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Fig. 7


Difference between the SFR averaged over 100 Myr and the instantaneous one given by CIGALE plotted as a function of the age of the youngest stellar population (tf for the τ-models and tySP for the two-populations model). Triangles are for the two-populations model, small circles for the rising-τ model and large circles for the τ model. The absolute value of the decreasing rate τ is color coded for τ-models.

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