Table 3.
Parameters and results of a run time comparison similar to Table 1 but now for a sample with N = 1.36 million galaxies (XI) and a random subsample with N = 105 galaxies (X) in a cube with side length 325 Mpc h−1.
N | Nr (RR) | N2x3d | Nr (DR) | Nsh | TDD | TRR | TRR, 2x3d | TDR | TDR, shell | T(ξLS) |
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Ratio | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
X | 105 | 3 × 105 | 1.5 × 105 | 4 × 105 | 1 | 4 | 3 × 101 | 1 × 101 | 3 × 101 | 9 × 10−1 | 6 × 101 | 2 × 101 | 3 |
XI | All | 3 × 105 | 1.5 × 105 | 3 × 105 | 1 | 7 × 102 | 3 × 101 | 1 × 101 | 3 × 102 | 1 × 101 | 1 × 103 | 7 × 102 | 1.4 |
Notes. We use the radius interval [2, 3] Mpc h−1 and the targeted accuracy is Δ = 10−2. The run times for DD and so on are given in seconds.
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