Examples of detected clusters and associated cluster members. Left panel: two clusters located along the same line of sight, but at two different redshifts (z = 0.233 ± 0.005 and z = 0.391 ± 0.005) displayed together with the map of the amplitude A measured by AMICO (cyan and red isodensity contours, respectively); the galaxy members with a probabilistic association P > 0.5 are indicated by circles. The filter response of AMICO is shown with the isocontours, blue for the lower redshift cluster and red for the higher redshift cluster. Right panel: most massive cluster in the sample having an X-ray mass of M = 8.6 ± 0.7 × 10¹³ M_⊙ and located at z = 0.29. Here the colour of the circles indicate the probabilistic membership association of the members. The white lines represent the masked areas and the survey limit. In both panels the magenta contours show the extended X-ray emission.