Fig. 7.

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Inferred magnitude of satellite anisotropy in the low-z and high-z DESI ELG catalogues. We display the ratio of the correlation function in the best-fit SHAMe catalogue to a version where the angular position of haloes has been randomly shuffled among each halo. Solid (dashed) lines and shaded (circle-hatched) regions indicate the mean and 1σ region after marginalisation over all SHAMe parameters when shuffling all satellites (only satellites within r200c). For comparison, we display the same quantity estimated in our mock DESI catalogues.
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