WB Clean Image Sky Model: Image Sky Model implementing a Wide-Band multi frequency synthesis algorithm.
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| WBCleanImageSkyModel () |
| Create a WBCleanImageSkyModel - default scale size = 1 pixel. More...
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| WBCleanImageSkyModel (const casacore::Int ntaylor, const casacore::Int nscales, const casacore::Double reffreq) |
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| WBCleanImageSkyModel (const casacore::Int ntaylor, const casacore::Vector< casacore::Float > &userScaleSizes, const casacore::Double reffreq) |
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| ~WBCleanImageSkyModel () |
| destructor More...
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casacore::Bool | solve (SkyEquation &se) |
| Solve for this SkyModel. More...
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casacore::Bool | solveResiduals (SkyEquation &se, casacore::Bool modelToMS=false) |
| casacore::Int add(casacore::ImageInterface<casacore::Float>& iimage, const casacore::Int maxNumXfr=100); casacore::Bool addResidual(casacore::Int thismodel, casacore::ImageInterface<casacore::Float>& iresidual); void initializeGradients(); More...
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casacore::Bool | makeNewtonRaphsonStep (SkyEquation &se, casacore::Bool incremental=false, casacore::Bool modelToMS=false) |
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casacore::Int | numberOfTaylorTerms () |
| MFS : Number of taylor terms per model. More...
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casacore::Double | getReferenceFrequency () |
| MFS : Reference Frequency. More...
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casacore::Int | getModelIndex (casacore::uInt model, casacore::uInt taylor) |
| Major axis for ordering : Taylor. More...
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casacore::Int | getTaylorIndex (casacore::uInt index) |
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casacore::Int | getFieldIndex (casacore::uInt index) |
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casacore::Bool | calculateCoeffResiduals () |
| MFS : In-place coefficient residual calculations. More...
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casacore::Bool | calculateAlphaBeta (const casacore::Vector< casacore::String > &restoredNames, const casacore::Vector< casacore::String > &residualNames) |
| MFS : Calculate restored alpha and beta. More...
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| CleanImageSkyModel () |
| Empty constructor. More...
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| CleanImageSkyModel (const CleanImageSkyModel &sm) |
| Copy constructor. More...
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casacore::Bool | hasMask (casacore::Int model=0) |
| Has a mask for model? More...
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virtual casacore::Bool | add (ComponentList &compList) |
| Add a componentlist. More...
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virtual casacore::Int | add (casacore::ImageInterface< casacore::Float > &image, const casacore::Int maxNumXfr=100) |
| Add an image. More...
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virtual casacore::Bool | addMask (casacore::Int image, casacore::ImageInterface< casacore::Float > &mask) |
| Add an mask. More...
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casacore::Bool | hasFluxMask (casacore::Int model=0) |
| Has a flux mask? More...
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virtual casacore::Bool | addFluxMask (casacore::Int image, casacore::ImageInterface< casacore::Float > &fluxMask) |
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casacore::ImageInterface
< casacore::Float > & | fluxMask (casacore::Int model=0) |
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virtual | ~CleanImageSkyModel () |
| Destructor. More...
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CleanImageSkyModel & | operator= (const CleanImageSkyModel &other) |
| Assignment operator. More...
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casacore::ImageInterface
< casacore::Float > & | mask (casacore::Int model=0) |
| Return masks. More...
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virtual void | setJointStokesClean (casacore::Bool joint=true) |
| set to search for peak in I^2+Q^2+U^2+V^2 domain or each stokes plane seperately Ignored for hogbom and msclean for now More...
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virtual casacore::Float | maxField (casacore::Vector< casacore::Float > &imagemax, casacore::Vector< casacore::Float > &imagemin) |
| Return the maximum absolute value from residual images per field. More...
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| ImageSkyModel (const casacore::Int maxNumModels=1) |
| Empty constructor. More...
