\begin{table}%t1
\caption{\label{X_rays}Summary of \xmm\  Spectral Analysis.}
%\centerline
{\begin{tabular}{cc cc}
%\multicolumn{7}{c}{ MIPS 24  detected cluster members with spectroscopic redshifts} \\
\hline\hline\noalign{\smallskip}
$kT$       &  $f_{\rm{x} }$ (0.5--2.0 keV)  &  $L_{\rm{X,bol} }$  & $\chi^2$/d.o.f.$^{\dagger}$ \\
(keV)    & ($10^{-14}~$erg~s$^{-1}~$cm$^{-2}$) & (${h}_{70}^{2} 10^{44}~$erg s$^{-1}$) & \\
\noalign{\smallskip}\hline
% & & & \\[-6pt]
 $\rm 3.6^{+2.9}_{-1.2}$ &$ 2.2 \pm1.1$ & $\rm 2.0 ^{+2.9}_{-1.2}$ & 64.06/64\\[1pt]
\hline
\end{tabular}}
\smallskip
$^{\dagger}$ Best fit thermal bremsstrahlung model; $Z = 0.4~Z_{\odot}$ fixed.
\end{table}