The eROSITA view of the Abell 3391/95 field: The Northern Clump - The largest infalling structure in the longest known gas filament observed with eROSITA, XMM-Newton, and Chandra

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

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Fig. D.3

XMM-Newton and RASS background spectra (black) of the central bin fitted with the three different central AGN models in the energy range of 0.7–7.0 keV. Top: Method 1 - with 15′′ mask to mask the central AGN. Middle: Method 2 - AGN component is modeled from Chandra best fit values. Bottom: Method 3 - AGN is modeled and additional thermal component is added.

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