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void | setMaxNumberModels (const casacore::Int maxNumModels) |
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| ImageSkyModel (const ImageSkyModel &sm) |
| Copy constructor. More...
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virtual casacore::Bool | updatemodel (ComponentList &compList) |
| update componentlist More...
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virtual casacore::Bool | updatemodel (const casacore::Int thismodel, casacore::ImageInterface< casacore::Float > &image) |
| update model image...you have to have added it before...nmodels_p held has to be bigger that image here its left to the caller to make sure the image is conformant...otherwise you are in trouble. More...
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virtual casacore::Bool | addResidual (casacore::Int image, casacore::ImageInterface< casacore::Float > &residual) |
| Add a residual image. More...
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virtual | ~ImageSkyModel () |
| Destructor. More...
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ImageSkyModel & | operator= (const ImageSkyModel &other) |
| Assignment operator. More...
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virtual casacore::Int | numberOfModels () |
| Number of models contained. More...
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virtual casacore::Int | getTaylorIndex (casacore::Int index) |
| MFS : Index of Taylor term in array of nmodels x ntaylorterms
virtual casacore::Int getTaylorIndex(casacore::Int index){return 0;} More...
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casacore::Bool | isSolveable (casacore::Int model=0) |
| Is this model solveable? More...
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casacore::Bool | free (casacore::Int model=0) |
| Free and fix the model (returns previous status). More...
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casacore::Bool | fix (casacore::Int model=0) |
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virtual void | initializeGradients () |
| Initialize for gradient search. More...
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virtual void | finalizeGradients () |
| Finalize for gradient search. More...
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casacore::Bool | hasComponentList () |
| Does this have a component list? More...
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casacore::Bool | isEmpty (casacore::Int model=0) |
| Is this model empty. More...
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virtual ComponentList & | componentList () |
| Return the component list. More...
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casacore::ImageInterface
< casacore::Float > & | image (casacore::Int model=0) |
| Return actual images to be used by SkyEquation. More...
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casacore::ImageInterface
< casacore::Complex > & | cImage (casacore::Int model=0) |
| casacore::Complex image (needed for e.g. More...
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casacore::ImageInterface
< casacore::Complex > & | XFR (casacore::Int model=0, casacore::Int numXFR=0) |
| casacore::Complex XFR More...
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casacore::ImageInterface
< casacore::Float > & | PSF (casacore::Int model=0) |
| PSF. More...
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casacore::ImageInterface
< casacore::Float > & | gS (casacore::Int model=0) |
| Gradient of chi-squared wrt pixels. More...
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casacore::ImageInterface
< casacore::Float > & | residual (casacore::Int model=0) |
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casacore::ImageInterface
< casacore::Float > & | ggS (casacore::Int model=0) |
| Grad Grad chi-squared wrt pixels (diagonal elements only) More...
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casacore::ImageInterface
< casacore::Float > & | fluxScale (casacore::Int model=0) |
| if (doFluxScale(mod)) image(mod) * fluxScale(mod) gives actual brightness distribution More...
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casacore::ImageInterface
< casacore::Float > & | work (casacore::Int model=0) |
| Work image. More...
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casacore::ImageInterface
< casacore::Float > & | deltaImage (casacore::Int model=0) |
| Increment in the image. More...
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casacore::Bool | doFluxScale (casacore::Int model=0) |
| tells if this model needs to be multiplied by a flux scale image More...
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void | mandateFluxScale (casacore::Int model=0) |
| require use of flux scale image More...
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casacore::Bool | hasXFR (casacore::Int model=0) |
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void | addStatistics (casacore::Float sumwt, casacore::Float chisq) |
| Add to Sum weights, Chi-Squared. More...
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casacore::Matrix
< casacore::Float > & | weight (casacore::Int model=0) |
| Weight per model (channels, polarizations) More...
