Open Access
Table 2.
Sample of galaxy clusters with redshift (first column) and diameter angular distances (second column), taken from De Filippis et al. (2005).
| z | D(z) |
|---|---|
| (Mpc) | |
| 0.023 | 103 ± 42 |
| 0.058 | 242 ± 61 |
| 0.072 | 165 ± 45 |
| 0.074 | 369 ± 62 |
| 0.084 | 749 ± 385 |
| 0.088 | 448 ± 185 |
| 0.091 | 335 ± 70 |
| 0.142 | 478 ± 126 |
| 0.176 | 809 ± 263 |
| 0.182 | 451 ± 189 |
| 0.183 | 604 ± 84 |
| 0.202 | 387 ± 141 |
| 0.202 | 806 ± 163 |
| 0.217 | 1465 ± 407 |
| 0.224 | 1118 ± 283 |
| 0.252 | 946 ± 131 |
| 0.282 | 1099 ± 308 |
| 0.288 | 934 ± 331 |
| 0.322 | 885 ± 207 |
| 0.327 | 697 ± 183 |
| 0.375 | 1231 ± 441 |
| 0.451 | 1166 ± 262 |
| 0.541 | 1635 ± 391 |
| 0.550 | 1073 ± 238 |
| 0.784 | 2479 ± 1023 |
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