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LSSTDataManagementBasePackage
SimpleAstrometryModel.cc
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1 // -*- LSST-C++ -*-
2 /*
3  * This file is part of jointcal.
4  *
5  * Developed for the LSST Data Management System.
6  * This product includes software developed by the LSST Project
7  * (https://www.lsst.org).
8  * See the COPYRIGHT file at the top-level directory of this distribution
9  * for details of code ownership.
10  *
11  * This program is free software: you can redistribute it and/or modify
12  * it under the terms of the GNU General Public License as published by
13  * the Free Software Foundation, either version 3 of the License, or
14  * (at your option) any later version.
15  *
16  * This program is distributed in the hope that it will be useful,
17  * but WITHOUT ANY WARRANTY; without even the implied warranty of
18  * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
19  * GNU General Public License for more details.
20  *
21  * You should have received a copy of the GNU General Public License
22  * along with this program. If not, see <https://www.gnu.org/licenses/>.
23  */
24 
25 #include <memory>
26 #include <string>
27 
28 #include "astshim.h"
29 #include "lsst/log/Log.h"
33 #include "lsst/jointcal/CcdImage.h"
35 #include "lsst/pex/exceptions.h"
37 
38 namespace {
39 LOG_LOGGER _log = LOG_GET("jointcal.SimpleAstrometryModel");
40 }
41 
42 namespace lsst {
43 namespace jointcal {
44 
47  bool initFromWcs, unsigned nNotFit, unsigned order)
48  : _skyToTangentPlane(projectionHandler)
49 
50 {
51  unsigned count = 0;
52 
53  for (auto i = ccdImageList.cbegin(); i != ccdImageList.cend(); ++i, ++count) {
54  const CcdImage &im = **i;
55  if (count < nNotFit) {
58  id->setIndex(-1); // non sense, because it has no parameters
59  _myMap[im.getHashKey()] = std::move(id);
60  } else
61  // Given how AssignIndices works, only the SimplePolyMappings
62  // will actually be fitted, as nNotFit requests.
63  {
64  // first check that there are enough measurements for the requested polynomial order.
65  size_t nObj = im.getCatalogForFit().size();
66  if (nObj == 0) {
67  LOGLS_WARN(_log, "Empty catalog from image: " << im.getName());
68  continue;
69  }
71  if (pol.getOrder() > 0) // if not, it cannot be decreased
72  {
73  while (unsigned(pol.getNpar()) > 2 * nObj) {
74  LOGLS_WARN(_log, "Reducing polynomial order from "
75  << pol.getOrder() << ", due to too few sources (" << nObj
76  << " vs. " << pol.getNpar() << " parameters)");
77  pol.setOrder(pol.getOrder() - 1);
78  }
79  }
80  /* We have to center and normalize the coordinates so that
81  the fit matrix is not too ill-conditionned. Basically, x
82  and y in pixels are mapped to [-1,1]. When the
83  transformation of SimplePolyMapping transformation is
84  accessed, the combination of the normalization and the
85  fitted transformation is returned, so that the trick
86  remains hidden
87  */
88  const Frame &frame = im.getImageFrame();
90  if (initFromWcs) {
91  pol = AstrometryTransformPolynomial(im.getPixelToTangentPlane().get(), frame, order);
92  pol = pol * shiftAndNormalize.inverted();
93  }
94  _myMap[im.getHashKey()] =
96  }
97  }
98 }
99 
101  return findMapping(ccdImage);
102 }
103 
104 unsigned SimpleAstrometryModel::assignIndices(std::string const &whatToFit, unsigned firstIndex) {
105  if (whatToFit.find("Distortions") == std::string::npos) {
106  LOGLS_ERROR(_log, "AssignIndices was called and Distortions is *not* in whatToFit.");
107  return 0;
108  }
109  unsigned index = firstIndex;
110  for (auto i = _myMap.begin(); i != _myMap.end(); ++i) {
111  SimplePolyMapping *p = dynamic_cast<SimplePolyMapping *>(&*(i->second));
112  if (!p) continue; // it should be AstrometryTransformIdentity
113  p->setIndex(index);
114  index += p->getNpar();
115  }
116  return index;
117 }
118 
119 void SimpleAstrometryModel::offsetParams(Eigen::VectorXd const &delta) {
120  for (auto &i : _myMap) {
121  auto mapping = i.second.get();
122  mapping->offsetParams(delta.segment(mapping->getIndex(), mapping->getNpar()));
123  }
124 }
125 
127  for (auto &i : _myMap) i.second->freezeErrorTransform();
128 }
129 
131  int total = 0;
132  for (auto &i : _myMap) {
133  total += i.second->getNpar();
134  }
135  return total;
136 }
137 
139  return dynamic_cast<const SimplePolyMapping *>(findMapping(ccdImage))->getTransform();
140 }
141 
143  auto proj = std::dynamic_pointer_cast<const TanRaDecToPixel>(getSkyToTangentPlane(ccdImage));
144  jointcal::Point tangentPoint(proj->getTangentPoint());
145 
146  auto polyMap = getTransform(ccdImage).toAstMap(ccdImage.getImageFrame());
147  ast::Frame pixelFrame(2, "Domain=PIXELS");
148  ast::Frame iwcFrame(2, "Domain=IWC");
149 
150  // make a basic SkyWcs and extract the IWC portion
151  auto iwcToSkyWcs = afw::geom::makeSkyWcs(
152  afw::geom::Point2D(0, 0),
153  afw::geom::SpherePoint(tangentPoint.x, tangentPoint.y, afw::geom::degrees),
155  auto iwcToSkyMap = iwcToSkyWcs->getFrameDict()->getMapping("PIXELS", "SKY");
156  auto skyFrame = iwcToSkyWcs->getFrameDict()->getFrame("SKY");
157 
158  ast::FrameDict frameDict(pixelFrame, *polyMap, iwcFrame);
159  frameDict.addFrame("IWC", *iwcToSkyMap, *skyFrame);
160  return std::make_shared<afw::geom::SkyWcs>(frameDict);
161 }
162 
163 AstrometryMapping *SimpleAstrometryModel::findMapping(CcdImage const &ccdImage) const {
164  auto i = _myMap.find(ccdImage.getHashKey());
165  if (i == _myMap.end())
167  "SimpleAstrometryModel cannot find CcdImage " + ccdImage.getName());
168  return i->second.get();
169 }
170 
171 } // namespace jointcal
172 } // namespace lsst
#define LOGLS_WARN(logger, message)
Log a warn-level message using an iostream-based interface.
