lsst.jointcal g93dcef90ea+f540a5a95e
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Namespace List
Here is a list of all namespaces with brief descriptions:
[detail level 1234]
 Nlsst
 Njointcal
 NcameraGeometry
 CCameraModel
 Ncheck_logged_chi2
 CChi2Data
 CLogParser
 Njointcal
 CJointcalConfig
 CJointcalInputData
 CJointcalTask
 CJointcalTaskConnections
 NtestUtils
 Nversion
 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 between AstrometryFit and the combinations of Mappings from pixels to some tangent plane (aka distortions)
 CAstrometryTransformVirtual (interface) class for geometric transformations
 CAstrometryTransformCompositionPrivate class to handle AstrometryTransform compositions (i.e
 CAstrometryTransformIdentityA do-nothing transformation. It anyway has dummy routines to mimick a AstrometryTransform
 CAstrometryTransformInverse
 CAstrometryTransformLinearImplements the linear transformations (6 real coefficients)
 CAstrometryTransformLinearRotJust here to provide a specialized constructor, and fit
 CAstrometryTransformLinearScaleJust here to provide specialized constructors. AstrometryTransformLinear fit routine
 CAstrometryTransformLinearShiftJust here to provide a specialized constructor, and fit
 CAstrometryTransformPolynomialPolynomial transformation class
 CAstrometryTransformSkyWcsA AstrometryTransform that holds a SkyWcs
 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
 CChipVisitAstrometryMappingThe mapping with two transforms in a row
 CChipVisitFluxMapping
 CChipVisitMagnitudeMapping
 CChipVisitPhotometryMappingA two-level photometric transform: one for the ccd and one for the visit
 CConstrainedAstrometryModelA multi-component model, fitting mappings for sensors and visits simultaneously
 CConstrainedFluxModel
 CConstrainedMagnitudeModel
 CConstrainedPhotometryModelPhotometry model with constraints, \(M(x,y) = M_CCD(x,y)*M_visit(u,v)\)
 CPrepPhotoCalibTo hold the return of prepPhotoCalib
 CFastFinderThis is an auxillary class for matching objects from starlists
 CIteratorIterator meant to traverse objects within some limiting distance
 CFatPointA Point with uncertainties
 CFittedStarFittedStars are objects whose position or flux is going to be fitted, and which come from the association of multiple MeasuredStars
 CFittedStarListA list of FittedStar s. Such a list is typically constructed by Associations
 CFitterBaseBase class for fitters
 CFluxTransformChebyshevNth-order 2d Chebyshev photometry transform, times the input flux
 CFluxTransformSpatiallyInvariantPhotometric offset independent of position, defined as (fluxMag0)^-1
 CFrameRectangle with sides parallel to axes
 CHisto2d
 CIdentityProjectionHandlerThe simplest implementation of ProjectionHandler
 CJointcalControl
 CMagnitudeTransformChebyshevNth-order 2d Chebyshev photometry transform, plus the input flux
 CMagnitudeTransformSpatiallyInvariantPhotometric offset independent of position, defined as -2.5 * log(flux / fluxMag0)
 CMatchConditionsParameters to be provided to combinatorial searches
 CMeasuredStarSources measured on 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 photometryTransform
 CPhotometryMappingBaseRelates transform(s) to their position in the fitting matrix and allows interaction with the transform(s)
 CPhotometryModel
 CPhotometryTransformA photometric transform, defined in terms of the input flux or magnitude
 CPhotometryTransformChebyshevNth-order 2d Chebyshev photometry transform
 CPhotometryTransformSpatiallyInvariantPhotometry offset independent of position
 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)
 CProperMotionProper motion data for a reference star or fitted star
 CRefStarObjects used as position/flux anchors (e.g
 CRefStarList
 CSegment
 CSegmentList
 CSegmentPair
 CSimpleAstrometryMappingClass for a simple mapping implementing a generic AstrometryTransform
 CSimpleAstrometryModelA model where there is one independent transform per CcdImage
 CSimpleFluxModel
 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
 CTanPixelToRaDecThe transformation that handles pixels to sideral transformations (Gnomonic, possibly with polynomial distortions)
 CTanRaDecToPixelThis one is the Tangent Plane (called gnomonic) projection (from celestial sphere to tangent plane)
 CTanSipPixelToRaDecImplements the (forward) SIP distorsion scheme
 CTripletList
 CUserTransformA run-time transform that allows users to define a AstrometryTransform with minimal coding (just the apply routine)
 NstdSTL namespace
 Chash< lsst::jointcal::CcdImageKey >Hash a ccdImage by its visit and ccd IDs