1 ABSTRACT

1 INTRODUCTION

2 FORTHCOMING RADIO SURVEYS  
2.1 LOFAR  
2.2 EMU  
2.3 WODAN  

3 SOURCE POPULATION MODELS  
3.1 Number densities  
3.2 Galaxy Bias  

4 COSMOLOGICAL PROBES  
4.1 The Auto-Correlation Function  
4.2 The Integrated Sachs-Wolfe Effect  
4.3 Magnification bias  

5 PREDICTIONS FOR MEASUREMENTS WITH FORTHCOMING SURVEYS  
5.1 Auto correlation predictions  
5.2 Cross-correlation predictions  
5.3 Magnification Bias  

6 COSMOLOGICAL MODEL CONSTRAINTS  
6.1 Dynamical Dark Energy  
6.2 Modified Gravity  
6.3 Observables and Fisher Matrices  

7 RESULTS

8 DISCUSSION AND CONCLUSIONS  
8.1 Implications for Survey Design  
8.2 Additional Measurements  
8.3 Conclusions