1. INTRODUCTION  
2. OBSERVATIONS AND MEASUREMENTS  
2.1. The AURORA Survey  
2.2. Data Reduction  
2.3. Slit Loss Correction  
2.4. Flux Calibration  
2.5. Photometric Catalogs and SED Fitting  
2.6. Emission Line Measurements  
3. RESULTS  
4. DISCUSSION  
5. SUMMARY AND CONCLUSIONS