Fig. 10
Covariance matrix 
as a function of j, for i = 4 associated with the
distance bin
12.3 < r < 16.6 h-1 Mpc,
for the “2ℓ = 2” mutipole of the redshift-space correlation. 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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