Fig. 4
Longitude profiles of scattered XB radiation in comparison with a near-infrared-inferred GRXE profile in energy ranges 3−10, 10−20, 17−25, and 25−60 keV for real sources. The sum of the scattered component is 10-30% of the stellar contribution to the GRXE. Data for the sources responsible for the labeled peaks are listed in Table A.1.
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