1 INTRODUCTION

2 SURVEY OBSERVATIONS AND DATA PROCESSING  
2.1 VPHAS+ specification  
2.2 VPHAS+ observations  
2.3 Data pipeline  
2.4 Limiting magnitudes and errors  

3 THE NARROWBAND Hα FILTER  
3.1 Overview  

4 SIMULATION OF VPHAS+ STELLAR COLOURS  

5 PHOTOMETRY VALIDATION: A COMPARISON OF SDSS AND VST DATA  

6 AN EXAMPLE OF POINT-SOURCE PHOTOMETRY DERIVED FROM A VPHAS+ FIELD  

7 NEBULAR ASTROPHYSICS WITH VPHAS+ IMAGES  

8 VPHAS+ PHOTOMETRY AS A REFERENCE SET FOR VARIABILITY STUDIES  

9 SUMMARY AND CONCLUDING REMARKS