| 1 | /* ======================================================================== *\ | 
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| 2 | ! | 
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| 3 | ! * | 
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| 4 | ! * This file is part of MARS, the MAGIC Analysis and Reconstruction | 
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| 5 | ! * Software. It is distributed to you in the hope that it can be a useful | 
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| 6 | ! * and timesaving tool in analysing Data of imaging Cerenkov telescopes. | 
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| 7 | ! * It is distributed WITHOUT ANY WARRANTY. | 
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| 8 | ! * | 
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| 9 | ! * Permission to use, copy, modify and distribute this software and its | 
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| 10 | ! * documentation for any purpose is hereby granted without fee, | 
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| 11 | ! * provided that the above copyright notice appear in all copies and | 
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| 12 | ! * that both that copyright notice and this permission notice appear | 
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| 13 | ! * in supporting documentation. It is provided "as is" without express | 
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| 14 | ! * or implied warranty. | 
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| 15 | ! * | 
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| 16 | ! | 
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| 17 | ! | 
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| 18 | !   Author(s): Marcos Lopez  10/2003 <mailto:marcos@gae.ucm.es> | 
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| 19 | ! | 
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| 20 | !   Copyright: MAGIC Software Development, 2000-2003 | 
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| 21 | ! | 
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| 22 | ! | 
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| 23 | \* ======================================================================== */ | 
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| 24 |  | 
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| 25 | ////////////////////////////////////////////////////////////////////////////// | 
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| 26 | // | 
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| 27 | //  MMcWeightEnergySlopeCalc | 
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| 28 | // | 
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| 29 | //  Change the spectrum of the MC showers simulated with Corsika (a power law) | 
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| 30 | //  to a new one, which can be either, again a power law but with a different | 
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| 31 | //  spectral index, or a generalizeed spectrum. The new spectrum can be | 
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| 32 | //  pass to this class in different ways: | 
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| 33 | //    1. Is the new spectrum will be a power law, just introduce the slope | 
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| 34 | //       of this power law. | 
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| 35 | //    2. Is the new spectrum will have a general shape, different options are | 
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| 36 | //       available: | 
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| 37 | //       a) The new spectrum is pass as a TF1 function | 
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| 38 | //       b) The new spectrum is pass as a char* | 
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| 39 | //       c) The new spectrum is pass as a "interpreted function", i.e., a | 
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| 40 | //          function defined inside a ROOT macro, which will be invoked by the | 
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| 41 | //          ROOT Cint itself. This is the case when we use ROOT macros. | 
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| 42 | //       d) The new spectrum is pass as a "real function", i.e., a | 
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| 43 | //          function defined inside normal c++ file. | 
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| 44 | // | 
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| 45 | //  Method: | 
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| 46 | //  ------ | 
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| 47 | // | 
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| 48 | //  -Corsika spectrun: dN/dE = A * E^(a) | 
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| 49 | //    with a = fCorsikaSlope, and A = N/integral{E*de} from ELowLim to EUppLim | 
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| 50 | // | 
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| 51 | //  -New spectrum:     dN/dE = B * g(E) | 
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| 52 | //    where B = N/integral{g*dE} from ELowLim to EUppLim, and N=NumEvents | 
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| 53 | // | 
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| 54 | //  For converting the spectrum simulated with Corsika to the new one, we apply | 
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| 55 | //  a weight to each event, given by: | 
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| 56 | // | 
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| 57 | //     W(E) = B/A * g(E)/E^(a) | 
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| 58 | // | 
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| 59 | //  In the case the new spectrum is simply a power law: dN/dE = B * E^(b), we | 
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| 60 | //  have: | 
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| 61 | // | 
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| 62 | //     W(E) = B/A * E^(b-a) | 
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| 63 | // | 
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| 64 | //  (The factor B/A is used in order both the original and new spectrum have | 
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| 65 | //   the same area (i.e. in order they represent the same number of showers)) | 
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| 66 | // | 
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| 67 | //  Note: | 
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| 68 | //  ------ | 
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| 69 | //   -If the the new spectrum is just a power law (i.e. the user only specify | 
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| 70 | //     the slope), the needed calculations (such as the integral of the | 
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| 71 | //     spectrum) are done analytically. But if the new spectrum is given as a | 
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| 72 | //     TF1 object, the calculations is done numerically. | 
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| 73 | // | 
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| 74 | //  ToDo: | 
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| 75 | //  ----- | 
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| 76 | //   -Give to the user also the possibility to specify the integral of the | 
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| 77 | //    spectrum as another TF1 object (or C++ function) | 
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| 78 | // | 
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| 79 | // | 
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| 80 | //  Input Containers: | 
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| 81 | //   MMcEvt, MMcRunHeader, MMcCorsikaRunHeader | 
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| 82 | // | 
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| 83 | //  Output Container: | 
