1 INTRODUCTION  
2 OBSERVATIONAL AND MODEL DATA USED  
2.1 Spitzer imaging and catalogues  
2.2 Redshift distributions from colour cuts  
2.3 Simulated data used  
3 METHODS  
3.1 Estimating correlation functions  
3.2 Spatial clustering  
4 RESULTS  
4.1 Estimates for all galaxies  
4.2 Estimates for colour selected subsamples  
4.3 Clustering predictions for the SHARK models  
4.4 Estimates for magnitude selected subsamples  
5 DISCUSSION AND CONCLUSIONS