Table 1
Properties of the clusters.
| Name | RAJ2000 | DecJ2000 | z | LX (0.1−2.4 keV) | kpc /′′ | Morph. |
| hh mm ss | ° ′ ′′ | 1044 erg s-1 | status | |||
|
|
||||||
| A68 | 00 36 59.4 | +09 08 30 | 0.254 | 9.47 | 3.96 | M |
| Z1953(ZwCl0847.2+3617) | 08 50 10.1 | +36 05 09 | 0.373 | 23.463 | 5.15 | M |
| Z3146 (ZwCL1021.0+0426) | 10 23 39.6 | +04 11 10 | 0.290 | 17.26 | 4.35 | R |
| Z5247 (RXC J1234.2+0947) | 12 34 17.3 | +09 46 12 | 0.229 | 6.32 | 3.66 | M |
| A1722 | 13 19 43.0 | +70 06 17 | 0.327 | 10.78 | 4.72 | R |
| RX J2129.6+0005 | 21 29 37.9 | +00 05 39 | 0.235 | 11.66 | 3.73 | R |
| A2552 | 23 11 33.1 | +03 38 07 | 0.305 | 10.07 | 4.50 | R |
|
|
||||||
| RXC J1212.3−1816 | 12 12 18.9 | −18 16 43 | 0.269 | 6.20 | 4.12 | M4 |
| A2485 | 22 48 32.9 | −16 06 23 | 0.247 | 5.10 | 3.89 | R |
| RXC J1504.1-0248 | 15 04 07.7 | −02 48 18 | 0.2153 | 28.08 | 3.50 | R |
| RXC J0510.7-0801 | 05 10 44.7 | −08 01 06 | 0.2195 | 8.55 | 3.55 | M |
Notes. The clusters in the first sector belong to the EGRHS sample (K13) and those in the second belong to the GRHS sample. Columns are 1. Cluster name; 2. Right ascension; 3. Declination; 4. Redshift; 5. X-ray luminosity1 (0.1−2.4 keV) in units 1044 erg s-1 (Ebeling et al. 1998, 2000; Böhringer et al. 2004); 6. Linear scale in kpc /′′; 7. Morphological status (R = Relaxed and M = Merging)2.
Cassano et al. (2010) and Sect. 5.3.
Possibly contaminated by point sources (Crawford et al. 1999).
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