1. INTRODUCTION  
2. OBSERVATIONS AND DATA REDUCTION  
2.1. ALMA Data and the Sample  
2.2. Herschel/PACS  
2.3. Herschel/SPIRE  
2.4. Ancillary HST and Spitzer Data  
2.5. Redshift Catalogs  
3. HERSCHEL SOURCE EXTRACTION  
3.1. Preparation  
3.2. Iterative Herschel Photometry  
3.3. Non-detections  
3.4. Special Sources  
3.5. Statistics of Herschel Detections  
4. SED FITTING  
4.1. Methodology  
4.2. Validity of Far-IR Photometric Redshifts  
4.3. Herschel-Faint Galaxies  
5. LENS MODELING  
5.1. Models, Magnifications and Multiple Images  
5.2. Uncertainties  
6. DISCUSSION  
6.1. Far-IR Colors  
6.2. Redshift versus 1.15 mm Flux Density  
6.3. Statistics of Intrinsic (Source-Plane) Properties  
6.4. Dust Temperature versus IR Luminosity  
6.5. Gas Depletion Time Scale  
6.6. Dust Temperature of a [C II]-Emitter at $z=6.07$  
7. SUMMARY