Left: XMM-Newton X-ray temperature map of RX J1347 in keV. X-ray iso-contours from the Chandra [0.5, 2.5] keV band image are superimposed in black. Total intensity radio contours are overlaid in white. They start at 3σ level and are spaced by a factor of . The inset shows the ICM brightness profile corresponding to the sector illustrated by the dashed lines on the main image. A shock model corresponding to density and temperature jumps of and gives the fitted brightness profile indicated by dotted lines in the inset. Right: total intensity 614 MHz map and contours (white) of RX J1347. Contours of the MUSTANG SZE image of the cluster are overlaid in green (levels: −1.5, −1.0 and −0.5 mJy/beam, from the inner contour outward, as in Mason et al. 2010, Fig. 6). The two panels have exactly the same physical scale.