We present results from the 2D anisotropic Baryon Acoustic Oscillation ( BAO ) signal present in the final dataset from the WiggleZ Dark Energy Survey .
We analyse the WiggleZ data in two ways : firstly using the full shape of the 2D correlation function and secondly focussing only on the position of the BAO peak in the reconstructed data set .
When fitting for the full shape of the 2D correlation function we use a multipole expansion to compare with theory .
When we use the reconstructed data we marginalise over the shape and just measure the position of the BAO peak , analysing the data in wedges separating the signal along the line of sight from that parallel to the line of sight .

We verify our method with mock data and find the results to be free of bias or systematic offsets .
We also redo the pre-reconstruction angle averaged ( 1D ) WiggleZ BAO analysis with an improved covariance and present an updated result .
The final results are presented in the form of \Omega _ { c } h ^ { 2 } , H ( z ) , and D _ { A } ( z ) for three redshift bins with effective redshifts z = 0.44 , 0.60 , and 0.73 .
Within these bins and methodologies , we recover constraints between 5 % and 22 % error .
Our cosmological constraints are consistent with Flat \Lambda CDM cosmology and agree with results from the Baryon Oscillation Spectroscopic Survey ( BOSS ) .