1. INTRODUCTION

2. METHOD
2.1. Chandra Observations
2.2. ChIcAGO Multi-wavelength Analysis Pipeline (MAP)
2.3. ChIcAGO Sources Spectral Investigation
2.4. Multi-wavelength Follow-up Observations

3. RESULTS
3.1. Chandra Results
3.2. Quantile Analysis and Spectral Modeling Results
3.3. Infrared and Optical Counterparts
3.4. Radio Counterparts

4. DISCUSSION
4.2. Unidentified ChIcAGO Sources with Infrared Counterparts
4.3. Further Discussion of Interesting ChIcAGO and AGPS Sources
4.4. ChIcAGO Sources Identified with SIMBAD
4.5. Confirmed and Tentative Identifications of the AGPS Sources

5. CONCLUSIONS