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Fig. 10.
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1 and 2σ constraints on (w0, wa) from tomographic Pseudo-Cℓ measurements of the full 3 × 2 pt signal in our noisy simulation. We show constraints measured for different numbers of equipopulated bins used for the tomographic analysis. The cross marks the fiducial cosmology (w0, wa) = (−1, 0) used for the simulation.
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