, and Sa) and late-type (Sb, Sbc, Sc, and Sd) galaxies. The contribution of the inner (R < 0.5 HLR) and outer (1 < R < 2 HLR) regions of ETGs and LTGs are listed in the central and right panels, respectively.

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