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Fig. 4.

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Predicted Magneticum X-ray surface brightness profiles per bin of halo mass. The profiles are obtained by convolving the PHOX projected profiles with the eROSITA PSF. The blue-shaded regions indicate the total X-ray emission within 1σ of the mean. The magenta blue-shaded regions indicate the AGN contribution, while the gray-shaded regions indicate XRB emission. The green-shaded region indicates the IGrM emission.

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