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2019-03-16add GPLv3 licensetlatorre
2018-11-17speed up likelihood function and switch to using fixed dxtlatorre
This commit speeds up the likelihood function by about ~20% by using the precomputed track positions, directions, times, etc. instead of interpolating them on the fly. It also switches to computing the number of points to integrate along the track by dividing the track length by a specified distance, currently set to 1 cm. This should hopefully speed things up for lower energies and result in more stable fits at high energies.
2018-10-18update fit to fit for electrons and protonstlatorre
2018-10-17fix a bug in the theta0 calculation for a pathtlatorre
This commit fixes a bug in the calculation of the average rms width of the angular distribution for a path with a KL expansion. I also made a lot of updates to the test-path program: - plot the distribution of the KL expansion coefficients - plot the standard deviation of the angular distribution as a function of distance along with the prediction - plot the simulated and reconstructed path in 3D
2018-09-17update muon kinetic energy calculationtlatorre
This commit updates the calculation of the muon kinetic energy as a function of distance along the track. Previously I was using an approximation from the PDG, but it doesn't seem to be very accurate and won't generalize to the case of electrons. The kinetic energy is now calculated using the tabulated values of dE/dx as a function of energy.
2018-08-31add theta0 argument to path_eval in test-path.ctlatorre
2018-08-27add code to expand the track of a particle using a KL expansiontlatorre
To fit the path of muons and electrons I use the Karhunen-Loeve expansion of a random 2D walk in the polar angle in x and y. This allows you to decompose the path into a sum over sine functions whose coefficients become random variables. The nice thing about fitting the path in this way is that you can capture *most* of the variation in the path using a small number of variables by only summing over the first N terms in the expansion and it is easy to calculate the probability of the coefficients since they are all uncorrelated.