lsst.jointcal  16.0-17-g0bdc215
Class List
Here are the classes, structs, unions and interfaces with brief descriptions:
[detail level 1234]
 NlsstClass for a simple mapping implementing a generic Gtransfo
 Njointcal
 NdataIds
 CPerTractCcdDataIdContainer
 Njointcal
 CJointcalConfig
 CJointcalRunner
 CJointcalTask
 NjointcalCoadd
 CJointcalCoaddTask
 CJointcalCoaddTaskConfig
 Nutils
 CJointcalStatistics
 CAssociationsThe class that implements the relations between MeasuredStar and FittedStar
 CAstrometryFitClass that handles the astrometric least squares problem
 CAstrometryMappingVirtual class needed in the abstraction of the distortion model
 CAstrometryModelInterface class between AstrometryFit and an actual model for the Mapping (s) from pixels to some tangent plane (aka distortions)
 CBaseStarThe base class for handling stars. Used by all matching routines
 CBaseTanWcs
 CCcdImageHandler of an actual image from a single CCD
 CCcdImageKeyFor hashing a ccdImage: the pair of (visit, ccd) IDs should be unique to each ccdImage
 CChi2AccumulatorBase class for Chi2Statistic and Chi2List, to allow addEntry inside Fitter for either class
 CChi2ListStructure to accumulate the chi2 contributions per each star (to help find outliers)
 CChi2Star
 CChi2StatisticSimple structure to accumulate chi2 and ndof
 CChipVisitFluxMapping
 CChipVisitMagnitudeMapping
 CChipVisitPhotometryMappingA two-level photometric transform: one for the ccd and one for the visit
 CConstrainedAstrometryModelThis is the model used to fit mappings as the combination of a transformation depending on the chip number (instrument model) and a transformation per visit (anamorphism)
 CConstrainedFluxModel
 CConstrainedMagnitudeModel
 CConstrainedPhotometryModelPhotometry model with constraints, \(M(x,y) = M_CCD(x,y)*M_visit(u,v)\)
 CFastFinderThis is an auxillary class for matching objects from starlists
 CIteratorIterator meant to traverse objects within some limiting distance
 CFatPointA Point with uncertainties
 CFittedStarThe objects which have been measured several times
 CFittedStarListA list of FittedStar s. Such a list is typically constructed by Associations
 CFitterBaseBase class for fitters
 CFluxTransfoChebyshevNth-order 2d Chebyshev photometry transfo, times the input flux
 CFluxTransfoSpatiallyInvariantPhotometric offset independent of position, defined as (fluxMag0)^-1
 CFrameRectangle with sides parallel to axes
 CGtransfoVirtual (interface) class for geometric transformations
 CGtransfoCompositionPrivate class to handle Gtransfo compositions (i.e
 CGtransfoIdentityA do-nothing transformation. It anyway has dummy routines to mimick a Gtransfo
 CGtransfoInverse
 CGtransfoLinImplements the linear transformations (6 real coefficients)
 CGtransfoLinRotJust here to provide a specialized constructor, and fit
 CGtransfoLinScaleJust here to provide specialized constructors. GtransfoLin fit routine
 CGtransfoLinShiftJust here to provide a specialized constructor, and fit
 CGtransfoPolyPolynomial transformation class
 CGtransfoSkyWcsA Gtransfo that holds a SkyWcs
 CHisto2d
 CIdentityProjectionHandlerThe simplest implementation of ProjectionHandler
 CJointcalControl
 CMagnitudeTransfoChebyshev
 CMagnitudeTransfoSpatiallyInvariantPhotometric offset independent of position, defined as -2.5 * log(flux / fluxMag0)
 CMatchConditionsParameters to be provided to combinatorial searches
 CMeasuredStarObjects measured on actual images
 CMeasuredStarListA list of MeasuredStar. They are usually filled in Associations::createCcdImage
 COneTPPerVisitHandlerA projection handler in which all CCDs from the same visit have the same tangent point
 CPhotometryFitClass that handles the photometric least squares problem
 CPhotometryMappingA mapping containing a single photometryTransfo
 CPhotometryMappingBaseRelates transfo(s) to their position in the fitting matrix and allows interaction with the transfo(s)
 CPhotometryModelInterface class for PhotometryFit
 CPhotometryTransfoA photometric transform, defined in terms of the input flux or magnitude
 CPhotometryTransfoChebyshevNth-order 2d Chebyshev photometry transfo
 CPhotometryTransfoSpatiallyInvariantPhotometry offset independent of position
 CPmBlockObjects whose position is going to be fitted. Coordinates in Common Tangent Plane
 CPointA point in a plane
 CPolyXY
 CProjectionHandlerThis is a virtual class that allows a lot of freedom in the choice of the projection from "Sky" (where coodinates are reported) to tangent plane (where they are compared to transformed measurements)
 CRefStarObjects used as position anchors, typically USNO stars
 CRefStarList
 CSegment
 CSegmentList
 CSegmentPair
 CSimpleAstrometryModelThis is the model used to fit independent CCDs, meaning that there is no instrument model
 CSimpleFluxModel
 CSimpleGtransfoMapping
 CSimpleMagnitudeModel
 CSimplePhotometryModelPhotometric response model which has a single photometric factor per CcdImage
 CSimplePolyMappingMapping implementation for a polynomial transformation
 CSparseHisto4dA class to histogram in 4 dimensions
 CStarListStd::lists of Stars
 CStarMatchA hanger for star associations
 CStarMatchList
 CTanPix2RaDecTransformation that handles pix to sideral transfos (Gnomonic, possibly with polynomial distortions)
 CTanRaDec2PixThis one is the Tangent Plane (called gnomonic) projection (from celestial sphere to tangent plane)
 CTanSipPix2RaDecImplements the (forward) SIP distorsion scheme
 CTripletList
 CTwoTransfoMappingThe mapping with two transfos in a row
 CUserTransfoRun-time transfo that allows users to define a Gtransfo with minimal coding (just the transfo routine)
 NstdSTL namespace
 Chash< lsst::jointcal::CcdImageKey >Hash a ccdImage by its visit and ccd IDs
 CCholmodSimplicialLDLT2