Table 3
Spectroscopic redshift for 12 clusters in the redshift range z = 0 − 0.4.
| ID |
|
|
zphoto |
|
|
|
|
|||||
| 70 | 0.152 | 0.152 | 0.17 ± 0.03 | 0.12 | |
| 94 | 0.269 | 0.29 ± 0.04 | |||
| 127 | 0.207 | 0.209 | 0.22 ± 0.02 | ||
| 139 | 0.169 | 0.18 ± 0.01 | |||
| 150 | 0.176 | 0.173 | 0.20 ± 0.02 | 0.14 | |
| 152 | 0.139 | 0.17 ± 0.02 | |||
| 227 | 0.346 | 0.35 ± 0.04 | |||
| 430 | 0.206 | 0.205 | 0.18 ± 0.01 | ||
| 457 | 0.1 | 0.10 ± 0.01 | |||
| 476 | 0.102 | 0.10 ± 0.01 | 0.1 | ||
| 511 | 0.269 | 0.26 ± 0.02 | 0.2 | ||
| 547 | 0.241 | 0.22 ± 0.02 | 0.18 | ||
Notes. The redshifts were obtained from long-slit spectroscopic observations at the NTT telescope. The redshifts of the BCG galaxies are in the column. Four clusters have a redshift for one additional member galaxy (). Photometric redshifts zphoto are taken from Table 2. For five systems we also provide the photometric redshifts from the SCS survey (M09, M10).
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