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isrMock.py
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1# This file is part of ip_isr.
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__ = ["IsrMockConfig", "IsrMock", "RawMock", "TrimmedRawMock", "RawDictMock",
23 "CalibratedRawMock", "MasterMock",
24 "BiasMock", "DarkMock", "FlatMock", "FringeMock", "UntrimmedFringeMock",
25 "BfKernelMock", "DefectMock", "CrosstalkCoeffMock", "TransmissionMock",
26 "MockDataContainer", "MockFringeContainer"]
27
28import copy
29import numpy as np
30import tempfile
31import astropy.time
32
33from datetime import datetime, timezone
34
35import lsst.geom
36import lsst.afw.geom as afwGeom
37import lsst.afw.image as afwImage
38from lsstDebug import getDebugFrame
39
40import lsst.afw.cameraGeom.utils as afwUtils
41import lsst.afw.cameraGeom.testUtils as afwTestUtils
42from lsst.afw.cameraGeom import ReadoutCorner
43import lsst.pex.config as pexConfig
44import lsst.pipe.base as pipeBase
45from .crosstalk import CrosstalkCalib
46from .defects import Defects
47
48
49class IsrMockConfig(pexConfig.Config):
50 """Configuration parameters for isrMock.
51
52 These parameters produce generic fixed position signals from
53 various sources, and combine them in a way that matches how those
54 signals are combined to create real data. The camera used is the
55 test camera defined by the afwUtils code.
56 """
57 # Detector parameters. "Exposure" parameters.
58 isLsstLike = pexConfig.Field(
59 dtype=bool,
60 default=False,
61 doc="If True, products have one raw image per amplifier, otherwise, one raw image per detector.",
62 )
63 plateScale = pexConfig.Field(
64 dtype=float,
65 default=20.0,
66 doc="Plate scale used in constructing mock camera.",
67 )
68 radialDistortion = pexConfig.Field(
69 dtype=float,
70 default=0.925,
71 doc="Radial distortion term used in constructing mock camera.",
72 )
73 isTrimmed = pexConfig.Field(
74 dtype=bool,
75 default=True,
76 doc="If True, amplifiers have been trimmed and mosaicked to remove regions outside the data BBox.",
77 )
78 detectorIndex = pexConfig.Field(
79 dtype=int,
80 default=20,
81 doc="Index for the detector to use. The default value uses a standard 2x4 array of amps.",
82 )
83 rngSeed = pexConfig.Field(
84 dtype=int,
85 default=20000913,
86 doc="Seed for random number generator used to add noise.",
87 )
88 # TODO: DM-18345 Check that mocks scale correctly when gain != 1.0
89 gain = pexConfig.Field(
90 dtype=float,
91 default=1.0,
92 doc="Gain for simulated data in electron/adu.",
93 )
94 readNoise = pexConfig.Field(
95 dtype=float,
96 default=5.0,
97 doc="Read noise of the detector in electron.",
98 )
99 expTime = pexConfig.Field(
100 dtype=float,
101 default=5.0,
102 doc="Exposure time for simulated data.",
103 )
104
105 # Signal parameters
106 skyLevel = pexConfig.Field(
107 dtype=float,
108 default=1000.0,
109 doc="Background contribution to be generated from 'the sky' in "
110 "adu (IsrTask) or electron (IsrTaskLSST).",
111 )
112 sourceFlux = pexConfig.ListField(
113 dtype=float,
114 default=[45000.0],
115 doc="Peak flux level of simulated 'astronomical sources' in "
116 "adu (IsrTask) or electron (IsrTaskLSST).",
117 )
118 sourceAmp = pexConfig.ListField(
119 dtype=int,
120 default=[0],
121 doc="Amplifier to place simulated 'astronomical sources'.",
122 )
123 sourceX = pexConfig.ListField(
124 dtype=float,
125 default=[50.0],
126 doc="Peak position (in amplifier coordinates) of simulated 'astronomical sources'.",
127 )
128 sourceY = pexConfig.ListField(
129 dtype=float,
130 default=[25.0],
131 doc="Peak position (in amplifier coordinates) of simulated 'astronomical sources'.",
132 )
133 overscanScale = pexConfig.Field(
134 dtype=float,
135 default=100.0,
