LSST Applications  21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
LSST Data Management Base Package
Public Member Functions | Protected Attributes | List of all members
lsst::jointcal::BaseTanWcs Class Referenceabstract

#include <AstrometryTransform.h>

Inheritance diagram for lsst::jointcal::BaseTanWcs:
lsst::jointcal::AstrometryTransform lsst::jointcal::TanPixelToRaDec lsst::jointcal::TanSipPixelToRaDec

Public Member Functions

 BaseTanWcs (AstrometryTransformLinear const &pixToTan, Point const &tangentPoint, const AstrometryTransformPolynomial *corrections=nullptr)
 
 BaseTanWcs (const BaseTanWcs &original)
 
void operator= (const BaseTanWcs &original)
 
void apply (const double xIn, const double yIn, double &xOut, double &yOut) const
 Transform pixels to ICRS RA, Dec in degrees. More...
 
Point getTangentPoint () const
 Get the sky origin (CRVAL in FITS WCS terminology) in degrees. More...
 
AstrometryTransformLinear getLinPart () const
 The Linear part (corresponding to CD's and CRPIX's) More...
 
const AstrometryTransformPolynomialgetCorr () const
 Get a non-owning pointer to the correction transform polynomial. More...
 
void setCorrections (std::unique_ptr< AstrometryTransformPolynomial > corrections)
 Assign the correction polynomial (what it means is left to derived classes) More...
 
Point getCrPix () const
 Get the pixel origin of the WCS (CRPIX in FITS WCS terminology, but zero-based) More...
 
virtual AstrometryTransformPolynomial getPixelToTangentPlane () const =0
 Get a transform from pixels to tangent plane (degrees) This is a linear transform plus the effects of the correction. More...
 
virtual void pixToTangentPlane (double xPixel, double yPixel, double &xTangentPlane, double &yTangentPlane) const =0
 Transform from pixels to tangent plane (degrees) More...
 
 ~BaseTanWcs ()
 
virtual void apply (const double xIn, const double yIn, double &xOut, double &yOut) const=0
 
void apply (Point const &in, Point &out) const
 applies the tranfo to in and writes into out. Is indeed virtual. More...
 
Point apply (Point const &in) const
 All these apply(..) shadow the virtual one in derived classes, unless one writes "using AstrometryTransform::apply". More...
 
Frame apply (Frame const &inputframe, bool inscribed) const
 Transform a bounding box, taking either the inscribed or circumscribed box. More...
 
void apply (Point const &in, Point &out) const
 applies the tranfo to in and writes into out. Is indeed virtual. More...
 
Point apply (Point const &in) const
 All these apply(..) shadow the virtual one in derived classes, unless one writes "using AstrometryTransform::apply". More...
 
Frame apply (Frame const &inputframe, bool inscribed) const
 Transform a bounding box, taking either the inscribed or circumscribed box. More...
 
virtual void print (std::ostream &out) const =0
 prints the transform coefficients to stream. More...
 
std::string __str__ ()
 
virtual double fit (StarMatchList const &starMatchList)=0
 fits a transform to a std::list of Point pairs (p1,p2, the Point fields in StarMatch). More...
 
void transformStar (FatPoint &in) const
 
virtual double getJacobian (Point const &point) const
 returns the local jacobian. More...
 
virtual double getJacobian (const double x, const double y) const
 returns the local jacobian. More...
 
virtual std::unique_ptr< AstrometryTransformclone () const =0
 returns a copy (allocated by new) of the transformation. More...
 
virtual std::unique_ptr< AstrometryTransformcomposeAndReduce (AstrometryTransform const &right) const
 Return a reduced composition of newTransform = this(right()), or nullptr if it cannot be reduced. More...
 
virtual void computeDerivative (Point const &where, AstrometryTransformLinear &derivative, const double step=0.01) const
 Computes the local Derivative of a transform, w.r.t. More...
 
virtual AstrometryTransformLinear linearApproximation (Point const &where, const double step=0.01) const
 linear (local) approximation. More...
 
