- [model] is a number running from 21-24, indicating the model number that this file corresponds to (see below).
- [map] is a number running from 1-16 indicating the realization.
- [src] is a number describing what the source distribution assumed is
- 01: Sources with zbar=1.0, beta=1.5
- 02: Sources with zbar=1.5, beta=1.5
- 03: Sources with zbar=1.0, beta=1.0
- 04: Sources with zbar=1.5, beta=1.0

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*