Intrinsic alignments in the FLAMINGO simulations with two-point statistics

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Fig. 10.

Corner plot of α_M and β_M from Eq. (22) for each of the FLAMINGO feedback models. These are posteriors from the fits on A₁ vs halo mass from Fig. 9. By fitting a power law to the variation of A₁ with halo mass, the dependence on halo mass is removed, after which all the feedback modes become consistent with each other.

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