| Age | Commit message (Collapse) | Author | |
|---|---|---|---|
| 2019-05-14 | add --plot-likelihood option to fit | tlatorre | |
| 2019-03-26 | update plotting scripts to handle case when there is no fit | tlatorre | |
| 2019-03-16 | add GPLv3 license | tlatorre | |
| 2019-01-15 | update zebra library to be able to use links | tlatorre | |
| This commit updates the zebra library files zebra.{c,h} so that it's now possible to traverse the data structure using links! This was originally motivated by wanting to figure out which MC particles were generated from the MCGN bank (from which it's only possible to access the tracks and vertices using structural links). I've also added a new test to test-zebra which checks the consistency of all of the next/up/orig, structural, and reference links in a zebra file. | |||
| 2018-12-03 | update plot | tlatorre | |
| 2018-12-03 | add a goodness of fit parameter psi to the fit | tlatorre | |
| 2018-11-30 | update plot-fit-results to handle masked arrays properly | tlatorre | |
| 2018-11-30 | rename plot.py -> plot | tlatorre | |
| 2018-11-25 | add a script to plot the fit results as a function of energy | tlatorre | |
| 2018-11-14 | update plot.py to plot the distribution of fit times | tlatorre | |
| 2018-11-14 | update plot.py | tlatorre | |
| 2018-11-14 | update plot.py | tlatorre | |
| 2018-11-14 | update plot.py to plot the log likelihood ratio | tlatorre | |
| 2018-11-14 | update yaml format to store fit results as a dictionary indexed by the ↵ | tlatorre | |
| particle id | |||
| 2018-10-22 | update plot.py | tlatorre | |
| 2018-10-22 | update plot.py to plot the angular resolution | tlatorre | |
| 2018-10-11 | update plot.py | tlatorre | |
| - determine bin width using the Freedman Diaconis rule - print out error on the standard deviation | |||
| 2018-10-03 | move python scripts into utils/ directory | tlatorre | |
 |
index : sddm | |
| Code for the self-destructing dark matter search in SNO | Anthony LaTorre |
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