Fig. 10.
Observables associated with the X-ray emission. Left: X-ray spectrum within R500 shown for both MEKAL and APEC models, as well as with and without galactic photoelectric absorption. The MEKAL model is difficult to distinguish because it coincides very well with the APEC model. Right: surface brightness profile in the band 0.1−2.4 keV. The dynamical range of the profile amplitude has been set to the same value for all observables.
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