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authorAaron LI <aly@aaronly.me>2017-10-18 16:14:59 +0800
committerAaron LI <aly@aaronly.me>2017-10-18 16:16:18 +0800
commit375198fb380933ea1b00f2e42401550ae20da76d (patch)
tree966fa37fd3e1b5f5f32c0ad30f927524f7d40f39 /tests/context.py
parent3dadf7b53f28af00f3170a10629c91e8d2888e0e (diff)
downloadfg21sim-375198fb380933ea1b00f2e42401550ae20da76d.tar.bz2
clusters: Update radio halo radius estimation
The simulated radio halo is assumed to have a radius of the falling sub-cluster; while previously it is assumed to be 1/4 of the virial radius of the merged cluster. The new estimation can agree better with the currently observed radio halos, which generally have a angular diameter size of ~2-7 [arcmin].
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