Temperature map in keV units of the Bullet Cluster derived from the Chandra data following the method described in Markevitch et al. (2000) and Wang et al. (2016). Contours show the radio emission from the MeerKAT discrete source-subtracted image spaced by a factor of 2 starting from 3 × rms. Dashed arcs mark the positions of the radio surface brightness discontinuities. The corresponding error map is reported in Appendix A.