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Fig. 3

image

Evolution of the SFR of CALIFA galaxies as a function of Hubble type; for the whole galaxy (left), the inner (middle), and outer regions (right). Solid lines are the average sSFR(t) of the galaxies in each morphology bin, removing only the 5% of galaxies with smallest t0. Shaded bands around the average curves represent ± the error in the mean.

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