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| 84 | //   MWeight | 
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| 85 | // | 
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| 86 | ////////////////////////////////////////////////////////////////////////////// | 
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| 87 |  | 
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| 88 | #include "MMcWeightEnergySpecCalc.h" | 
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| 89 |  | 
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| 90 | #include "MParList.h" | 
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| 91 | #include "MLog.h" | 
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| 92 | #include "MLogManip.h" | 
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| 93 | #include "MMcEvt.hxx" | 
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| 94 | #include "MMcRunHeader.hxx" | 
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| 95 | #include "MMcCorsikaRunHeader.h" | 
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| 96 | #include "MWeight.h" | 
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| 97 |  | 
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| 98 | #include "TF1.h" | 
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| 99 | #include "TGraph.h" | 
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| 100 |  | 
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| 101 | ClassImp(MMcWeightEnergySpecCalc); | 
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| 102 |  | 
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| 103 | using namespace std; | 
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| 104 |  | 
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| 105 |  | 
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| 106 |  | 
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| 107 | void MMcWeightEnergySpecCalc::Init(const char *name, const char *title) | 
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| 108 | { | 
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| 109 |  | 
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| 110 | fName  = name  ? name  : "MMcWeightEnergySpecCalc"; | 
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| 111 | fTitle = title ? title : "Task to calculate weights to change the energy spectrum"; | 
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| 112 |  | 
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| 113 | AddToBranchList("MMcEvt.fEnergy"); | 
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| 114 |  | 
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| 115 | fAllEvtsTriggered         =  kFALSE; | 
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| 116 | fTotalNumSimulatedShowers =  0; | 
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| 117 | } | 
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| 118 |  | 
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| 119 |  | 
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| 120 | // --------------------------------------------------------------------------- | 
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| 121 | // | 
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| 122 | // Constructor. The new spectrum will be just a power law. | 
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| 123 | // | 
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| 124 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(Float_t slope, | 
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| 125 | const char *name, const char *title) | 
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| 126 | { | 
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| 127 | fNewSpecIsPowLaw = kTRUE; | 
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| 128 | fNewSlope = slope; | 
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| 129 |  | 
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| 130 | fNewSpectrum = NULL; | 
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| 131 |  | 
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| 132 | Init(name,title); | 
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| 133 | } | 
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| 134 |  | 
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| 135 | // --------------------------------------------------------------------------- | 
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| 136 | // | 
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| 137 | // Constructor. The new spectrum will have a general shape, given by the user | 
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| 138 | // as a TF1 function. | 
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| 139 | // | 
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| 140 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(const TF1& spectrum, | 
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| 141 | const char *name, const char *title) | 
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| 142 | { | 
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| 143 | fNewSpecIsPowLaw = kFALSE; | 
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| 144 | fNewSpectrum = (TF1*)spectrum.Clone(); | 
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| 145 |  | 
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| 146 | Init(name,title); | 
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| 147 | } | 
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| 148 |  | 
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| 149 | // --------------------------------------------------------------------------- | 
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| 150 | // | 
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| 151 | // As before, but the function which represent the new spectrum is given as | 
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| 152 | // a char* . Starting from it, we build a TF1 function | 
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| 153 | // | 
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| 154 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(const char* spectrum, | 
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| 155 | const char *name, const char *title) | 
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| 156 | { | 
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| 157 | fNewSpecIsPowLaw = kFALSE; | 
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| 158 | fNewSpectrum = new TF1("NewSpectrum",spectrum); | 
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| 159 |  | 
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| 160 | Init(name,title); | 
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| 161 | } | 
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| 162 |  | 
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| 163 | // --------------------------------------------------------------------------- | 
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| 164 | // | 
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| 165 | // As before, but the new spectrum is given as a intrepreted C++ function. | 
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| 166 | // Starting from it we build a TF1 function. | 
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| 167 | // This constructor is called for interpreted functions by CINT, i.e., when | 
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| 168 | // the functions are declared inside a ROOT macro. | 
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| 169 | // | 
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| 170 | // NOTE: you muss do a casting to (void*) of the function that you pass to this | 
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| 171 | //       constructor before invoking it in a macro, e.g. | 
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| 172 | // | 
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| 173 | //       Double_t myfunction(Double_t *x, Double_t *par) | 
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| 174 | //         { | 
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| 175 | //           ... | 
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| 176 | //         } | 
