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Fig. A.9.

image

Top panel: fraction of the luminosity values LX,  ours used in this analysis over the values coming from MCXC (LX,  MCXC) over the full extragalactic sky. All the 313 clusters of our sample were used. The same distance-weighting was used as for the main A analysis. The color scale is the same as for the A/Aall maps throughout the paper. Bottom panel: same as in top panel, for the fraction of LX,  MCXC over the luminosity values coming from the parent catalogs LX,  parent.

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