Fig. 5.

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Collection of clusters that show several types of radio emission. PSZ2 G053.53+59.52 has a central radio halo and a number of sources of uncertain origin. PSZ2 G071.21+28.86 has a double radio relic. PSZ2 G088.53+41.18 is a system without diffuse cluster emission as the only emission detected is associated with an optical galaxy. PSZ2 G097.72+38.12 has a radio halo. PSZ2 G113.91–37.01 has a radio halo and two relics. PSZ2 G114.99+70.36 has emission of uncertain origin. PSZ2 G143.44+53.66 has emission of uncertain origin. PSZ2 G148.36+75.23 has a radio halo. PSZ2 G166.62+42.13 has a radio halo and multiple relics. We remark that the classification was done by inspecting all the sets of images available, while the images displayed in this gallery are only the reference ones (i.e., those with robust = −0.5 and no uv taper). For a more complete picture of the large variety of radio structures observed in our sample, we refer the reader to Fig. B.1 and to the project website.
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