Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription

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Fig. 3

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Redshift distribution of the CFHTLenS galaxies for all patches. The histogram is the recovered redshift distribution obtained by averaging the individual and the solid line represents the best-fit using Eq. (44). The best-fit values of λ, β, and z₀ are used in Eq. (5) for W^g.

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