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Fig. 11.

Fig. 11. Refer to the following caption and surrounding text.

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Contour areas enclosed by the 1 and 2σ constraints on the dark energy (w0, wa) parameters, measured for the full 3 × 2 pt signal in the presence of Gaussian shape noise and photo-z uncertainty. We vary the number of redshift bins used for each of the equipopulated, equally spaced in fiducial comoving distance, and equal redshift width binning strategies.

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