source: branches/MarsISDCBranchBasedOn17887/sponde_onoff.rc@ 20115

# -------------------- Define your energy estimator -------------------

# Manually optimized (for example using trainenergy.C)
EstimateEnergy.Rule: MHillas.fSize^0.906*pow(10, -0.831*(MHillasSrc.fDist*3.37e-3-0.161)^2*(MHillasSrc.fDist*3.37e-3>0.161) + 2.21*(MHillasSrc.fDist*3.37e-3-0.493)^2*(MHillasSrc.fDist*3.37e-3>0.493) + 8.18e-6*MPointingPos.fZd^2.82 - 0.1*MNewImagePar.fLeakage1^0.2)

# You can use instead the Random Forest energy estimator
#  (for example trained by trainenergy.C)
#EstimateEnergy: MRanForestCalc
#EstimateEnergy.NameOutput: MEnergyEst
#EstimateEnergy.FileName: rf-energy.root
#EstimateEnergy.Debug: No

# ------------------------ Define your binnings -----------------------

# The energy binning is mandatory
BinningEnergyEst.Raw:   18   53   35800 log

# Binnings used for the Energy- and Disp-tab
#BinningSize.Raw:            50  10  100000  log
#BinningLeakage.Raw:         50   0     0.3  lin
#BinningEnergyResidual.Raw:  51  -1       1  lin
#BinningResidualDist.Raw:    51  -1       1  lin

# A change of the theta binning must be done in ganymed (see below) :(
#BinningTheta.Raw: 101 -0.005 0.505 asin

# --------------- Setup the weighting for your spectrum ---------------
#            For more details see MMcSpectrumWeight::ReadEnv

# A simple power law with a differential spectral index of -4
#MMcSpectrumWeight.NewSlope: -4

# Give a formula for the spectrum. Capital X is a place-holder
# for the energy (eg. the crab-spectrum from our publication)
#MMcSpectrumWeight.Formula: pow(X/300, -2.31-0.26*log10(X/300))

# ----------------------- Additional setup ----------------------------

# In the loop filling the ThetaSq histogram the theta cut is switched off
# and the theta-cut is implicitly done in the histogram. Reading the
# Monte Carlo for determining the collection area there is no theta-
# histogram involved, thus you need the theta cut switched on
Spectrum.Cut1.ThetaCut: On

# You may want to change the scale region to a different region than
# previously used in your ganymed-file. This might be usefull for
# on/off-data. Note, that the result can also depend on what else
# was setup for your MAlphaFitter in ganymed.
#MAlphaFitter.ScaleMin: 0.137
#MAlphaFitter.ScaleMax: 0.500

# You may use this to change the scale and/or fit region for
# determination of the excess vs energy (can be usefull in On/Off mode)
#MAlphaFitter.ScaleMode: Fixed

# You may want to allow scaling of each energy bin individually. (This
# can be useful if on- and off- data in wobble mode do not agree well)
#MAlphaFitter.ScaleMode: background
#MAlphaFitter.BackgroundFitMin: 0.09
#MAlphaFitter.BackgroundFitMax: 0.25

# ------------------------- Additional cut ----------------------------

# You can apply a cut in addition to all other cuts to your data and
# MOnte Carlos. This can be usefull for example to setup a second
# MFMagicCuts with a tighter behaviour assuming that your ganymed
# was written with a really loose cut.
#CutS.Inverted:  Yes
#CutS.Condition: MFMagicCuts
#CutS.ThetaCut: None
#CutS.HadronnesCut: Area
# Parametrization of Area
#CutS.Param2:   0.215468
#CutS.Param3:   5.63973
#CutS.Param4:   0.0836169

# --------------------------- Other binnings --------------------------

# Binnings that are used by sponde but can not/shoud not be changed
# because they are taken from the ganymed file
#BinningTheta
#BinningWidth
#BinningLength
#BinningDist
#BinningM3Long
#BinningM3Trans
#BinningSlope
#BinningAsym
#BinningConc1