Comparison of the two SFHs used in the CIGALEfitting process: the single burst model (x-axis) and the double burst model (y-axis). These graphs include the highly-magnified object described in the main text and removed from the MS fitting. In descending order, the graphs depict the comparison of the age of the main stellar population, the stellar mass, the SFR, and the statistic. Grey dots indicate galaxies for which the single burst model is a better fit and coloured dots indicate galaxies for which the double burst model is better. Red dots indicate galaxies for which the double burst model is significantly better than the single burst model. Error bars on these values are described in the caption of Fig. 3.