  We describe the `WiggleZ' spectroscopic survey of 280,000 star-forming
galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2
optical imaging. The fundamental goal is a detection of the baryonic acoustic
oscillations in galaxy clustering at high-redshift (0.5 < z < 1) and a precise
measurement of the equation of state of dark energy from this purely geometric
and robust method. The survey has already started on the 3.9m Anglo-Australian
Telescope using the AAOmega spectrograph, and planned to complete during 2009.
The WWW page for the survey can be found at
http://astronomy.swin.edu.au/wigglez
