22 __all__ = [
"FitTanSipWcsTask",
"FitTanSipWcsConfig"]
33 from .setMatchDistance
import setMatchDistance
34 from .sip
import makeCreateWcsWithSip
38 """Config for FitTanSipWcsTask."""
39 order = pexConfig.RangeField(
40 doc=
"order of SIP polynomial",
45 numIter = pexConfig.RangeField(
46 doc=
"number of iterations of fitter (which fits X and Y separately, and so benefits from "
52 numRejIter = pexConfig.RangeField(
53 doc=
"number of rejection iterations",
58 rejSigma = pexConfig.RangeField(
59 doc=
"Number of standard deviations for clipping level",
64 maxScatterArcsec = pexConfig.RangeField(
65 doc=
"maximum median scatter of a WCS fit beyond which the fit fails (arcsec); "
66 "be generous, as this is only intended to catch catastrophic failures",
74 """Fit a TAN-SIP WCS given a list of reference object/source matches.
76 ConfigClass = FitTanSipWcsConfig
77 _DefaultName =
"fitWcs"
80 def fitWcs(self, matches, initWcs, bbox=None, refCat=None, sourceCat=None, exposure=None):
81 """Fit a TAN-SIP WCS from a list of reference object/source matches
85 matches : `list` of `lsst.afw.table.ReferenceMatch`
86 The following fields are read:
88 - match.first (reference object) coord
89 - match.second (source) centroid
91 The following fields are written:
93 - match.first (reference object) centroid,
94 - match.second (source) centroid
95 - match.distance (on sky separation, in radians)
97 initWcs : `lsst.afw.geom.SkyWcs`
99 bbox : `lsst.geom.Box2I`
100 the region over which the WCS will be valid (an lsst:afw::geom::Box2I);
101 if None or an empty box then computed from matches
102 refCat : `lsst.afw.table.SimpleCatalog`
103 reference object catalog, or None.
104 If provided then all centroids are updated with the new WCS,
105 otherwise only the centroids for ref objects in matches are updated.
106 Required fields are "centroid_x", "centroid_y", "coord_ra", and "coord_dec".
107 sourceCat : `lsst.afw.table.SourceCatalog`
108 source catalog, or None.
109 If provided then coords are updated with the new WCS;
110 otherwise only the coords for sources in matches are updated.
111 Required fields are "slot_Centroid_x", "slot_Centroid_y", and "coord_ra", and "coord_dec".
112 exposure : `lsst.afw.image.Exposure`
113 Ignored; present for consistency with FitSipDistortionTask.
117 result : `lsst.pipe.base.Struct`
118 with the following fields:
120 - ``wcs`` : the fit WCS (`lsst.afw.geom.SkyWcs`)
121 - ``scatterOnSky`` : median on-sky separation between reference
122 objects and sources in "matches" (`lsst.afw.geom.Angle`)
130 wcs = self.
initialWcsinitialWcs(matches, initWcs)
131 rejected = np.zeros(len(matches), dtype=bool)
132 for rej
in range(self.config.numRejIter):
133 sipObject = self.
_fitWcs_fitWcs([mm
for i, mm
in enumerate(matches)
if not rejected[i]], wcs)
134 wcs = sipObject.getNewWcs()
135 rejected = self.
rejectMatchesrejectMatches(matches, wcs, rejected)
136 if rejected.sum() == len(rejected):
137 raise RuntimeError(
"All matches rejected in iteration %d" % (rej + 1,))
139 "Iteration {0} of astrometry fitting: rejected {1} outliers, "
140 "out of {2} total matches.".
format(
141 rej, rejected.sum(), len(rejected)
145 print(
"Plotting fit after rejection iteration %d/%d" % (rej + 1, self.config.numRejIter))
146 self.
plotFitplotFit(matches, wcs, rejected)
148 sipObject = self.
_fitWcs_fitWcs([mm
for i, mm
in enumerate(matches)
if not rejected[i]], wcs)
149 wcs = sipObject.getNewWcs()
151 print(
"Plotting final fit")
152 self.
plotFitplotFit(matches, wcs, rejected)
154 if refCat
is not None:
155 self.log.
debug(
"Updating centroids in refCat")
158 self.log.
warn(
"Updating reference object centroids in match list; refCat is None")
161 if sourceCat
is not None:
162 self.log.
debug(
"Updating coords in sourceCat")
165 self.log.
warn(
"Updating source coords in match list; sourceCat is None")
168 self.log.
debug(
"Updating distance in match list")
171 scatterOnSky = sipObject.getScatterOnSky()
173 if scatterOnSky.asArcseconds() > self.config.maxScatterArcsec:
174 raise pipeBase.TaskError(
175 "Fit failed: median scatter on sky = %0.3f arcsec > %0.3f config.maxScatterArcsec" %
176 (scatterOnSky.asArcseconds(), self.config.maxScatterArcsec))
178 return pipeBase.Struct(
180 scatterOnSky=scatterOnSky,
184 """Generate a guess Wcs from the astrometric matches
186 We create a Wcs anchored at the center of the matches, with the scale
187 of the input Wcs. This is necessary because matching returns only
188 matches with no estimated Wcs, and the input Wcs is a wild guess.
