Relative importance of the non-Gaussian contributions (solid line) and (dashed line) to the redshift-space covariance matrix , along the diagonal, i = j. We show the results obtained for halos in the redshift range 0 < z < 0.8 with an angular window of 50 deg². (The contribution for M > 10¹⁴   h^-1   M_⊙ does not appear because it is less than 10^-2.)