virtual void transformPosAndErrors (const FatPoint &in, FatPoint &out) const
 
virtual void transformErrors (Point const &where, const double *vIn, double *vOut) const
 transform errors (represented as double[3] in order V(xx),V(yy),Cov(xy)) More...
 
virtual std::unique_ptr< AstrometryTransforminverseTransform (const double precision, const Frame &region) const
 returns an inverse transform. Numerical if not overloaded. More...
 
void getParams (double *params) const
 params should be at least Npar() long More...
 
void offsetParams (Eigen::VectorXd const &delta)
 
virtual double paramRef (Eigen::Index const i) const
 
virtual double & paramRef (Eigen::Index const i)
 
virtual void paramDerivatives (Point const &where, double *dx, double *dy) const
 Derivative w.r.t parameters. More...
 
virtual std::unique_ptr< AstrometryTransformroughInverse (const Frame &region) const
 Rough inverse. More...
 
virtual std::size_t getNpar () const
 returns the number of parameters (to compute chi2's) More...
 
virtual std::shared_ptr< ast::MappingtoAstMap (jointcal::Frame const &domain) const
 Create an equivalent AST mapping for this transformation, including an analytic inverse if possible. More...
 
void write (const std::string &fileName) const
 
virtual void write (std::ostream &stream) const
 

Protected Attributes

AstrometryTransformLinear linPixelToTan
 
std::unique_ptr< AstrometryTransformPolynomialcorr
 
double ra0
 
double dec0
 
double cos0
 
double sin0
 

Detailed Description

Definition at line 574 of file AstrometryTransform.h.

Constructor & Destructor Documentation

◆ BaseTanWcs() [1/2]

lsst::jointcal::BaseTanWcs::BaseTanWcs ( AstrometryTransformLinear const &  pixToTan,
Point const &  tangentPoint,
const AstrometryTransformPolynomial corrections = nullptr 
)

Definition at line 1395 of file AstrometryTransform.cc.

1396  {
1397  // the angles returned by linPixelToTan should be in degrees.
1398  linPixelToTan = pixToTan;
1399  ra0 = deg2rad(tangentPoint.x);
1400  dec0 = deg2rad(tangentPoint.y);
1401  cos0 = std::cos(dec0);
1402  sin0 = std::sin(dec0);
1403  corr = nullptr;
1404  if (corrections) corr.reset(new AstrometryTransformPolynomial(*corrections));
1405 }
std::unique_ptr< AstrometryTransformPolynomial > corr
AstrometryTransformLinear linPixelToTan
T cos(T... args)
T sin(T... args)

◆ BaseTanWcs() [2/2]

lsst::jointcal::BaseTanWcs::BaseTanWcs ( const BaseTanWcs original)

Definition at line 1411 of file AstrometryTransform.cc.

1411  : AstrometryTransform() {
1412  corr = nullptr;
1413  *this = original;
1414 }

◆ ~BaseTanWcs()

lsst::jointcal::BaseTanWcs::~BaseTanWcs ( )

Definition at line 1472 of file AstrometryTransform.cc.

1472 {}

Member Function Documentation

◆ __str__()

std::string lsst::jointcal::AstrometryTransform::__str__ ( )
inlineinherited

Definition at line 94 of file AstrometryTransform.h.

94  {
96  print(s);
97  return s.str();
98  }
virtual void print(std::ostream &out) const =0
prints the transform coefficients to stream.
T str(T... args)

◆ apply() [1/8]

void lsst::jointcal::BaseTanWcs::apply ( const double  xIn,
const double  yIn,
double &  xOut,
double &  yOut 
) const
virtual

Transform pixels to ICRS RA, Dec in degrees.

Implements lsst::jointcal::AstrometryTransform.

Definition at line 1426 of file AstrometryTransform.cc.

