source: trunk/src/Cubes/spectraUtils.cc @ 884

Last change on this file since 884 was 884, checked in by MatthewWhiting, 12 years ago

A large set of changes aimed at making the use of indexing variables consistent. We have moved to size_t as much as possible to represent the location in memory. This includes making the dimension array within DataArray? and derived classes an array of size_t variables. Still plenty of compilation warnings (principally comparing signed and unsigned variables) - these will need to be cleaned up.

File size: 10.3 KB
Line 
1// -----------------------------------------------------------------------
2// spectraUtils.cc: Utility functions to obtain & manipulate spectra
3// -----------------------------------------------------------------------
4// Copyright (C) 2006, Matthew Whiting, ATNF
5//
6// This program is free software; you can redistribute it and/or modify it
7// under the terms of the GNU General Public License as published by the
8// Free Software Foundation; either version 2 of the License, or (at your
9// option) any later version.
10//
11// Duchamp is distributed in the hope that it will be useful, but WITHOUT
12// ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or
13// FITNESS FOR A PARTICULAR PURPOSE.  See the GNU General Public License
14// for more details.
15//
16// You should have received a copy of the GNU General Public License
17// along with Duchamp; if not, write to the Free Software Foundation,
18// Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307, USA
19//
20// Correspondence concerning Duchamp may be directed to:
21//    Internet email: Matthew.Whiting [at] atnf.csiro.au
22//    Postal address: Dr. Matthew Whiting
23//                    Australia Telescope National Facility, CSIRO
24//                    PO Box 76
25//                    Epping NSW 1710
26//                    AUSTRALIA
27// -----------------------------------------------------------------------
28#include <iostream>
29#include <fstream>
30#include <iomanip>
31#include <sstream>
32#include <string>
33#include <vector>
34#include <math.h>
35#include <wcslib/wcs.h>
36#include <duchamp/Cubes/cubeUtils.hh>
37#include <duchamp/param.hh>
38#include <duchamp/duchamp.hh>
39#include <duchamp/fitsHeader.hh>
40#include <duchamp/PixelMap/Object3D.hh>
41#include <duchamp/Cubes/cubes.hh>
42#include <duchamp/Utils/utils.hh>
43
44using namespace PixelInfo;
45
46namespace duchamp
47{
48
49  void getSpecAbscissae(Detection &object, FitsHeader &head, size_t zdim, float *abscissae)
50  {
51    /// @details
52    ///  A function that returns an array of
53    ///  frequency/velocity/channel/etc values (that can be used as the
54    ///  abscissae on the spectral plot).
55    ///  \param object The object on which our spectrum is centered (in
56    ///  case the spectral value changes with x & y
57    ///  \param head The FitsHeader set of parameters that determine the coordinate transformation.
58    ///  \param zdim The length of the spectral axis
59    ///  \param abscissae The array of spectral values -- must be allocated first
60
61    getSpecAbscissae(head,object.getXcentre(),object.getYcentre(),zdim, abscissae);
62  }
63
64  void getSpecAbscissae(FitsHeader &head, float xpt, float ypt, size_t zdim, float *abscissae)
65  {
66    /// @details
67    ///  A function that returns an array of
68    ///  frequency/velocity/channel/etc values (that can be used as the
69    ///  horizontal axis on the spectral plot).
70    ///  \param head The FitsHeader set of parameters that determine the coordinate transformation.
71    ///  \param xpt The x-value of the spatial position on which our spectrum is centred.
72    ///  \param ypt The y-value of the spatial position on which our spectrum is centred.
73    ///  \param zdim The length of the spectral axis
74    ///  \param abscissae The array of spectral values -- must be allocated first.
