Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential - Effect of the redshift bin mismatch

Open Access

Fig. C.2.

Average cross-power spectrum between galaxy over-density and CMB convergence reconstructed from 300 simulations after adding photometric redshift errors (complementary to Fig. 4). The error bars are computed from the covariance matrix of simulations using Eq. (9).

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