| 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): Harald Kornmayer 1/2001 (harald@mppmu.mpg.de)
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| 19 | ! Author(s): Thomas Bretz 12/2000 (tbretz@uni-sw.gwdg.de)
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| 20 | !
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| 21 | ! Copyright: MAGIC Software Development, 2000-2001
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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 | // //
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| 28 | // MHillas //
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| 29 | // //
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| 30 | // Storage Container for the Hillas parameter //
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| 31 | // //
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| 32 | // FIXME: Here everybody should find an explanation of the parameters //
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| 33 | // //
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| 34 | /////////////////////////////////////////////////////////////////////////////
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| 35 | #include "MHillas.h"
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| 36 |
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| 37 | #include <math.h>
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| 38 |
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| 39 | #include <TEllipse.h>
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| 40 |
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| 41 | #include "MCerPhotEvt.h"
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| 42 | #include "MCerPhotPix.h"
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| 43 | #include "MGeomCam.h"
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| 44 |
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| 45 | #include "MLog.h"
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| 46 |
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| 47 | ClassImp(MHillas)
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| 48 |
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| 49 | MHillas::MHillas(const char *name, const char *title) :
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| 50 | fAlpha(0), fTheta(0), fWidth(0), fLength(0), fSize(0), fDist(0), fEllipse(NULL)
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| 51 | {
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| 52 | *fName = name ? name : "MHillas";
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| 53 | *fTitle = title ? title : "Storage container for Hillas parameter of one event";
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| 54 |
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| 55 | // FIXME: Initialization of values missing
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| 56 | }
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| 57 |
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| 58 | MHillas::~MHillas()
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| 59 | {
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| 60 | Clear();
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| 61 | }
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| 62 |
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| 63 | void MHillas::Print(Option_t *)
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| 64 | {
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| 65 | *fLog << "Hillas Parameter:" << endl;
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| 66 | *fLog << " - Alpha = " << fabs(fAlpha) << endl;
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| 67 | *fLog << " - Width = " << fWidth << endl;
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| 68 | *fLog << " - Length = " << fLength << endl;
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| 69 | *fLog << " - Size = " << fSize << endl;
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| 70 | *fLog << " - Dist = " << fDist << endl;
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| 71 | }
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| 72 |
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| 73 | void MHillas::Paint(Option_t *)
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| 74 | {
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| 75 | if (!fEllipse)
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| 76 | return;
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| 77 |
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| 78 | fEllipse->Paint();
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| 79 | }
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| 80 |
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| 81 | void MHillas::Draw(Option_t *)
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| 82 | {
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| 83 | //
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| 84 | // Instead of adding MHillas itself to the Pad
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| 85 | // (s. AppendPad in TObject) we create an ellipse,
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| 86 | // which is added to the Pad by it's Draw function
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| 87 | // You can remove it by deleting the Ellipse Object
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| 88 | // (s. Clear() )
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| 89 | //
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| 90 |
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| 91 | Clear();
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| 92 |
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| 93 | fEllipse = new TEllipse(cos(fTheta)*fDist, sin(fTheta)*fDist,
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| 94 | fLength, fWidth,
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| 95 | 0, 360, fTheta*kRad2Deg+fAlpha-180);
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| 96 |
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| 97 | fEllipse->SetLineWidth(2);
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| 98 | fEllipse->Draw();
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| 99 |
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| 100 | /*
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| 101 | This is from TH1
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| 102 | TString opt = option;
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| 103 | opt.ToLower();
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| 104 | if (gPad && !opt.Contains("same")) {
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| 105 | //the following statement is necessary in case one attempts to draw
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| 106 | //a temporary histogram already in the current pad
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| 107 | if (TestBit(kCanDelete)) gPad->GetListOfPrimitives()->Remove(this);
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| 108 | gPad->Clear();
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| 109 | }
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| 110 | AppendPad(opt.Data());
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| 111 | */
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| 112 | }
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| 113 |
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| 114 | void MHillas::Clear(Option_t *)
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| 115 | {
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| 116 | if (!fEllipse)
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| 117 | return;
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| 118 |
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| 119 | delete fEllipse;
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| 120 |
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| 121 | fEllipse = NULL;
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| 122 | }
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| 123 |
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| 124 | Bool_t MHillas::Calc(MGeomCam &geom, MCerPhotEvt &evt)
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| 125 | {
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| 126 | //
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| 127 | // Calculate the Hillas parameters from a cerenkov photon event
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| 128 | // (The calcualtion is some kind of two dimentional statistics)
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| 129 | //
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| 130 |
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| 131 | const UInt_t nevt = evt.GetNumPixels();
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| 132 |
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| 133 | //
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| 134 | // sanity check
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| 135 | //
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| 136 | if (nevt <= 2)
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| 137 | return kFALSE;
