Therefore, the original version’s conclusion that the impact of the baryon effect on cosmological constraints is not significant remains unchanged. This results in an underestimation of |$S_8=\sigma _8\sqrt$|. Owing to this bug, the nonlinear matter power spectrum on quasi-nonlinear scales was overestimated by >8%, leading to an overestimation of the cosmic shear two-point correlation function (TPCF) of approximately 6% on scales used in this study. Mention the characteristics of TEM waves. Write down the expression for cut off frequency when the wave is propagated in between two parallel plates. ( 2012) as an improvement in the halofit model of Smith et al. It is the wavelength below which there is wave propagation and above which there is no wave propagation. We found that an incorrect numerical coefficient was used in the code to compute the fitting function of the nonlinear matter power spectrum, given by Takahashi et al. The first bug affects the fiducial model adopted in this study. Here we present revised results obtained from corrected computations. In the original publication of “Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data”, we discovered a couple of bugs in the software used for numerical computations.
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