sddm - Code for the self-destructing dark matter search in SNO

Age	Commit message (Collapse)	Author
2019-07-29	switch to using the multiphoton PCA time	tlatorre
	This commit updates the likelihood to use the multiphoton PCA time instead of the usual pt time. When looking at the reconstruction of muons in run 10,000 I noticed that the PMT hit times for the PMTs which had really high charge was all over the place. There were PMTs that were very close to each other with hit times differing by ~ 20 ns. I'm still not entirely sure what causes this (is it some hardware issue with the discriminator or is it a problem with the charge walk correction which always assumes a single PE?), but the multiphoton PCA times looked a lot more reasonable. Eventually I need to look into the ptms variable which is the multiphoton PCA transit time RMS.
2019-07-16	update neck tube cut to include time difference changes due to cable changes	tlatorre

2019-07-16	use QLX if QHS is railed	tlatorre

2019-06-14	add trigger word and trigger time in ns to the YAML file	tlatorre

2019-06-14	update flasher cut to use pt1 instead of ept	tlatorre
	Small update to the flasher cut to use the non-walk corrected time instead of just the ECA calibrated time. Also added some comments to the variables in the event structure.
2019-06-14	forgot to add event.h	tlatorre

2019-06-10	add a bunch of SNO data quality cuts	tlatorre
	This commit adds the following data quality cuts used in SNOMAN: - neck - qvnhit - crate isotropy - junk Still need to test these.
2019-03-16	add GPLv3 license	tlatorre

2019-03-07	update fit to automatically load DQXX file based on run number	tlatorre

2019-03-04	add a function to tag flasher events	tlatorre

2018-08-14	update pmt hit array in event struct to be MAX_PMTS long	tlatorre

2018-08-14	move everything to src directory	tlatorre