DFRD for models with dust masses computed by CIGALE with DL2014 dust models. Only models with a delayed star formation history are plotted. A delayed star formation history only was consistently used in the SED fitting with CIGALE to estimate sM_dust and sSFR. The models shown do not have any grain growth in the ISM. We also show the other models in light gray to show which parameter space the models cover. On this figure, we superimposed the three lines that show the respective linear fits as in Fig. 11. The models shown are from Burgarella et al. (2020) and Nanni et al. (2020). This figure shows that most of the objects (ALMA detections and ALMA upper limits) are approximately located at the same positions as the models. Only HZ9 is found at larger sSFR and sM_dust. If confirmed at this location in the DFRD, these objects would be very difficult to explain with these models.