136 doc="Amplitude of the ramp function to add to overscan data in "
137 "adu (IsrTask) or electron (IsrTaskLSST)",
138 )
139 biasLevel = pexConfig.Field(
140 dtype=float,
141 default=8000.0,
142 doc="Background contribution to be generated from the bias offset in adu.",
143 )
144 darkRate = pexConfig.Field(
145 dtype=float,
146 default=5.0,
147 doc="Background level contribution (in electron/s) to be generated from dark current.",
148 )
149 darkTime = pexConfig.Field(
150 dtype=float,
151 default=5.0,
152 doc="Exposure time for the dark current contribution.",
153 )
154 flatDrop = pexConfig.Field(
155 dtype=float,
156 default=0.1,
157 doc="Fractional flux drop due to flat from center to edge of detector along x-axis.",
158 )
159 fringeScale = pexConfig.ListField(
160 dtype=float,
161 default=[200.0],
162 doc="Peak fluxes for the components of the fringe ripple in "
163 "adu (IsrTask) or electron (IsrTaskLSST).",
164 )
165 fringeX0 = pexConfig.ListField(
166 dtype=float,
167 default=[-100],
168 doc="Center position for the fringe ripples.",
169 )
170 fringeY0 = pexConfig.ListField(
171 dtype=float,
172 default=[-0],
173 doc="Center position for the fringe ripples.",
174 )
175
176 # Inclusion parameters
177 doAddSky = pexConfig.Field(
178 dtype=bool,
179 default=True,
180 doc="Apply 'sky' signal to output image.",
181 )
182 doAddSource = pexConfig.Field(
183 dtype=bool,
184 default=True,
185 doc="Add simulated source to output image.",
186 )
187 doAddCrosstalk = pexConfig.Field(
188 dtype=bool,
189 default=False,
190 doc="Apply simulated crosstalk to output image. This cannot be corrected by ISR, "
191 "as detector.hasCrosstalk()==False.",
192 )
193 doAddOverscan = pexConfig.Field(
194 dtype=bool,
195 default=True,
196 doc="If untrimmed, add overscan ramp to overscan and data regions.",
197 )
198 doAddBias = pexConfig.Field(
199 dtype=bool,
200 default=True,
201 doc="Add bias signal to data.",
202 )
203 doAddDark = pexConfig.Field(
204 dtype=bool,
205 default=True,
206 doc="Add dark signal to data.",
207 )
208 doAddFlat = pexConfig.Field(
209 dtype=bool,
210 default=True,
211 doc="Add flat signal to data.",
212 )
213 doAddFringe = pexConfig.Field(
214 dtype=bool,
215 default=True,
216 doc="Add fringe signal to data.",
217 )
218
219 # Datasets to create and return instead of generating an image.
220 doTransmissionCurve = pexConfig.Field(
221 dtype=bool,
222 default=False,
223 doc="Return a simulated transmission curve.",
224 )
225 doDefects = pexConfig.Field(
226 dtype=bool,
227 default=False,
228 doc="Return a simulated defect list.",
229 )
230 doBrighterFatter = pexConfig.Field(
231 dtype=bool,
232 default=False,
233 doc="Return a simulated brighter-fatter kernel.",
234 )
235 doDeferredCharge = pexConfig.Field(
236 dtype=bool,
237 default=False,
238 doc="Return a simulated deferred charge calibration.",
239 )
240 doCrosstalkCoeffs = pexConfig.Field(
241 dtype=bool,
242 default=False,
243 doc="Return the matrix of crosstalk coefficients.",
244 )
245 doLinearizer = pexConfig.Field(
246 dtype=bool,
247 default=False,
248 doc="Return linearizer dataset.",
249 )
250 doDataRef = pexConfig.Field(
251 dtype=bool,
252 default=False,
253 doc="Return a simulated gen2 butler dataRef.",
254 )
255 doGenerateImage = pexConfig.Field(
256 dtype=bool,
257 default=False,
258 doc="Return the generated output image if True.",
259 )
260 doGenerateData = pexConfig.Field(
261 dtype=bool,
262 default=False,
263 doc="Return a non-image data structure if True.",
264 )
265 doGenerateAmpDict = pexConfig.Field(
266 dtype=bool,
267 default=False,
268 doc="Return a dict of exposure amplifiers instead of an afwImage.Exposure.",
269 )
270
271
272class IsrMock(pipeBase.Task):
273 """Class to generate consistent mock images for ISR testing.
