1. INTRODUCTION  
2. DATA  
2.1. Sample Properties  
2.2. ALMA Observations  
2.3. NOEMA Observations  
3. RESULTS  
3.1. Continuum Emission  
3.2. Line Emission and Absorption  
3.3. Position Offsets  
4. ANALYSIS AND DISCUSSION  
4.1. Spectral Energy Distribution Modeling  
4.2. Scaling Relations  
5. CONCLUSIONS