1. INTRODUCTION
2. OBSERVATIONS AND DATA REDUCTION
2.1. Data Reduction
2.2. Point Spread Functions
3. SOURCE DETECTION AND PHOTOMETRY
3.1. Source Detection
3.2. Band-merging
3.3. Photometry
3.4. Hardness Ratios
3.5. Sensitivity Maps
4. POINT SOURCE CATALOG
4.1. Flux Limit
4.2. Comparison with wavdetect
4.3. Comparison with N05 GWS Analysis
4.4. Astrometric Accuracy
4.5. False Source Contamination
4.6. Final AEGIS-X Catalog
5. OPTICAL AND IR IDENTIFICATIONS
5.1. Optical Identifications
5.2. IRAC Identifications
6. CONCLUSIONS