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Table 2

Spectral fits to background data for CXB and Galactic components.

Γ Norma k T MWH NormMWHb k T LHB NormLHBb χ2/d.o.f.
(×10-4) [keV] (×10-3) [keV] (×10-2)

1.40(fixed) 38.7/38



Photon flux of power-law model, in units of photons   keV-1   cm-2   s-1 at 1 keV.


Normalization of the APEC model, . DA is the angular diameter distance to the source. An r = 20′ uniform sky is assumed.

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