Fig. 1
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Constraints on the parameters in Eq. (19) fitted to the unbiased standard deviation of the 200 PINOCCHIO mocks with C0 cosmology. We fitted α and β considering k ≤ 0.05 h Mpc−1, assuming a Gaussian likelihood with error bar estimated from the measurements for 0.05 ≤ k/h Mpc−1 ≤ 0.2 and assuming it to be constant in k and equivalent to the unbiased standard deviation.
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