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

Age	Commit message (Collapse)	Author
2019-06-14	add a function to compute the most likely number of PE given an observed charge	tlatorre
	Also, call this function when computing the psi parameter in nll_best().
2019-03-26	small update to the charge likelihood calculation	tlatorre
	This commit updates the charge likelihood calculation to calculate: P(hit,q\|n) = P(q\|hit,n)*P(hit\|n) This has almost no effect on the fit results, but is technically correct.
2019-03-16	add GPLv3 license	tlatorre

2018-11-28	update sno_charge.c	tlatorre
	This commit adds lots of comments to sno_charge.c and makes a couple of other changes: - use interp1d() instead of the GSL interpolation routines - increase MAX_PE to 100 I increased MAX_PE because I determined that it had a rather large impact on the likelihood function for 500 MeV electrons. This unfortunately slows down the initialization by a lot. I think I could speed this up by convolving the single PE charge distribution with a gaussian before convolving the charge distributions to compute the charge distributions for multiple PE.
2018-11-27	a bunch of small changes to speed things up	tlatorre

2018-09-18	add free_charge() to free memory used to interpolate the charge distributions	tlatorre

2018-09-10	add a fast likelihood function	tlatorre
	This commit adds a fast function to calculate the expected number of PE at a PMT without numerically integrating over the track. This calculation is much faster than integrating over the track (~30 ms compared to several seconds) and so we use it during the "quick" minimization phase of the fit to quickly find the best position.
2018-08-14	move everything to src directory	tlatorre