Fig. A.2
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Variation of the best-fit parameters of the X-ray background model components is shown over Galactic latitude (gal b): (a) best-fit reduced fit statistic (cstat/d.o.f.), (b) LHB normalisation, (c) CGM plasma temperature (APEC), (d) CGM normalisation, (e) normalisation of the hot corona component (kT = 0.7 keV) with two Galactic mass profiles, based on Bienayme et al. (1987) and McMillan (2017), and (f) normalisation of the extra-galactic component (double-broken-powerlaw). In each diagram the solid line is the average, while the dashed lines show the 1σ standard deviation. For (b)-(f) the triangles facing down indicate Galactic l < 280° while facing up triangles are used for l > 280°.
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