Fig. 4

Redshift-space (solid line, for 2ℓ = 0) and real-space (dashed
line) covariance matrices,
and Ci,j, as a function of
j, for i = 4 associated with the distance bin
12.3 < r < 16.6 h-1 Mpc.
We show the results obtained for halos in the redshift range
0 < z < 0.8
with an angular window of 50 deg2.
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