Residual images of the X-ray and SZE surface brightness. Left: the residual image of Chandra X-ray surface brightness after subtracting the mean profile, excluding the southeast quadrant. The original surface brightness is the same as in the left panel of Figure 1. For reference, the position of the central AGN is marked by a cross. Right: same as the left panel but for the ALMA 92 GHz brightness in mJy beam⁻¹ with the effective beam size of 5″ FWHM. The original surface brightness is shown in the right panel of Figure 1.