casa::ImageFit1D< T > Class Template Reference

Fit spectral components to a Vector of data from an image. More...

#include <ImageFit1D.h>

List of all members.

Public Types

enum  AbcissaType {
  PIXEL,
  IM_NATIVE,
  VELOCITY,
  N_TYPES
}

Public Member Functions

 ImageFit1D (SHARED_PTR< const ImageInterface< T > > image, uInt axis=0)
 Constructor.
 ImageFit1D (SHARED_PTR< const ImageInterface< T > > image, SHARED_PTR< const ImageInterface< T > > weights, uInt axis=0)
 Constructor with fitting weights image.
 ~ImageFit1D ()
 Destructor.
 ImageFit1D (const ImageFit1D &other)
 Copy constructor.
ImageFit1Doperator= (const ImageFit1D &other)
 Assignment operator.
void setData (const IPosition &pos, Array< FitterType >(*yfunc)(const Array< FitterType > &)=0)
 Set the data to be fit.
void setData (const IPosition &pos, const ImageFit1D< T >::AbcissaType type, const Bool doAbs=True, const Double *const &abscissaDivisor=0, Array< Double >(*xfunc)(const Array< Double > &)=0, Array< FitterType >(*yfunc)(const Array< FitterType > &)=0)
void setElements (const SpectralList &list)
 Set a SpectralList of SpectralElements to fit for.
void addElement (const SpectralElement &el)
 Add new SpectralElement(s) to the SpectralList (can be empty) of SpectralElements to be fit for.
void addElements (const SpectralList &list)
void setGaussianElements (uInt nGauss)
 Set a SpectralList of Gaussian SpectralElements to fit for.
void clearList ()
 Clear the SpectralList of elements to be fit for.
Bool fit ()
 Do the fit and return convergence status.
Double getChiSquared () const
 Get Chi Squared of fit.
Double getNumberIterations () const
 Get number of iterations for last fit.
const SpectralListgetList (Bool fit=True) const
 Recover the list of elements.
Vector< T > getEstimate (Int which=-1) const
 Recover vectors for the estimate, fit and residual.
Vector< T > getFit (Int which=-1) const
Vector< T > getResidual (Int which=-1, Bool fit=True) const
Bool setXMask (const std::set< uInt > &indices, Bool specifiedPixelsAreGood)
Vector< Bool > getDataMask () const
 get data mask
Vector< Bool > getTotalMask () const
 Get Total Mask (data and range mask).
Bool succeeded () const
 did the fit succeed? should only be called after fit().
Bool converged () const
 did the fit converge? should only be called after fit().
void invalidate ()
 flag the solution as invalid based on external criteria.
Bool isValid () const
 is the solution valid? If False, some external logic has called invalidate()
void setAbscissa (const Vector< Double > &x)
 Set the abscissa values prior to running setData.
Vector< Double > makeAbscissa (ImageFit1D< T >::AbcissaType type, Bool doAbs, const Double *const &abscissaDivisor)
 make the abscissa values, x.

Static Public Member Functions

static Bool setAbcissaState (String &errMsg, ImageFit1D< T >::AbcissaType &type, CoordinateSystem &cSys, const String &xUnit, const String &doppler, uInt pixelAxis)
 Helper function.

Private Member Functions

 ImageFit1D ()
 Disallow default constructor.
void check () const
void checkType () const
void _construct ()
void copy (const ImageFit1D< T > &other)
void _resetFitter ()
 void setWeightsImage (const ImageInterface<T>& im);

Private Attributes

SHARED_PTR< const
ImageInterface< T > > 
_image
SHARED_PTR< const
ImageInterface< T > > 
_weights
uInt _axis
ProfileFit1D< FitterType > _fitter
 In the future I will be able to template the fitter on T.
Bool _converged
Bool _success
Bool _isValid
Vector< Double > _x
Vector< Double > _unityWeights
Vector< Double > _weightSlice
IPosition _sliceShape

Detailed Description

template<class T>
class casa::ImageFit1D< T >

Fit spectral components to a Vector of data from an image.

