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############################################################################### * * .oooooo..o oooooooooo. ooooo ooo .o88o. o8o . * d8P' `Y8 `888' `Y8b `888b. `8' 888 `" `"' .o8 * Y88bo. 888 888 8 `88b. 8 o888oo oooo .o888oo * `"Y8888o. 888oooo888' 8 `88b. 8 888 `888 888 * `"Y88b 888 `88b 8 `88b.8 888 888 888 * oo .d8P 888 .88P 8 `888 888 888 888 . * 8""88888P' o888bood8P' o8o `8 o888o o888o "888" * * SBNfit, fitter, oscillator, covariance matrix maker, collapser * originally for sterile decays at SBL facilities * but actually pretty generic * * If you have any questions, queries or comments please contact the authors; * [email protected] * [email protected] * *The authors make no guarrentee of the behaviour, stability or bug-free-ness of this code. ###################################################i############################# This is a trimmed down version of SBNfit for usage in uBooNE. It does not have full functionality yet, things are being migrated in/checked and documentated. ########################################## Building and compiling ######################################## The CMakeLists should be a standard and generic enough to work on most machines, although I have not tested it everywhere. It should also be simple enough to fix if it doesn't work out-of-the-box. For an introduction see: https://microboone-docdb.fnal.gov/cgi-bin/private/ShowDocument?docid=17092 Attention: Please see the github wiki for most up to date documentation https://github.com/markrosslonergan/whipping_star/wiki #Instructions for GPVM based building and running. While in base git directory source .setup.sh #To Build, should work out of the box on GPVM with above setup cd build cmake .. make This will build the SBNfit source and libraries, as well as executable example programs in build/example The included simple examples are not physically accurate, just toy MC! cd examples #The first example builds a covariance matrix from eventweight std::map<std::string,std::vector<double>> objects ./example1 --xml example.xml --print should have 4 output files, first two data, second two human readable plots EXAMPLE1.SBNspec.root : The central value spectra EXAMPLE1.SBNcovar.root : The full and fractional covariance matricies SBNfit_spectrum_plots_EXAMPLE1.root : The central value plots, but subchannels stacked to represent a channel SBNfit_covariance_plots_EXAMPLE1.root : The covariance matricies plotted as TH2D nicely. Inside directory individualDir is all the individual variation matricies #The second example loads up the computed covariance matrix and makes a plot of the chi^2 as you scale the signal for stats and stats+sys ./example2 --xml example.xml should have 1 output. EXAMPLE2_plots.root containing a simple TCanvas showing the chi^2 behaviour For an older out of date tutorial: https://docs.google.com/presentation/d/1vLYPDaID0a4nbx5rnKTda_RzhdTavLdyrkpkGMVZLgE/edit#slide=id.g35c91f84c5_0_194 ############################################################################ ############## TODO ######################################## ############################################################################ (1) Being able to fill SBNfit histograms (subchannels) from functions of inputted variables. e.g fill "ereco" to nu_uBooNE_elike_intrinsic if "nupdg==1" or nu_uBooNE_mlike_otherwise (2) DONE. -- Being able to see all individual histograms and how they change for all the universes (3) Being able to make covariance matrix from detetcor systematic MC files (4) Pull terms (5) Examples for oscillations (6) DONE. -- Example for Frequentist Studies
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