Comparison plots between the geometry-corrected X-ray pressure map (top left), the geometry-corrected trend-divided X-ray pressure map (top-right), followed by SZ MUSTANG2 data (bottom-left), next to a kinetic and relativistic SZ corrected version of the data, shown here in Kelvin_CMB units (bottom-right). The white contours are from the radio images seen in van Weeren et al. (2017) and the green contours corresponds to the MUSTANG2 data in the bottom-left. The circles represent the strong lensing sub-cluster centres given in Limousin et al. (2016), which were used to reproduce the kSZ+rSZ model used in Adam et al. (2017b), displayed in Table 7. The full FOV of the MUSTANG2 data can be seen in Appendix C.