Unclustered tracers remain unclustered - The lack of primordial non-Gaussianity response of bias-zero tracers

Open Access

Fig. B.1.

PNG response b_ϕ as a function of linear bias b₁ for haloes classified as a function of local matter density δ_m, R using all PNG-UNITsim (f_NL = 100) haloes above 20 particles.

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