Temperature of the excess component in units of keV (left) and its statistical error (right) inferred from the ALMA SZE and Chandra X-ray images, assuming a constant line-of-sight length of L_excess = 150 kpc. The values are approximately proportional to ﹩{({L}_{\mathrm{excess}}/150\mathrm{kpc})}^{-1/2}﹩. Regions for which the S/Ns of either data sets are less than 4σ are left blank (black). For reference, the elliptical annuli shown in Figure 3 are overlaid. Note that X-ray spectra are not used in computing the quantities plotted in this figure.