\begin{table}%t1 \caption {\label{tab1}Radio and X-ray properties of clusters used in this paper.} %\centerline {\begin{tabular}{llllllllllll} \hline \hline Cluster's & $z$ & $L_{\rm X}$ & $L_{\rm bol}$ & $P_{1.4}$ & Ref. \\ name & & [$10^{44}$ erg/s ]& [$10^{44}$ erg/s ]& [$10^{24}$ Watt/Hz] & \\ \hline 1E50657-558 & 0.2994 & $23.03\pm 1.81$ & $87.10\pm 6.82$ & $28.21\pm 1.97$ & 1, 7 \\ {\bf A2163} & 0.2030 & $23.17\pm 1.48$ & $86.50\pm 5.52$ & $18.44\pm 0.24$ & 1, 8 \\ {\bf A2744} & 0.3080 & $12.92\pm 2.41$ & $36.81\pm 6.88$ & $17.16\pm 1.71$ & 1, 9 \\ {\bf A2219} & 0.2280 & $12.73\pm 1.37$ & $38.55\pm 4.05$ & $12.23\pm 0.59$ & 2, 10 \\ CL0016+16 & 0.5545 & $18.83\pm 1.88$ & $55.59\pm 5.56$ & ~$\:6.74\pm 0.67$ & 4, 11\\ A1914 & 0.1712 & $10.71\pm 1.02$ & $34.51\pm 3.28$ & ~$\:5.21\pm 0.24$ & 3, 10 \\ A665 & 0.1816 & ~$\:9.84\pm 1.54$ & $27.61\pm 4.32$ & ~$\:3.98\pm 0.39$ & 2, 11 \\ A520 & 0.2010 & ~$\:8.83\pm 1.99$ & $23.77\pm 5.34$ & ~$\:3.91\pm 0.39$ & 2, 10 \\ {\bf A521} & 0.2475 & ~$\:8.18\pm 1.36$ & $19.63\pm 3.26$ & ~$\:1.16\pm 0.11$ & 1, 12 \\ A2254 & 0.1780 & ~$\:4.32\pm 0.92$ & $11.35\pm 2.43$ & ~$\:2.94\pm 0.29$ & 3, 10 \\ A2256 & 0.0581 & ~$\:3.81\pm 0.17$ & ~$\:9.54\pm 0.43$& ~$\:0.68\pm 0.12$ & 3, 13, 14 \\ {\bf A773} & 0.2170 & ~$\:8.10\pm 1.35$ & $22.70\pm 3.78$ & ~$\:1.73\pm 0.17$ & 2, 9 \\ A545 & 0.1530 & ~$\:5.66\pm 0.49$ & $12.50\pm 1.09$ & ~$\:1.48\pm 0.06$ & 1, 10 \\ A2319 & 0.0559 & ~$\:7.40\pm 0.40$ & $21.42\pm 1.16$ & ~$\:1.12\pm 0.11$ & 3, 15 \\ {\bf A1300} & 0.3071 & $13.96\pm 2.05$ & $41.97\pm 6.17$ & ~$\:6.09\pm 0.61$ & 1, 15 \\ A1656 (Coma) & 0.0231 & ~$\:3.77\pm 0.10$ & $10.44\pm 0.28$ & ~$\:0.72^{+0.07}_{-0.04}$ & 3, 16, 17 \\ A2255 & 0.0808 & ~$\:2.65\pm 0.12$ & ~$\:6.61\pm 0.30$& ~$\:0.89\pm 0.05$ & 3, 18 \\ A754 & 0.0535 & ~$\:4.31\pm 0.33$ & $12.94\pm 0.99$ & ~$\:1.08\pm 0.06$ & 3, 10 \\ {\bf A209} & 0.2060 & ~$\:6.29\pm 0.65$ & $16.26\pm1.69$ & ~$\:1.19\pm 0.26$ & 1, 19* \\ {\bf RXJ2003}& 0.3171 & ~$\:9.25\pm 1.53$ & $27.23\pm4.95$ & $12.30\pm 0.71$ & 1, 20 \\ MACS J0717 & 0.5548 & $24.6\pm 0.3$ & $84.18\pm1.01$ & $50.0\pm 10.0$ & 5, 21, 22 \\ {\bf A2390} & 0.228 & $13.49\pm 3.16$ & & ~$\:9.77 \pm 0.45$ & 2, 10 \\ {\bf Z7160} & 0.258 & ~$\:8.51\pm 2.12$ & & ~$\:2.19 \pm 0.26$ & 2, 23 \\ {\bf RXJ1314}& 0.2439 & $10.96 \pm 1.81$ & & ~$\:0.75 \pm 0.15$ & 1, 19*, 24* \\ {\bf A2697} & 0.2320 & ~$\:6.88 \pm 0.85$ & & $<$0.40 & 1, 25 \\ {\bf A141} & 0.2300 & ~$\:5.76 \pm 0.90$ & & $<$0.36 & 1, 25 \\ {\bf A3088} & 0.2537 & ~$\:6.95 \pm 1.20$ & & $<$0.42 & 1, 25 \\ {\bf RXJ1115.8} & 0.3499 & $13.58\pm 2.99$ & & $<$0.45 & 1, 25 \\ {\bf S780} & 0.2357 & $15.53\pm 2.80$ & & $<$0.36 & 1, 25 \\ {\bf RXJ1512.2} & 0.3152 & $10.19\pm 