Star-formation rate versus lookback time (redshifts), enabling a comparison of the SFHs from different PROSPECTOR runs with varying priors and models. In purple is the fiducial bursty continuity prior run. In orange is the Leja et al. (2019) style continuity prior run. In green is a run with no dust parameters (i.e. dust free), and in red is a run with no f_esc parameter (i.e. f_esc = 0). In brown is a run with no nebular component, and in pink is a run with the most recent star-formation bin spanning 10 Myrs instead of the fiducial setup. Despite the varying models, we obtained a consistent interpretation of a rapidly quenched SFH.