Comparison between the simulated SFHs from Narayanan et al. (2024), binned as the CIGALE non-parametric SFHs, and the recovered SFR in the same time bins obtained with CIGALE. Bin 1 corresponds to the latest bin, at time of the observation, while bin 9 corresponds to the earliest time bin. The light green dots are obtained using a non-parametric SFH with bursty continuity prior while the dark green dots are obtained with the non-parametric SFH without prior proposed in this work.