source: trunk/external-alma/components/SpectralComponents/SpectralFit2.tcc @ 2980

Last change on this file since 2980 was 2980, checked in by Malte Marquarding, 10 years ago

Add a copy of casacore/components/SpectralComponents to external-alma directory to prepare for its removal from casacore-trunk. DOn;t activate in SConscript yet.

File size: 5.8 KB
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1//# SpectralFit2.cc: Least Squares fitting of spectral elements: templated part
2//# Copyright (C) 2001,2002,2004
3//# Associated Universities, Inc. Washington DC, USA.
4//#
5//# This library is free software; you can redistribute it and/or modify it
6//# under the terms of the GNU Library General Public License as published by
7//# the Free Software Foundation; either version 2 of the License, or (at your
8//# option) any later version.
9//#
10//# This library is distributed in the hope that it will be useful, but WITHOUT
11//# ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or
12//# FITNESS FOR A PARTICULAR PURPOSE.  See the GNU Library General Public
13//# License for more details.
14//#
15//# You should have received a copy of the GNU Library General Public License
16//# along with this library; if not, write to the Free Software Foundation,
17//# Inc., 675 Massachusetts Ave, Cambridge, MA 02139, USA.
18//#
19//# Correspondence concerning AIPS++ should be addressed as follows:
20//#        Internet email: aips2-request@nrao.edu.
21//#        Postal address: AIPS++ Project Office
22//#                        National Radio Astronomy Observatory
23//#                        520 Edgemont Road
24//#                        Charlottesville, VA 22903-2475 USA
25//#
26//# $Id: SpectralFit2.tcc 21465 2014-06-19 05:56:56Z gervandiepen $
27
28//# Includes
29#include <components/SpectralComponents/SpectralFit.h>
30
31#include <casa/Utilities/PtrHolder.h>
32#include <components/SpectralComponents/CompiledSpectralElement.h>
33#include <components/SpectralComponents/GaussianSpectralElement.h>
34#include <components/SpectralComponents/LogTransformedPolynomialSpectralElement.h>
35#include <components/SpectralComponents/LorentzianSpectralElement.h>
36#include <components/SpectralComponents/PolynomialSpectralElement.h>
37#include <components/SpectralComponents/PowerLogPolynomialSpectralElement.h>
38#include <scimath/Fitting/NonLinearFitLM.h>
39#include <scimath/Functionals/CompiledFunction.h>
40#include <scimath/Functionals/CompoundFunction.h>
41#include <scimath/Functionals/CompoundParam.h>
42#include <scimath/Functionals/Gaussian1D.h>
43#include <scimath/Functionals/Lorentzian1D.h>
44#include <scimath/Functionals/Polynomial.h>
45#include <scimath/Functionals/PowerLogarithmicPolynomial.h>
46
47namespace casa { //# NAMESPACE CASA - BEGIN
48
49//# Templated member functions
50
51template <class MT>
52Bool SpectralFit::fit(const Vector<MT> &y,
53                      const Vector<MT> &x,
54                      const Vector<Bool> *mask) {
55  Vector<MT> sigma(x.nelements());
56  sigma = 1.0;
57  return fit(sigma, y, x, mask);
58}
59
60template <class MT>
61Bool SpectralFit::fit(
62        const Vector<MT> &sigma, const Vector<MT> &y,
63        const Vector<MT> &x, const Vector<Bool> *mask
64) {
65        NonLinearFitLM<MT> fitter;
66        iter_p = 0;
67        // The functions to fit
68        CompoundFunction<AutoDiff<MT> > func;
69        uInt ncomps = slist_p.nelements();
70        PtrHolder<Function<AutoDiff<MT> > > autodiff;
71        for (uInt i=0; i<ncomps; i++) {
72                SpectralElement *elem = slist_p[i];
73                uInt nparms = elem->getOrder();
74                SpectralElement::Types type = slist_p[i]->getType();
75                switch(type) {
76                case SpectralElement::GAUSSIAN: {
77                        autodiff.set(new Gaussian1D<AutoDiff<MT> >());
78                }
79                break;
80                case SpectralElement::POLYNOMIAL: {
81                        PolynomialSpectralElement *x = dynamic_cast<PolynomialSpectralElement *>(elem);
82                        autodiff.set(new Polynomial<AutoDiff<MT> >(x->getDegree()));
