Table 1
Optical properties of all clusters studied.
| Cluster | Alt. name | RA | Dec | z | Δz | Ngals | Observing mode |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|
|||||||
| RXCJ0052.4-5746 | 13.1093 | –57.7806 | 0.2559 | 2.37 | 3 | MOS | |
| RXCJ0129.4-6432 | 22.3730 | –64.5409 | 0.3264 | 1.98 | 6 | MOS | |
| RXCJ0139.5-2629 | 24.8888 | –26.4886 | 0.2445 | 1.56 | 4 B | LS | |
| RXCJ0343.5-7152 | 55.8775 | –71.8764 | 0.2136 | 1.61 | 3 | MOS | |
| RXCJ0347.4-2149 | A3168 | 56.8724 | –21.8224 | 0.2399 | 1.77 | 5 | MOS |
| RXCJ0425.5-0045 | ZwCl0423.2-0053 | 66.3798 | –0.7577 | 0.2240 | 1.75 | 6 | MOS |
| RXCJ0521.4-2754 | 80.3581 | –27.9065 | 0.3175 | 2.79 | 2 B | LS | |
| RXCJ1253.8-2622 | A1633 | 193.4682 | –26.3828 | 0.2179 | 1.65 | 9 B | MOS |
| RXCJ1617.6-0714 | 244.4099 | –7.2446 | 0.2523 | 2.36 | 3 B | MOS | |
| RXCJ1914.5-5928 | PLCKG337.1-26.0 | 288.6333 | –59.4767 | 0.2636 | 1.74 | 4 | MOS |
| RXCJ2006.4-1912 | 301.6046 | –19.2106 | 0.2769 | 1.83 | 4 | MOS | |
| RXCJ2041.2-1324 | 310.3188 | –13.4149 | 0.3311 | 2.11 | 5 B | MOS | |
| RXCJ2049.9-3029 | A3715 | 312.4885 | –30.4926 | 0.2088 | 1.55 | 3 | MOS |
| RXCJ2126.1-3202 | AS0946 | 321.5441 | –32.0338 | 0.2797 | 1.66 | 2 B | MOS |
| RXCJ2149.0-3228 | 327.2524 | –32.4744 | 0.2326 | 1.94 | 4 | MOS | |
| RXCJ2149.9-1859 | 327.4500 | –19.0050 | 0.2836 | 3.64 | 2 B | LS | |
| RXCJ2308.3-0155 | 347.0873 | –1.9210 | 0.3047 | 2.07 | 4 | MOS | |
| RXCJ2317.9-3534 | A3989 | 349.4828 | –35.5794 | 0.2041 | 2.04 | 3 | MOS |
| RXCJ2351.0-1954 | 357.7703 | –19.9132 | 0.2477 | 1.90 | 2 | MOS | |
|
|
|||||||
| RXCJ1013.1-1641 | 153.2794 | –16.6884 | 0.2240 | 2.00 | 3 | LS | |
| RXCJ1023.2-0636 | A1001 | 155.8268 | –6.6046 | 0.2544 | 1.06 | 3 | LS |
| RXCJ1355.6-2623 | A1816 | 208.9334 | –26.3833 | 0.2035 | 1.43 | 5 | MOS |
Notes. (1) RA and Dec for J2000 in degrees. (2) The centre of RXCJ1914.5-5928 is 4.3 arcmin away from that of PLCKG337.1-26.0. There are three different redshifts associated with this Planck cluster (Planck collaboration 2011a, 2011b). We take the redshift of the component with the largest contribution to the Fe line at 0.26 in the Table 2 of Planck Collaboration (2011b). (6) Errors in units of 10-4 (7) Number of galaxies with concurrent redshifts, B indicates when the BCG redshift is available. LS marks the redshift obtained from a single long-slit observation. The last three entries are based on the observation in March 2004 with the EFOSC2 instrument, which forms part of the REFLEX III supplementary catalogue.
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