Fig.3
A gri composite image of the central 
of PLCKG147.3−16.6, based on imaging data from NOT/MOSCA (g and i) and TNG/DOLORES (r and i). Boxes: cluster galaxies spectroscopically confirmed with Gemini (excluding the two galaxies at z = 0.68). North is up and East to the left. The green contours are isocontours of the wavelet filtered XMM-Newton image. The white contours show the luminosity distribution of the red sequence galaxies indicated by red symbols in Fig. A.2, smoothed with a σ = 14″ Gaussian filter. The plotted contour levels are at (10, 20, 30) times the rms variation in the luminosity distribution.
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