\begin{table}%t1
%%\centering
\par
\caption{\label{table:1}400 SD low redshift sample.} 
\begin{tabular}{llllllll} 
\hline\hline\noalign{\smallskip}                
Cluster  &  Obs ID & $z$ & $c_{\rm SB}$ & $T$ (keV) & $T_{\rm core}$ & $L_{\rm X}$  & $R_{\rm src}$ \\   
(1)      & (2)  & (3)     & (4) &  (5) & (6)  & (7) & (8) \\
\hline                        
A3395	  & 4944  &  0.0506   & 0.081~$\pm$~0.006 & 5.13 (5.10) & 5.3 & 1.09 & -- \\
A754	  & 577, 6796, 6797  & 0.0542   & 0.036~$\pm$~0.001 & 9.94 (8.73) & 8.3 & 2.78  & no \\
A3391    & 4943 & 0.0551   & 0.045~$\pm$~0.002 & 6.07 (5.39) & 7.0 & 1.05  & -- \\
A3667	  & 513, 5751, 5752, 6296, 6292  & 0.0557   & 0.029~$\pm$~0.001 & 6.72 (6.33) & 5.4 & 3.14 & -- \\
A85	      & 904 & 0.0557   & 0.167~$\pm$~0.001 & 6.90 (6.45) & 3.2 & 2.91  & yes \\
A133 	  & 2203, 9897 & 0.0569   & 0.259~$\pm$~0.003 & 3.71 (4.01) & 2.3 & 0.96 & yes \\	
A2256	  & 2419, 965, 1386 & 0.0581   & 0.024~$\pm$~0.001 & 6.90 (8.37) & 6.8 & 2.66  & no \\
A3158	  & 3201, 3712 & 0.0583   & 0.045~$\pm$~0.001 & 4.94 (4.67) & 5.9 & 1.72  & -- \\
A3266    & 899 & 0.0602   & 0.047~$\pm$~0.002 & 8.35 (8.63) & 8.0 & 2.69  & -- \\
A1795	  & 5289, 5290, 6159, 6161, 6162, 6163  & 0.0622   & 0.180~$\pm$~0.001 & 7.80 (6.14) & 3.3 & 3.52  & yes \\
A399	  & 3230 & 0.0713   & 0.040~$\pm$~0.001 & 5.80 (6.49) & 7.1 & 2.01  & no \\
A2065    & 3182 & 0.0723   & 0.087~$\pm$~0.002 & 5.35 (5.44) & 4.2 & 1.82  & yes \\
A401	  & 518, 2309 & 0.0743   & 0.040~$\pm$~0.001 & 8.07 (7.72) & 7.1 & 3.90  & no \\
A3112	  & 2216, 2516 & 0.0759   & 0.273~$\pm$~0.001 & 4.28 (5.19) & 2.7 & 2.43  & -- \\
A3822 	  & 8269 & 0.0760   & 0.045~$\pm$~0.004 & 5.45 (5.23) & 5.6 & 1.91  & -- \\
ZCl1215 & 4184 & 0.0767   & 0.040~$\pm$~0.002 & 6.00 (6.54) & 6.5 & 1.80  & no \\
A2029	  & 891, 4977, 6101 & 0.0779   & 0.169~$\pm$~0.003 & 7.38 (8.22) & 4.2 & 5.72  & yes \\
A1650 	  & 5822, 5823, 6356, 6357, 6358, 7242, 7691 & 0.0823   & 0.112~$\pm$~0.001 & 5.89 (5.29) & 5.1 & 2.33  & no \\
A2597 	  & 922, 6934  & 0.0830   & 0.332~$\pm$~0.001 & 3.58 (3.87) & 2.7 & 2.09  & yes \\
A1651	  & 4185  & 0.0853   & 0.082~$\pm$~0.003 & 7.00 (6.41) & 6.7 & 2.93  & yes \\
A478	  & 1669  & 0.0881   & 0.194~$\pm$~0.001 & 7.07 (7.96) & 3.1 & 7.24  & yes \\
A2142	  & 7692, 5005 & 0.0904   & 0.082~$\pm$~0.001 & 8.24 (10.04) & 6.3 & 7.20  & no \\
A2244	  & 7693 & 0.0989   & 0.103~$\pm$~0.005 & 5.57 (5.37) & 5.4 & 2.98  & no \\
A2204    & 6104, 7940 & 0.1511   & 0.315~$\pm$~0.002 & 6.97 (8.55) & 3.5 & 9.35  & yes \\
A2163	  & 1653 & 0.2030   & 0.025~$\pm$~0.002 & 12.12 (14.72) & 16 & 13.7  & no  \\
RXC J1504.1-0248 & 5793 & 0.2169   & 0.333~$\pm$~0.003 & 8.90 (9.89) & 4.6 & 15.6  & yes \\
Hydra\tablefootmark{*}    & 4969, 4970 & 0.0549   &  -- & 4.30 (3.64) & 2.9 & 1.93  & yes \\
S1101\tablefootmark{*}   &  1668 & 0.0564   & --  & 2.65 (2.44) & 2.0 & 1.03 & -- \\
\hline  
\end{tabular}
\tablefoot{(1) Cluster name; (2)~Chandra observation identifier; (3)~redshift; (4)~surface brightness concentration without $K$-correction; (5)~global temperature from Cavagnolo  et~al.  \cite{cav} (the values in parentheses are from Vikhlinin et~al. \cite{vikhlinin09}); (6)~core 
temperature from Cavagnolo et~al. (\cite{cav}); (7)~soft-band luminosity in units $10^{44}$~[erg~s$^{-1}$]; and (8)~presence of a radio source according to the NVSS archive. \tablefoottext{*}{Strong cool-core clusters observed only with ACIS-S which we did not consider in our analysis.}}
\vspace*{-2mm}
\end{table}