Comparison between the true parameters of the mock SEDs and the results from the SED modeling with CIGALE. A parameter is well-constrained when there is a one-to-one relation between the two. Statistics on the ratio between the output and the input parameters are provided for the stellar mass and SFR: the first quartile of the ratio, the median, and the third quartile. The red dashed line in the r_SFR panel indicates the threshold adopted in this study.