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Table 2:

Properties of the clusters in the sample: the first 14 entries are LEC clusters, while the remaining are non-LEC.

Name 		Redshift Temperature R180 $\sigma $ Core Cl. Dyn.  Cl.
    (keV) (Mpc)      
A2199 0.0301 $4.101 \pm 0.025$ 1.58 $ 0.4216 \pm 0.0033 $ CC NOM
A496 0.0329 $4.990 \pm 0.038$ 1.75 $ 0.3109 \pm 0.0028$ CC NOM*
2A0335+096 0.035 $3.649 \pm 0.009$ 1.49 $ 0.2644 \pm 0.0007 $ CC NOM
A2052 0.035 $2.884 \pm 0.014$ 1.33 $0.4274 \pm 0.0028$ CC NOM
A4059 0.047 $3.968 \pm 0.028$ 1.55 $0.4394 \pm 0.0044$ CC NOM
Hydra A 0.054 $3.413 \pm 0.024 $ 1.43 $0.4138 \pm 0.0040 $ CC NOM
A85 0.055 $5.491 \pm 0.048$ 1.82 $0.3857 \pm 0.0050$ CC MRG
A1795 0.062 $5.416 \pm 0.026$ 1.80 $0.3524 \pm 0.0023$ CC NOM
A3112 0.075 $ 4.319 \pm 0.033$ 1.59 $0.3855 \pm 0.0038$ CC NOM
A2597 0.085 $ 3.491 \pm 0.018 $ 1.43 $ 0.3568 \pm 0.0026$ CC NOM
A478 0.088 $7.057 \pm 0.034$ 2.03 $0.3706 \pm 0.0024$ CC NOM*
PKS0745-191 0.103 $7.765 \pm 0.12$ 2.11 $0.2957 \pm 0.0056$ CC NOM*
A2204 0.152 $7.412 \pm 0.092$ 2.01 $0.2972 \pm 0.0046$ CC NOM
A2029 0.077 $ 6.173 \pm 0.056$ 1.90 $0.4505 \pm 0.0057$ CC NOM
A4038 0.030 $2.957 \pm 0.015$ 1.35 $0.5093 \pm 0.0037$ INT NOM
A576 0.039 $3.777 \pm 0.044 $ 1.52 $0.6226 \pm 0.0135 $ INT MRG
A3571 0.039 $6.253 \pm 0.045 $ 1.95 $0.6220 \pm 0.0078$ INT NOM
A119 0.044 $6.032 \pm 0.082$ 1.92 $0.7621 \pm 0.0279$ NCC MRG
MKW3s 0.045 $3.325 \pm 0.018$ 1.42 $0.4860 \pm 0.0039$ CC NOM
A1644 0.047 $4.156 \pm 0.056 $ 1.59 $0.5318 \pm 0.0132 $ INT NOM
A3558 0.048 $5.221 \pm 0.025$ 1.78 $0.6155 \pm 0.0057$ INT NOM
A3562 0.048 $4.344 \pm 0.032$ 1.62 $0.6089 \pm 0.0083$ NCC MRG
Triangulum Australis 0.051 $9.224 \pm 0.095$ 2.36 $0.6845 \pm 0.0164$ NCC NOM
A3158 0.060 $4.903 \pm 0.042 $ 1.71 $0.7488 \pm 0.0153$ NCC MRG
A399 0.072 $5.984 \pm 0.109$ 1.88 $0.7086 \pm 0.0319$ NCC MRG
A401 0.074 $ 7.268 \pm 0.084$ 2.07 $ 0.7028 \pm 0.0212$ NCC MRG
A2255 0.081 $ 6.197 \pm 0.154 $ 1.91 $ 0.8853 \pm 0.0714 $ NCC MRG
A1650 0.084 $ 5.427 \pm 0.0539 $ 1.78 $0.5323 \pm 0.0089$ INT NOM
A1689 0.183 $ 8.612 \pm 0.102 $ 2.13 $0.4724 \pm 0.0089$ INT NOM
A2319 0.056 $8.962 \pm 0.091 $ 2.32 $ 0.5643 \pm 0.0113$ NCC MRG
A3532 0.055 $ 4.839 \pm 0.104 $ 1.70 $0.7285 \pm 0.0336$ INT NOM*
A3667 0.056 $ 5.461 \pm 0.029 $ 1.81 $ 0.6378 \pm 0.0078$ NCC MRG*
A754 0.054 $ 8.544 \pm 0.102 $ 2.27 $ 0.5289 \pm 0.0120$ NCC MRG
A3266 0.055 $ 7.351 \pm 0.081 $ 2.10 $ 0.6772 \pm 0.0170$ NCC MRG*
A2256 0.057 $ 5.709 \pm 0.0763 $ 1.85 $ 0.6300 \pm 0.0197$ NCC MRG*

Notes. (*) Properties and the references for the clusters not included in the sample in Paper I. A496: CC and no evidence for a major merger (Tamura et al. 2001, and references therein). A478: CC and no evidence for a major merger (Sanderson et al. 2005, and references therein). PKS0745-191: CC and no evidence for a major merger (Chen et al. 2003, and references therein). A3532: INT (moderate temperature drop) and no evidence for a major merger (the indications of optical substructures, Bardelli et al. 2000, are insufficient to claim a major merger). A3667: NCC and MRG (evidence of radio relics Rottgering et al. 1997; optical substructures Owers et al. 2009; and disturbed thermodynamical maps Briel et al. 2004; Vikhlinin et al. 2001). A3266: NCC and MRG (even if extended radio emission has not been detected, Buote 2001, there are evidences of optical substructures; Quintana et al. 1996; and disturbed thermodynamical maps Finoguenov et al. 2006). A2256: NCC and MRG (radio halo and relic, Kim 1999, optical substructures; Berrington et al. 2002, and disturbed temperature maps; Bourdin & Mazzotta 2008; Sun et al. 2002).


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