Fig. 9
Covariance matrix 
along the diagonal, i = j, 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. Points from numerical simulations are
obtained from 138 fields separated by a 10 degree gap (squares) or from 34 fields
separated by 20 degree gap (crosses).
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