Comparison between the true parameters of the mock SEDs and the results from the SED modeling with CIGALE (from top left panel) for the SFR, stellar mass (M_*), dust luminosity (L_dust), dust mass (M_dust), attenuation in the V band (Att_V) of the birth clouds and the ISM, color excess (B-V), age of the main stellar population (age_⋆), and the attenuation in the FUV (Att_FUV). A parameter is considered to be well estimated and constrained when there is a one-to-one relation between the two.