To simplify downloads and file management, maps have been grouped into tar files.
Model | OmegaM | w | h | n | sig8 |
21&22 | 0.25 | -1.0 | 0.72 | 0.97 | 0.80 |
23&24 | 0.25 | -1.0 | 0.72 | 0.97 | 0.75 |
Parameters for the models run.
For each cosmological model two independent sets of initial conditions are
generated. All models are spatially flat, so Omega_de=1-OmegaM.
For all models the baryon density OmegaBh^2=0.0224 -- our results are very
insensitive to this choice.
All models have power-law spectra (no running) with index n and the dark
energy has a constant equation of state w.
Name | Size (MB) | Last modified |
shear.021.01.tar | 192 | 2006/10/03 |
shear.021.02.tar | 192 | 2006/10/03 |
shear.021.03.tar | 192 | 2006/10/03 |
shear.021.04.tar | 192 | 2006/10/03 |
shear.022.01.tar | 192 | 2006/10/03 |
shear.022.02.tar | 192 | 2006/10/03 |
shear.022.03.tar | 192 | 2006/10/03 |
shear.022.04.tar | 192 | 2006/10/03 |
shear.023.01.tar | 192 | 2006/10/03 |
shear.023.02.tar | 192 | 2006/10/03 |
shear.023.03.tar | 192 | 2006/10/03 |
shear.023.04.tar | 192 | 2006/10/03 |
shear.024.01.tar | 192 | 2006/10/03 |
shear.024.02.tar | 192 | 2006/10/03 |
shear.024.03.tar | 192 | 2006/10/03 |
shear.024.04.tar | 192 | 2006/10/03 |
Last modified Tue Oct 3 17:41:43 2006