1. Introduction  
2. Data and sample selection  
3. Panchromatic SED modelling of the data  
3.1. Tools: CIGALE  
3.2. Statistical properties of our sample  
4. ISM diagnostics of the general population of QGs from hCOSMOS  
4.1. Evolution of $M_{\mathrm{dust}}/M_{\star}$ with redshift  
4.2. Evolution of $M_{\mathrm{dust}}/M_{\star}$ with sSFR  
5. Morphological impact on the evolution of dust abundance in QGs  
6. Interpretation of results with models  
6.1. Models  
6.2. Comparison between models and data  
6.3. Sources of dust in QGs at intermediate redshifts: insights from models  
6.4. To what extent does the specific dust mass mirror the molecular gas fraction in QGs?  
7. Conclusions