1. INTRODUCTION

2. THE CARNEGIE-SPITZER-IMACS SURVEY
2.1. The limitations of optically-selected surveys
2.2. The potential of an IRAC-selected survey

3. DATA
3.1. Photometry
3.2. Aperture Photometry
3.3. Spectroscopy

4. SED FITTING
4.1. Ingredients
4.2. Fixing the Flux Calibration
4.3. Fitting for the Galaxy Components
4.4. Likelihood Analysis
4.5. Using M-estimators to Probe Data Quality
4.6. Defining Data Quality Flags
4.7. Success Rates and Completeness
4.8. Redshift Uncertainties

6. SUMMARY