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| author | tlatorre <tlatorre@uchicago.edu> | 2020-08-17 11:10:03 -0500 |
|---|---|---|
| committer | tlatorre <tlatorre@uchicago.edu> | 2020-08-17 11:10:03 -0500 |
| commit | 3bcde006dcff72bfb1f3dd7ff052b501393f1125 (patch) | |
| tree | 6df17555932ce3234a67d02b4d598c86d82d6243 /snoman.ratdb | |
| parent | 5b4efebc67641001660bbfca1458d9a5f99ae886 (diff) | |
| download | sddm-3bcde006dcff72bfb1f3dd7ff052b501393f1125.tar.gz sddm-3bcde006dcff72bfb1f3dd7ff052b501393f1125.tar.bz2 sddm-3bcde006dcff72bfb1f3dd7ff052b501393f1125.zip | |
update function to tag atmospherics
Previously the function to tag atmospherics was looking at the *first*
event to come after a prompt event and checking to see if it was a
neutron. However, this has a huge issue in that for large energy events,
there is often secondary events caused by afterpulsing.
I've now updated the algorithm to look for any events in which there is
*any* follower event that passes the neutron criteria.
Diffstat (limited to 'snoman.ratdb')
0 files changed, 0 insertions, 0 deletions