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| author | tlatorre <tlatorre@uchicago.edu> | 2019-01-27 21:08:25 -0600 |
|---|---|---|
| committer | tlatorre <tlatorre@uchicago.edu> | 2019-01-27 21:08:25 -0600 |
| commit | 1d77bacaae25d40d160f2bcd14ba3a355921213e (patch) | |
| tree | ad283c9c0d7bfd5326690bc43af7c82c5a1bb40d /src/find_peaks.c | |
| parent | b9491718282f86b77c2594f161b096903706edc1 (diff) | |
| download | sddm-1d77bacaae25d40d160f2bcd14ba3a355921213e.tar.gz sddm-1d77bacaae25d40d160f2bcd14ba3a355921213e.tar.bz2 sddm-1d77bacaae25d40d160f2bcd14ba3a355921213e.zip | |
add photons from delta rays to likelihood calculation
This commit updates the likelihood function to take into account Cerenkov light
produced from delta rays produced by muons. The angular distribution of this
light is currently assumed to be constant along the track and parameterized in
the same way as the Cerenkov light from an electromagnetic shower. Currently I
assume the light is produced uniformly along the track which isn't exactly
correct, but should be good enough.
Diffstat (limited to 'src/find_peaks.c')
0 files changed, 0 insertions, 0 deletions