274
275 ISR testing currently relies on one-off fake images that do not
276 accurately mimic the full set of detector effects. This class
277 uses the test camera/detector/amplifier structure defined in
278 `lsst.afw.cameraGeom.testUtils` to avoid making the test data
279 dependent on any of the actual obs package formats.
280 """
281 ConfigClass = IsrMockConfig
282 _DefaultName = "isrMock"
283
284 def __init__(self, **kwargs):
285 super().__init__(**kwargs)
286 self.rng = np.random.RandomState(self.config.rngSeed)
287 # The coefficients have units adu for IsrTask and have
288 # units electron for IsrTaskLSST.
289 self.crosstalkCoeffs = np.array([[0.0, 0.0, 0.0, 0.0, 0.0, -1e-3, 0.0, 0.0],
290 [1e-2, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
291 [1e-2, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
292 [1e-2, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
293 [1e-2, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
294 [1e-2, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
295 [1e-2, 0.0, 0.0, 2.2e-2, 0.0, 0.0, 0.0, 0.0],
296 [1e-2, 5e-3, 5e-4, 3e-3, 4e-2, 5e-3, 5e-3, 0.0]])
297 if getDebugFrame(self._display, "mockCrosstalkCoeffs"):
298 self.crosstalkCoeffs = np.array([[0.0, 1.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
299 [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
300 [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
301 [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
302 [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
303 [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
304 [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0],
305 [0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0]])
306 # Generic gaussian BF kernel
307 self.bfKernel = np.array([[1., 4., 7., 4., 1.],
308 [4., 16., 26., 16., 4.],
309 [7., 26., 41., 26., 7.],
310 [4., 16., 26., 16., 4.],
311 [1., 4., 7., 4., 1.]]) / 273.0
312
313 def run(self):
314 """Generate a mock ISR product, and return it.
315
316 Returns
317 -------
318 image : `lsst.afw.image.Exposure`
319 Simulated ISR image with signals added.
320 dataProduct :
321 Simulated ISR data products.
322 None :
323 Returned if no valid configuration was found.
324
325 Raises
326 ------
327 RuntimeError
328 Raised if both doGenerateImage and doGenerateData are specified.
329 """
330 if self.config.doGenerateImage and self.config.doGenerateData:
331 raise RuntimeError("Only one of doGenerateImage and doGenerateData may be specified.")
332 elif self.config.doGenerateImage:
333 return self.makeImage()
334 elif self.config.doGenerateData:
335 return self.makeData()
336 else:
337 return None
338
339 def makeData(self):
340 """Generate simulated ISR data.
341
342 Currently, only the class defined crosstalk coefficient
343 matrix, brighter-fatter kernel, a constant unity transmission
344 curve, or a simple single-entry defect list can be generated.
345
346 Returns
347 -------
348 dataProduct :
349 Simulated ISR data product.
350 """
351 if sum(map(bool, [self.config.doBrighterFatter,
352 self.config.doDeferredCharge,
353 self.config.doDefects,
354 self.config.doTransmissionCurve,
355 self.config.doCrosstalkCoeffs,
356 self.config.doLinearizer])) != 1:
357 raise RuntimeError("Only one data product can be generated at a time.")
358 elif self.config.doBrighterFatter:
359 return self.makeBfKernel()
360 elif self.config.doDeferredCharge:
361 return self.makeDeferredChargeCalib()
362 elif self.config.doDefects:
363 return self.makeDefectList()
364 elif self.config.doTransmissionCurve:
365 return self.makeTransmissionCurve()
366 elif self.config.doCrosstalkCoeffs:
367 return self.crosstalkCoeffs
368 elif self.config.doLinearizer:
369 return self.makeLinearizer()
370 else:
371 return None
372
373 def makeBfKernel(self):
374 """Generate a simple Gaussian brighter-fatter kernel.
375
376 Returns
377 -------
378 kernel : `numpy.ndarray`
379 Simulated brighter-fatter kernel.
380 """
381 return self.bfKernel
382
384 """Generate a CTI calibration.
