Corner plot of the posterior for the joint fits to w_gg with non-linear galaxy bias and w_g+ with TATT for the different FLAMINGO feedback variations. The galaxy sample was selected from the 1 Gpc runs and consists only of objects with a dark matter mass of more than 10¹² M_⊙ and more than 300 stellar particles. Feedback does not strongly change the derived constraints on A₁, except for the case of ‘M*-σ’ shown in orange, and the strong jet variation ‘Jet fgas-4σ’ shown in light green. These changes are consequences of the different stellar masses of the samples after the same stellar particle cut is applied.