\begin{table}%t8
\caption{\label{Table8}General information for each cluster: the overall (defined here to be from $0{-}2r_{\rm{c}}$) temperature and iron abundance, the overall luminosity, the total number of counts in the cluster, the calculations relevant to the cooling time, and finally the subset as defined in Table~\ref{Table7}.}
\par
\small%%\centerline

 {
\begin{tabular}{c c c c c c c c c c c } 
\hline \hline
\multicolumn{6}{c }{Temperatures and Iron abundances for each full cluster} & \multicolumn{4}{c}{Cooling calculations for each central region} & \multicolumn{1}{c}{Analysis Subset}\\ 
\multicolumn{1}{ c  }{cluster name}  & \multicolumn{1}{ c  }{$ \it z$} & \multicolumn{1}{c }{temperature} & \multicolumn{1}{c }{iron abundance} & \multicolumn{1}{c}{\# of Counts} &
  \multicolumn{1}{c}{$\mathcal{L}_{0-2}$} &
  \multicolumn{1}{c}{$\mathcal{L}_{0-0.5}$}
  & \multicolumn{1}{c}{proton density } &
  \multicolumn{1}{c}{cooling time} & \multicolumn{1}{c}{age} & \multicolumn{1}{c}{subset \#} \\ \hline
Abell 1413$^{\dagger}$  & 0.142 & $7.0 \pm 0.3$ &
$0.46 \pm 0.08$ & 11164 & 5.11 & 1.95 & 0.019 & 3.79 & 8.55 & 2 \\
Abell 2204$^{\dagger}$  & 0.152 & $4.3 \pm 0.1$ &
$0.86 \pm 0.08$ & 16382 & 5.17 & 1.09 & 0.22 & 0.24 & 8.44  & 1\\ 
Abell 665$^{\dagger}$ & 0.182 & $8.0 \pm 0.4$ & $0.40 \pm
0.08$ & 12526 & 3.89 & 0.87 & 0.012 & 6.91 & 8.11 & 2\\
RX J0439.0+0520$^{\dagger}$  & 0.208 & $3.6 \pm 0.2$ &
$0.76 \pm 0.17$ & 2018 & 1.96 & 0.75 & 0.08 & 0.57 &
 7.83 & 1\\ 
Abell 773 & 0.217 & $8.0 \pm 0.7$ & $0.32 \pm 0.13$ &
8351 & 9.24 & 5.24 & 0.0058 & 14.72 & 7.74 & 4\\
Abell 1763 & 0.223 & $7.9 \pm 0.2$ & $0.34 \pm 0.04$ &
48845 & 8.81  & 3.52 & 0.0062 & 12.93 & 7.68 & 4\\
Abell 2390$^{\dagger}$ & 0.228 & $8.5 \pm 0.2$ & $0.43 \pm
0.04$ & 36705 & 10.70 & 3.41 & 0.038 & 1.94 &
7.63 & 2\\
Abell 1835$^{\dagger}$ & 0.253 & $6.0 \pm 0.1$ & $0.39 \pm 0.01$ &
242214 & 18.20 & 7.20 & 0.088 & 0.71 & 7.38 & 1\\ 
Abell 697 & 0.282 & ${9.7 \pm 0.7}$ & ${0.35 \pm 0.08}$ &
13442 & 16.6 & 7.75 & 0.0082 & 11.15 & 7.10 & 4\\ 
Abell 611$^{\dagger}$  & 0.288 & $7.0 \pm 0.3$ &
$0.31 \pm 0.06$ & 15213 & 6.53 & 2.64 & 0.019 & 3.92 & 7.04 & 2 \\ 
MS 1008.1-1224  & 0.306 & $6.3 \pm 0.4$ &
$0.35 \pm 0.08$ & 7257 & 4.18 & 1.28 & 0.0082 & 8.49 & 6.88 & 3\\ 
MS 2137.3-2353$^{\dagger}$  & 0.313 & $4.6 \pm 0.1$ &
$0.35 \pm 0.04$ & 16958 & 8.29 & 2.87 & 0.10 & 0.60 & 6.81 & 1\\ 
Abell 1995 & 0.319 & ${8.9 \pm 0.5}$ & ${0.28 \pm 0.10}$ &
34062 & 15.20 & 5.73 & 0.0062 & 13.58 & 6.73 & 4\\
ZWCL 1358+6245$^{\dagger}$  & 0.328 & $6.1 \pm 0.3$ &