83                }
84                break;
85                case SpectralElement::COMPILED:
86                        // Allow fall through; these use the same code
87                case SpectralElement::GMULTIPLET: {
88                        CompiledSpectralElement *x = dynamic_cast<CompiledSpectralElement *>(elem);
89                        autodiff.set(new CompiledFunction<AutoDiff<MT> >());
90                        dynamic_cast<CompiledFunction<AutoDiff<MT> > *>(
91                                autodiff.ptr()
92                        )->setFunction(x->getFunction());
93                }
94                break;
95                case SpectralElement::LORENTZIAN: {
96                        autodiff.set(new Lorentzian1D<AutoDiff<MT> >());
97                }
98                break;
99                case SpectralElement::POWERLOGPOLY: {
100                        Vector<Double> parms = elem->get();
101                        autodiff.set(new PowerLogarithmicPolynomial<AutoDiff<MT> > (nparms));
102                }
103                break;
104                case SpectralElement::LOGTRANSPOLY: {
105                        LogTransformedPolynomialSpectralElement *x = dynamic_cast<
106                                LogTransformedPolynomialSpectralElement*
107                        >(elem);
108                        // treated as a polynomial for fitting purposes. The caller is responsible for passing the ln's of
109                        // the ordinate and obscissa values to the fitter.
110                        autodiff.set(new Polynomial<AutoDiff<MT> > (x->getDegree()));
111                }
112                break;
113                default:
114                        throw AipsError("SpectralFit::fit(): Logic Error: Unhandled SpectralElement type");
115                }
116                Vector<Double> parms = elem->get();
117                Vector<Bool> fixed = elem->fixed();
118                for (uInt j=0; j<nparms; j++) {
119                        (*autodiff)[j] = AutoDiff<MT>(parms[j], nparms, j);
120                        if (j == PCFSpectralElement::WIDTH && type == SpectralElement::GAUSSIAN) {
121                                (*autodiff)[j] *= GaussianSpectralElement::SigmaToFWHM;
122                        }
123                        autodiff->mask(j) = ! fixed[j];
124                }
125                func.addFunction(*autodiff);
126        }
127        fitter.setFunction(func);
128        // Max. number of iterations
129        fitter.setMaxIter(50+ ncomps*10);
130        // Convergence criterium
131        fitter.setCriteria(0.001);
132        // Fit
133        Vector<MT> sol;
134        Vector<MT> err;
135        sol = fitter.fit(x, y, sigma, mask);
136        err = fitter.errors();
137        // Number of iterations
138        iter_p = fitter.currentIteration();
139        chiSq_p = fitter.getChi2();
140        uInt j = 0;
141        Vector<Double> tmp, terr;
142        for (uInt i=0; i<ncomps; i++) {
143                SpectralElement *element = slist_p[i];
144                uInt nparms = element->getOrder();
145                tmp.resize(nparms);
146                terr.resize(nparms);
147                SpectralElement::Types type = element->getType();
148                for (uInt k=0; k<nparms; k++) {
149                        Bool convertGaussWidth = k==PCFSpectralElement::WIDTH && type == SpectralElement::GAUSSIAN;
150                        tmp(k) = convertGaussWidth
151                                ? sol(j) / GaussianSpectralElement::SigmaToFWHM
152                                : sol(j);
153                        terr(k) = convertGaussWidth
154                                ? err(j) / GaussianSpectralElement::SigmaToFWHM
155                                : err(j);
156                        j++;
157                };
158                element->set(tmp);
159                element->setError(terr);
160        }
161        return fitter.converged();
162}
163
164
165} //# NAMESPACE CASA - END
166
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