lsst.jointcal  master-g9041cab851+10
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Class List
Here are the classes, structs, unions and interfaces with brief descriptions:
[detail level 1234]
oNlsstClass for a simple mapping implementing a generic Gtransfo
|\Njointcal
| oNdataIds
| |\CPerTractCcdDataIdContainer
| oNjointcal
| |oCJointcalRunner
| |oCJointcalConfig
| |\CJointcalTask
| oNjointcalCoadd
| |\CJointcalCoaddTask
| oNutils
| |\CJointcalStatistics
| oNversion
| oCAssociationsThe class that implements the relations between MeasuredStar and FittedStar
| oCAstrometryFitClass that handles the astrometric least squares problem
| oCAstrometryModelInterface class between AstrometryFit and an actual model for the Mapping (s) from pixels to some tangent plane (aka distortions)
| oCBaseStarThe base class for handling stars. Used by all matching routines
| oCCcdImageHandler of an actual image from a single CCD
| oCChi2AccumulatorBase class for Chi2Statistic and Chi2List, to allow addEntry inside Fitter for either class
| oCChi2StatisticSimple structure to accumulate chi2 and ndof
| oCChi2Star
| oCChi2ListStructure to accumulate the chi2 contributions per each star (to help find outliers)
| oCConstrainedPhotometryModel
| oCConstrainedPolyModelThis 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)
| oCFastFinderThis is an auxillary class for matching objects from starlists
| |\CIteratorIterator meant to traverse objects within some limiting distance
| oCFatPointA Point with uncertainties
| oCPmBlockObjects whose position is going to be fitted. Coordinates in Common Tangent Plane
| oCFittedStarThe objects which have been measured several times
| oCFittedStarListA list of FittedStar s. Such a list is typically constructed by Associations
| oCFitterBaseBase class for fitters
| oCFrameRectangle with sides parallel to axes
| oCGtransfoVirtual (interface) class for geometric transformations
| oCGtransfoIdentityA do-nothing transformation. It anyway has dummy routines to mimick a Gtransfo
| oCGtransfoPolyPolynomial transformation class
| oCGtransfoLinImplements the linear transformations (6 real coefficients)
| oCGtransfoLinShiftJust here to provide a specialized constructor, and fit
| oCGtransfoLinRotJust here to provide a specialized constructor, and fit
| oCGtransfoLinScaleJust here to provide specialized constructors. GtransfoLin fit routine
| oCBaseTanWcs
| oCTanPix2RaDecTransformation that handles pix to sideral transfos (Gnomonic, possibly with polynomial distortions)
| oCTanSipPix2RaDecImplements the (forward) SIP distorsion scheme
| oCTanRaDec2PixThis one is the Tangent Plane (called gnomonic) projection (from celestial sphere to tangent plane)
| oCUserTransfoRun-time transfo that allows users to define a Gtransfo with minimal coding (just the transfo routine)
| oCHisto2d
| oCSparseHisto4dA class to histogram in 4 dimensions
| oCJointcalControl
| oCMatchConditionsParameters to be provided to combinatorial searches
| oCMappingVirtual class needed in the abstraction of the distortion model
| oCMeasuredStarObjects measured on actual images
| oCMeasuredStarListA list of MeasuredStar. They are usually filled in Associations::AddImage
| oCPhotometryFitClass that handles the photometric least squares problem
| oCPhotometryMapping
| oCPhotometryModelInterface class for PhotometryFit
| oCPhotometryTransfo
| oCPhotometryTransfoSpatiallyInvariant
| oCPointA point in a plane
| oCProjectionHandlerThis 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)
| oCIdentityProjectionHandlerThe simplest implementation of ProjectionHandler
| oCOneTPPerVisitHandlerA projection handler in which all CCDs from the same visit have the same tangent point
| oCRefStarObjects used as position anchors, typically USNO stars
| oCRefStarList
| oCSimplePhotometryModelPhotometric response model which has a single photometric factor per CcdImage
| oCSimpleGtransfoMapping
| oCSimplePolyMappingMapping implementation for a polynomial transformation
| oCSimplePolyModelThis is the model used to fit independent CCDs, meaning that there is no instrument model
| oCStarListStd::lists of Stars
| oCStarMatchA hanger for star associations
| oCStarMatchList
| oCTripletList
| oCTwoTransfoMappingThe mapping with two transfos in a row
| oCGtransfoInverse
| oCGtransfoCompositionPrivate class to handle Gtransfo compositions (i.e
| oCPolyXY
| oCSegment
| oCSegmentList
| \CSegmentPair
\CCholmodSimplicialLDLT2