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Table 3.
Bulk flow of galaxies with more than 100 particles.
| Run # | Galaxies | Bulk flow | z0 | Ωm′ |
|---|---|---|---|---|
| vx | vy | vz | ||
| 111 | 260 | 7472 | 33 000 | |
| –1466 | 6154 | –3976 | 98%* | |
| ± | 174 | 543 | 325 | 3 × 10−6 |
| 112 | 487 | 5872 | 30 000 | |
| –2707 | 4137 | 3168 | 98%* | |
| ± | 370 | 300 | 219 | 0 |
| 113† | 107 | 1073 | 10 000 | |
| 78 | 993 | 400 | 98%* | |
| ± | 270 | 280 | 256 | 5 × 10−5 |
| 114 | 404 | 758 | 10 000 | |
| 527 | –353 | –415 | 98%* | |
| ± | 115 | 111 | 65 | 0 |
| 115 | 193 | 1124 | 500 | |
| 443 | –620 | 827 | ||
| ± | 399 | 300 | 489 | 0 |
Notes. *98% signifies a < 2% probability that the 3D bulk flow was nonzero by chance. z0 is the initial redshift. †Mass-loss method (2).
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