Fig. 7.
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Simulated and theoretical Rsim(δw, σ, z) responses in ΛCDM cosmology for the L = 60 Mpc h−1 window size at z = 1 and 3 redshifts. The new power-law response function fits the simulated responses well, especially in the low density regions. At higher redshifts, the SPT and power-law responses converge as the density field becomes more Gaussian.
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