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Fig. 8.

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Errors for estimates of the correlation function at r ∈ [2, 3] Mpc h−1 from 1.36 million galaxies and a subsample of 100 k galaxies in a box with side-length 325 Mpc h−1. Upper plot: absolute error Δ1 shown for the standard RR (solid lines) and for RR2x3d (dashed lines) pair-counts. Lower plot: absolute error Δ2 is shown for the standard DR (solid lines), the DR using a low-discrepancy sequence (dotted lines), and for DRshell also using a low-discrepancy sequence (dashed lines). The black dotted lines are proportional to (upper) and 1/N2x3d (lower).

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