| Age | Commit message (Collapse) | Author | |
|---|---|---|---|
| 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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