\begin{table}%t2 \caption{\label{clusters}Properties of the clusters in the sample: the~first 14~entries are LEC~clusters, while the remaining are non-LEC.} %\centering \par \begin{tabular}{c c c c c c c} \hline\hline \noalign{\smallskip} Name & Redshift & Temperature & $R_{180}$ & $\sigma$ & Core Cl. & Dyn.~ Cl. \\ & & (keV) & (Mpc) & & \\ \hline 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\tablefootmark{*} \\ 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\tablefootmark{*} \\ PKS0745-191 & 0.103 & $7.765 \pm 0.12$ & 2.11 & $0.2957 \pm 0.0056$& CC & NOM\tablefootmark{*} \\ 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 \\ \hline 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\tablefootmark{*}\\ A3667 & 0.056 & $ 5.461 \pm 0.029 $ & 1.81 & $ 0.6378 \pm 0.0078$& NCC & MRG\tablefootmark{*}\\ 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\tablefootmark{*} \\ A2256 & 0.057 & $ 5.709 \pm 0.0763 $ & 1.85 & $ 0.6300 \pm 0.0197$& NCC & MRG\tablefootmark{*}\\ \hline \end{tabular} \tablefoot {\tablefoottext{*}{Properties and the references for the clusters not included in the sample in Paper~I. A496: CC and no evidence for a major merger (\citealt{tamura01}, and references therein). A478: CC and no evidence for a major merger (\citealt{sanderson05}, and references therein). PKS0745-191: CC and no evidence for a major merger (\citealt{chen03}, and references therein). A3532: INT (moderate temperature drop) and no evidence for a major merger (the~indications of optical substructures, \citealt{bardelli00}, are insufficient to claim a major merger). A3667: NCC and MRG (evidence of radio relics \citealt{rott97}; optical substructures \citealt{owers09}; and disturbed thermodynamical maps \citealt{briel04, vikh01b}). A3266: NCC and MRG (even~if extended radio emission has not been detected, \citealt{buote01}, there are evidences of optical substructures; \citealt{quintana96}; and disturbed thermodynamical maps \citealt{finog06}). A2256: NCC and MRG (radio halo and relic, \citealt{kim99}, optical substructures; \citealt{berrington02}, and disturbed temperature maps; \citealt{sun02, bourdin08}).}} \end{table}