Fig. 13
The covariance matrices 
(solid line) and Ci,j (dashed line) of the estimators 
and 
, for i = 4 associated with the distance bin 12.3 < r < 16.6 h-1 Mpc, as a function of j. We show the results obtained for halos in the redshift range 0 < z < 0.8 with an angular window of 50 deg2. Here we only consider the low-order terms given by Eqs. (67) and (69).
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