1426  {
1427  double l, m; // radians in the tangent plane
1428  pixToTangentPlane(xIn, yIn, l, m); // l, m in degrees.
1429  l = deg2rad(l);
1430  m = deg2rad(m); // now in radians
1431  // Code inspired from worldpos.c in wcssubs (ancestor of the wcslib)
1432  /* At variance with wcslib, it collapses the projection to a plane
1433  and expression of sidereal cooordinates into a single set of
1434  operations. */
1435  double dect = cos0 - m * sin0;
1436  if (dect == 0) {
1437  LOGL_WARN(_log, "No sidereal coordinates at pole!");
1438  xOut = 0;
1439  yOut = 0;
1440  return;
1441  }
1442  double rat = ra0 + atan2(l, dect);
1443  dect = atan(std::cos(rat - ra0) * (m * cos0 + sin0) / dect);
1444  if (rat - ra0 > M_PI) rat -= (2. * M_PI);
1445  if (rat - ra0 < -M_PI) rat += (2. * M_PI);
1446  if (rat < 0.0) rat += (2. * M_PI);
1447  // convert to degree
1448  xOut = rad2deg(rat);
1449  yOut = rad2deg(dect);
1450 }
#define M_PI
Definition: ListMatch.cc:31
#define LOGL_WARN(logger, message...)
Log a warn-level message using a varargs/printf style interface.
Definition: Log.h:547
int m
Definition: SpanSet.cc:48
T atan2(T... args)
T atan(T... args)
virtual void pixToTangentPlane(double xPixel, double yPixel, double &xTangentPlane, double &yTangentPlane) const =0
Transform from pixels to tangent plane (degrees)

◆ apply() [2/8]

virtual void lsst::jointcal::AstrometryTransform::apply

◆ apply() [3/8]

Frame lsst::jointcal::AstrometryTransform::apply ( Frame const &  inputframe,
bool  inscribed 
) const
inherited

Transform a bounding box, taking either the inscribed or circumscribed box.

Parameters
[in]inputframeThe frame to be transformed.
[in]inscribedReturn the inscribed (true) or circumscribed (false) box.
Returns
The transformed frame.

Definition at line 76 of file AstrometryTransform.cc.

76  {
77  // 2 opposite corners
78  double xtmin1, xtmax1, ytmin1, ytmax1;
79  apply(inputframe.xMin, inputframe.yMin, xtmin1, ytmin1);
80  apply(inputframe.xMax, inputframe.yMax, xtmax1, ytmax1);
81  Frame fr1(std::min(xtmin1, xtmax1), std::min(ytmin1, ytmax1), std::max(xtmin1, xtmax1),
82  std::max(ytmin1, ytmax1));
83  // 2 other corners
84  double xtmin2, xtmax2, ytmin2, ytmax2;
85  apply(inputframe.xMin, inputframe.yMax, xtmin2, ytmax2);
86  apply(inputframe.xMax, inputframe.yMin, xtmax2, ytmin2);
87  Frame fr2(std::min(xtmin2, xtmax2), std::min(ytmin2, ytmax2), std::max(xtmin2, xtmax2),
88  std::max(ytmin2, ytmax2));
89 
90  if (inscribed) return fr1 * fr2;
91  return fr1 + fr2;
92 }
virtual void apply(const double xIn, const double yIn, double &xOut, double &yOut) const =0
T max(T... args)
T min(T... args)

◆ apply() [4/8]

Frame lsst::jointcal::AstrometryTransform::apply

Transform a bounding box, taking either the inscribed or circumscribed box.

Parameters
[in]inputframeThe frame to be transformed.
[in]inscribedReturn the inscribed (true) or circumscribed (false) box.
Returns
The transformed frame.

Definition at line 89 of file AstrometryTransform.cc.

76  {
77  // 2 opposite corners
78  double xtmin1, xtmax1, ytmin1, ytmax1;
79  apply(inputframe.xMin, inputframe.yMin, xtmin1, ytmin1);
80  apply(inputframe.xMax, inputframe.yMax, xtmax1, ytmax1);
81  Frame fr1(std::min(xtmin1, xtmax1), std::min(ytmin1, ytmax1), std::max(xtmin1, xtmax1),
82  std::max(ytmin1, ytmax1));
83  // 2 other corners
84  double xtmin2, xtmax2, ytmin2, ytmax2;
85  apply(inputframe.xMin, inputframe.yMax, xtmin2, ytmax2);
86  apply(inputframe.xMax, inputframe.yMin, xtmax2, ytmin2);
87  Frame fr2(std::min(xtmin2, xtmax2), std::min(ytmin2, ytmax2), std::max(xtmin2, xtmax2),
88  std::max(ytmin2, ytmax2));
89 
90  if (inscribed) return fr1 * fr2;
91  return fr1 + fr2;
92 }
virtual void apply(const double xIn, const double yIn, double &xOut, double &yOut) const=0

