1 INTRODUCTION

2 OBSERVATIONAL DATA  
2.1 Observations  
2.2 Data Reduction  
2.3 Photometry  

3 CORRECTING STAR COUNT NUMBERS  
3.1 M32 Field Contamination  
3.2 Source Density Profiles  
3.3 Stellar Spatial Distribution  

4 RESULTS & DISCUSSION  
4.1 M32 Luminosity Functions  
4.2 IRAC Colour Distribution  
4.3 IRAC Colour-Magnitude Diagrams  
4.4 Mass-Loss Rates of the AGB Candidates  
4.5 Comparison to Davidge (2014)  

5 SUMMARY AND CONCLUSIONS