385 """
386
387 raise NotImplementedError("Mock deferred charge is not implemented for IsrMock.")
388
389 def makeDefectList(self):
390 """Generate a simple single-entry defect list.
391
392 Returns
393 -------
394 defectList : `lsst.meas.algorithms.Defects`
395 Simulated defect list
396 """
398 lsst.geom.Extent2I(40, 50))])
399
401 """Generate the simulated crosstalk coefficients.
402
403 Returns
404 -------
405 coeffs : `numpy.ndarray`
406 Simulated crosstalk coefficients.
407 """
408
409 return self.crosstalkCoeffs
410
412 """Generate a simulated flat transmission curve.
413
414 Returns
415 -------
416 transmission : `lsst.afw.image.TransmissionCurve`
417 Simulated transmission curve.
418 """
419
420 return afwImage.TransmissionCurve.makeIdentity()
421
422 def makeLinearity(self):
423 """Generate a linearity dataset.
424
425 Returns
426 -------
427 linearizer : `lsst.ip.isr.Linearizer`
428 """
429 raise NotImplementedError("Linearizer not implemented for isrMock.")
430
431 def makeImage(self):
432 """Generate a simulated ISR image.
433
434 Returns
435 -------
436 exposure : `lsst.afw.image.Exposure` or `dict`
437 Simulated ISR image data.
438
439 Notes
440 -----
441 This method currently constructs a "raw" data image by:
442
443 * Generating a simulated sky with noise
444 * Adding a single Gaussian "star"
445 * Adding the fringe signal
446 * Multiplying the frame by the simulated flat
447 * Adding dark current (and noise)
448 * Adding a bias offset (and noise)
449 * Adding an overscan gradient parallel to the pixel y-axis
450 * Simulating crosstalk by adding a scaled version of each
451 amplifier to each other amplifier.
452
453 The exposure with image data constructed this way is in one of
454 three formats.
455
456 * A single image, with overscan and prescan regions retained
457 * A single image, with overscan and prescan regions trimmed
458 * A `dict`, containing the amplifer data indexed by the
459 amplifier name.
460
461 The nonlinearity, CTE, and brighter fatter are currently not
462 implemented.
463
464 Note that this method generates an image in the reverse
465 direction as the ISR processing, as the output image here has
466 had a series of instrument effects added to an idealized
467 exposure.
468 """
469 exposure = self.getExposure()
470
471 for idx, amp in enumerate(exposure.getDetector()):
472 bbox = None
473 if self.config.isTrimmed is True:
474 bbox = amp.getBBox()
475 else:
476 bbox = amp.getRawDataBBox()
477
478 ampData = exposure.image[bbox]
479
480 if self.config.doAddSky is True:
481 self.amplifierAddNoise(ampData, self.config.skyLevel, np.sqrt(self.config.skyLevel))
482
483 if self.config.doAddSource is True:
484 for sourceAmp, sourceFlux, sourceX, sourceY in zip(self.config.sourceAmp,
485 self.config.sourceFlux,
486 self.config.sourceX,
487 self.config.sourceY):
488 if idx == sourceAmp:
489 self.amplifierAddSource(ampData, sourceFlux, sourceX, sourceY)
490
491 if self.config.doAddFringe is True:
492 self.amplifierAddFringe(amp, ampData, np.array(self.config.fringeScale),
493 x0=np.array(self.config.fringeX0),
494 y0=np.array(self.config.fringeY0))
495
496 if self.config.doAddFlat is True:
497 if ampData.getArray().sum() == 0.0:
498 self.amplifierAddNoise(ampData, 1.0, 0.0)
499 u0 = exposure.getDimensions().getX()
500 v0 = exposure.getDimensions().getY()
501 self.amplifierMultiplyFlat(amp, ampData, self.config.flatDrop, u0=u0, v0=v0)
502
503 if self.config.doAddDark is True:
504 self.amplifierAddNoise(ampData,
505 self.config.darkRate * self.config.darkTime / self.config.gain,
506 np.sqrt(self.config.darkRate
507 * self.config.darkTime / self.config.gain))
508
509 if self.config.doAddCrosstalk is True:
510 ctCalib = CrosstalkCalib()
511 # We use the regular subtractCrosstalk code but with a negative
512 # sign on the crosstalk coefficients so it adds instead of
513 # subtracts. We only apply the signal plane (ignoreVariance,
514 # subtrahendMasking) with a very large pixel to mask to ensure
515 # no crosstalk mask bits are set.
