Package iceCube.uhe.analysis

Package icecube.uhe.analysis

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Description

Class Summary

AtmMuonBundleFitter	This class provides methods to fit I3Particles with the CEL approximated AtmMuonBundle flux or precalculated fluxes by PropagatingAtmMuonFlux.
BHevapPropagationMatrixFlux	It calculates the detectable neutrino event intensity at the Earth Surface as I3ParticleFlux does but the calculation is made by using directly the zenith angle binned propagation matrix and the numerically calculated effective area (I3EffectiveArea.java) without relying on I3Particle MC events.
Criteria	Criteria class defines requrements of the IceCube EHE events that are subject to futher analysis.
CriteriaIC22
DrawAtmMuonBundle
DrawAtmMuonBundle2D
DrawAtmMuonBundleByElbertFluxTable
DrawAtmMuonBundleByRelativeWeight
DrawAtmMuonBundleCombined
DrawAtmMuonBundleFluxRatio
DrawBGSpectrumByJaidaHisto
DrawEffAreaTable
DrawInIceEffArea	Draw the in-ice effective area table by running I3ParticleFlux.getInIceEffectiveArea(double logEnergy, double cosZenith, int flavor, int doublet).
DrawNuEffAreaByAreaTable	Calculate the neutrino detection effective area [km^2 sr] (neutrino interaction probability convoluted) by running PropagationMatrixFlux with EffAreaTable class.
DrawNuEffAreaByI3Particle	Calculate the neutrino detection effective area [km^2 sr] (neutrino interaction probability convoluted) by running I3ParticleFlux.
DumpQuickNCPropagationMatrixYield	Calculate the neutrino detection yield by running ProrpagationMatrixFlux and write it to the standard output.
DumpQuickPropagationMatrixYield	Calculate the neutrino detection yield by running ProrpagationMatrixFlux and write it to the standard output.
EffAreaTable	(In-ice) Effective Area is calculated from the numerical table stored in the classes/iceCube/uhe/analysis.
EnergyHistogramMaker	This class makes a 2D histogram of Energy correlations like Muon In-ice Energy Vs Primary Cosmic Ray enegry (obtained by AtmMuonBundleFlux.java in the MuonModel package) or Muon In-ice Energy Vs Muon Surface Energy (using PropagationMatrixFactory.java in the propahgation package) Written by S.
FitElbertModelFixedEthWithIC9Data	Fit the IC9 data with the Elbert Formula using AtmMuonBundleFetter class.
FitElbertModelWithIC9Data	Fit the IC9 data with the Elbert Formula using AtmMuonBundleFetter class.
I3ParticleAnalysisFactory	I3Particles Analysis Factory.
I3ParticleBuilder	Build IceCube event(s) reading from the f2k data via standard input.
I3ParticleBuilderDemo	I3Particle.class Demo program.
I3ParticleCorsikaWeightFiller
I3ParticleCREnergyDistFiller
I3ParticleFlux	I3ParticleFlux calculates the detectable neutrino event intensity at the Earth Surface using propagation matrix filled in each of I3Particle.
I3ParticleGZKWeightFiller
I3ParticleIC22AnalysisFactory	I3Particles Analysis Factory for the IC22 data.
I3ParticleMCPrimaryWeightFiller	This class provides the methods to fill I3Particles with MC primary spectrum weights.
I3ParticlePropMatrixFiller	This class provides the methods to fill I3Particles with the pregenerated propagation matrix.
I3ParticleWeightFiller	This class provides the methods to fill I3Particles with GZK and Atmospheric muon weights.
JaidaPlotStyleSetter
MakeBootstrapBGSpectrum
MakeEffAreaTable	Calculate the in-ice effective area table by running I3ParticleFlux.getInIceEffectiveArea(double logEnergy, double cosZenith, int flavor, int doublet).
MakeQuickPropagationYieldMap	Calculate the neutrino detection yield by running QuickProrpagationMatrixFlux and Make a Map(log(Neutrino Energy) Map(cross section, yield)).
MergeI3Particles
NPEthresholdOptimizer	Optimize NPE threshold to minimize either the model rejection potential or the signal discovery potential.
PlotAllSpectrum
PlotChi2ByJaidaHisto
PlotCRSpectrum
PlotEventNumberRatioByJaidaHisto
PlotIC22BG2DSpectrum
PlotIC22SIG2DSpectrum
PlotIC22Spectrum
PlotSpectrumByJaidaHisto
PropagationMatrixDrawer	This class makes a 2D/1D histogram of Energy correlations of In-ice Energy Vs Surface Energy (using PropagationMatrixFactory.java in the propahgation package) Written by S.
PropagationMatrixFlux	It calculates the detectable neutrino event intensity at the Earth Surface as I3ParticleFlux does but the calculation is made by using directly the zenith angle binned propagation matrix and the numerically calculated effective area (I3EffectiveArea.java) without relying on I3Particle MC events.
QuickNCPropagationMatrixFlux	It calculates the detectable neutrino event intensity at the Earth Surface as I3ParticleFlux does but the calculation is made by using directly the zenith angle binned propagation matrix and the numerically calculated effective area (I3EffectiveArea.java) without relying on I3Particle MC events.
QuickPropagationMatrixFlux	It calculates the detectable neutrino event intensity at the Earth Surface as I3ParticleFlux does but the calculation is made by using the calculated energy distribution by NeutrinoQuickPropagator class and the numerically calculated effective area (I3EffectiveArea.java) without relying on I3Particle MC events.
RunAnalysis
RunAtmMuonBundleCombinedFitter
RunAtmMuonBundleFitter
RunI3ParticleBuilder	Run I3ParticleBulder to generate a series of I3Particles.
RunI3ParticleFlux	Calculate the detectable Neutrino flux [GeV/cm^2 sec sr] at the surface by running I3ParticleFlux.
RunJaidaAnalysis
RunJaidaAnalysisIC22
RunJaidaAnalysisIC9
RunPropagationMatrixFlux	Calculate the detectable Neutrino flux [GeV/cm^2 sec sr] at the surface by running ProrpagationMatrixFlux.
RunQuickPropagationMatrixFlux	Calculate the detectable Neutrino flux [GeV/cm^2 sec sr] at the surface by running ProrpagationMatrixFlux.
YieldAnalysisFactory	This class makes and handles histograms of the neutrino detection yield[cm^2 sec sr] generated by DumpQuickPropagationMatrixYield class and neutrino cross section.

Package iceCube.uhe.analysis Description

Package icecube.uhe.analysis

This package contains the classes for the IceCube Extremely-High Energy Neutrino analysis with the I3Particle-based data. The factory class "I3ParticleAnalysisFactory" provides tools for the data analysis.

Last modified: Thu Jan 25 17:34:57 JST 2007