Fig. 3
NXB-subtracted spectra of A2255 (r < 5′). The XIS BI (black) and FI (red) spectra are fitted with the ICM model (phabs × Apec), along with the sum of the CXB and Galactic emission. The ICM component is shown with the cyan line. The CXB, LHB and MWH emissions are indicated with black, green, and blue curves, respectively. The sum of all sky background emissions is shown with an orange curve.
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