Open Access

Fig. 7.


Scaling relation between the prediction index output by the U-net p and the flux in the MILCA y map. In blue we plot the fluxes of the 20 204 sources that are detected on the full sky with the U-net, stacked on the SZ MILCA y map as a function of their associated prediction index p. For comparison, the average flux in the MILCA y map of the PSZ2 clusters is shown in orange, the average flux of the MCXC clusters is shown in green, and the average fluxes of the RM50 and the RM30 clusters are shown in red and purple, respectively. Error bars are computed with the bootstrap method.

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