COSMOLOGICAL PARAMETERS
Omega_m = 0.307115
Omega_Lambda = 0.692885
Omega_bar = 0.048206
sigma_8 = 0.8288
h = 0.6777
ns = 0.9611

SPECTRUM P(k)
Planck_z99.dat


SIMULATION PARAMETERS

--- L512 ---
Box = 32.0 Mpc/h
npart = 512^3
Mpart = 2e7 Msun/h
softening = 1.5 kpc/h
zinit = 99

--- L4km ---
Box = 32.0 Mpc/h
Mpart = 4e4 Msun/h (effective number of particles 4096^3)
softening = 0.2 kpc/h
zoom cnter x,y,z = 7, 18, 10 Mpc/h
zoom region radius = 3 Mpc/h
overdensity in zoom sphere = 1.02
zinit = 99

--- L4ku ---
Box = 32.0 Mpc/h
Mpart = 4e4 Msun/h (effective number of particles 4096^3)
softening = 0.2 kpc/h
zoom cnter x,y,z = 22, 12, 17 Mpc/h
zoom region radius = 5 Mpc/h
overdensity in zoom sphere = 0.37
zinit = 99

--- L4ko ---
Box = 32.0 Mpc/h
Mpart = 4e4 Msun/h (effective number of particles 4096^3)
softening = 0.2 kpc/h
zoom cnter x,y,z = 12, 23, 11 Mpc/h
zoom region radius = 3 Mpc/h
overdensity in zoom sphere = 2.15
zinit = 99



HALOS
Rockstar version: 0.99.9-RC3 with modification described in Pilipenko et al. 2017

Note that in the Pilipenko et al. 2017 we used only M200c and Vmax to calculate concentrations! I.e. we did not use rs and rs_klypin produced by Rockstar.

For zoom simulations, to safely select halos without contamination by heavy particles, one should use only halos within (R-0.4 Mpc/h) radius from the center of the zoom region.