◆ apply() [5/8]

Point lsst::jointcal::AstrometryTransform::apply ( Point const &  in) const
inlineinherited

All these apply(..) shadow the virtual one in derived classes, unless one writes "using AstrometryTransform::apply".

Definition at line 75 of file AstrometryTransform.h.

75  {
76  double xout, yout;
77  apply(in.x, in.y, xout, yout);
78  return Point(xout, yout);
79  }

◆ apply() [6/8]

Point lsst::jointcal::AstrometryTransform::apply
inline

All these apply(..) shadow the virtual one in derived classes, unless one writes "using AstrometryTransform::apply".

Definition at line 75 of file AstrometryTransform.h.

75  {
76  double xout, yout;
77  apply(in.x, in.y, xout, yout);
78  return Point(xout, yout);
79  }

◆ apply() [7/8]

void lsst::jointcal::AstrometryTransform::apply ( Point const &  in,
Point out 
) const
inlineinherited

applies the tranfo to in and writes into out. Is indeed virtual.

Definition at line 71 of file AstrometryTransform.h.

71 { apply(in.x, in.y, out.x, out.y); }

◆ apply() [8/8]

void lsst::jointcal::AstrometryTransform::apply
inline

applies the tranfo to in and writes into out. Is indeed virtual.

Definition at line 71 of file AstrometryTransform.h.

71 { apply(in.x, in.y, out.x, out.y); }

◆ clone()

virtual std::unique_ptr<AstrometryTransform> lsst::jointcal::AstrometryTransform::clone ( ) const
pure virtualinherited

◆ composeAndReduce()

std::unique_ptr< AstrometryTransform > lsst::jointcal::AstrometryTransform::composeAndReduce ( AstrometryTransform const &  right) const
virtualinherited

Return a reduced composition of newTransform = this(right()), or nullptr if it cannot be reduced.

"Reduced" in this context means that they are capable of being merged into a single transform, for example, for two polynomials:

\[ f(x) = 1 + x^2, g(x) = -1 + 3x \]

we would have h = f.composeAndReduce(g) == 2 - 6x + 9x^2.

To be overloaded by derived classes if they can properly reduce the composition.

Parameters
rightThe transform to apply first.
Returns
The new reduced and composed AstrometryTransform, or nullptr if no such reduction is possible.

Reimplemented in lsst::jointcal::AstrometryTransformIdentity.

Definition at line 94 of file AstrometryTransform.cc.

95  { // by default no way to compose
97 }

◆ computeDerivative()

void lsst::jointcal::AstrometryTransform::computeDerivative ( Point const &  where,
AstrometryTransformLinear derivative,
const double  step = 0.01 
) const
virtualinherited

Computes the local Derivative of a transform, w.r.t.

the Derivative is represented by a AstrometryTransformLinear, in which (hopefully), the offset terms are zero.

position.

Step is used for numerical derivation.

Derivative should transform a vector of offsets into a vector of offsets.

Reimplemented in lsst::jointcal::AstrometryTransformLinear, lsst::jointcal::AstrometryTransformPolynomial, and lsst::jointcal::AstrometryTransformIdentity.

Definition at line 118 of file AstrometryTransform.cc.