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| 177 | // | 
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| 178 | //        MMcWeightEnergySpecCalc wcalc((void*)myfunction); | 
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| 179 | // | 
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| 180 | //        tasklist.AddToList(&wcalc); | 
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| 181 | // | 
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| 182 | //        otherwise ROOT will invoke the constructor McWeightEnergySpecCalc( | 
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| 183 | //         const char* spectrum, const char *name, const char *title) | 
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| 184 | // | 
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| 185 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(void* function, | 
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| 186 | const char *name, const char *title) | 
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| 187 | { | 
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| 188 | fNewSpecIsPowLaw = kFALSE; | 
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| 189 | fNewSpectrum = new TF1("NewSpectrum",function,0,1,1); | 
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| 190 |  | 
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| 191 | Init(name,title); | 
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| 192 | } | 
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| 193 |  | 
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| 194 | // --------------------------------------------------------------------------- | 
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| 195 | // | 
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| 196 | // As before, but this is the constructor for real functions, i.e. it is called | 
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| 197 | // when invoked with the normal C++ compiler, i.e. not inside a ROOT macro. | 
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| 198 | // | 
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| 199 | MMcWeightEnergySpecCalc::MMcWeightEnergySpecCalc(Double_t (*function)(Double_t*x, Double_t* par), const Int_t npar,  const char *name, const char *title) | 
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| 200 | { | 
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| 201 | fNewSpecIsPowLaw = kFALSE; | 
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| 202 | fNewSpectrum = new TF1("NewSpectrum",function,0,1,1); | 
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| 203 |  | 
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| 204 | Init(name,title); | 
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| 205 | } | 
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| 206 |  | 
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| 207 |  | 
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| 208 |  | 
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| 209 | // ---------------------------------------------------------------------------- | 
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| 210 | // | 
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| 211 | // Destructor. Deletes the cloned fNewSpectrum. | 
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| 212 | // | 
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| 213 | MMcWeightEnergySpecCalc::~MMcWeightEnergySpecCalc() | 
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| 214 | { | 
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| 215 | if (fNewSpectrum) | 
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| 216 | delete fNewSpectrum; | 
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| 217 | } | 
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| 218 |  | 
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| 219 |  | 
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| 220 |  | 
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| 221 | // --------------------------------------------------------------------------- | 
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| 222 | // | 
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| 223 | // | 
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| 224 | Int_t MMcWeightEnergySpecCalc::PreProcess (MParList *pList) | 
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| 225 | { | 
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| 226 |  | 
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| 227 | fMcEvt = (MMcEvt*)pList->FindObject("MMcEvt"); | 
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| 228 | if (!fMcEvt) | 
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| 229 | { | 
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| 230 | *fLog << err << dbginf << "MMcEvt not found... exit." << endl; | 
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| 231 | return kFALSE; | 
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| 232 | } | 
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| 233 |  | 
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| 234 | fWeight = (MWeight*)pList->FindCreateObj("MWeight"); | 
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| 235 | if (!fWeight) | 
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| 236 | { | 
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| 237 | *fLog << err << dbginf << "MWeight not found... exit." << endl; | 
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| 238 | return kFALSE; | 
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| 239 | } | 
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| 240 |  | 
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| 241 | return kTRUE; | 
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| 242 | } | 
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| 243 |  | 
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| 244 |  | 
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| 245 |  | 
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| 246 | // ---------------------------------------------------------------------------- | 
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| 247 | // | 
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| 248 | // Executed each time a new root file is loaded | 
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| 249 | // We will need fCorsikaSlope and fE{Upp,Low}Lim to calculate the weights | 
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| 250 | // | 
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| 251 | Bool_t MMcWeightEnergySpecCalc::ReInit(MParList *plist) | 
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| 252 | { | 
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| 253 | MMcRunHeader *runheader = (MMcRunHeader*)plist->FindObject("MMcRunHeader"); | 
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| 254 | if (!runheader) | 
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| 255 | { | 
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| 256 | *fLog << err << dbginf << "Error - MMcRunHeader not found... exit." << endl; | 
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| 257 | return kFALSE; | 
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| 258 | } | 
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| 259 |  | 
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| 260 | MMcCorsikaRunHeader *corrunheader  = (MMcCorsikaRunHeader*)plist->FindObject("MMcCorsikaRunHeader"); | 
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| 261 | if (!corrunheader) | 
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| 262 | { | 
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| 263 | *fLog << err << dbginf << "Error - MMcCorsikaRunHeader not found... exit." << endl; | 
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| 264 | return kFALSE; | 
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| 265 | } | 
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| 266 |  | 
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| 267 |  | 
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| 268 | fCorsikaSlope = (Double_t)corrunheader->GetSlopeSpec(); | 
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| 269 | fELowLim      = (Double_t)corrunheader->GetELowLim(); | 
