1 INTRODUCTION

2 OBSERVATIONS
2.1 Infrared and Optical Observations
2.2 Radio Observations

3 SPECTRAL-ENERGY DISTRIBUTIONS
3.1 Photometric-Redshift Estimation
3.2 Stellar-Mass Estimation

4 DATA SELECTION
4.1 Galaxy Classification
4.2 Star-Galaxy Separation
4.3 Further Selection Considerations

5 STACKING

6 RESULTS
6.1 Calculating Specific Star-Formation Rates as a Function of Galaxy Type, Redshift and Stellar Mass

7 COMPARISON WITH SSFRS FROM OTHER ROUTES
7.1 SSFRs from Radio Stacking
7.2 Specific Star-Formation Rates for the Henriques et al. (2012) Semi-Analytic Model
7.3 Far-Infrared Star-Formation Rate Indicators
7.4 AGN Contamination

8 CONCLUSIONS