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Table 1
Best-fit parameters for the sky background components from Fig. 2.
| Component | Norm arcmin-2 |
|
|
|
| Local Bubble | (8.1 ± 0.5) × 10-7 |
| Galactic halo | (1.15 ± 0.08) × 10-6 |
| CXB | (9.7 ± 0.7) × 10-7 |
Notes. Column description: 1: Background component (see Sect. 2.2). 2: normalization of the model per arcmin2. For APEC (Local Bubble and Galactic halo), this corresponds to 
dV; for a power law (CXB), this is in units of photons keV-1 cm-2 s-1 at 1 keV.
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