Fig. 4.

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Galaxy clustering (wp, top left panel; ξℓ = 0, top right panel; ξℓ = 2, lower left panel) and galaxy-galaxy lensing (ΔΣ, lower right panel) for the FLAMINGO suite of simulations with different astrophysical implementations (symbols) and the SHAMe model (lines). The different colours represent the various astrophysical implementations, as labelled. All samples are displaced along the y axis for clarity. Only the results from the DESI BGS-like sample are shown in the plot. The middle subpanel shows the difference between the empirical model and FLAMINGO, normalised by the error. The bottom subpanel shows the difference between theFLAMINGO model variations and the fiducial FLAMINGO model. The fits are performed for all scales shown for the galaxy clustering statistics and for scales above 1 h−1 Mpc for galaxy-galaxy lensing.
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