119  {
120  double x = where.x;
121  double y = where.y;
122  double xp0, yp0;
123  apply(x, y, xp0, yp0);
124 
125  double xp, yp;
126  apply(x + step, y, xp, yp);
127  derivative.a11() = (xp - xp0) / step;
128  derivative.a21() = (yp - yp0) / step;
129  apply(x, y + step, xp, yp);
130  derivative.a12() = (xp - xp0) / step;
131  derivative.a22() = (yp - yp0) / step;
132  derivative.dx() = 0;
133  derivative.dy() = 0;
134 }
int const step
double x
int y
Definition: SpanSet.cc:48

◆ fit()

virtual double lsst::jointcal::AstrometryTransform::fit ( StarMatchList const &  starMatchList)
pure virtualinherited

◆ getCorr()

const AstrometryTransformPolynomial* lsst::jointcal::BaseTanWcs::getCorr ( ) const
inline

Get a non-owning pointer to the correction transform polynomial.

Definition at line 595 of file AstrometryTransform.h.

595 { return corr.get(); }

◆ getCrPix()

Point lsst::jointcal::BaseTanWcs::getCrPix ( ) const

Get the pixel origin of the WCS (CRPIX in FITS WCS terminology, but zero-based)

Definition at line 1460 of file AstrometryTransform.cc.

1460  {
1461  /* CRPIX's are defined by:
1462  ( CD1_1 CD1_2 ) (x - crpix1)
1463  transformed = ( ) * ( )
1464  ( CD2_1 CD2_2 ) (y - crpix2)
1465 
1466  so that CrPix is the point which transforms to (0,0)
1467  */
1468  const AstrometryTransformLinear inverse = linPixelToTan.inverted();
1469  return Point(inverse.Dx(), inverse.Dy());
1470 }
AstrometryTransformLinear inverted() const
returns the inverse: T1 = T2.inverted();

◆ getJacobian() [1/2]

double lsst::jointcal::AstrometryTransform::getJacobian ( const double  x,
const double  y 
) const
virtualinherited

returns the local jacobian.

Definition at line 99 of file AstrometryTransform.cc.

99  {
100  double x2, y2;
101  double eps = x * 0.01;
102  if (eps == 0) eps = 0.01;
103  apply(x, y, x2, y2);
104  double dxdx, dydx;
105  apply(x + eps, y, dxdx, dydx);
106  dxdx -= x2;
107  dydx -= y2;
108  double dxdy, dydy;
109  apply(x, y + eps, dxdy, dydy);
110  dxdy -= x2;
111  dydy -= y2;
112  return ((dxdx * dydy - dxdy * dydx) / (eps * eps));
113 }

◆ getJacobian() [2/2]

virtual double lsst::jointcal::AstrometryTransform::getJacobian ( Point const &  point) const
inlinevirtualinherited

returns the local jacobian.

Definition at line 110 of file AstrometryTransform.h.

110 { return getJacobian(point.x, point.y); }
virtual double getJacobian(Point const &point) const
returns the local jacobian.

◆ getLinPart()

AstrometryTransformLinear lsst::jointcal::BaseTanWcs::getLinPart ( ) const

The Linear part (corresponding to CD's and CRPIX's)

Definition at line 1454 of file AstrometryTransform.cc.

1454 { return linPixelToTan; }

◆ getNpar()

virtual std::size_t lsst::jointcal::AstrometryTransform::getNpar ( ) const
inlinevirtualinherited

◆ getParams()

void lsst::jointcal::AstrometryTransform::getParams ( double *  params) const
inherited

params should be at least Npar() long

Definition at line 216 of file AstrometryTransform.cc.

216  {
217  std::size_t npar = getNpar();
218  for (std::size_t i = 0; i < npar; ++i) params[i] = paramRef(i);
219 }
virtual double paramRef(Eigen::Index const i) const
virtual std::size_t getNpar() const
returns the number of parameters (to compute chi2's)

◆ getPixelToTangentPlane()

virtual AstrometryTransformPolynomial lsst::jointcal::BaseTanWcs::getPixelToTangentPlane ( ) const
pure virtual

Get a transform from pixels to tangent plane (degrees) This is a linear transform plus the effects of the correction.

Implemented in lsst::jointcal::TanSipPixelToRaDec, and lsst::jointcal::TanPixelToRaDec.

◆ getTangentPoint()

Point lsst::jointcal::BaseTanWcs::getTangentPoint ( ) const

Get the sky origin (CRVAL in FITS WCS terminology) in degrees.

