1. INTRODUCTION  
2. OBSERVATIONS AND DATA  
2.1. The Sample  
2.2. Herschel  
2.3. ALMA  
2.4. Spitzer/IRAC  
2.5. Other Ancillary Data  
3. RESULTS  
3.1. ALMA Detection and Photometry  
3.2.2. Spitzer/IRAC  
3.3. Quantitative Morphological Modeling  
3.4. Summary of ALMA and IRAC Counterparts  
4. PHYSICAL PROPERTIES OF THE DETECTED LENSED SMGS  
4.1. SED Fitting and Photometric Redshift  
4.2. Multi-wavelength Color and Redshift  
4.3. Star Formation in Lensed SMGs  
4.4. Dust to Stellar Mass Ratio  
4.6. IR Surface Luminosity and Dust Temperature  
4.7. Dust-to-Stellar Size Ratio Versus IR Surface Luminosity  
4.8. Stellar Surface Density  
5. DISCUSSION  
5.2. Central Starburst vs. Galaxy-Wide Star Formation  
5.3. Structural Evolution of SMGs  
5.4. The Evolutionary Picture of SMGs  
5.4.1. Trigger Mechanism of SMGs  
5.4.2. The Connection Between SMGs and cQs  
6. SUMMARY