Fig. 4
A2163. Left panels: X-ray emission overlaid on galaxy maps. Optical observations performed at the MPI 2.2 m telescope, see Paper I (Maurogordato et al. 2008). X-ray images obtained from wavelet analyses of a Chandra exposure in the 0.5–2.0 keV band. Top-left: overall cluster emission. Bottom-left: high resolution analysis of the ICM emission near the cluster centre, see Sect. 3.3 for details. Right panels: ICM temperature maps obtained from wavelet spectral-imaging analysis of the EPIC-XMM-Newton data set. Top-right: black iso-contours from the Chandra image (same as top-left map). Bottom-right: black iso-contours from high resolution Chandra residue (same as bottom-left map); white iso-contours from projected galaxy density map (see also Fig. 6 in Paper I).
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