Definition: Log.h:633
AstrometryTransform const & getTransform(CcdImage const &ccdImage) const
Access to mappings.
#define LOG_LOGGER
Definition: Log.h:688
void setOrder(const unsigned order)
Sets the polynomial order (the highest sum of exponents of the largest monomial). ...
implements the linear transformations (6 real coefficients).
SimpleAstrometryModel(CcdImageList const &ccdImageList, const std::shared_ptr< ProjectionHandler const > projectionHandler, bool initFromWCS, unsigned nNotFit=0, unsigned order=3)
Sky2TP is just a name, it can be anything.
A point in a plane.
Definition: Point.h:36
const AstrometryMapping * getMapping(CcdImage const &) const override
Mapping associated to a given CcdImage.
void offsetParams(Eigen::VectorXd const &delta) override
Offset the parameters by the provided amounts (by -delta).
std::shared_ptr< AstrometryTransform > const getPixelToTangentPlane() const
Definition: CcdImage.h:140
std::string getName() const
Return the _name that identifies this ccdImage.
Definition: CcdImage.h:79
Mapping implementation for a polynomial transformation.
unsigned getNpar() const
Number of parameters in total.
const std::shared_ptr< AstrometryTransform const > getSkyToTangentPlane(CcdImage const &ccdImage) const override
the mapping of sky coordinates (i.e.
T cend(T... args)
table::Key< int > id
Definition: Detector.cc:163
STL class.
LSST DM logging module built on log4cxx.
std::shared_ptr< afw::geom::SkyWcs > makeSkyWcs(CcdImage const &ccdImage) const override
Make a SkyWcs that contains this model.
rectangle with sides parallel to axes.
Definition: Frame.h:38
AstrometryTransformLinear normalizeCoordinatesTransform(const Frame &frame)
Returns the transformation that maps the input frame along both axes to [-1,1].
AngleUnit constexpr degrees
constant with units of degrees
Definition: Angle.h:109
A base class for image defects.
void addFrame(int iframe, Mapping const &map, Frame const &frame) override
Add a new Frame and an associated Mapping to this FrameSet so as to define a new coordinate system...
Definition: FrameDict.cc:32
Frame is used to represent a coordinate system.
Definition: Frame.h:157
int getTotalParameters() const override
Return the total number of parameters in this model.
This one is the Tangent Plane (called gnomonic) projection (from celestial sphere to tangent plane) ...
T dynamic_pointer_cast(T... args)
T move(T... args)
T count(T... args)
int getNpar() const override
total number of parameters
A do-nothing transformation. It anyway has dummy routines to mimick a AstrometryTransform.
T find(T... args)
T size(T... args)
#define LSST_EXCEPT(type,...)
Create an exception with a given type.
Definition: Exception.h:48
STL class.
AstrometryTransformLinear inverted() const
returns the inverse: T1 = T2.inverted();
a virtual (interface) class for geometric transformations.
Point in an unspecified spherical coordinate system.
Definition: SpherePoint.h:57
T cbegin(T... args)
MeasuredStarList const & getCatalogForFit() const
Gets the catalog to be used for fitting, which may have been cleaned-up.
Definition: CcdImage.h:94
std::shared_ptr< SkyWcs > makeSkyWcs(daf::base::PropertySet &metadata, bool strip=false)
Construct a SkyWcs from FITS keywords.
Definition: SkyWcs.cc:476
Eigen::Matrix2d makeCdMatrix(lsst::geom::Angle const &scale, lsst::geom::Angle const &orientation=0 *lsst::geom::degrees, bool flipX=false)
Make a WCS CD matrix.
Definition: SkyWcs.cc:139
Reports invalid arguments.
Definition: Runtime.h:66
virtual class needed in the abstraction of the distortion model
CcdImageKey getHashKey() const
Definition: CcdImage.h:152
Handler of an actual image from a single CCD.
Definition: CcdImage.h:64
#define LOG_GET(logger)
Returns a Log object associated with logger.
Definition: Log.h:75
virtual std::shared_ptr< ast::Mapping > toAstMap(jointcal::Frame const &domain) const
Create an equivalent AST mapping for this transformation, including an analytic inverse if possible...
A FrameSet whose frames can be referenced by domain name.
Definition: FrameDict.h:67
unsigned assignIndices(std::string const &whatToFit, unsigned firstIndex) override
Positions the various parameter sets into the parameter vector, starting at firstIndex.
#define LOGLS_ERROR(logger, message)
Log a error-level message using an iostream-based interface.
Definition: Log.h:653
unsigned getOrder() const
Returns the polynomial order.
Frame const & getImageFrame() const
Frame in pixels.
Definition: CcdImage.h:191