516 ctCalib.subtractCrosstalk(
517 exposure,
518 crosstalkCoeffs=-1*self.crosstalkCoeffs,
519 doSubtrahendMasking=True,
520 minPixelToMask=np.inf,
521 ignoreVariance=True,
522 fullAmplifier=False,
523 )
524
525 for amp in exposure.getDetector():
526 bbox = None
527 if self.config.isTrimmed is True:
528 bbox = amp.getBBox()
529 else:
530 bbox = amp.getRawDataBBox()
531
532 ampData = exposure.image[bbox]
533
534 if self.config.doAddBias is True:
535 self.amplifierAddNoise(ampData, self.config.biasLevel,
536 self.config.readNoise / self.config.gain)
537
538 if self.config.doAddOverscan is True:
539 oscanBBox = amp.getRawHorizontalOverscanBBox()
540 oscanData = exposure.image[oscanBBox]
541 self.amplifierAddNoise(oscanData, self.config.biasLevel,
542 self.config.readNoise / self.config.gain)
543
544 self.amplifierAddYGradient(ampData, -1.0 * self.config.overscanScale,
545 1.0 * self.config.overscanScale)
546 self.amplifierAddYGradient(oscanData, -1.0 * self.config.overscanScale,
547 1.0 * self.config.overscanScale)
548
549 if self.config.doGenerateAmpDict is True:
550 expDict = dict()
551 for amp in exposure.getDetector():
552 expDict[amp.getName()] = exposure
553 return expDict
554 else:
555 return exposure
556
557 # afw primatives to construct the image structure
558 def getCamera(self, isForAssembly=False):
559 """Construct a test camera object.
560
561 Parameters
562 -------
563 isForAssembly : `bool`
564 If True, construct a camera with "super raw"
565 orientation (all amplifiers have LL readout
566 corner but still contains the necessary flip
567 and offset info needed for assembly. This is
568 needed if isLsstLike is True. If False, return
569 a camera with bboxes flipped and offset to the
570 correct orientation given the readout corner.
571
572 Returns
573 -------
574 camera : `lsst.afw.cameraGeom.camera`
575 Test camera.
576 """
577 cameraWrapper = afwTestUtils.CameraWrapper(
578 plateScale=self.config.plateScale,
579 radialDistortion=self.config.radialDistortion,
580 isLsstLike=self.config.isLsstLike and isForAssembly,
581 )
582 camera = cameraWrapper.camera
583 return camera
584
585 def getExposure(self, isTrimmed=None):
586 """Construct a test exposure.
587
588 The test exposure has a simple WCS set, as well as a list of
589 unlikely header keywords that can be removed during ISR
590 processing to exercise that code.
591
592 Parameters
593 ----------
594 isTrimmed : `bool` or `None`, optional
595 Override the configuration isTrimmed?
596
597 Returns
598 -------
599 exposure : `lsst.afw.exposure.Exposure`
600 Construct exposure containing masked image of the
601 appropriate size.
602 """
603 if isTrimmed is None:
604 _isTrimmed = self.config.isTrimmed
605 else:
606 _isTrimmed = isTrimmed
607
608 camera = self.getCamera(isForAssembly=self.config.isLsstLike)
609 detector = camera[self.config.detectorIndex]
610 image = afwUtils.makeImageFromCcd(
611 detector,
612 isTrimmed=_isTrimmed,
613 showAmpGain=False,
614 rcMarkSize=0,
615 binSize=1,
616 imageFactory=afwImage.ImageF,
617 )
618
619 var = afwImage.ImageF(image.getDimensions())
620 mask = afwImage.Mask(image.getDimensions())
621 image.assign(0.0)
622
623 maskedImage = afwImage.makeMaskedImage(image, mask, var)
624 exposure = afwImage.makeExposure(maskedImage)
625 exposure.setDetector(detector)
626 exposure.setWcs(self.getWcs())
627
628 visitInfo = afwImage.VisitInfo(exposureTime=self.config.expTime, darkTime=self.config.darkTime)
629 exposure.getInfo().setVisitInfo(visitInfo)
630 # Set a dummy ID.
