Results of Bayesian analysis of the mock catalog. Each plot corresponds to an output parameter considered in this work and discussed in the text. The first six output parameters are related to the star formation history (M_star, SFR, D4000, τ₁, t₂, and f_ySP); the next five output parameters characterize the dust attenuation (δ, A_V,ySP, f_att, A_V, and A_FUV) and the two last ones define the IR dust emission (L_IR and α). The “exact” values are plotted on the x-axis, the results applying the SED fitting method to the mock data are plotted on the y-axis, and the standard error given by the Bayesian analysis is over plotted as an error bar for each value. The linear Pearson correlation coefficient (r) is indicated on each plot.