Contour plots for the redshift-space correlation matrices , defined as in Eq. (41). There are ten distance bins, over 5 < r < 100   h^-1 Mpc, equally spaced in log    (r), as in previous figures. We considered halos in the redshift range 0 < z < 0.8, within an angular window of 50 deg², above the mass thresholds M > 2 × 10¹³   h^-1   M_⊙ in the upper row, and M > 10¹⁴   h^-1   M_⊙ in the lower row. Left panels: correlation matrix associated with the Gaussian part (34) of the covariance matrix. Right panels: full correlation matrix, associated with the full matrix (33).