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Fig. 7

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Predicted signal-to-noise ratio of the relative band powers fmn for different redshift bins (see key for line styles in the top panel). Minimum variance estimators and Bayesian analysis give comparable results except for the matter band power fδ,mn (top panel), which here combines constraints from lensing and galaxy clustering with priors b ≤ 4 and  | r |  ≤ 2 in the Bayesian approach. The bottom panels shows the signal-to-noise of the minimum variance estimates.

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