1. Introduction

2. Survey Motivation

3. Observation Strategy
3.1. Pointing Grid
3.2. Resolution
3.3. 74 MHz Specific Considerations
3.4. Time per Pointing
3.5. Re-Observations

4. Data Reduction Method
4.1. Calibration
4.2. RFI Excision
4.3. Producing Images

5. Survey Assessment
5.1. Sky Area Imaged
5.2. Sensitivity Achieved
5.3. Image Quality

6. Extracting the Catalog
6.1. Source Finding
6.2. False Detections
6.3. Derived Parameters

7. Derivation of Source Parameters and Their Accuracy
7.1. Source Positions
7.2. Source Sizes
7.3. Flux Densities

8. Completeness of the Catalog

9. Accessing the Data

10. Conclusion and Future Work