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fitTanSipWcs.py
Go to the documentation of this file.
1# This file is part of meas_astrom.
2#
3# Developed for the LSST Data Management System.
4# This product includes software developed by the LSST Project
5# (https://www.lsst.org).
6# See the COPYRIGHT file at the top-level directory of this distribution
7# for details of code ownership.
8#
9# This program is free software: you can redistribute it and/or modify
10# it under the terms of the GNU General Public License as published by
11# the Free Software Foundation, either version 3 of the License, or
12# (at your option) any later version.
13#
14# This program is distributed in the hope that it will be useful,
15# but WITHOUT ANY WARRANTY; without even the implied warranty of
16# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
17# GNU General Public License for more details.
18#
19# You should have received a copy of the GNU General Public License
20# along with this program. If not, see <https://www.gnu.org/licenses/>.
21
22__all__ = ["FitTanSipWcsTask", "FitTanSipWcsConfig"]
23
24
25import numpy as np
26
27import lsst.geom
28import lsst.sphgeom
29import lsst.afw.geom as afwGeom
30import lsst.afw.table as afwTable
31import lsst.pex.config as pexConfig
32import lsst.pipe.base as pipeBase
33from lsst.utils.timer import timeMethod
34from .setMatchDistance import setMatchDistance
35from .sip import makeCreateWcsWithSip
36
37
38class FitTanSipWcsConfig(pexConfig.Config):
39 """Config for FitTanSipWcsTask."""
40 order = pexConfig.RangeField(
41 doc="order of SIP polynomial",
42 dtype=int,
43 default=2,
44 min=0,
45 )
46 numIter = pexConfig.RangeField(
47 doc="number of iterations of fitter (which fits X and Y separately, and so benefits from "
48 "a few iterations",
49 dtype=int,
50 default=3,
51 min=1,
52 )
53 numRejIter = pexConfig.RangeField(
54 doc="number of rejection iterations",
55 dtype=int,
56 default=1,
57 min=0,
58 )
59 rejSigma = pexConfig.RangeField(
60 doc="Number of standard deviations for clipping level",
61 dtype=float,
62 default=3.0,
63 min=0.0,
64 )
65 maxScatterArcsec = pexConfig.RangeField(
66 doc="maximum median scatter of a WCS fit beyond which the fit fails (arcsec); "
67 "be generous, as this is only intended to catch catastrophic failures",
68 dtype=float,
69 default=10,
70 min=0,
71 )
72
73
74class FitTanSipWcsTask(pipeBase.Task):
75 """Fit a TAN-SIP WCS given a list of reference object/source matches.
76 """
77 ConfigClass = FitTanSipWcsConfig
78 _DefaultName = "fitWcs"
79
80 @timeMethod
81 def fitWcs(self, matches, initWcs, bbox=None, refCat=None, sourceCat=None, exposure=None):
82 """Fit a TAN-SIP WCS from a list of reference object/source matches
83
84 Parameters
85 ----------
86 matches : `list` of `lsst.afw.table.ReferenceMatch`
87 The following fields are read:
88
89 - match.first (reference object) coord
90 - match.second (source) centroid
91
92 The following fields are written:
93
94 - match.first (reference object) centroid,
95 - match.second (source) centroid
96 - match.distance (on sky separation, in radians)
97
98 initWcs : `lsst.afw.geom.SkyWcs`
99 initial WCS
100 bbox : `lsst.geom.Box2I`
101 the region over which the WCS will be valid (an lsst:afw::geom::Box2I);
102 if None or an empty box then computed from matches
104 reference object catalog, or None.
105 If provided then all centroids are updated with the new WCS,
106 otherwise only the centroids for ref objects in matches are updated.
107 Required fields are "centroid_x", "centroid_y", "coord_ra", and "coord_dec".
108 sourceCat : `lsst.afw.table.SourceCatalog`
109 source catalog, or None.
110 If provided then coords are updated with the new WCS;
111 otherwise only the coords for sources in matches are updated.
