Key: - To do p Partially done ^ Done ? Not sure if it's done - write cross section section in paper - explain integral in paper p develop signal generator - made signal generator for two particle decays p develop high energy and multi-ring fitter ^ write talk for Monday - write a section on atmospheric backgrounds in paper ^ check index of refraction calculation against tables in the paper ^ write more tests for the solid angle calculation - use table from paper ^ make sure normal direction is normalized ^ speed up likelihood calculation - rotate and translate path points in path_init - create fast interp1d for equally spaced points - optimize with -O2 - only calculate average time if mu_direct[i] is not too small and PMT is hit - add likelihood function which calculates total expected charge and only loops over hit PMTs - add fast likelihood which doesn't use a 2D lookup table - add function to compute the Hessian via finite differences - add function to calculate covariance matrix - add function to compute the approximate volume in the likelihood space where the likelihood is greater than some value ^ add output to likelihood ^ add a set of seed points to start the likelihood ^ minimize the likelihood in a do while loop until it converges to a single point ^ once the first position is found, compute the Hough transform to look for other rings p add rayleigh scattering to likelihood function - Done, but it's pretty hacky p add muon shower PDF? delta rays? - Done for delta rays, but need to add shower photons - calculate path length through acrylic? p update estar table with energies above 1 GeV - added values up to 10 GeV ^ speed up normalize() and interp1d() ^ add shower PDF to get_total_charge_approx() x compute mean of starting points ^ speed up time PDF calculation for fast likelihood p calculate psi parameter as a goodness of fit test - Still need to tweak this. It seems to have a strong nhit dependence ^ add a maximum length for the range - now only fit to the end of the PSUP ^ add a time limit for the fit ^ multi-particle fit p optimize CHARGE_FRACTION ? find out why likelihood is sometimes returning nan ^ add pdf for cerenkov light from delta rays - tweak find peaks algorithm ^ update zebra to allow use of links - minimum energy for each particle type ^ check all zebra links ^ fix zero logical record size bug in zebra.c p speed up fit - have optimized most of the likelihood function. I think further optimization will require a different technique for evaluating the integrals ^ nhit cut p add flasher cut p default max particles - submit-grid-jobs fits up to 3 particles by default ^ add environment variable to control where to look for pmt.txt and titles files p update charge code to handle highest values for qhs and qlx - don't have this coded into the charge probability code, but I now use QHL if QHS is railed and flag any PMT with a railed QHL ^ use qhs and qlx based on variable in PMT bank - Note: I don't use the best charge variable in the PMT bank, but I do select QHL when QHS is railed ^ fix bug in path_init() ^ load DQXX file based on run number ^ update rayleigh scattering lengths ^ fix delta ray calculation p figure out why electron energy bias is +10% - updated code to use a more accurate approximation for the number of shower photons which seems to bring the bias down to 5% - update find peaks algorithm to do single particle quick fits ^ figure out how to combine SNO fitter data with my fitter for final analysis. For example, how to apply neutron follower cut? - double check that zdab-reprocess is correct for the D2O and salt phases since it appears to be from the NCD phase - add code to compute expected deviation from nll_best to normalize psi - add term to likelihood for probability that a channel is misccalibrated or didn't make it into the event - when calculating the first order statistic for a gaussian is alpha = pi/8 a better choice than 0.375? - speed up charge initialization - determine *real* mean and standard deviation of single PE charge distribution. TELLIE SNO+ data? - extend electron range table - fix time PDF. Currently take the first order statistic of dark noise + indirect light + direct light all together, but this isn't correct.