\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}