Latitude profiles of scattered XB radiation in comparison with the near-infrared-inferred GRXE profile in the energy range 3−10 keV for the field of view of 16 × 16 arcmin centered at l = 0.08°, b =  −1.42°. In this region between 80 and 90% of the GRXE has been resolved into point sources (Revnivtsev et al. 2009). Percentages quoted show the fractional contribution of the diffuse GRXE component in each case. Because of the coincidental presence near this field of view of a luminous simulated source, we also quote the same value on the other side of the Galactic plane in the case of Monte Carlo sources.