no code implementations • 22 May 2018 • Xiangchong Li, Nobuhiko Katayama, Masamune Oguri, Surhud More
(i) For simulations which only contain isolated galaxies, the amplitude of multiplicative bias is below 1 % .
Cosmology and Nongalactic Astrophysics
1 code implementation • 13 Aug 2012 • Ryuichi Takahashi, Masanori Sato, Takahiro Nishimichi, Atsushi Taruya, Masamune Oguri
The simulation results are used to re-calibrate the fitting parameters of the halofit model so as to reproduce small-scale power spectra of the $N$-body simulations, while keeping the precision at large scales.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