Definition at line 1452 of file AstrometryTransform.cc.

1452 { return Point(rad2deg(ra0), rad2deg(dec0)); }

◆ inverseTransform()

std::unique_ptr< AstrometryTransform > lsst::jointcal::AstrometryTransform::inverseTransform ( const double  precision,
const Frame region 
) const
virtualinherited

returns an inverse transform. Numerical if not overloaded.

precision and region refer to the "input" side of this, and hence to the output side of the returned AstrometryTransform.

Reimplemented in lsst::jointcal::AstrometryTransformInverse, lsst::jointcal::AstrometryTransformLinear, lsst::jointcal::TanRaDecToPixel, lsst::jointcal::TanSipPixelToRaDec, and lsst::jointcal::TanPixelToRaDec.

Definition at line 303 of file AstrometryTransform.cc.

304  {
305  return std::unique_ptr<AstrometryTransform>(new AstrometryTransformInverse(this, precision, region));
306 }

◆ linearApproximation()

AstrometryTransformLinear lsst::jointcal::AstrometryTransform::linearApproximation ( Point const &  where,
const double  step = 0.01 
) const
virtualinherited

linear (local) approximation.

Reimplemented in lsst::jointcal::AstrometryTransformLinear, and lsst::jointcal::AstrometryTransformIdentity.

Definition at line 136 of file AstrometryTransform.cc.

137  {
138  Point outwhere = apply(where);
139  AstrometryTransformLinear der;
140  computeDerivative(where, der, step);
141  return AstrometryTransformLinearShift(outwhere.x, outwhere.y) * der *
142  AstrometryTransformLinearShift(-where.x, -where.y);
143 }
virtual void computeDerivative(Point const &where, AstrometryTransformLinear &derivative, const double step=0.01) const
Computes the local Derivative of a transform, w.r.t.

◆ offsetParams()

void lsst::jointcal::AstrometryTransform::offsetParams ( Eigen::VectorXd const &  delta)
inherited

Definition at line 221 of file AstrometryTransform.cc.

221  {
222  std::size_t npar = getNpar();
223  for (std::size_t i = 0; i < npar; ++i) paramRef(i) += delta[i];
224 }

◆ operator=()

void lsst::jointcal::BaseTanWcs::operator= ( const BaseTanWcs original)

Definition at line 1416 of file AstrometryTransform.cc.

1416  {
1417  linPixelToTan = original.linPixelToTan;
1418  ra0 = original.ra0;
1419  dec0 = original.dec0;
1420  cos0 = std::cos(dec0);
1421  sin0 = std::sin(dec0);
1422  corr = nullptr;
1423  if (original.corr) corr.reset(new AstrometryTransformPolynomial(*original.corr));
1424 }

◆ paramDerivatives()

void lsst::jointcal::AstrometryTransform::paramDerivatives ( Point const &  where,
double *  dx,
double *  dy 
) const
virtualinherited

Derivative w.r.t parameters.

Derivatives should be al least 2*NPar long. first Npar, for x, last Npar for y.

Reimplemented in lsst::jointcal::AstrometryTransformPolynomial.

Definition at line 236 of file AstrometryTransform.cc.

236  {
237  throw LSST_EXCEPT(pex::exceptions::InvalidParameterError,
238  "AstrometryTransform::paramDerivatives() should never be called ");
239 }
#define LSST_EXCEPT(type,...)
Create an exception with a given type.
Definition: Exception.h:48

◆ paramRef() [1/2]

double & lsst::jointcal::AstrometryTransform::paramRef ( Eigen::Index const  i)
virtualinherited

Reimplemented in lsst::jointcal::AstrometryTransformPolynomial.

Definition at line 231 of file AstrometryTransform.cc.

231  {
232  throw LSST_EXCEPT(pex::exceptions::InvalidParameterError,
233  "AstrometryTransform::paramRef should never be called ");
234 }

◆ paramRef() [2/2]

double lsst::jointcal::AstrometryTransform::paramRef ( Eigen::Index const  i) const
virtualinherited

Reimplemented in lsst::jointcal::AstrometryTransformPolynomial.

