| Commit message (Collapse) | Author | Age | Files | Lines | |
|---|---|---|---|---|---|
| * | halo.py: Rewrite "_coef_acceleration()" method | Aaron LI | 2017-06-01 | 1 | -15/+44 |
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| * | Bind ClusterFormation to HaloSingle | Aaron LI | 2017-06-01 | 1 | -1/+4 |
| | | | | | Also add logging messages to simulate_mergertree() | ||||
| * | Update to use custom units.py instead of astropy's | Aaron LI | 2017-06-01 | 1 | -40/+26 |
| | | | | | Also fix a parameter error in "formation.py" | ||||
| * | halo.py: Update to match MergerTree structures | Aaron LI | 2017-06-01 | 1 | -8/+8 |
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| * | halo.py: Force a minimal value on acceleration coefficient | Aaron LI | 2017-06-01 | 1 | -1/+25 |
| | | | | | | | | To avoid the too small (or zero) values for the diffusion coefficient of the Fokker-Planck equation. Also change config "extragalactic/halo/pmax" from 1e4 to 1e5 | ||||
| * | clusters/halo: Add missing config "buffer_np" | Aaron LI | 2017-06-01 | 1 | -0/+2 |
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| * | Add clusters/halo.py: simulate single halo for cluster | Aaron LI | 2017-06-01 | 1 | -0/+698 |
| Simulate (giant) radio halos following the "statistical magneto-turbulent model" proposed by Cassano & Brunetti (2005). | |||||
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index : fg21sim.git | |
| Simulate foreground for 21cm EoR signal detection | Git Repositories Owner |
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