Fig. 14.
Example fit of the total spectrum for region 16 in Perseus, rebinned for display to have a signal to noise ratio of 10 in each spectral bin. The vertical line is at an energy of 6.55 keV. (Top panel) Fitted data and best-fitting cluster model (fitted redshift), showing its cluster and background components. Also shown is the cluster component with the redshift changed to the Hitomi cluster value. (Centre panel) Residuals of the total best-fitting model. (Bottom panel) Residuals of the total model with the APEC redshift changed to the Hitomi value.
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