\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}