$0.39 \pm 0.08$  & 8208 & 3.37 & 0.94 & 0.035 & 1.65 & 6.68 & 1\\ 
RX J0256.5+0006  & 0.360 & $ 5.0 \pm 0.2$ &
$0.34 \pm 0.06$ & 8608 & 4.49 & 1.36 & 0.0061 & 11.32 & 6.40 & 3\\ 
RX J0318.2-0301  & 0.370 & $5.7 \pm 0.3$ &
$0.28 \pm 0.08$ & 7879 & 3.76 & 1.31 & 0.0064 & 9.16 & 6.32  & 3\\
RX J0426.1+1655$^{\dagger}$  & 0.380 & $5.4 \pm 0.4$ &
$0.19 \pm 0.07$ & 33174 & 1.55 & 0.77 & 0.021 & 2.83 &
6.23  & 1\\
MACS J2228.5+2036 & 0.412 & $7.1 \pm 0.5$ &
$0.33 \pm 0.10 $ & 6199 & 15.29 & 6.24 & 0.0081 & 10.30 & 5.97 & 8\\
MACS J2214.9-1359  & 0.483 & $8.8 \pm 0.8 $&
$0.29 \pm 0.12$ & 3399 & 14.36  & 5.20 & 0.011 & 7.61 & 5.43 & 8\\
MACS J1311.0-0310${\dagger}$  & 0.490 & $6.5 \pm 0.6$&
$0.45 \pm 0.13$ & 2111 & 10.57 & 4.60 & 0.021 & 3.09 & 5.38 & 5\\ 
MS 0015.9+1609  & 0.541 & $9.8 \pm 0.6 $ &
$0.28 \pm 0.06$ & 17837 & 23.57  & 3.28& 0.0041 & 21.99 &5.02 & 8\\ 
MACS 1423.8+2404$^{\dagger}$  & 0.545 & $5.3 \pm 0.1 $&
$0.54 \pm 0.05$ & 17674  & 10.06  & 3.31& 0.12 & 0.50 & 4.99 & 5
\\ 
MS 0451.6-0305  & 0.550 & $9.4 \pm 0.7 $&
$0.40 \pm 0.11$ & 14303 & 22.11 & 7.34 & 0.011 & 8.32 &4.96 & 8\\ 
MACS J2129.4-0741 & 0.570 & $7.0 \pm 1.1 $&
$0.41 \pm 0.23$  & 1755 & 10.63 & 2.59 & 0.018 &4.64 & 4.82 & 6\\
MS 2053.7-0449 & 0.583 & $4.9 \pm 0.5 $ & $0.28 \pm 0.10$ & 1733 &
1.95 & 0.41 & 0.0083 & 7.75 & 4.74 & 7\\
MACS J0647.7+7015  & 0.584 & $11.5_{\rm -2.0}^{+2.8}  $&
$0.19_{\rm -0.19}^{+0.26} $ &2717 & 16.27 & 7.58 & 0.013 & 8.79 &4.73 & 8 \\ 
RX J1120.1+4318 & 0.600 & $5.2 \pm 0.4$ &
$0.37 \pm 0.11$ & 10239 & 7.22 & 3.28 & 0.0063 & 11.21 & 4.63 & 7\\ 
MACS J0744.8+3927${\dagger}$  & 0.686 & $6.8 \pm 0.7$ &
$0.51 \pm 0.18$ & 1153 & 9.36  &2.66 & 0.063 & 1.09& 4.11 & 6\\
MS 1137.5+6625  & 0.782 & $7.2 \pm 0.6$ &
$0.26 \pm 0.13$ & 4073 &6.03  & 2.07 & 0.014 & 5.61 & 3.59 & 8\\ 
RX J1716.9+6708  & 0.813 & $4.6 \pm 0.5$ &
$0.57 \pm 0.23$ & 1649 & 6.16 & 2.21 & 0.0088 & 9.69 & 3.43 & 7\\
CL J1226.9+3332  & 0.890 & $11.1 \pm 0.3$ &$ 0.20
\pm 0.05$ & 29846 & 20.56 & 10.06 & 0.014 & 7.42 & 3.07 & 8\\
\hline
\end{tabular}}
\medskip
The column $\mathcal{L}_{0-0.5}$ is the luminosity from $0{-}0.5 r_{\rm{c}}$, and $\mathcal{L}_{0-2}$ is the luminosity from $0{-}2r_{\rm{c}}$. The luminosities are in~$\rm erg-s^{-1}$, the times are in~Gyr, and the densities are in units of~$\rm cm^{-3}$.  Galaxy clusters with a dagger ($\dagger$) next to them have confirmed radio sources likely associated with the cluster.  The temperature and iron abundance have the same units as in Table~\ref{Table6}.
\end{table}