TabularSpectrum.h

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//# SpectralIndex.h: Models the spectral variation with a spectral index
//# Copyright (C) 2010
//# Associated Universities, Inc. Washington DC, USA.
//#
//# This library is free software; you can redistribute it and/or modify it
//# under the terms of the GNU Library General Public License as published by
//# the Free Software Foundation; either version 2 of the License, or (at your
//# option) any later version.
//#
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//# ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or
//# FITNESS FOR A PARTICULAR PURPOSE.  See the GNU Library General Public
//# License for more details.
//#
//# You should have received a copy of the GNU Library General Public License
//# along with this library; if not, write to the Free Software Foundation,
//# Inc., 675 Massachusetts Ave, Cambridge, MA 02139, USA.
//#
//# Correspondence concerning AIPS++ should be addressed as follows:
//#        Internet email: aips2-request@nrao.edu.
//#        Postal address: AIPS++ Project Office
//#                        National Radio Astronomy Observatory
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//#
//# $Id: TabularSpectrum.h 21282 2012-11-05 11:04:19Z gervandiepen $

#ifndef COMPONENTS_TABULARSPECTRUM_H
#define COMPONENTS_TABULARSPECTRUM_H

#include <casa/aips.h>
#include <components/ComponentModels/ComponentType.h>
#include <components/ComponentModels/SpectralModel.h>
#include <components/ComponentModels/Flux.h>
namespace casa { //# NAMESPACE CASA - BEGIN

class MFrequency;
class RecordInterface;
class String;
template <class T> class Vector;

// <summary>Models the spectral variation with a spectral index</summary>

// <use visibility=export>

// <reviewed reviewer="" date="yyyy/mm/dd" tests="tSpectralIndex" demos="dSpectralModel">
// </reviewed>

// <prerequisite>
//   <li> <linkto class="SpectralModel">SpectralModel</linkto>
// </prerequisite>
//
// <synopsis>

// This class models the spectral variation of a component with measured 
// values at given frequencies. The values are interpolated in betweenm

// This class like the other spectral models becomes more useful when used
// through the <linkto class=SkyComponent>SkyComponent</linkto> class, which
// incorperates the flux and spatial variation of the emission, or through the
// <linkto class=ComponentList>ComponentList</linkto> class, which handles
// groups of SkyComponent objects.


// As with all classes derived from SpectralModel the basic operation of this
// class is to model the flux as a function of frequency. This class does not
// know what the flux is at the reference frequency. Instead the sample
// functions return factors that are used to scale the flux and calculate the
// amount of flux at a specified frequency. 

// Besides the reference frequency this class has one parameter; the spectral
// index. This parameter can be set & queried using the general purpose
// <src>parameters</src> functions or the class specific <src>index</src>
// functions.

// This class also contains functions (<src>toRecord</src> &
// <src>fromRecord</src>) which perform the conversion between Records and
// SpectralIndex objects. These functions define how a SpectralIndex
// object is represented in glish. The format of the record that is generated
// and accepted by these functions is:
// <srcblock>
// c = {'type' : 'tabular',
//       'frequency' : {'type' : 'frequency',
//                    refer : 'lsr',
//                    m0 :{'value' : [1,1.1, 1.2, 1.3, 1.4], 'unit' : 'GHz'}
//                   },
          
//       'flux' : {'value' : [1.0,1.1, 1.2, 1.3, 1.4], 'unit' : 'Jy'}
//      }
// </srcblock>
// The frequency field contains a record representation of a vector frequency 
// measure
// and its format is defined in the Measures module. Its refer field defines
// the reference frame for the direction and the m0 field defines the value of
// the reference frequency. The parsing of the type field is case
// insensitive. The index field contains the spectral index.
// </synopsis>

//
// <example>
// These examples are coded in the tSpectralModel.h file.
// <h4>Example 1:</h4>
// In this example a SpectralIndex object is created and used to calculate the
// flux at a number of frequencies.
// <srcblock>
//  SpectralIndex siModel;
//  siModel.setRefFrequency(MFrequency(Quantity(1.0, "GHz")));
//  siModel.setIndex(1.0, Stokes::I);  
//  siModel.setIndex(0.5, Stokes::Q);  
//  siModel.setIndex(0.5, Stokes::U);  
//  siModel.setIndex(-1.0, Stokes::V);
//  const Flux<Double> LBandFlux(1.0, 1.0, 1.0, 1.0);
//  const MVFrequency step(Quantity(100.0, "MHz"));
//  MVFrequency sampleFreq = siModel.refFrequency().getValue();
//  Flux<Double> sampleFlux;
//  cout << "Frequency\t I-Flux\t Q-Flux\t U-Flux\t V-Flux\n";
//  for (uInt i = 0; i < 11; i++) {
//    sampleFlux = LBandFlux.copy();
//    sampleFlux.convertPol(ComponentType::LINEAR);
//    sampleFlux.convertUnit(Unit("WU"));
//    siModel.sample(sampleFlux,
//                   MFrequency(sampleFreq, siModel.refFrequency().getRef()));
//    cout << setprecision(3) << sampleFreq.get("GHz")
//         << "\t\t " << sampleFlux.value(0u).re
//         << "\t " << sampleFlux.value(1u).re
//         << "\t " << sampleFlux.value(2u).re
//         << "\t " << sampleFlux.value(3u).re
//         << " " << sampleFlux.unit().getName() << endl;
//    sampleFreq += step;
//  }
// </srcblock>
// </example>
//
// <motivation> A Spectral Index frequency variation is the  most widely used
// model in radio astronomy. In particular the NFRA package 'newstar' uses it
// extensively.
// </motivation>
//
// <todo asof="1999/11/23">
//   <li> Nothing I hope
// </todo>

