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2020-09-07update python scripts to not call plt.show() when run with --savetlatorre
2020-08-31add estimate_errors to chi2 analysistlatorre
This commit updates the estimate_errors() function so that it works without a list of constraints and uses arrays of low and high bounds passed in instead of hardcoded constraints. I can now call this function from the chi2 analysis to get the stepsizes before running the MCMC.
2020-08-30update dc scriptstlatorre
- delete instrumental tags in both scripts since we already tag them in get_events() - apply the same cuts to the MC as to the data - add a comment about the fitted fraction - quit if we don't have at least 1 type of each instrumental
2020-07-27add 20 MeV cut to dc, dc-closure-test, and plot-dctlatorre
2020-07-27loop over runs in dc, dc-closure-test, and plot-dc to prevent using too much ↵tlatorre
memory
2020-06-14update dc and dc-closure-test to take into account fitted fraction of ↵tlatorre
instrumentals This commit updates the contamination analysis scripts to take into account the fact that we only fit a fraction of some of the instrumental events. Based on the recent rate at which my jobs have been running on the grid, fitting all the events would take *way* too long. Therefore, I'm now planning to only fit 10% of muon, flasher, and neck events. With this commit the contamination analysis will now correctly take into account the fact that we aren't fitting all the instrumental events.
2020-05-31update contamination analysis step sizetlatorre
This commit updates the step size used for the MCMC in the contamination analysis to 0.5 times the error returned by scanning near the minimum. I ran some tests and this seemed to be pretty efficient compared to either the full error or 0.1 times the error. I also reduced the number of workers to 10.
2020-05-25update contamination analysis stufftlatorre
- fix Constraint.renormalize_no_fix() which could enter an infinite loop if the fixed parameter was greater than 1 - EPSILON - don't divide by psi twice in get_events() - only use prompt events and cut on nhit_cal < 100
2020-05-12speed up the contamination analysis scripttlatorre
2020-05-12add a script to do a closure test on the contamination analysistlatorre
2020-05-11update ockham factor, remove hack, and don't submit all flasherstlatorre
This commit contains the following updates: - remove hack to get rid of low energy events in plot-energy since while writing the unidoc I realized it's not necessary now that we add +100 to multi-particle fits - update Ockham factor to use an energy resolution of 5% - update submit-grid-jobs to submit jobs according to the following criteria: - always submit prompt events with no data cleaning cuts - submit 10% of prompt flasher events - submit all other prompt events - submit followers only if they have no data cleaning cuts - update submit-grid-jobs to place the nhit cut of 100 on the calibrated nhit
2020-05-11update utils/ folder to make a python package called sddmtlatorre
This commit adds an sddm python package to the utils/ folder. This allows me to consolidate code used across all the various scripts. This package is now installed by default to /home/tlatorre/local/lib/python2.7/site-packages so you should add the following to your .bashrc file: export PYTHONPATH=$HOME/local/lib/python2.7/site-packages/:$PYTHONPATH before using the scripts installed to ~/local/bin.
2020-01-13update script to calculate contaminationtlatorre
This commit updates the dc script to calculate the instrumental contamination to now treat all 4 high level variables as correlated for muons. Previously I had assumed that the reconstructed radius was independent from udotr, z, and psi, but based on the corner plots it seems like the radius is strongly correlated with udotr. I also updated the plotting code when using the save command line argument to be similar to plot-fit-results.
2020-01-06add script to calculate background contaminationtlatorre
This commit adds a script to calculate the background contamination using a method inspired by the bifurcated analysis method used in SNO. The method works by looking at the distribution of several high level variables (radius, udotr, psi, and reconstructed z position) for events tagged by the different data cleaning cuts and assuming that any background events which sneak past the data cleaning cuts will have a similar distribution (for certain backgrounds this is assumed and for others I will actually test this assumption. For more details see the unidoc). Then, by looking at the distribution of these high level variables for all the untagged events we can use a maximum likelihood fit to determine the residual contamination. There are also a few other updates to the plot-energy script: - add a --dc command line argument to plot corner plots for the high level variables used in the contamination analysis - add a fudge factor to the Ockham factor of 100 per extra particle - fix a bug by correctly setting the final kinetic energy to the sum of the individual kinetic energies instead of just the first particle - fix calculation of prompt events by applying at the run level