1.76$ & & $<$0.63 & 1, 25 \\ {\bf A2537} & 0.2966 & $10.17\pm 1.45$ & & $<$0.50 & 1, 25 \\ {\bf A2631} & 0.2779 & ~$\:7.57 \pm 1.50$ & & $<$0.39 & 1, 25 \\ {\bf A2667} & 0.2264 & $13.65\pm 1.38$ & & $<$0.42 & 1, 25 \\ {\bf RXJ0027.6} & 0.3649 & $12.29\pm 3.88$ & & $<$0.68 & 6, 25 \\ {\bf A611} & 0.2880 & ~$\:8.86 \pm 2.53$ & & $<$0.40 & 6, 25 \\ {\bf A781} & 0.2984 & $11.29\pm 2.82$ & & $<$0.36 & 2, 25 \\ {\bf Z2089} & 0.2347 & ~$\:6.79 \pm 1.76$ & & $<$0.27 & 2, 25 \\ {\bf Z2701} & 0.2140 & ~$\:6.59 \pm 1.15$ & & $<$0.42 & 2, 25 \\ {\bf A1423} & 0.2130 & ~$\:6.19 \pm 1.34$ & & $<$0.41 & 2, 25 \\ {\bf Z5699} & 0.3063 & ~$\:8.96 \pm 2.24$ & & $<$0.54 & 6, 25 \\ {\bf Z5768} & 0.2660 & ~$\:7.47 \pm 1.66$ & & $<$0.36 & 6, 25 \\ {\bf Z7215} & 0.2897 & ~$\:7.34 \pm 1.91$ & & $<$0.55 & 6, 25 \\ {\bf RXJ1532.9} & 0.3450 & $16.49\pm 4.50$ & & $<$0.62 & 2, 25 \\ {\bf RXJ2228.6} & 0.4177 & $19.44\pm 5.55$ & & $<$0.91 & 6, 25 \\ \hline \end{tabular}} \par \smallskip Giant radio halos (first sector), mini-halos in cool core clusters (second sector), small scale halos (tirdth sector), clusters with no Mpc-scale radio emission (last sector). GMRT clusters are reported in bold. In Col.~(1): Cluster name. Column~(2): Cluster redshift. Column~(3): X-ray luminosity in the energy range $[0.1{-}2.4]$~keV in unit of $h_{70}^{-2}~10^{44}$~erg/s. Column~(4): Bolometric X-ray luminosity in the energy range $[0.01{-}40]$~keV in unit of $h_{70}^{-2}~10^{44}$~erg/s. Column~(5): Radio power at $1.4$~GHz in unit of $h_{70}^{-2}~ 10^{24}$~Watt/Hz. Column~(6) References: 1 = Boehringer et~al. (2004), 2 = Ebeling et~al. (\cite{Ebeling98}), 3 = Ebeling et~al. (\cite{Ebeling96}), 4 = Tsuru et~al. (\cite{Tsuru96}), 5 = Ebeling et~al. (\cite{Ebeling07}), 6 = Ebeling et~al. (\cite{Ebeling00}), 7 = Liang et~al. (\cite{Liang00}), 8 = Feretti et~al. (\cite{Feretti01}), 9 = Govoni et~al. (\cite{Govoni01}), 10 = Bacchi et~al. (\cite{Bacchi03}), 11 = Giovannini \& Feretti (\cite{Giovannini00}), 12 = Dallacasa et~al. (\cite{Dallacasa09}), 13 = Clarke \& Ensslin (\cite{Clarke06}), 14 = Brentjens (\cite{Brentjens08}), 15 = Feretti (\cite{Feretti02}), 16 = Kim et~al. (\cite{Kim90}), 17 = Deiss et~al. (\cite{Deiss97}), 18 = Govoni et~al. (\cite{Govoni05}), 19 = Venturi et~al. (\cite{Venturi07}), 20 = Giacintucci et~al. (\cite{Giacintucci09}), 21 = van Weeren et~al. (\cite{vanWeeren09}), 22 = Bonafede et~al. (\cite{Bonafede09}), 23 = Cassano et~al. (\cite{Cassano08}b), 24 = Giacintucci (\cite{Giacintucci07}) (integrating the diffuse radio emission between the two radio relics). (*) $P_{1.4}$ of A209 and RXJ1314 is estimated from that at 610~MHz by adopting $\alpha =1.2$. \vspace*{-1.5mm} \end{table}