1. Introduction

2. Sample, Observations & Data Reduction
2.1. Sample Selection
2.2. SMA & APEX Observations
2.3. Joint Imaging of Data
2.4. Dust Observations with Herschel

3. Narrow Lines & Linewidth–Size Relation

4. Suppression of CMZ Star Formation
4.1. Observations of Star Formation in CMZ Clouds
4.2. Estimates of the Star Formation Rate
4.3. SF Suppression in CMZ Clouds

5. Discussion
5.2. SF is Suppressed in Individual Clouds
5.3. Young Cloud Ages Unlikely to Explain Suppressed SF

6. Summary