\begin{table}%t1
%\centering
\par
\caption{The CXB components determined in a region free of clusters emission outside of the virial radii of the clusters. The unabsorbed fluxes are determined in the 0.3--10.0~keV band. $f$ indicates parameters kept fixed during spectral fitting.}\label{tab:back}
\small\begin{tabular}{lcccc}
\hline
\hline
Comp. & $k~T$/$\Gamma$ & Flux  			 \\
  & (keV / phot. ind.) & (10$^{-12}$~erg~cm$^{-2}$~s$^{-1}$~deg$^{-2}$) \\
\hline
LHB & $k~T=0.08^f$  		& $3.4\pm1.1$ 	\\
GH  & $k~T=0.17\pm0.03$      & 	$2.9\pm0.9$ 	\\  
EPL  & $\Gamma=1.41^f$    		& $22^f$       \\
PL & $\Gamma=0.78\pm0.16$	& $49\pm7$ \\
\hline
\end{tabular}
\end{table}