631 exposure.getInfo().setId(12345)
632
633 metadata = exposure.getMetadata()
634 metadata.add("SHEEP", 7.3, "number of sheep on farm")
635 metadata.add("MONKEYS", 155, "monkeys per tree")
636 metadata.add("VAMPIRES", 4, "How scary are vampires.")
637
638 # Add the current time
639 now = datetime.now(timezone.utc)
640 currentMjd = astropy.time.Time(now, format='datetime', scale='utc').mjd
641 metadata.add("MJD", currentMjd, "Modified Julian Date that the file was written")
642
643 ccd = exposure.getDetector()
644 newCcd = ccd.rebuild()
645 newCcd.clear()
646 readoutMap = {
647 'LL': ReadoutCorner.LL,
648 'LR': ReadoutCorner.LR,
649 'UR': ReadoutCorner.UR,
650 'UL': ReadoutCorner.UL,
651 }
652 for amp in ccd:
653 newAmp = amp.rebuild()
654 newAmp.setLinearityCoeffs((0., 1., 0., 0.))
655 newAmp.setLinearityType("Polynomial")
656 newAmp.setGain(self.config.gain)
657 newAmp.setSuspectLevel(25000.0)
658 newAmp.setSaturation(32000.0)
659 readoutCorner = amp.getReadoutCorner().name
660
661 # Apply flips to bbox where needed
662 imageBBox = amp.getRawDataBBox()
663 rawBbox = amp.getRawBBox()
664 parallelOscanBBox = amp.getRawParallelOverscanBBox()
665 serialOscanBBox = amp.getRawSerialOverscanBBox()
666 prescanBBox = amp.getRawPrescanBBox()
667
668 if self.config.isLsstLike:
669 # This follows cameraGeom.testUtils
670 xoffset, yoffset = amp.getRawXYOffset()
671 offext = lsst.geom.Extent2I(xoffset, yoffset)
672 flipx = bool(amp.getRawFlipX())
673 flipy = bool(amp.getRawFlipY())
674 if flipx:
675 xExt = rawBbox.getDimensions().getX()
676 rawBbox.flipLR(xExt)
677 imageBBox.flipLR(xExt)
678 parallelOscanBBox.flipLR(xExt)
679 serialOscanBBox.flipLR(xExt)
680 prescanBBox.flipLR(xExt)
681 if flipy:
682 yExt = rawBbox.getDimensions().getY()
683 rawBbox.flipTB(yExt)
684 imageBBox.flipTB(yExt)
685 parallelOscanBBox.flipTB(yExt)
686 serialOscanBBox.flipTB(yExt)
687 prescanBBox.flipTB(yExt)
688 if not flipx and not flipy:
689 readoutCorner = 'LL'
690 elif flipx and not flipy:
691 readoutCorner = 'LR'
692 elif flipx and flipy:
693 readoutCorner = 'UR'
694 elif not flipx and flipy:
695 readoutCorner = 'UL'
696 rawBbox.shift(offext)
697 imageBBox.shift(offext)
698 parallelOscanBBox.shift(offext)
699 serialOscanBBox.shift(offext)
700 prescanBBox.shift(offext)
701 newAmp.setReadoutCorner(readoutMap[readoutCorner])
702 newAmp.setRawBBox(rawBbox)
703 newAmp.setRawDataBBox(imageBBox)
704 newAmp.setRawParallelOverscanBBox(parallelOscanBBox)
705 newAmp.setRawSerialOverscanBBox(serialOscanBBox)
706 newAmp.setRawPrescanBBox(prescanBBox)
707 newAmp.setRawFlipX(False)
708 newAmp.setRawFlipY(False)
709 no_offset = lsst.geom.Extent2I(0, 0)
710 newAmp.setRawXYOffset(no_offset)
711
712 newCcd.append(newAmp)
713
714 exposure.setDetector(newCcd.finish())
715
716 exposure.image.array[:] = np.zeros(exposure.getImage().getDimensions()).transpose()
717 exposure.mask.array[:] = np.zeros(exposure.getMask().getDimensions()).transpose()
718 exposure.variance.array[:] = np.zeros(exposure.getVariance().getDimensions()).transpose()
719
720 return exposure
721
722 def getWcs(self):
723 """Construct a dummy WCS object.
