\begin{table}%T3
\par
%\centering
\par
\caption{\label{tab:bkgd_ratio} The scaling ratio of the $>$10~keV count rates outside 
(Col.~2) and inside (Col.~3) the telescope FOV in the background 
template files compared to the cluster files. The former ratio is an 
indication of the particle (cosmic ray) background rate, while the 
latter indicates the level of the soft proton background rate. These ratios are 
plotted as a function of Julian date in Fig.~\ref{fig:cray}.}  
\begin{tabular}{l cc }\hline\hline 
Cluster ID&Outside FOV &Inside FOV\\\hline 
RX~J0337.7--2522 & 0.72&1.82   \\ 
RX~J0505.3--2849&0.70& 1.27\\ 
RX~J0847.2+3449 & 0.68&2.14\\ 
RX~J1120.1+4318 &0.99&1.05\\ 
RX~J1325.5--3826 & 1.05\\ 
RX~J1334.3+5030 &1.00&1.23\\ 
RX~J1354.2--0222&0.52&3.44\\ 
RX~J1701.3+6414 &0.48&5.13\\\hline 
\end{tabular} 
\end{table}