Open Access

Fig. 5.


Stack of the 18 415 sources detected with the U-net that do not belong to the Planck or the MCXC catalogue in 16 different maps to determine statistical counterparts of galaxy cluster components in different wavelengths: the SZ MILCA y map, the six Planck HFI frequency maps, the IRIS map at 100 μm, the CMB lensing map, the four galaxy over-density maps based on all, and on passive, transitioning, and active populations of galaxies from the WISExSCOS photometric redshift catalogue (in the redshift range 0.1 <  z <  0.3), and the ROSAT X-ray map. Each of them shows statistical indications of galaxy cluster emissions. Patches are 3.4° ×3.4° in order to show the large-scale contribution around the sources.

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