Intended use:

Public interface

Review Status

Test programs:
tImageFit1D

Prerequisite

Synopsis

Fit lists (held in class SpectralList) of SpectralElements to a Vector of data from the image. Each SpectralElement can be one from a variety of types. The values of the parameters for each SpectralElement provide the initial starting guesses for the fitting process.

You specify the domain in which the fit is to be done via the enum AbcissaType. The CoordinateSystem in the image is used to convert the pixel coordinates to the desired abcissa. You can change the units of the CoordinateSystem if you want to fit in different units. If you set an estimate yourself (function setElements or addElement) it is the callers responsibility that the elements are in the correct abcissa domain. Function setGaussianElements will automatically make an estimate in the correct domain.

Also, a SpectralElement object holds a mask indicating whether a parameter should be held fixed or solved for. After the fitting is done, a new SpectralList holding SpectralElements with the fitted parameters is created.

For all the functions that return a status Bool, True is good. If False is returned, an error message can be recovered with function errorMessage, You should not proceed if False is returned.

Exceptions will be thrown if you do not set the Image and axis via the constructor or setImage function.

Example

 PagedImage<Float> im("myimage");
 Int axis = 2;
 ImageFit1D<Float> fitter(image, axis);
 IPosition pos(in.ndim(),0);
 fitter.setData(pos, ImageFit1D<Float>::IM_NATIVE);     // Fit in native coordinate space
 fitter.setGaussianElements(3);                      // FIt 3 Gaussians
 if (fitter.fit()) {
 cerr << fitter.getList() << endl;                // Print result
 }

To Do

Definition at line 117 of file ImageFit1D.h.


Member Enumeration Documentation

template<class T>
enum casa::ImageFit1D::AbcissaType
Enumerator:
PIXEL 
IM_NATIVE 
VELOCITY 
N_TYPES 

Definition at line 122 of file ImageFit1D.h.


Constructor & Destructor Documentation

template<class T>
casa::ImageFit1D< T >::ImageFit1D ( SHARED_PTR< const ImageInterface< T > >  image,
uInt  axis = 0 
)

Constructor.

Fitting weights are assumed all unity.

template<class T>
casa::ImageFit1D< T >::ImageFit1D ( SHARED_PTR< const ImageInterface< T > >  image,
SHARED_PTR< const ImageInterface< T > >  weights,
uInt  axis = 0 
)

Constructor with fitting weights image.

The data and weights images must be the same shape.

template<class T>
casa::ImageFit1D< T >::~ImageFit1D (  ) 

Destructor.

template<class T>
casa::ImageFit1D< T >::ImageFit1D ( const ImageFit1D< T > &  other  ) 

Copy constructor.

Uses reference semantics.

template<class T>
casa::ImageFit1D< T >::ImageFit1D (  )  [inline, private]

Disallow default constructor.

Definition at line 304 of file ImageFit1D.h.


Member Function Documentation

template<class T>
void casa::ImageFit1D< T >::_construct (  )  [private]
template<class T>
void casa::ImageFit1D< T >::_resetFitter (  )  [private]

void setWeightsImage (const ImageInterface<T>& im);

reset the fitter, for example if we've done a fit and want to move to the next position in the image

template<class T>
void casa::ImageFit1D< T >::addElement ( const SpectralElement el  )  [inline]

Add new SpectralElement(s) to the SpectralList (can be empty) of SpectralElements to be fit for.

You must have already called setData to call this function.

Definition at line 204 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, and casa::ProfileFit1D< T >::addElement().

template<class T>
void casa::ImageFit1D< T >::addElements ( const SpectralList list  )  [inline]
template<class T>
void casa::ImageFit1D< T >::check (  )  const [private]
template<class T>
void casa::ImageFit1D< T >::checkType (  )  const [private]
template<class T>
void casa::ImageFit1D< T >::clearList (  )  [inline]

Clear the SpectralList of elements to be fit for.

Definition at line 217 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, and casa::ProfileFit1D< T >::clearList().

template<class T>
Bool casa::ImageFit1D< T >::converged (  )  const

did the fit converge? should only be called after fit().

template<class T>
void casa::ImageFit1D< T >::copy ( const ImageFit1D< T > &  other  )  [private]
template<class T>
Bool casa::ImageFit1D< T >::fit (  ) 

Do the fit and return convergence status.

Errors in the fitting process will generate an AipsError exception and you should catch these yourself.

Referenced by casa::ImageFit1D< T >::getList().

template<class T>
Double casa::ImageFit1D< T >::getChiSquared (  )  const [inline]

Get Chi Squared of fit.

Definition at line 225 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, and casa::ProfileFit1D< T >::getChiSquared().

template<class T>
Vector<Bool> casa::ImageFit1D< T >::getDataMask (  )  const [inline]

get data mask

Definition at line 252 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, and casa::ProfileFit1D< T >::getDataMask().

template<class T>
Vector<T> casa::ImageFit1D< T >::getEstimate ( Int  which = -1  )  const

Recover vectors for the estimate, fit and residual.

If you don't specify which element, all elements are included If the Vectors are returned with zero length, it means an error condition exists (e.g. asking for fit before you do one). In this case an error message can be recovered with function errorMessage.

template<class T>
Vector<T> casa::ImageFit1D< T >::getFit ( Int  which = -1  )  const
template<class T>
const SpectralList& casa::ImageFit1D< T >::getList ( Bool  fit = True  )  const [inline]

Recover the list of elements.

You can get the elements as initially estimated (fit=False), or after fitting (fit=True). In the latter case, the SpectralElements hold the parameters and errors of the fit.

Definition at line 234 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, casa::ImageFit1D< T >::fit(), and casa::ProfileFit1D< T >::getList().

template<class T>
Double casa::ImageFit1D< T >::getNumberIterations (  )  const [inline]

Get number of iterations for last fit.

Definition at line 228 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, and casa::ProfileFit1D< T >::getNumberIterations().

template<class T>
Vector<T> casa::ImageFit1D< T >::getResidual ( Int  which = -1,
Bool  fit = True 
) const
template<class T>
Vector<Bool> casa::ImageFit1D< T >::getTotalMask (  )  const [inline]

Get Total Mask (data and range mask).

Definition at line 255 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, and casa::ProfileFit1D< T >::getTotalMask().

template<class T>
void casa::ImageFit1D< T >::invalidate (  ) 

flag the solution as invalid based on external criteria.

template<class T>
Bool casa::ImageFit1D< T >::isValid (  )  const

is the solution valid? If False, some external logic has called invalidate()

template<class T>
Vector<Double> casa::ImageFit1D< T >::makeAbscissa ( ImageFit1D< T >::AbcissaType  type,
Bool  doAbs,
const Double *const &  abscissaDivisor 
)

make the abscissa values, x.

If type=IN_NATIVE and abscissaDivisor is not null, then divide the native values by the value pointed to by <src>abscissaDivisor in making the abscissa values.

template<class T>
ImageFit1D& casa::ImageFit1D< T >::operator= ( const ImageFit1D< T > &  other  ) 

Assignment operator.

Uses reference semantics.

template<class T>
static Bool casa::ImageFit1D< T >::setAbcissaState ( String &  errMsg,
ImageFit1D< T >::AbcissaType type,
CoordinateSystem &  cSys,
const String &  xUnit,
const String &  doppler,
uInt  pixelAxis 
) [static]

Helper function.

Sets up the CoordinateSystem to reflect the choice of abcissa unit and the doppler (if the axis is spectral).

template<class T>
void casa::ImageFit1D< T >::setAbscissa ( const Vector< Double > &  x  )  [inline]

Set the abscissa values prior to running setData.

If this is done, then the abscissa values will not be recomputed when setData is called. This can imporove performance if, for example, you are looping over several fitters for which you know the abscissa values do not change.

Definition at line 281 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_x.

template<class T>
void casa::ImageFit1D< T >::setData ( const IPosition &  pos,
const ImageFit1D< T >::AbcissaType  type,
const Bool  doAbs = True,
const Double *const &  abscissaDivisor = 0,
Array< Double >(*)(const Array< Double > &)  xfunc = 0,
Array< FitterType >(*)(const Array< FitterType > &)  yfunc = 0 
)
template<class T>
void casa::ImageFit1D< T >::setData ( const IPosition &  pos,
Array< FitterType >(*)(const Array< FitterType > &)  yfunc = 0 
)

Set the data to be fit.

