1. INTRODUCTION  
3. DESIGN OF THE SURVEY  
3.2. Narrow-Band Filters  
3.3. Planned Survey Size and Location of Survey Fields  
4. PRELIMINARY RESULTS FROM THE PILOT STUDY  
4.1. Results from the Imaging Survey  
4.2. Results from the Spectroscopic Follow-Up Observations  
4.3. Properties of the SFACT Emission-Line Objects: A Preliminary View  
5. COMPARISON WITH PREVIOUS NARROWBAND SURVEYS  
6. APPLICATIONS OF THE SFACT SURVEY  
6.1. Evolution of the Star-Formation Rate Density to $z=1$ and Beyond  
6.2. Characterization of the Strong-Lined AGN Population  
6.3. Demographics of Dwarf Star-forming Galaxies to $z=0.5$  
6.4. Environments of Star-Forming Galaxies and AGNs  
6.5. Evolution of Galaxy Abundances to $z=0.9$  
6.6. Detection of Rare Objects  
7. STATUS AND FUTURE PLANS  
8. SUMMARY & CONCLUSIONS