1 INTRODUCTION
2 WIGGLEZ DARK ENERGY SURVEY DESIGN AND ANALYSIS METHODS
2.1 Survey fields
2.2 Photometry
2.3 Galaxy Selection
2.4 Spectroscopy
2.5 Redshift Reliability and Distribution
2.6 Stellar mass estimates
2.7 Stacked spectra and spectral line fitting
2.8 Active galactic nuclei in stacked spectra
2.9 Direct method metallicity and star formation rate estimation
3 RESULTS: PROPERTIES OF WIGGLEZ GALAXIES
3.1 Two-component Emission Lines
3.2 Mass Metallicity Relation
4 DISCUSSION
4.1 Resolving the [OII] doublet.
4.2 Active galaxies in the WiggleZ sample
4.3 The metallicity of high-mass star forming galaxies
5 FINAL PUBLIC DATA RELEASE
5.1 Tabular Data
5.2 Spectral Data
5.3 WiggleZ Data Access
6 SUMMARY