Fig. 8

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Left: instrument independent, absorption corrected, and background subtracted sX profiles of Chandra (green), XMM-Newton (blue), and eROSITA (red) in the energy band 0.5–2.0 keV. The blue, red, and black horizontal dashed lines are the CXB levels of XMM-Newton, eROSITA, and eROSITA with XMM-Newton defined CXB region, respectively. Black points are the CXB corrected XMM-Newton sX. The various radii are plotted in brown. Right: XMM-Newton Sx profiles in different directions of the Northern Clump using the box annuli setup (top) and the relative differences with respect to the average surface brightness (bottom). The grey shaded areas in both plots are the lσ confidence region of the average Sx The various radii are plotted in brown. The CXB and QPB level are plotted in orange and cyan dashed lines.
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