Chandra and MUSE images of the targets. For each object, we show in the left panel a (background-subtracted and exposure-corrected) Chandra image in the 0.5−7 keV band of the large-scale ICM emission. Contours start from the peak of the X-ray emission and decrease in steps by a factor of two. The images have been smoothed with a Gaussian of σ = 3 pixels. The middle panel shows a RGB Chandra image of the central region of each cluster, with the bands 0.3−1.2, 1.2−2.5, and 2.5−7.0 keV being shown as red (R), green (G), and blue (B), respectively. Overlaid in black are the total intensity Hα contours from the MUSE data. In the right panels, we show the warm gas kinematics (top) and velocity dispersion (bottom).