Probing the timescale of the 1.4 GHz radio emissions as a star formation tracer

Open Access

Fig. 7.

Ratio of the SFR and the SFR_radio as a function of the SFR gradient over the last 300 Myr (∇SFR₃₀₀). Black dots represent galaxies that agree in both SFRs indicators, green dots show outliers in the SFH delayed scenario, and red dots show outliers for the two SFH models. 90% of the outliers would be selected as outliers with the flexible or nonparametric SFHs.

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