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| 270 | fEUppLim      = (Double_t)corrunheader->GetEUppLim(); | 
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| 271 |  | 
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| 272 | fTotalNumSimulatedShowers += runheader->GetNumSimulatedShowers(); | 
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| 273 | fAllEvtsTriggered |= runheader->GetAllEvtsTriggered(); | 
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| 274 |  | 
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| 275 |  | 
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| 276 |  | 
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| 277 | *fLog << inf << "Slope of primaries' energy spectrum of Simulated showers: " << fCorsikaSlope << endl; | 
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| 278 | *fLog << inf << "Limits of energy range of Simulated showers: " | 
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| 279 | << fELowLim <<" - " << fEUppLim << endl; | 
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| 280 | *fLog << inf << "New Slope for Simulated showers: " << fNewSlope << endl; | 
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| 281 | *fLog << inf << "Total Number of Simulated showers: " | 
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| 282 | << fTotalNumSimulatedShowers << endl; | 
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| 283 | *fLog << inf << "Only triggered events avail: " << (fAllEvtsTriggered?"yes":"no") << endl; | 
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| 284 |  | 
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| 285 |  | 
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| 286 |  | 
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| 287 | // | 
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| 288 | // Sanity checks to be sure that we won't divide by zero later on | 
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| 289 | // | 
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| 290 | if(fCorsikaSlope == -1. || fNewSlope == -1.) | 
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| 291 | { | 
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| 292 | *fLog << err << "The Slope of the power law must be different of -1... exit" << endl; | 
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| 293 | return kFALSE; | 
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| 294 | } | 
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| 295 |  | 
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| 296 |  | 
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| 297 | // | 
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| 298 | // Starting from fCorsikaSlope and fE{Upp,Low}Lim, calculate the integrals | 
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| 299 | // of both, the original Corsika spectrum and the new one. | 
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| 300 | // | 
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| 301 | // | 
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| 302 | // For the Corsika simulated spectrum (just a power law), we have: | 
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| 303 | // | 
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| 304 | fCorSpecInt = ( pow(fEUppLim,1+fCorsikaSlope) - pow(fELowLim,1+fCorsikaSlope) ) / ( 1+fCorsikaSlope ); | 
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| 305 |  | 
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| 306 |  | 
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| 307 | // | 
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| 308 | // For the new spectrum: | 
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| 309 | // | 
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| 310 | if (fNewSpecIsPowLaw)     // just the integral of a power law | 
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| 311 | { | 
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| 312 | fNewSpecInt = ( pow(fEUppLim,1+fNewSlope) - pow(fELowLim,1+fNewSlope) )/ ( 1+fNewSlope ); | 
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| 313 | } | 
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| 314 | else | 
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| 315 | { | 
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| 316 | fNewSpectrum->SetRange(fELowLim, fEUppLim); | 
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| 317 |  | 
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| 318 | // In this case we have to integrate the new spectrum numerically. We | 
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| 319 | // could do simply fNewSpectrum->Integral(fELowLim,fEUppLim), but ROOT | 
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| 320 | // fails integrating up to fEUppLim for a sharp cutoff spectrum | 
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| 321 |  | 
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| 322 | // | 
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| 323 | // Trick to calculate the integral numerically (it works better than | 
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| 324 | // fNewSpectrum->Integral(fELowLim,fEUppLim) (although not perfectlly) | 
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| 325 | // | 
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| 326 | fNewSpectrum->SetNpx(1000); | 
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| 327 | TGraph gr(fNewSpectrum,"i"); | 
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| 328 | Int_t Npx = gr.GetN(); | 
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| 329 | Double_t* y = gr.GetY(); | 
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| 330 |  | 
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| 331 | const Double_t integral = y[Npx-1]; | 
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| 332 | fNewSpecInt = integral; | 
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| 333 | } | 
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| 334 |  | 
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| 335 |  | 
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| 336 | return kTRUE; | 
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| 337 | } | 
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| 338 |  | 
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| 339 |  | 
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| 340 |  | 
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| 341 | // ---------------------------------------------------------------------------- | 
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| 342 | // | 
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| 343 | // | 
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| 344 | Int_t MMcWeightEnergySpecCalc::Process() | 
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| 345 | { | 
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| 346 | const Double_t energy = fMcEvt->GetEnergy(); | 
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| 347 |  | 
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| 348 | const Double_t C = fCorSpecInt / fNewSpecInt; | 
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| 349 | Double_t weight; | 
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| 350 |  | 
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| 351 |  | 
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| 352 | if (fNewSpecIsPowLaw) | 
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| 353 | weight = C * pow(energy,fNewSlope-fCorsikaSlope); | 
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| 354 | else | 
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| 355 | weight = C * fNewSpectrum->Eval(energy) / pow(energy,fCorsikaSlope); | 
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| 356 |  | 
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| 357 |  | 
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| 358 | fWeight->SetWeight( weight ); | 
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| 359 |  | 
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| 360 | return kTRUE; | 
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| 361 | } | 
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