75
76    if(head.isWCS()){
77      double xval = double(xpt);
78      double yval = double(ypt);
79      for(double zval=0;zval<zdim;zval++)
80        abscissae[int(zval)] = head.pixToVel(xval,yval,zval);
81    }
82    else
83      for(double zval=0;zval<zdim;zval++) abscissae[int(zval)] = zval;
84
85  }
86  //--------------------------------------------------------------------
87
88  void getIntSpec(Detection &object, float *fluxArray, size_t *dimArray, std::vector<bool> mask,
89                  float beamCorrection, float *spec)
90  {
91    /// @details
92    ///  The base function that extracts an integrated spectrum for a
93    ///  given object from a pixel array. The spectrum is returned as
94    ///  the integrated flux, corrected for the beam using the given
95    ///  correction factor.
96    ///   \param object The Detection in question
97    ///   \param fluxArray The full array of pixel values.
98    ///   \param dimArray The axis dimensions for the fluxArray
99    ///   \param mask A mask array indicating whether given pixels are valid
100    ///   \param beamCorrection How much to divide the summed spectrum
101    ///   by to return the integrated flux.
102    ///   \param spec The integrated spectrum for the object -- must be allocated first.
103
104    for(int i=0;i<dimArray[2];i++) spec[i] = 0.;
105    size_t xySize = dimArray[0]*dimArray[1];
106    bool *done = new bool[xySize];
107    for(int i=0;i<xySize;i++) done[i]=false;
108    std::vector<Voxel> voxlist = object.getPixelSet();
109    std::vector<Voxel>::iterator vox;
110    for(vox=voxlist.begin();vox<voxlist.end();vox++){
111      int pos = vox->getX() + dimArray[0] * vox->getY();
112      if(!done[pos]){
113        done[pos] = true;
114        for(int z=0;z<dimArray[2];z++){
115          if(mask[pos+z*xySize]){
116            spec[z] += fluxArray[pos + z*xySize] / beamCorrection;
117          }         
118        }
119      }
120    }
121    delete [] done;
122
123  }
124  //--------------------------------------------------------------------
125
126  void getPeakSpec(Detection &object, float *fluxArray, size_t *dimArray, bool *mask, float *spec)
127  {
128    /// @details
129    ///  The base function that extracts an peak spectrum for a
130    ///  given object from a pixel array. The spectrum is returned as
131    ///  the integrated flux, corrected for the beam using the given
132    ///  correction factor.
133    ///   \param object The Detection in question
134    ///   \param fluxArray The full array of pixel values.
135    ///   \param dimArray The axis dimensions for the fluxArray
136    ///   \param mask A mask array indicating whether given pixels are valid
137    ///   \param spec The peak spectrum for the object -- must be allocated first
138
139    size_t xySize = dimArray[0]*dimArray[1];
140    int pos = object.getXPeak() + dimArray[0]*object.getYPeak();
141    for(int z=0;z<dimArray[2];z++){
142      if(mask[pos + z*xySize])
143        spec[z] = fluxArray[pos + z*xySize];
144    }
145  }
146  //--------------------------------------------------------------------
147
148
149  void Cube::getSpectralArrays(int objNum, float *specx, float *specy,
150                               float *specRecon, float *specBase)
151  {
152    /// @details
153    ///  A utility function that goes and calculates, for a given
154    ///  Detection, the spectral arrays, according to whether we want
155    ///  the peak or integrated flux. The arrays can be used by
156    ///  Cube::plotSpectrum() and Cube::writeSpectralData(). The arrays
157    ///  calculated are listed below. Their length is given by the
158    ///  length of the Cube's spectral dimension.
159    ///
160    ///  Note that the arrays need to be allocated prior to calling
161    ///  this function.
162    ///
163    ///  \param objNum The number of the object under consideration
164    ///  \param specx The array of frequency/velocity/channel/etc
165    ///         values (the x-axis on the spectral plot).
166    ///  \param specy The array of flux values, matching the specx
167    ///         array.
168    ///  \param specRecon The reconstructed or smoothed array, done in
169    ///         the same way as specy.
170    ///  \param specBase The fitted baseline values, done in the same
171    ///         way as specy.