724
725 Taken from the deprecated ip_isr/examples/exampleUtils.py.
726
727 This is not guaranteed, given the distortion and pixel scale
728 listed in the afwTestUtils camera definition.
729
730 Returns
731 -------
732 wcs : `lsst.afw.geom.SkyWcs`
733 Test WCS transform.
734 """
735 return afwGeom.makeSkyWcs(crpix=lsst.geom.Point2D(0.0, 100.0),
736 crval=lsst.geom.SpherePoint(45.0, 25.0, lsst.geom.degrees),
737 cdMatrix=afwGeom.makeCdMatrix(scale=1.0*lsst.geom.degrees))
738
739 def localCoordToExpCoord(self, ampData, x, y):
740 """Convert between a local amplifier coordinate and the full
741 exposure coordinate.
742
743 Parameters
744 ----------
745 ampData : `lsst.afw.image.ImageF`
746 Amplifier image to use for conversions.
747 x : `int`
748 X-coordinate of the point to transform.
749 y : `int`
750 Y-coordinate of the point to transform.
751
752 Returns
753 -------
754 u : `int`
755 Transformed x-coordinate.
756 v : `int`
757 Transformed y-coordinate.
758
759 Notes
760 -----
761 The output is transposed intentionally here, to match the
762 internal transpose between numpy and afw.image coordinates.
763 """
764 u = x + ampData.getBBox().getBeginX()
765 v = y + ampData.getBBox().getBeginY()
766
767 return (v, u)
768
769 # Simple data values.
770 def amplifierAddNoise(self, ampData, mean, sigma, rng=None):
771 """Add Gaussian noise to an amplifier's image data.
772
773 This method operates in the amplifier coordinate frame.
774
775 Parameters
776 ----------
777 ampData : `lsst.afw.image.ImageF`
778 Amplifier image to operate on.
779 mean : `float`
780 Mean value of the Gaussian noise.
781 sigma : `float`
782 Sigma of the Gaussian noise.
783 rng : `np.random.RandomState`, optional
784 Random state to use instead of self.rng.
785 """
786 if rng is not None:
787 _rng = rng
788 else:
789 _rng = self.rng
790
791 ampArr = ampData.array
792 ampArr[:] = ampArr[:] + _rng.normal(mean, sigma,
793 size=ampData.getDimensions()).transpose()
794
795 def amplifierAddYGradient(self, ampData, start, end):
796 """Add a y-axis linear gradient to an amplifier's image data.
797
798 This method operates in the amplifier coordinate frame.
799
800 Parameters
801 ----------
802 ampData : `lsst.afw.image.ImageF`
803 Amplifier image to operate on.
804 start : `float`
805 Start value of the gradient (at y=0).
806 end : `float`
807 End value of the gradient (at y=ymax).
808 """
809 nPixY = ampData.getDimensions().getY()
810 ampArr = ampData.array
811 ampArr[:] = ampArr[:] + (np.interp(range(nPixY), (0, nPixY - 1), (start, end)).reshape(nPixY, 1)
812 + np.zeros(ampData.getDimensions()).transpose())
813
814 def amplifierAddSource(self, ampData, scale, x0, y0):
815 """Add a single Gaussian source to an amplifier.
816
817 This method operates in the amplifier coordinate frame.
818
819 Parameters
820 ----------
821 ampData : `lsst.afw.image.ImageF`
822 Amplifier image to operate on.
823 scale : `float`
824 Peak flux of the source to add.
825 x0 : `float`
826 X-coordinate of the source peak.
827 y0 : `float`
828 Y-coordinate of the source peak.
829 """
830 for x in range(0, ampData.getDimensions().getX()):
831 for y in range(0, ampData.getDimensions().getY()):
832 ampData.array[y][x] = (ampData.array[y][x]
833 + scale * np.exp(-0.5 * ((x - x0)**2 + (y - y0)**2) / 3.0**2))
834
835 # Functional form data values.
836 def amplifierAddFringe(self, amp, ampData, scale, x0=100, y0=0):
837 """Add a fringe-like ripple pattern to an amplifier's image data.
