1 INTRODUCTION

2 OBSERVATIONS

3 DATA REDUCTION  
3.1 Chandra data reduction with CIAO

4 SIMULATED DATA AND OPTIMIZED POINT SOURCE DETECTION  
4.1 Creating the simulated data  
4.2 Source Detection Algorithm  
4.3 Characterizing the Quality of the Source Detection Algorithm  

5 REAL DATA PRODUCTS  
5.1 Astrometric Correction of the Individual Observations  
5.2 Main Source Catalog  
5.3 Sensitivity Maps  
5.4 Flux Upper Limit Maps in Overlapped Mosaics  
5.5 Low Likelihood Source Catalog

6 DISCUSSION  
6.1 log N – log S  
6.2 NH Column Densities from Hardness Ratios  
6.3 Cross-identification between X-ray and Optical Regime  
6.4 Cross-identification between X-ray and Infrared Regimes

7 SUMMARY