Definition at line 226 of file AstrometryTransform.cc.

226  {
227  throw LSST_EXCEPT(pex::exceptions::InvalidParameterError,
228  std::string("AstrometryTransform::paramRef should never be called "));
229 }

◆ pixToTangentPlane()

virtual void lsst::jointcal::BaseTanWcs::pixToTangentPlane ( double  xPixel,
double  yPixel,
double &  xTangentPlane,
double &  yTangentPlane 
) const
pure virtual

Transform from pixels to tangent plane (degrees)

Implemented in lsst::jointcal::TanSipPixelToRaDec, and lsst::jointcal::TanPixelToRaDec.

◆ print()

virtual void lsst::jointcal::AstrometryTransform::print ( std::ostream out) const
pure virtualinherited

◆ roughInverse()

std::unique_ptr< AstrometryTransform > lsst::jointcal::AstrometryTransform::roughInverse ( const Frame region) const
virtualinherited

Rough inverse.

Stored by the numerical inverter to guess starting point for the trials. Just here to enable overloading.

Reimplemented in lsst::jointcal::TanRaDecToPixel, lsst::jointcal::TanPixelToRaDec, and lsst::jointcal::AstrometryTransformInverse.

Definition at line 195 of file AstrometryTransform.cc.

195  {
196  // "in" and "out" refer to the inverse direction.
197  Point centerOut = region.getCenter();
198  Point centerIn = apply(centerOut);
199  AstrometryTransformLinear der;
200  computeDerivative(centerOut, der, std::sqrt(region.getArea()) / 5.);
201  der = der.inverted();
202  der = AstrometryTransformLinearShift(centerOut.x, centerOut.y) * der *
203  AstrometryTransformLinearShift(-centerIn.x, -centerIn.y);
204  return std::unique_ptr<AstrometryTransform>(new AstrometryTransformLinear(der));
205 }
T sqrt(T... args)

◆ setCorrections()

void lsst::jointcal::BaseTanWcs::setCorrections ( std::unique_ptr< AstrometryTransformPolynomial corrections)

Assign the correction polynomial (what it means is left to derived classes)

Definition at line 1456 of file AstrometryTransform.cc.

1456  {
1457  corr = std::move(corrections);
1458 }
T move(T... args)

◆ toAstMap()

virtual std::shared_ptr<ast::Mapping> lsst::jointcal::AstrometryTransform::toAstMap ( jointcal::Frame const &  domain) const
inlinevirtualinherited

Create an equivalent AST mapping for this transformation, including an analytic inverse if possible.

Parameters
domainThe domain of the transform, to help find an inverse.
Returns
An AST Mapping that represents this transformation.

Reimplemented in lsst::jointcal::AstrometryTransformPolynomial, and lsst::jointcal::AstrometryTransformIdentity.

Definition at line 189 of file AstrometryTransform.h.

189  {
190  throw std::logic_error("toAstMap is not implemented for this class.");
191  }

◆ transformErrors()

void lsst::jointcal::AstrometryTransform::transformErrors ( Point const &  where,
const double *  vIn,
double *  vOut 
) const
virtualinherited

transform errors (represented as double[3] in order V(xx),V(yy),Cov(xy))

Definition at line 162 of file AstrometryTransform.cc.

162  {
163  AstrometryTransformLinear der;
164  computeDerivative(where, der, 0.01);
165  double a11 = der.A11();
166  double a22 = der.A22();
167  double a21 = der.A21();
168  double a12 = der.A12();
169 
170  /* (a11 a12) (vxx vxy)
171  M = ( ) and V = ( )
172  (a21 a22) (xvy vyy)
173 
174  Vxx = Vin[0], vyy = Vin[1], Vxy = Vin[2];
175  we want to compute M*V*tp(M)
176  A lin alg light package would be perfect...
177  */
178  int xx = 0;
179  int yy = 1;
180  int xy = 2;
181  // M*V :
182 
183  double b11 = a11 * vIn[xx] + a12 * vIn[xy];
184  double b22 = a21 * vIn[xy] + a22 * vIn[yy];
185  double b12 = a11 * vIn[xy] + a12 * vIn[yy];
186  double b21 = a21 * vIn[xx] + a22 * vIn[xy];
187 
188  // (M*V) * tp(M)
189 
190  vOut[xx] = b11 * a11 + b12 * a12;
191  vOut[xy] = b11 * a21 + b12 * a22;
192  vOut[yy] = b21 * a21 + b22 * a22;
193 }

