Fig. 1.
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Distribution of the galaxies in the field of PLCK1, between z = 0.4 and z = 0.52. Left: VLT/VIMOS galaxies overlaid on the XMM-Newton brown-filled contours for PLCK1. The colors of the dots correspond to the redshift of the galaxies determined with MARZ (Sect. 4.1). Right: 3D distribution of the galaxies in the field of PLCK1 in the redshift range [0.4, 0.52]. The color of the dots correspond to the galaxy types assigned with MARZ (Sect. 4.1). The blue spheres indicate the spatial extensions of the different components with radius R500 in the RA/Dec. plane and 3σ in the z axis.
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