I. INTRODUCTION

II. THE WIGGLEZ DARK ENERGY SURVEY
A. Data
B. The GiggleZ simulation

III. TAKING FIDUCIAL MODEL AND WINDOW FUNCTION INTO ACCOUNT

IV. MODELLING THE GALAXY POWER SPECTRUM
A. Seven approaches to modelling P(k)
B. Bias
C. A comparison of the approaches
D. Systematics
E. WiggleZ power spectrum fit

V. COSMOLOGICAL CONSTRAINTS
A. Cosmological Models
B. Parameters and the physics being constrained
C. Analysis method
D. Results
E. Comparison of all models

VI. CONCLUSIONS