GLAM simulations are done using a Parallel Particle-Mesh (PM) code. See Klypin & Prada (2016) for details.
We provide a number of different products for these simulations. This includes raw particle data for some simulations. For A-series simulations we provide the non-linear dark matter power spectra and density distribution functions (PDF). Halo catalogs are provided for C-series simulations.
We provide a number of different products for these simulations. This includes raw particle data for some simulations. For A-series simulations we provide the non-linear dark matter power spectra and density distribution functions (PDF). Halo catalogs are provided for C-series simulations.
C1.4_1.36Gpc
Box :        1360 Mpc/h
Particles:   1400**3
Ngrid :       3400**3
Mass_p :   7.8e10 Msun/h
Dx :          0.4 Mpc/h
Realizations:   300
40 snapshots with BDM
Box :        1360 Mpc/h
Particles:   1400**3
Ngrid :       3400**3
Mass_p :   7.8e10 Msun/h
Dx :          0.4 Mpc/h
Realizations:   300
40 snapshots with BDM
C1.0_1.0Gpc
Box :        1000 Mpc/h
Particles:   1500**3
Ngrid :       3000**3
Mass_p :   2.5e10 Msun/h
Dx :          0.33 Mpc/h
Realizations:   700
30 snapshots with BDM
Box :        1000 Mpc/h
Particles:   1500**3
Ngrid :       3000**3
Mass_p :   2.5e10 Msun/h
Dx :          0.33 Mpc/h
Realizations:   700
30 snapshots with BDM
C1.2_1.2Gpc
Box :        1200 Mpc/h
Particles:   2000**3
Ngrid :       5000**3
Mass_p :   1.84e10 Msun/h
Dx :          0.24 Mpc/h
Realizations:   70
30 snapshots with BDM
Box :        1200 Mpc/h
Particles:   2000**3
Ngrid :       5000**3
Mass_p :   1.84e10 Msun/h
Dx :          0.24 Mpc/h
Realizations:   70
30 snapshots with BDM