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Fig. 1.


Merged, exposure-corrected 0.5–7 keV map of the Chandra observations of SPT-CL J2106-5844. The image is binned into 8 × 8 pixels from the native Chandra pixel size of 0.492″. The asymmetric X-ray brightness distribution hints at the disturbed dynamical state of SPT-CL J2106-5844 (Foley et al. 2011; Kim et al. 2019). Overlaid are contours from a smoothed version of the X-ray surface brightness image.

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