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Fig. 8


Signal-to-noise ratio per band of the reconstructed matter power spectrum fδ,mn in a Bayesian analysis, either for an analysis of the shear tomography alone (“independent”), or when combining galaxy clustering, lensing with priors b ≤ 4,  | r |  ≤ 2 (“combined”). Plotted are the three first redshift bins (top to bottom line).

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