112 Required fields are "slot_Centroid_x", "slot_Centroid_y", and "coord_ra", and "coord_dec".
113 exposure : `lsst.afw.image.Exposure`
114 Ignored; present for consistency with FitSipDistortionTask.
115
116 Returns
117 -------
118 result : `lsst.pipe.base.Struct`
119 with the following fields:
120
121 - ``wcs`` : the fit WCS (`lsst.afw.geom.SkyWcs`)
122 - ``scatterOnSky`` : median on-sky separation between reference
123 objects and sources in "matches" (`lsst.afw.geom.Angle`)
124 """
125 if bbox is None:
126 bbox = lsst.geom.Box2I()
127
128 import lsstDebug
129 debug = lsstDebug.Info(__name__)
130
131 wcs = self.initialWcs(matches, initWcs)
132 rejected = np.zeros(len(matches), dtype=bool)
133 for rej in range(self.config.numRejIter):
134 sipObject = self._fitWcs([mm for i, mm in enumerate(matches) if not rejected[i]], wcs)
135 wcs = sipObject.getNewWcs()
136 rejected = self.rejectMatches(matches, wcs, rejected)
137 if rejected.sum() == len(rejected):
138 raise RuntimeError("All matches rejected in iteration %d" % (rej + 1,))
139 self.log.debug(
140 "Iteration %d of astrometry fitting: rejected %f outliers, out of %d total matches.",
141 rej, rejected.sum(), len(rejected)
142 )
143 if debug.plot:
144 print("Plotting fit after rejection iteration %d/%d" % (rej + 1, self.config.numRejIter))
145 self.plotFit(matches, wcs, rejected)
146 # Final fit after rejection
147 sipObject = self._fitWcs([mm for i, mm in enumerate(matches) if not rejected[i]], wcs)
148 wcs = sipObject.getNewWcs()
149 if debug.plot:
150 print("Plotting final fit")
151 self.plotFit(matches, wcs, rejected)
152
153 if refCat is not None:
154 self.log.debug("Updating centroids in refCat")
155 afwTable.updateRefCentroids(wcs, refList=refCat)
156 else:
157 self.log.warning("Updating reference object centroids in match list; refCat is None")
158 afwTable.updateRefCentroids(wcs, refList=[match.first for match in matches])
159
160 if sourceCat is not None:
161 self.log.debug("Updating coords in sourceCat")
162 afwTable.updateSourceCoords(wcs, sourceList=sourceCat)
163 else:
164 self.log.warning("Updating source coords in match list; sourceCat is None")
165 afwTable.updateSourceCoords(wcs, sourceList=[match.second for match in matches])
166
167 self.log.debug("Updating distance in match list")
168 setMatchDistance(matches)
169
170 scatterOnSky = sipObject.getScatterOnSky()
171
172 if scatterOnSky.asArcseconds() > self.config.maxScatterArcsec:
173 raise pipeBase.TaskError(
174 "Fit failed: median scatter on sky = %0.3f arcsec > %0.3f config.maxScatterArcsec" %
175 (scatterOnSky.asArcseconds(), self.config.maxScatterArcsec))
176
177 return pipeBase.Struct(
178 wcs=wcs,
179 scatterOnSky=scatterOnSky,
180 )
181
182 def initialWcs(self, matches, wcs):
183 """Generate a guess Wcs from the astrometric matches
184
185 We create a Wcs anchored at the center of the matches, with the scale
186 of the input Wcs. This is necessary because matching returns only
187 matches with no estimated Wcs, and the input Wcs is a wild guess.
188 We're using the best of each: positions from the matches, and scale
189 from the input Wcs.
190
191 Parameters
192 ----------
193 matches : `list` of `lsst.afw.table.ReferenceMatch`
194 List of sources matched to references.
196 Current WCS.
197
198 Returns
199 -------
200 newWcs : `lsst.afw.geom.SkyWcs`
201 Initial WCS guess from estimated crpix and crval.
202 """
203 crpix = lsst.geom.Extent2D(0, 0)
204 crval = lsst.sphgeom.Vector3d(0, 0, 0)
205 for mm in matches:
206 crpix += lsst.geom.Extent2D(mm.second.getCentroid())
207 crval += mm.first.getCoord().getVector()
208 crpix /= len(matches)
209 crval /= len(matches)
210 newWcs = afwGeom.makeSkyWcs(crpix=lsst.geom.Point2D(crpix),
211 crval=lsst.geom.SpherePoint(crval),
212 cdMatrix=wcs.getCdMatrix())
213 return newWcs
214
215 def _fitWcs(self, matches, wcs):
216 """Fit a Wcs based on the matches and a guess Wcs.
217
218 Parameters
219 ----------
220 matches : `list` of `lsst.afw.table.ReferenceMatch`
221 List of sources matched to references.
223 Current WCS.
224
225 Returns
226 -------
228 Fitted SIP object.
229 """
230 for i in range(self.config.numIter):
231 sipObject = makeCreateWcsWithSip(matches, wcs, self.config.order)
232 wcs = sipObject.getNewWcs()
233 return sipObject
234
235 def rejectMatches(self, matches, wcs, rejected):
236 """Flag deviant matches
237
238 We return a boolean numpy array indicating whether the corresponding
239 match should be rejected. The previous list of rejections is used
240 so we can calculate uncontaminated statistics.
