Table 2.
ζ metric in km s−1.
| Cluster | CLONE/CF2 | CLONE/CF3 | Random/CF3 | ||
|---|---|---|---|---|---|
| Cylinder | 10 | 2.5 | 10 | 2.5 | 2.5 |
| radius | Mpc | Mpc | Mpc | Mpc | Mpc |
| Virgo | 163 | 304 | 157 | 304 | 11 200 |
| Centaurus | 173 | 348 | 171 | 343 | 11 221 |
| Abell 569 | 294 | 1998 | 155 | 1392 | 7272 |
| Coma | 275 | 722 | 485 | 820 | 6276 |
| Abell 85 | 386 | 727 | 718 | 1082 | 2392 |
| Abell 2256 | 1453 | 1454 | 1491 | 1491 | 2882 |
| PGC 765572 | 1137 | 1137 | 1066 | 1067 | 2447 |
| PGC 999654 | 747 | 747 | 685 | 685 | 2769 |
| PGC 340526 | 875 | 907 | 704 | 736 | 1728 |
| PGC 46604 | 1341 | 1341 | 1341 | 1341 | 2800 |
Notes. It measures the difference between the simulated and observed lines of sight. The higher ζ is, the more different the lines of sight are. The last column gives the average ζ value when comparing 1100 random simulated lines of sight and the observed ones. The random lines of sight were selected to contain at least one halo more massive than 1014 M⊙; see the text for a detailed explanation.
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