Intrinsic alignments in the FLAMINGO simulations with two-point statistics

Open Access

Fig. 4.

Variations in the non-linear bias parameters b₁ and the NLA alignment amplitude A₁ with halo mass M_h (in our case, we use M_200mean as the mass of the halo) for our galaxy sample. b₂ is not shown for the sake of clarity. Error bars on the bias parameter and amplitude were calculated by taking the 68th percentile values of the IA posteriors.

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