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Fig. 1.

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Forward-modelling of the X-GAP selection. We started from a dark matter halo light cone generated from the Uchuu simulation, built a novel method for assigning cluster and group X-ray profiles and temperatures as a function of the halo mass and redshift, and used abundance-matching schemes to simulate galaxies and AGN. We generated X-ray events and accounted for the telescope response. Finally, we reproduced the detection schemes in X-ray and optical bands to select an X-GAP-like sample from our simulation.

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