GLAM simulations
If you use this data please cite the paper by
Klypin & Prada (2018)

GLAM simulations are done using the new Parallel Particle-Mesh GLAM code, see also Klypin & Prada (2018) for details. We provide a number of different products for these simulations. These include non-linear dark matter power spectra and density distribution functions (PDF), halo catalogs, and raw particle data for some simulations.

For A-series simulations we provide non-linear dark matter power spectra and density distribution functions (PDF). The GLAM A-series simulations have been performed on the Finisterrae II supercomputer at the Centro de Supercomputación de Galicia (CESGA).

GLAM_Aseries

Halo catalogs are provided for the PMILL (P-Millennium), MD (MultiDark) and Uchuu series. We also provide galaxy mock catalogs for some of them, and raw particle data if indicated.

PMILL_1.0Gpc
Cosmo: P-Millennium
Box
: 1000 Mpc/h
Particles
: 2000**3
Ngrid: 4000**3
M_p: 1.06e10 Msun/h
Time-steps: 136
Soft. length:
0.25 Mpc/h
Realizations:
1000
Run: DiRAC@Durham
MD_1.0Gpc
Cosmo: MD-Planck
Box
: 1000 Mpc/h
Particles
: 2000**3
Ngrid: 4000**3
M_p: 1.06e10 Msun/h
Time-steps: 136
Soft. length:
0.25 Mpc/h
Realizations:

Run:
Uchuu_1.0Gpc
Cosmo: Uchuu
Box
: 1000 Mpc/h
Particles
: 2000**3
Ngrid: 4000**3
M_p: 1.06e10 Msun/h
Time-steps: 136
Soft. length:
0.25 Mpc/h
Realizations:

Run: