\begin{table}%T2 \caption{\label{table2}Radio halos.} \small%\centerline { \begin{tabular}{lclrrrrrccc} \hline\hline\noalign{\smallskip} Name & $z$ & kpc/$''$ & $S$(1.4) & $\Delta S$ &log $P$(1.4) & LLS & Lx(10$^{44}$) & Ref. & Ref. & Notes \\ & & &~mJy &~mJy & W/Hz & Mpc & erg/s & Radio& X-ray & \\ \hline A209 & 0.2060 & 3.34 & 16.9 & 1.0 & 24.31 & 1.40 & 6.17 & * & 21 &a relic could be present \\ A401 & 0.0737 & 1.38 & 17.0 & 1.0 & 23.34 & 0.52 & 6.52 & 1 & 15 & elongated and irregular \\ A520 & 0.1990 & 3.25 & 34.4 & 1.5 & 24.58 & 1.11 & 8.30 & 2 & 16 & \\ A521 & 0.2533 & 3.91 & 5.9 & 0.5 & 24.05 & 1.17 & 8.47 & * & 21 & a relic is also present \\ A545 & 0.1540 & 2.64 & 23.0 & 1.0 & 24.16 & 0.89 & 5.55 & 1 & 21 & \\ A665 & 0.1819 & 3.03 & 43.1 & 2.2 & 24.59 & 1.82 & 9.65 & 3 & 16 & \\ A697 & 0.2820 & 4.23 & 7.8 & 1.0 & 24.28 & 0.65 &10.40 & * & 16 &from NVSS, see text \\ A754 & 0.0542 & 1.04 & 86.0 & 4.0 & 23.77 & 0.99 & 2.21 & 1 & 15 & a relic is also present \\ A773 & 0.2170 & 3.48 & 12.7 & 1.3 & 24.23 & 1.25 & 7.95 & 2 & 16 & \\ A851 & 0.4069 & 5.40 & 3.7 & 0.3 & 24.33 & 1.08 & 5.04 & * & 17 & \\ A1213 & 0.0469 & 0.91 & 72.2 & 3.5 & 23.56 & 0.22 & 0.10 & * & 18 & asymmetric \\ A1300 & 0.3072 & 4.49 & 20.0 & 2.0 & 24.78 & 1.3 &13.73 &4,5& 21 & a relic is also present \\ A1351 & 0.3224 & 4.64 & 39.6 & 3.5 & 25.12 & 0.84 & 5.47 & * & 17 & \\ A1656 & 0.0231 & 0.46 &530.0 &50.0 & 23.80 & 0.83 & 3.99 & 6 & 15 & a relic is also present \\ A1758 & 0.2790 & 4.20 & 16.7 & 0.8 & 24.60 & 1.51 & 7.09 & * & 19 &total diffuse emission H+R \\ & & & 3.9 & 0.4 & 23.97 & 0.63 & & * & & central halo \\ A1914 & 0.1712 & 2.88 & 64.0 & 3.0 & 24.71 & 1.04 &10.42 & 1 & 15 & \\ A1995 & 0.3186 & 4.61 & 4.1 & 0.7 & 24.13 & 0.83 & 8.83 & * & 17 & \\ A2034 & 0.1130 & 2.03 & 13.6 & 1.0 & 23.64 & 0.61 & 3.81 & * & 16 & \\ A2163 & 0.2030 & 3.31 &155.0 & 2.0 & 25.26 & 2.28 &22.73 & 7 & 14 & a relic is also present \\ A2218 & 0.1756 & 2.94 & 4.7 & 0.1 & 23.60 & 0.38 & 5.77 & 3 & 16 & asymmetric \\ A2219 & 0.2256 & 3.58 & 81.0 & 4.0 & 25.08 & 1.72 &12.19 & 1 & 16 & \\ A2254 & 0.1780 & 2.98 & 33.7 & 1.8 & 24.47 & 0.92 & 4.55 & 2 & 16 & irregular asymmetric shape\\ A2255 & 0.0806 & 1.50 & 56.0 & 3.0 & 23.94 & 0.90 & 2.64 & 8 & 16 & a relic is also present \\ A2256 & 0.0581 & 1.11 &103.4 & 1.1 & 23.91 & 0.81 & 3.75 &9 & 16 & a relic is also present \\ A2294 & 0.1780 & 2.98 & 5.8 & 0.5 & 23.71 & 0.54 & 3.90 & * & 16 & \\ A2319 & 0.0557 & 1.07 &153.0 & 8.0 & 24.04 & 1.02 & 8.46 &10 & 15 & spectral steepening \\ A2744 & 0.3080 & 4.50 & 57.1 & 2.9 & 25.24 & 1.89 &12.86 & 2 & 21 & a relic is also present \\ A3444 & 0.2533 & 3.91 & 14.6 & 1.0 & 24.45 & 3.3 &13.42 & * & 21 & Filament; see text \\ A3562 & 0.0490 & 0.95 & 20.0 & 2.0 & 23.04 & 0.28 & 1.57 &11 & 15 & spectral steepening \\ 1E0657-56&0.2960 & 4.38 & 78.0 & 5.0 & 25.33 & 2.1 &22.59 &12 & 21 & bullet cluster \\ RXC~J1314.4-2515&0.2439&3.81& 20.3&0.8&24.55&1.83 &10.75 &13 & 21 & Double relics are present\\ CL1446+26&0.3700&5.08 &9.2 & 0.5 & 24.63& 0.36 & 3.42 & * & 20 & relic source \\ RXC~J2003.5-2323&0.3171 &4.59&35.0 &2.0 &25.09 &1.40&9.12 &14 & 21 & \\ \hline \end{tabular}} \smallskip Column~1: cluster name; Col.~2: redshift; Col.~3: angular to linear conversion; Col. 4: radio flux density at 1.4~GHz; Col. 5: Estimated flux density error; Col.~6: radio power at 1.4~GHz; Col.~7: radio largest linear size; Col.~8: X-ray luminosity in the 0.1$-$2.4~keV band in 10$^{44}$ units; Col.~9: references for radio data: * = this work; 1 = \citet{bac03}; 2 = \citet{gov01a}; 3 = \citet{gf00}; 4 = \citet{ven09}; 5 = \citet{rei99}; 6 = \citet{kim90}; 7 = \citet{fer01}; 8 = \citet{gov05}; 9 = \citet{ce06}; 10 = \citet{fer97}; 11 = \citet{ven03}; 12 = \citet{lia00}; 13 = \citet{fer05}; 14 = \citet{gia09}; Col.~10: references for X-ray data: 15 = \citet{rb02}; 16 = \citet{ebe98}; 17 = \citet{boe00}; 18 = \citet{led03}; 19 = \citet{ebe96}; 20 = \citet{wu99}; 21 = \citet{boe04}; Col.~11: notes. \end{table}