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| 138 |
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| 139 | //
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| 140 | // calculate mean valu of pixels
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| 141 | //
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| 142 | float xmean =0;
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| 143 | float ymean =0;
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| 144 |
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| 145 | fSize = 0;
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| 146 |
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| 147 | //
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| 148 | // FIXME! npix should be retrieved from MCerPhotEvt
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| 149 | //
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| 150 | UShort_t npix=0;
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| 151 | for (UInt_t i=0; i<nevt; i++)
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| 152 | {
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| 153 | const MCerPhotPix &pix = evt[i];
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| 154 |
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| 155 | if (!pix.IsPixelUsed())
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| 156 | continue;
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| 157 |
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| 158 | const MGeomPix &gpix = geom[pix.GetPixId()];
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| 159 |
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| 160 | const float nphot = pix.GetNumPhotons();
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| 161 |
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| 162 | fSize += nphot;
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| 163 | xmean += nphot * gpix.GetX(); // [mm]
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| 164 | ymean += nphot * gpix.GetY(); // [mm]
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| 165 |
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| 166 | npix++;
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| 167 | }
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| 168 |
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| 169 | //
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| 170 | // sanity check
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| 171 | //
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| 172 | if (fSize==0 || npix<=2)
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| 173 | return kFALSE;
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| 174 |
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| 175 | xmean /= fSize; // [mm]
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| 176 | ymean /= fSize; // [mm]
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| 177 |
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| 178 | //
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| 179 | // calculate sdev
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| 180 | //
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| 181 | float sigmaxx=0;
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| 182 | float sigmaxy=0;
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| 183 | float sigmayy=0;
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| 184 |
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| 185 | for (UInt_t i=0; i<nevt; i++)
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| 186 | {
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| 187 | const MCerPhotPix &pix = evt[i];
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| 188 |
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| 189 | if (!pix.IsPixelUsed())
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| 190 | continue;
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| 191 |
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| 192 | const MGeomPix &gpix = geom[pix.GetPixId()];
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| 193 |
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| 194 | const float dx = gpix.GetX() - xmean;
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| 195 | const float dy = gpix.GetY() - ymean;
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| 196 |
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| 197 | const float nphot = pix.GetNumPhotons();
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| 198 |
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| 199 | sigmaxx += nphot * dx*dx; // [mm^2]
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| 200 | sigmaxy += nphot * dx*dy; // [mm^2]
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| 201 | sigmayy += nphot * dy*dy; // [mm^2]
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| 202 | }
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| 203 |
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| 204 | //
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| 205 | // check for orientation
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| 206 | //
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| 207 | const float theta = atan(sigmaxy/(sigmaxx-sigmayy)*2)/2;
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| 208 |
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| 209 | float c = cos(theta); // [1]
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| 210 | float s = sin(theta); // [1]
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| 211 |
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| 212 | //
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| 213 | // calculate the length of the two axis
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| 214 | //
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| 215 | float axis1 = 2.0*c*s*sigmaxy + c*c*sigmaxx + s*s*sigmayy; // [mm^2]
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| 216 | float axis2 = -2.0*c*s*sigmaxy + s*s*sigmaxx + c*c*sigmayy; // [mm^2]
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| 217 |
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| 218 | axis1 /= fSize; // [mm^2]
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| 219 | axis2 /= fSize; // [mm^2]
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| 220 |
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| 221 | //
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| 222 | // check for numerical negatives
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| 223 | // (very small number can get negative by chance)
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| 224 | //
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| 225 | if (axis1 < 0) axis1=0;
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| 226 | if (axis2 < 0) axis2=0;
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| 227 |
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| 228 | //
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| 229 | // calculate the main Hillas parameters
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| 230 | //
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| 231 | // fLength, fWidth describes the two axis of the ellipse
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| 232 | // fAlpha is the angle between the length-axis and the center
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| 233 | // of the camera
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| 234 | // fDist is the distance between the center of the camera and the
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| 235 | // denter of the ellipse
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| 236 | //
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| 237 | const int rotation = axis1<axis2;
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| 238 |
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| 239 | fLength = rotation ? sqrt(axis2) : sqrt(axis1); // [mm]
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| 240 | fWidth = rotation ? sqrt(axis1) : sqrt(axis2); // [mm]
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| 241 |
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| 242 | const float a = c*xmean + s*ymean;
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| 243 | const float b = c*ymean - s*xmean;
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| 244 |
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| 245 | fAlpha = rotation ? atan(a/b) : atan(-b/a); // [rad]
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| 246 | fAlpha *= kRad2Deg; // [deg]
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| 247 |
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| 248 | fDist = sqrt(xmean*xmean + ymean*ymean); // [mm]
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| 249 |
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| 250 | fTheta = atan(ymean/xmean); // [rad]
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| 251 | if (xmean<0) fTheta += kPI; // [rad]
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| 252 |
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| 253 | return kTRUE;
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| 254 | }
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