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Fig. 3.

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Power spectrum of the simulation volume at its initial condition (z ∼ 127). Blue shows the power of the constrained field (large scales) in the 34 × 28 × 450 cMpc3/h3 volume. Orange shows the theoretically expected linear power. The shaded region shows the composite realization for the cosmosTNG simulations: modes are from the constrained field up to kcutoff = 1 h/cMpc above which we randomly draw modes according to linear theory.

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