Fig. 13.

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Projected surface brightness profile ΣX as a function of projected distance Rproj from the Galactic center (as seen by an observer far from the MW) in comparison to stacking experiments (Comparat et al. 2022; Chadayammuri et al. 2022) and simulations (taken from Chadayammuri et al. 2022). The dotted and dashed lines show the β halo and disk-like emission components, respectively. The blue triangles indicate upper limits from Comparat et al. (2022).
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