◆ transformPosAndErrors()

void lsst::jointcal::AstrometryTransform::transformPosAndErrors ( const FatPoint in,
FatPoint out 
) const
virtualinherited

Reimplemented in lsst::jointcal::AstrometryTransformPolynomial, and lsst::jointcal::TanRaDecToPixel.

Definition at line 145 of file AstrometryTransform.cc.

145  {
146  FatPoint res; // in case in and out are the same address...
147  res = apply(in);
148  AstrometryTransformLinear der;
149  // could save a call here, since Derivative needs the transform of where that we already have
150  // 0.01 may not be a very good idea in all cases. May be we should provide a way of altering that.
151  computeDerivative(in, der, 0.01);
152  double a11 = der.A11();
153  double a22 = der.A22();
154  double a21 = der.A21();
155  double a12 = der.A12();
156  res.vx = a11 * (a11 * in.vx + 2 * a12 * in.vxy) + a12 * a12 * in.vy;
157  res.vy = a21 * a21 * in.vx + a22 * a22 * in.vy + 2. * a21 * a22 * in.vxy;
158  res.vxy = a21 * a11 * in.vx + a22 * a12 * in.vy + (a21 * a12 + a11 * a22) * in.vxy;
159  out = res;
160 }

◆ transformStar()

void lsst::jointcal::AstrometryTransform::transformStar ( FatPoint in) const
inlineinherited

Definition at line 107 of file AstrometryTransform.h.

107 { transformPosAndErrors(in, in); }
virtual void transformPosAndErrors(const FatPoint &in, FatPoint &out) const

◆ write() [1/2]

void lsst::jointcal::AstrometryTransform::write ( const std::string fileName) const
inherited

Definition at line 246 of file AstrometryTransform.cc.

246  {
247  ofstream s(fileName.c_str());
248  write(s);
249  bool ok = !s.fail();
250  s.close();
251  if (!ok)
252  throw LSST_EXCEPT(pex::exceptions::InvalidParameterError,
253  "AstrometryTransform::write, something went wrong for file " + fileName);
254 }
T c_str(T... args)
void write(const std::string &fileName) const

◆ write() [2/2]

void lsst::jointcal::AstrometryTransform::write ( std::ostream stream) const
virtualinherited

Reimplemented in lsst::jointcal::AstrometryTransformPolynomial, and lsst::jointcal::AstrometryTransformIdentity.

Definition at line 256 of file AstrometryTransform.cc.

256  {
257  throw LSST_EXCEPT(
258  pex::exceptions::InvalidParameterError,
259  "AstrometryTransform::write(ostream), should never be called. MEans that it is missing in some "
260  "derived class ");
261 }

Member Data Documentation

◆ corr

std::unique_ptr<AstrometryTransformPolynomial> lsst::jointcal::BaseTanWcs::corr
protected

Definition at line 616 of file AstrometryTransform.h.

◆ cos0

double lsst::jointcal::BaseTanWcs::cos0
protected

Definition at line 618 of file AstrometryTransform.h.

◆ dec0

double lsst::jointcal::BaseTanWcs::dec0
protected

Definition at line 617 of file AstrometryTransform.h.

◆ linPixelToTan

AstrometryTransformLinear lsst::jointcal::BaseTanWcs::linPixelToTan
protected

Definition at line 614 of file AstrometryTransform.h.

◆ ra0

double lsst::jointcal::BaseTanWcs::ra0
protected

Definition at line 617 of file AstrometryTransform.h.

◆ sin0

double lsst::jointcal::BaseTanWcs::sin0
protected

Definition at line 618 of file AstrometryTransform.h.


The documentation for this class was generated from the following files: