1. Introduction, Motivation and History

2. Survey Goals and Observational Design
2.1. Passband Selection
2.2. Survey Requirements and Exposure Details
2.3. Photometric Calibration
2.4. Field Selection

3. Data Processing
3.1. Processing of MOSAIC2 images
3.2. Instrumental Photometry from MOSAIC2 Images
3.3. Processing of the 0.9m CFCCD images
3.4. Instrumental Photometry from CFCCD Images
3.5. Calibrated Photometry from the CFCCD Data
3.6. Transfer of Calibrated Magnitudes to the MOSAIC2 results

4. Color-Magnitude Diagrams of Fields along a northern extension from the LMC
4.1. Comparison with Isochrones
4.2. Identifying giants using the DDO 51 photometry

5. Analysis of Star Counts

6. Discussion
6.1. Further Characterization of the LMC Disk
6.2. Can there be an undetected LMC halo?
6.3. Summary