deletions | additions       diff --git a/reconstructed_wedges.tex b/reconstructed_wedges.tex  index 0f79b0b..402881a 100644  --- a/reconstructed_wedges.tex  +++ b/reconstructed_wedges.tex 
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Here we apply the techhnique of reconstruction of the baroynic acoustic feature (cite Eisenstein) on the WiggleZ data, present the results in the form of clustering wedges, and describe constraints on $H$ and $D_{\rm A}$. We test our methodology and compare our results with results of application on the WiZCOLA mocks.   In \cite{Kazin14} \cite{Kazin_2014} we reported application of the reconstruction of the density field technique as presented by (cite Eisenstein). We succesfully shown that ...  Here we examine implications of the technique on the anistorpic baryonic signature. Figure (currently experienceing referencing problems ...) displays our results for the $\xi$ in the range $0.6