Fig. 7.

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MCMC results for the top-hat and adapted filter using the model and the T17 simulations as our data vector and a covariance matrix calculated from ten T17 realisations each divided into 48 sub-patches. For the adapted filter a systematic bias for σ8 and Ωm is found, although it cancels out for the parameter. The contours here are marginalised over the lens galaxy bias parameters.
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