this is the model used to fit independent CCDs, meaning that there is no instrument model. More...
#include <simplepolymodel.h>
Public Member Functions | |
| SimplePolyModel (const CcdImageList &L, const ProjectionHandler *ProjH, bool InitFromWCS, unsigned NNotFit=0) | |
| Sky2TP is just a name, it can be anything. | |
| const Mapping * | GetMapping (const CcdImage &) const |
| Mapping associated to a given CcdImage. | |
| unsigned | AssignIndices (unsigned FirstIndex, std::string &WhatToFit) |
| Positions the various parameter sets into the parameter vector, starting at FirstIndex. | |
| void | OffsetParams (const Eigen::VectorXd &Delta) |
| Offset the parameters by the provided amounts. More... | |
| const Gtransfo * | Sky2TP (const Mapping *M, const CcdImage &C) const |
this is the model used to fit independent CCDs, meaning that there is no instrument model.
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virtual |
Offset the parameters by the provided amounts.
The shifts are applied according to the indices given in AssignIndices.
Implements DistortionModel.
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inlinevirtual |
the mapping of sky coordinates (i.e. the coordinate system in which fitted stars are reported) onto the Tangent plane (into which the pixel coordinates are transformed)
Implements DistortionModel.
1.8.6