Table 1: 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.
Comp. k T/$\Gamma$ Flux
  (keV / phot. ind.) (10-12 erg cm-2 s-1 deg-2)
LHB k T=0.08f $3.4\pm1.1$
GH $k~T=0.17\pm0.03$ $2.9\pm0.9$
EPL $\Gamma=1.41^f$ 22f
PL $\Gamma=0.78\pm0.16$ $49\pm7$

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