189 We're using the best of each: positions from the matches, and scale
194 matches : `list` of `lsst.afw.table.ReferenceMatch`
195 List of sources matched to references.
196 wcs : `lsst.afw.geom.SkyWcs`
201 newWcs : `lsst.afw.geom.SkyWcs`
202 Initial WCS guess from estimated crpix and crval.
208 crval += mm.first.getCoord().getVector()
209 crpix /= len(matches)
210 crval /= len(matches)
213 cdMatrix=wcs.getCdMatrix())
216 def _fitWcs(self, matches, wcs):
217 """Fit a Wcs based on the matches and a guess Wcs.
221 matches : `list` of `lsst.afw.table.ReferenceMatch`
222 List of sources matched to references.
223 wcs : `lsst.afw.geom.SkyWcs`
228 sipObject : `lsst.meas.astrom.sip.CreateWcsWithSip`
231 for i
in range(self.config.numIter):
233 wcs = sipObject.getNewWcs()
237 """Flag deviant matches
239 We return a boolean numpy array indicating whether the corresponding
240 match should be rejected. The previous list of rejections is used
241 so we can calculate uncontaminated statistics.
245 matches : `list` of `lsst.afw.table.ReferenceMatch`
246 List of sources matched to references.
247 wcs : `lsst.afw.geom.SkyWcs`
249 rejected : array-like of `bool`
250 Array of matches rejected from the fit. Unused.
254 rejectedMatches : `ndarray` of type `bool`
255 Matched objects found to be outside of tolerance.
257 fit = [wcs.skyToPixel(m.first.getCoord())
for m
in matches]
258 dx = np.array([ff.getX() - mm.second.getCentroid().getX()
for ff, mm
in zip(fit, matches)])
259 dy = np.array([ff.getY() - mm.second.getCentroid().getY()
for ff, mm
in zip(fit, matches)])
260 good = np.logical_not(rejected)
261 return (dx > self.config.rejSigma*dx[good].
std()) | (dy > self.config.rejSigma*dy[good].
std())
266 We create four plots, for all combinations of (dx, dy) against
267 (x, y). Good points are black, while rejected points are red.
271 matches : `list` of `lsst.afw.table.ReferenceMatch`
272 List of sources matched to references.
273 wcs : `lsst.afw.geom.SkyWcs`
275 rejected : array-like of `bool`
276 Array of matches rejected from the fit.
279 import matplotlib.pyplot
as plt
280 except ImportError
as e:
281 self.log.
warn(
"Unable to import matplotlib: %s", e)
284 fit = [wcs.skyToPixel(m.first.getCoord())
for m
in matches]
285 x1 = np.array([ff.getX()
for ff
in fit])
286 y1 = np.array([ff.getY()
for ff
in fit])
287 x2 = np.array([m.second.getCentroid().getX()
for m
in matches])
288 y2 = np.array([m.second.getCentroid().getY()
for m
in matches])
293 good = np.logical_not(rejected)
295 figure = plt.figure()
296 axes = figure.add_subplot(2, 2, 1)
297 axes.plot(x2[good], dx[good],
'ko')
298 axes.plot(x2[rejected], dx[rejected],
'ro')
300 axes.set_ylabel(
"dx")
302 axes = figure.add_subplot(2, 2, 2)
303 axes.plot(x2[good], dy[good],
'ko')
304 axes.plot(x2[rejected], dy[rejected],
'ro')
306 axes.set_ylabel(
"dy")
308 axes = figure.add_subplot(2, 2, 3)
309 axes.plot(y2[good], dx[good],
'ko')
310 axes.plot(y2[rejected], dx[rejected],
'ro')
312 axes.set_ylabel(
"dx")
314 axes = figure.add_subplot(2, 2, 4)
315 axes.plot(y2[good], dy[good],
'ko')
316 axes.plot(y2[rejected], dy[rejected],
'ro')
318 axes.set_ylabel(
"dy")
An integer coordinate rectangle.
Point in an unspecified spherical coordinate system.
def _fitWcs(self, matches, wcs)
def initialWcs(self, matches, wcs)
def fitWcs(self, matches, initWcs, bbox=None, refCat=None, sourceCat=None, exposure=None)
def plotFit(self, matches, wcs, rejected)
def rejectMatches(self, matches, wcs, rejected)
Vector3d is a vector in ℝ³ with components stored in double precision.
std::shared_ptr< SkyWcs > makeSkyWcs(daf::base::PropertySet &metadata, bool strip=false)
Construct a SkyWcs from FITS keywords.
void updateRefCentroids(geom::SkyWcs const &wcs, ReferenceCollection &refList)
Update centroids in a collection of reference objects.
void updateSourceCoords(geom::SkyWcs const &wcs, SourceCollection &sourceList)
Update sky coordinates in a collection of source objects.
def setMatchDistance(matches)
CreateWcsWithSip< MatchT > makeCreateWcsWithSip(std::vector< MatchT > const &matches, afw::geom::SkyWcs const &linearWcs, int const order, geom::Box2I const &bbox=geom::Box2I(), int const ngrid=0)
Factory function for CreateWcsWithSip.
def format(config, name=None, writeSourceLine=True, prefix="", verbose=False)