All non-profile axes data are averaged. For the profile axis, the full spectrum is taken. The abscissa world values are computed when you call these functions unless they have been set previously by a call to setAbscissa() in which case the values that were passed to that method are used. Use the first form of setData() in this case. The domain of the abscissa values is controlled by AbcissaType and doAbs (absolute coordinates). The CoordinateSystem in the image is used to convert from pixels to world values. If type=IN_NATIVE and abscissaDivisor is not null, the world abscissa values will be divided by the value pointed to by abscissaDivisor. This mitigates having very large or very small abscissa values when fitting. If xfunc and/or yfunc is not NULL, the x and/or y values are fed to the specified function and the resultant values are what are used for the x and/or y values in the fit. If xfunc is not NULL and setAbscissa values has been called prior, no abscissa value transformation occurs. Thus if you want to apply a function to the abscissa values, the caller should pass the result of that function into setAbscissaValues.

template<class T>
void casa::ImageFit1D< T >::setElements ( const SpectralList list  )  [inline]

Set a SpectralList of SpectralElements to fit for.

These elements must be in the correct abcissa domain set in function setData. You must have already called setData to call this function. The SpectralElements in the list hold the initial estimates. They also contain the information about whether specific parameters are to be held fixed or allowed to vary in the fitting process. You can recover the list of elements with function getList.

Definition at line 198 of file ImageFit1D.h.

References casa::ImageFit1D< T >::_fitter, and casa::ProfileFit1D< T >::setElements().

template<class T>
void casa::ImageFit1D< T >::setGaussianElements ( uInt  nGauss  ) 

Set a SpectralList of Gaussian SpectralElements to fit for.

The initial estimates for the Gaussians will be automatically determined in the correct abcissa domain. All of the parameters created by this function will be solved for by default. You can recover the list of elements with function getList. Status is returned, if False, error message can be recovered with errorMessage

template<class T>
Bool casa::ImageFit1D< T >::setXMask ( const std::set< uInt > &  indices,
Bool  specifiedPixelsAreGood 
) [inline]
template<class T>
Bool casa::ImageFit1D< T >::succeeded (  )  const

did the fit succeed? should only be called after fit().


Member Data Documentation

template<class T>
uInt casa::ImageFit1D< T >::_axis [private]

Definition at line 293 of file ImageFit1D.h.

template<class T>
Bool casa::ImageFit1D< T >::_converged [private]

Definition at line 299 of file ImageFit1D.h.

template<class T>
ProfileFit1D<FitterType> casa::ImageFit1D< T >::_fitter [private]
template<class T>
SHARED_PTR<const ImageInterface<T> > casa::ImageFit1D< T >::_image [private]

Definition at line 292 of file ImageFit1D.h.

template<class T>
Bool casa::ImageFit1D< T >::_isValid [private]

Definition at line 299 of file ImageFit1D.h.

template<class T>
IPosition casa::ImageFit1D< T >::_sliceShape [private]

Definition at line 301 of file ImageFit1D.h.

template<class T>
Bool casa::ImageFit1D< T >::_success [private]

Definition at line 299 of file ImageFit1D.h.

template<class T>
Vector<Double> casa::ImageFit1D< T >::_unityWeights [private]

Definition at line 300 of file ImageFit1D.h.

template<class T>
SHARED_PTR<const ImageInterface<T> > casa::ImageFit1D< T >::_weights [private]

Definition at line 292 of file ImageFit1D.h.

template<class T>
Vector<Double> casa::ImageFit1D< T >::_weightSlice [private]

Definition at line 300 of file ImageFit1D.h.

template<class T>
Vector<Double> casa::ImageFit1D< T >::_x [private]

Definition at line 300 of file ImageFit1D.h.

Referenced by casa::ImageFit1D< T >::setAbscissa().


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