1. Introduction
2. Survey design
2.1. Sample selection
2.2. Catalog completeness
3. Observations and data reduction
3.1. Observations
3.2. Parallel data reduction at the SURFsara Data Processing Facility
3.3. Flux extraction
4. Results
4.1. Disk luminosities and masses
4.2. Disk mass distribution in SODA
4.3. Comparison to literature results
4.4. The most massive disks in Orion A
5. Discussion
5.1. Impact of age gradients
5.2. Disk masses: SODA and other star-forming regions
6. Conclusions