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Fig. A.1.
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Power spectrum of a bin with b1 ∼ 3.2 selected by halo mass (Mh, left) and by local halo overdensity (δh, R, right). Whereas the effect of introducing PNG (fNL = 100) has a strong effect on mass-selected bins, the δh, R bins show near identical clustering for fNL = 0 and fNL = 100.
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