241
242 Parameters
243 ----------
244 matches : `list` of `lsst.afw.table.ReferenceMatch`
245 List of sources matched to references.
247 Fitted WCS.
248 rejected : array-like of `bool`
249 Array of matches rejected from the fit. Unused.
250
251 Returns
252 -------
253 rejectedMatches : `ndarray` of type `bool`
254 Matched objects found to be outside of tolerance.
255 """
256 fit = [wcs.skyToPixel(m.first.getCoord()) for m in matches]
257 dx = np.array([ff.getX() - mm.second.getCentroid().getX() for ff, mm in zip(fit, matches)])
258 dy = np.array([ff.getY() - mm.second.getCentroid().getY() for ff, mm in zip(fit, matches)])
259 good = np.logical_not(rejected)
260 return (dx > self.config.rejSigma*dx[good].std()) | (dy > self.config.rejSigma*dy[good].std())
261
262 def plotFit(self, matches, wcs, rejected):
263 """Plot the fit
264
265 We create four plots, for all combinations of (dx, dy) against
266 (x, y). Good points are black, while rejected points are red.
267
268 Parameters
269 ----------
270 matches : `list` of `lsst.afw.table.ReferenceMatch`
271 List of sources matched to references.
273 Fitted WCS.
274 rejected : array-like of `bool`
275 Array of matches rejected from the fit.
276 """
277 try:
278 import matplotlib.pyplot as plt
279 except ImportError as e:
280 self.log.warning("Unable to import matplotlib: %s", e)
281 return
282
283 fit = [wcs.skyToPixel(m.first.getCoord()) for m in matches]
284 x1 = np.array([ff.getX() for ff in fit])
285 y1 = np.array([ff.getY() for ff in fit])
286 x2 = np.array([m.second.getCentroid().getX() for m in matches])
287 y2 = np.array([m.second.getCentroid().getY() for m in matches])
288
289 dx = x1 - x2
290 dy = y1 - y2
291
292 good = np.logical_not(rejected)
293
294 figure = plt.figure()
295 axes = figure.add_subplot(2, 2, 1)
296 axes.plot(x2[good], dx[good], 'ko')
297 axes.plot(x2[rejected], dx[rejected], 'ro')
298 axes.set_xlabel("x")
299 axes.set_ylabel("dx")
300
301 axes = figure.add_subplot(2, 2, 2)
302 axes.plot(x2[good], dy[good], 'ko')
303 axes.plot(x2[rejected], dy[rejected], 'ro')
304 axes.set_xlabel("x")
305 axes.set_ylabel("dy")
306
307 axes = figure.add_subplot(2, 2, 3)
308 axes.plot(y2[good], dx[good], 'ko')
309 axes.plot(y2[rejected], dx[rejected], 'ro')
310 axes.set_xlabel("y")
311 axes.set_ylabel("dx")
312
313 axes = figure.add_subplot(2, 2, 4)
314 axes.plot(y2[good], dy[good], 'ko')
315 axes.plot(y2[rejected], dy[rejected], 'ro')
316 axes.set_xlabel("y")
317 axes.set_ylabel("dy")
318
319 plt.show()
A 2-dimensional celestial WCS that transform pixels to ICRS RA/Dec, using the LSST standard for pixel...
Definition: SkyWcs.h:117
A class to contain the data, WCS, and other information needed to describe an image of the sky.
Definition: Exposure.h:72
Custom catalog class for record/table subclasses that are guaranteed to have an ID,...
Definition: SortedCatalog.h:42
An integer coordinate rectangle.
Definition: Box.h:55
Point in an unspecified spherical coordinate system.
Definition: SpherePoint.h:57
def fitWcs(self, matches, initWcs, bbox=None, refCat=None, sourceCat=None, exposure=None)
Definition: fitTanSipWcs.py:81
def plotFit(self, matches, wcs, rejected)
def rejectMatches(self, matches, wcs, rejected)
Measure the distortions in an image plane and express them a SIP polynomials.
Vector3d is a vector in ℝ³ with components stored in double precision.
Definition: Vector3d.h:44
std::shared_ptr< SkyWcs > makeSkyWcs(daf::base::PropertySet &metadata, bool strip=false)
Construct a SkyWcs from FITS keywords.
Definition: SkyWcs.cc:521
void updateRefCentroids(geom::SkyWcs const &wcs, ReferenceCollection &refList)
Update centroids in a collection of reference objects.
Definition: wcsUtils.cc:72
void updateSourceCoords(geom::SkyWcs const &wcs, SourceCollection &sourceList)
Update sky coordinates in a collection of source objects.
Definition: wcsUtils.cc:95
STL namespace.
Lightweight representation of a geometric match between two records.
Definition: Match.h:67