Same as Fig. A.2, but for comparison with Hyde. On the left column we also give the model's L_IR (since the SEDs are otherwise very similar). The first row shows a SFH which lasts steadily for several hundred million years but is composed of multiple bursts and dips, then slowly fades out 200 Myr before the observation. The second row shows an SFH with essentially two bursts happening at least 500 Myr prior observation. The third row shows an SFH with two burst, the last one happening when the galaxy is observed.