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Fig. 9.


Simulated 100 ksec observation of the starburst galaxy M 82 with the Athena X-IFU. The image in the center shows the inner arcminutes as simulated by SIXTE. For the two regions (indicated by green and blue) we extracted spectra, which are plotted in the left and right panels together with the input model (gray line). For each spectrum we provide a zoom into the region around 1.1 keV to highlight the difference in observed lines.

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