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casacore::Bool | solveResiduals (SkyEquation &me, casacore::Bool modelToMS=false) |
| Solve explicitly for the residuals: same as solve for this class modelToMs determines if predicted vis is put in the MODEL_DATA column. More...
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virtual void | makeApproxPSFs (SkyEquation &se) |
| Make the approximate PSFs needed for each model. More...
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virtual
casacore::ImageInterface
< casacore::Float > & | getResidual (casacore::Int model=0) |
| Get current residual image: this is either that image specified via addResidual, or a scratch image. More...
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casacore::ImageBeamSet & | beam (casacore::Int model=0) |
| Return the fitted beam for each model. More...
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void | setPGPlotter (casacore::PGPlotter &pgp) |
| Set casacore::PGPlotter to be used. More...
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void | setCycleFactor (float x) |
| This is the factor by which you multiply the worst outer sidelobe by to get the threshold for the current cycle. More...
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void | setCycleSpeedup (float x) |
| Cycle threshold will double in this number of iterations (ie, use a large number if you don't want cycle threshold to inch up) More...
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void | setCycleMaxPsfFraction (float x) |
| Yet another control for the minor cycle threshold. More...
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void | setDisplayProgress (const casacore::Bool display) |
| Set the variable that switches on the progress display. More...
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void | setDataPolFrame (StokesImageUtil::PolRep datapolrep) |
| Set a variable to indicate the polarization frame in the data (circular or linear). More...
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virtual void | setMemoryUse (casacore::Bool useMem=false) |
| try to make templattices use memory if possible if set to false then always use disk More...
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virtual casacore::Bool | getMemoryUse () |
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void | setTileVol (const casacore::Int tileVol=1000000) |
| Set templattice tile vol in pixels. More...
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| SkyModel () |
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void | setAlgorithm (const casacore::String &alg) |
| set Algorithm (e.g clean, mem, nnls) More...
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const casacore::String | getAlgorithm () |
| get Algorithm More...
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void | setSubAlgorithm (const casacore::String &alg) |
| set Sub Algorithm More...
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const casacore::String | getSubAlgorithm () |
| get Sub Algorithm More...
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void | setImageRegion (casacore::ImageRegion &ir) |
| Set the imageregion that will be used for the next XFR generation. More...
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void | unsetImageRegion () |
| use the default shape More...
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void | setImageNormalization (casacore::Bool val) |
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casacore::Bool | isImageNormalized () |
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| Iterate () |
| Constructor. More...
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virtual | ~Iterate () |
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void | setFree () |
| Is this a free variable? More...
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void | setNotFree () |
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casacore::Bool | free () |
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void | setNumberIterations (const casacore::Int n) |
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void | setGain (const casacore::Float g) |
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void | setTolerance (const casacore::Float t) |
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void | setThreshold (const casacore::Float t) |
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void | setMode (const casacore::String m) |
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casacore::Int | numberIterations () |
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casacore::Float | gain () |
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casacore::Float | tolerance () |
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virtual casacore::Float | threshold () |
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const casacore::String | mode () |
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WB Clean Image Sky Model: Image Sky Model implementing a Wide-Band multi frequency synthesis algorithm.
Intended use:
Public interface
Prerequisite
Etymology
WBCleanImageSkyModel implements the Wide Band Clean algorithm. It is derived from SkyModel.
Synopsis
The WB Clean is the multi-frequency synthesis deconvolution algorithm. It decomposes an image into a linear compbination of models convolved with spectral dirty beams of various order. A multiscale variant can be invoked by supplying a user vector of scale sizes. Default is 1, corresponding to a scale insensitive mfs deconvolution.
Masking is optionally performed using a mask image: only points where the mask is non-zero are searched for Gaussian components. This can cause some difficulty, as the different Gaussian scale sizes will extend beyond the mask by different amounts. If no mask is specified all points in the inner quarter of the image are cleaned.
Example
See the example for SkyModel.
Motivation
Definition at line 91 of file WBCleanImageSkyModel.h.