1. INTRODUCTION

2. OBSERVATIONS
2.1. The ALMA dataset
2.2. Ancillary Data

3. THE SAMPLE

4. CO-BASED MEASUREMENTS
4.1. CO luminosities and associated H₂ masses
4.2. Size of the CO-emitting region in ID.2
4.3. CO excitation

5. DISCUSSION
5.1. Location in the galaxy 'main sequence' plot
5.2. Star formation law
5.4. Gas to stellar mass ratios
5.5. CO vs. Dust-based ISM masses

6. SUMMARY