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Fig. 12.

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Comparison in different halo mass bins between the PHOX input IGrM profiles convolved with the eROSITA PSF and the results of the stacking procedure on the mock observations. The PHOX profiles are averaged in bins of input halo mass, while the stacked profiles are obtained in bins of halo mass proxy of the related prior catalog (blue for R11, violet for T17, and pink for Y05).

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