Fig. 6.
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Distribution (in logarithmic scale) of the ratio of the radio and SED SFRs. Each color corresponds to an SFRSED obtained by averaging the SFH over different timescales from 100 Myr up to 500 Myr. The inset presents the same statistics, but selects only galaxies with a declining SFH (∇SFR300 ≤ −20). The bias and the dispersion are indicated for each timescale.
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