Fig. 4.

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Observed X-ray luminosity of CGM as a function to M* (purple, brown points), compared to the relation derived by convolving the observed LX, CGM − M500c relation with the stellar-to-halo-mass relation (gray band). The LX, CGM − M* measurements from Anderson et al. (2015) is shifted by 0.1 dex to higher mass to account for the difference in M* estimation between Anderson et al. (2015) and this work.
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