// <linkfrom anchor="SpectralIndex" classes="SpectralModel ConstantSpectrum">
//  <here>SpectralIndex</here> - Uses a spectral index to model the spectrum
// </linkfrom>
 
class TabularSpectrum: public SpectralModel
{
public:
  // The default SpectralIndex has a reference frequency of 1 GHz in the LSR
  // frame and a spectral index of zero. As such it is no different from the
  // ConstantSpectrum class (except slower).
  TabularSpectrum();

  // Construct a Tabular  values with I and f specified
  // exponent.
  TabularSpectrum(const MFrequency& refFreq, const Vector<MFrequency::MVType>& freq,
                  const Vector<Flux<Double> >& flux, const MFrequency::Ref& refFrame);

  // The copy constructor uses copy semantics
  TabularSpectrum(const TabularSpectrum& other);

  // The destructor does nothing special.
  virtual ~TabularSpectrum();

  // The assignment operator uses copy semantics.
  TabularSpectrum& operator=(const TabularSpectrum& other);

  // return the actual spectral type ie., ComponentType::TABULAR_SPECTRUM
  virtual ComponentType::SpectralShape type() const;

  // set/get the Tabular values
  // <group>
  void values(Vector<MFrequency::MVType>& freq, Vector<Flux<Double> >& flux) const;
  void setValues(const Vector<MFrequency::MVType>& frequencies, const Vector<Flux<Double> >& flux, const MFrequency::Ref& refFrame);
  // </group>

  // Return the scaling factor that indicates what proportion of the flux is at
  // the specified frequency. ie. if the centreFrequency argument is the
  // reference frequency then this function will always return one. At other
  // frequencies it will return a non-negative number.
  virtual Double sample(const MFrequency& centerFrequency) const;

  // Same as the previous function except that many frequencies can be sampled
  // at once. The reference frame must be the same for all the specified
  // frequencies. Uses a customised implementation for improved speed.
  virtual void sample(Vector<Double>& scale, 
                      const Vector<MFrequency::MVType>& frequencies, 
                      const MFrequency::Ref& refFrame) const;

  // Return a pointer to a copy of this object upcast to a SpectralModel
  // object. The class that uses this function is responsible for deleting the
  // pointer. This is used to implement a virtual copy constructor.
  virtual SpectralModel* clone() const;

  // return the number of parameters. There is one parameter for this spectral
  // model, namely the spectral index. So you supply a unit length vector when
  // using these functions. Otherwise an exception (AipsError) may be thrown.
  // <group>
  virtual uInt nParameters() const;
  virtual void setParameters(const Vector<Double>& newSpectralParms);
  virtual Vector<Double> parameters() const;
  virtual void setErrors(const Vector<Double>& newSpectralErrs);
  virtual Vector<Double> errors() const;
  // </group>

  // These functions convert between a Record and a SpectralIndex. These
  // functions define how a SpectralIndex object is represented in glish and
  // this is detailed in the synopsis above. These functions return False if
  // the record is malformed and append an error message to the supplied string
  // giving the reason.
  // <group>
  virtual Bool fromRecord(String& errorMessage, const RecordInterface& record);
  virtual Bool toRecord(String& errorMessage, RecordInterface& record) const;
  // </group>

  // Convert the parameters of the spectral index object to the specified
  // units. Only one field of the supplied record is used, namely 'index'. This
  // field is optional as the spectral index is a unitless quantity. If the
  // index field is specified it must have the empty string as its value.  This
  // function always returns True unless the index field is specified and does
  // not contain an empty string.
  virtual Bool convertUnit(String& errorMessage,
                           const RecordInterface& record);

  // Function which checks the internal data of this class for consistant
  // values. Returns True if everything is fine otherwise returns False.
  virtual Bool ok() const;

private:
  
  MFrequency::Ref freqRef_p;
  Vector<Double> tabFreqVal_p;
  Vector<Flux<Double> > flux_p;
  Vector<Double> ival_p;
  Double referenceFreq_p;
  Double maxFreq_p;
  Double minFreq_p;
  
};

} //# NAMESPACE CASA - END

#endif