172
173    size_t xdim = this->axisDim[0];
174    size_t ydim = this->axisDim[1];
175    size_t zdim = this->axisDim[2];
176       
177    for(int i=0;i<zdim;i++) specy[i]     = 0.;
178    for(int i=0;i<zdim;i++) specRecon[i] = 0.;
179    for(int i=0;i<zdim;i++) specBase[i]  = 0.;
180       
181    if(this->head.isWCS()){
182      double xval = double(this->objectList->at(objNum).getXcentre());
183      double yval = double(this->objectList->at(objNum).getYcentre());
184      for(double zval=0;zval<zdim;zval++)
185        specx[int(zval)] = this->head.pixToVel(xval,yval,zval);
186    }
187    else
188      for(double zval=0;zval<zdim;zval++) specx[int(zval)] = zval;
189       
190    float beamCorrection;
191    if(this->header().needBeamSize())
192      beamCorrection = this->head.beam().area();
193    else beamCorrection = 1.;
194       
195    if(this->par.getSpectralMethod()=="sum"){
196      bool *done = new bool[xdim*ydim];
197      for(int i=0;i<xdim*ydim;i++) done[i]=false;
198      std::vector<Voxel> voxlist = this->objectList->at(objNum).getPixelSet();
199      std::vector<Voxel>::iterator vox;
200      for(vox=voxlist.begin();vox<voxlist.end();vox++){
201        int pos = vox->getX() + xdim * vox->getY();
202        if(!done[pos]){
203          done[pos] = true;
204          for(int z=0;z<zdim;z++){
205            if(!(this->isBlank(pos+z*xdim*ydim))){
206              specy[z] += this->array[pos + z*xdim*ydim] / beamCorrection;
207              if(this->reconExists)
208                specRecon[z] += this->recon[pos + z*xdim*ydim] / beamCorrection;
209              if(this->par.getFlagBaseline())
210                specBase[z] += this->baseline[pos + z*xdim*ydim] / beamCorrection;
211            }       
212          }
213        }
214      }
215      delete [] done;
216    }
217    else {// if(par.getSpectralMethod()=="peak"){
218      int pos = this->objectList->at(objNum).getXPeak() +
219        xdim*this->objectList->at(objNum).getYPeak();
220      for(int z=0;z<zdim;z++){
221        specy[z] = this->array[pos + z*xdim*ydim];
222        if(this->reconExists)
223          specRecon[z] = this->recon[pos + z*xdim*ydim];
224        if(this->par.getFlagBaseline())
225          specBase[z] = this->baseline[pos + z*xdim*ydim];
226      }
227    }
228
229//     size_t zdim = this->axisDim[2];
230//     Detection obj = this->objectList->at(objNum);
231//     getSpecAbscissae(obj, this->head, zdim, specx);
232
233//     float beamCorrection;
234//     if(this->header().needBeamSize())
235//       beamCorrection = this->par.getBeamSize();
236//     else beamCorrection = 1.;
237
238//     bool *mask = this->makeBlankMask();
239//     if(!this->reconExists)
240//       for(int i=0;i<this->axisDim[2];i++) specRecon[i] = 0.;
241//     if(!this->par.getFlagBaseline())
242//       for(int i=0;i<this->axisDim[2];i++) specBase[i]  = 0.;
243
244//     if(this->par.getSpectralMethod()=="sum"){
245//       getIntSpec(obj, this->array, this->axisDim, mask, beamCorrection, specy);
246//       if(this->reconExists){
247//      getIntSpec(obj, this->recon, this->axisDim, mask, beamCorrection, specRecon);
248//       }
249//       if(this->par.getFlagBaseline()){
250//      getIntSpec(obj, this->baseline, this->axisDim, mask, beamCorrection, specBase);
251//       }
252//     }
253//     else{ // if(.getSpectralMethod()=="peak"){
254//       getPeakSpec(obj, this->array, this->axisDim, mask, specy);
255//       if(this->reconExists)
256//      getPeakSpec(obj, this->recon, this->axisDim, mask, specRecon);
257//       if(this->par.getFlagBaseline())
258//      getPeakSpec(obj, this->baseline, this->axisDim, mask, specBase);
259//     }
260
261  }
262  //--------------------------------------------------------------------
263
264}
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