1 INTRODUCTION

2 THEORETICAL MODELLING OF THE ANGULAR POWER SPECTRA
2.1 Angular power spectra of biased tracers
2.2 Accounting for shot noise
2.3 Sub- and super-Poissonian shot noise
2.4 Accounting for sub- and super-Poissonian shot noise
2.5 Theory predictions for effective bias

3 DATA
3.1 Galaxy and cluster catalogues
3.2 Pixellated maps and survey mask
3.3 Subsets of data used

4 ANGULAR POWER SPECTRUM ESTIMATORS

5 RESULTS
5.1 Fitting the angular power spectra with a fixed shot noise contribution
5.2 Accounting for the effective noise contribution
5.3 Effective bias for volume-limited cluster sample
5.4 Results for low and high richness cluster samples

6 SUMMARY AND OUTLOOK