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| author | tlatorre <tlatorre@uchicago.edu> | 2019-06-26 14:45:26 -0500 | 
|---|---|---|
| committer | tlatorre <tlatorre@uchicago.edu> | 2019-06-26 14:45:26 -0500 | 
| commit | 5016143a42b57c47e9916bbb70de2ae2669cbc8f (patch) | |
| tree | 874ec6948abe3b0671c9962ac9d585e49d9a1422 /utils/gen-dark-matter | |
| parent | d4cb7e14b54e4f4510fd73d1b3e219eaaffbe081 (diff) | |
| download | sddm-5016143a42b57c47e9916bbb70de2ae2669cbc8f.tar.gz sddm-5016143a42b57c47e9916bbb70de2ae2669cbc8f.tar.bz2 sddm-5016143a42b57c47e9916bbb70de2ae2669cbc8f.zip  | |
plot Michel electrons and muons in plot-energy
This commit is a major update to the plot-energy script. The most significant
changes are:
- new prompt event selection
    We now define prompt events as any event >= 100 nhit which is at least 250
    ms away from the last 100 nhit event.
- add Michel electron event selection.
    Michel electrons are now selected as any event between 800 ns and 20
    microseconds after a muon or prompt event. Additionally they are required
    to be >= 100 nhit and pass an extra set of data cleaning cuts (compared to
    the prompt events).
- add an atmospheric "sideband"
    I also updated the script to plot the energy distribution and particle ID
    for all events that *do* have a neutron follower as a kind of sideband
    which should contain only atmospheric events.
- plot muon energy spectrum and angular distribution
Diffstat (limited to 'utils/gen-dark-matter')
0 files changed, 0 insertions, 0 deletions
