1 code implementation • 7 Aug 2020 • Masato Shirasaki, Eric M. Huff, Katarina Markovic, Jason D. Rhodes
At the length scales of $r=5-40\, [h^{-1}\, \mathrm{Mpc}]$, our model predicts the mean and dispersion of the pairwise velocity for dark matter halos with their masses of $10^{12. 5-13. 5} \, [h^{-1}M_{\odot}]$ at $0. 3 < z < 1$ with a 5%-level precision, while the model precision reaches a 20% level (mostly a 10% level) for other masses and redshifts explored in the simulations.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