838
839 Parameters
840 ----------
841 amp : `~lsst.afw.ampInfo.AmpInfoRecord`
842 Amplifier to operate on. Needed for amp<->exp coordinate
843 transforms.
844 ampData : `lsst.afw.image.ImageF`
845 Amplifier image to operate on.
846 scale : `numpy.array` or `float`
847 Peak intensity scaling for the ripple.
848 x0 : `numpy.array` or `float`, optional
849 Fringe center
850 y0 : `numpy.array` or `float`, optional
851 Fringe center
852
853 Notes
854 -----
855 This uses an offset sinc function to generate a ripple
856 pattern. True fringes have much finer structure, but this
857 pattern should be visually identifiable. The (x, y)
858 coordinates are in the frame of the amplifier, and (u, v) in
859 the frame of the full trimmed image.
860 """
861 for x in range(0, ampData.getDimensions().getX()):
862 for y in range(0, ampData.getDimensions().getY()):
863 (u, v) = self.localCoordToExpCoord(amp, x, y)
864 ampData.getArray()[y][x] = np.sum((ampData.getArray()[y][x]
865 + scale * np.sinc(((u - x0) / 50)**2
866 + ((v - y0) / 50)**2)))
867
868 def amplifierMultiplyFlat(self, amp, ampData, fracDrop, u0=100.0, v0=100.0):
869 """Multiply an amplifier's image data by a flat-like pattern.
870
871 Parameters
872 ----------
873 amp : `lsst.afw.ampInfo.AmpInfoRecord`
874 Amplifier to operate on. Needed for amp<->exp coordinate
875 transforms.
876 ampData : `lsst.afw.image.ImageF`
877 Amplifier image to operate on.
878 fracDrop : `float`
879 Fractional drop from center to edge of detector along x-axis.
880 u0 : `float`
881 Peak location in detector coordinates.
882 v0 : `float`
883 Peak location in detector coordinates.
884
885 Notes
886 -----
887 This uses a 2-d Gaussian to simulate an illumination pattern
888 that falls off towards the edge of the detector. The (x, y)
889 coordinates are in the frame of the amplifier, and (u, v) in
890 the frame of the full trimmed image.
891 """
892 if fracDrop >= 1.0:
893 raise RuntimeError("Flat fractional drop cannot be greater than 1.0")
894
895 sigma = u0 / np.sqrt(-2.0 * np.log(fracDrop))
896
897 for x in range(0, ampData.getDimensions().getX()):
898 for y in range(0, ampData.getDimensions().getY()):
899 (u, v) = self.localCoordToExpCoord(amp, x, y)
900 f = np.exp(-0.5 * ((u - u0)**2 + (v - v0)**2) / sigma**2)
901 ampData.array[y][x] = (ampData.array[y][x] * f)
902
903
905 """Generate a raw exposure suitable for ISR.
906 """
907 def __init__(self, **kwargs):
908 super().__init__(**kwargs)
909 self.config.isTrimmed = False
910 self.config.doGenerateImage = True
911 self.config.doGenerateAmpDict = False
912 self.config.doAddOverscan = True
913 self.config.doAddSky = True
914 self.config.doAddSource = True
915 self.config.doAddCrosstalk = False
916 self.config.doAddBias = True
917 self.config.doAddDark = True
918
919
921 """Generate a trimmed raw exposure.
922 """
923 def __init__(self, **kwargs):
924 super().__init__(**kwargs)
925 self.config.isTrimmed = True
926 self.config.doAddOverscan = False
927
928
930 """Generate a trimmed raw exposure.
931 """
932 def __init__(self, **kwargs):
933 super().__init__(**kwargs)
934 self.config.isTrimmed = True
935 self.config.doGenerateImage = True
936 self.config.doAddOverscan = False
937 self.config.doAddSky = True
938 self.config.doAddSource = True
939 self.config.doAddCrosstalk = False
940
941 self.config.doAddBias = False
942 self.config.doAddDark = False
943 self.config.doAddFlat = False
944 self.config.doAddFringe = True
945
946 self.config.biasLevel = 0.0
947 self.config.readNoise = 10.0
948
949
951 """Generate a raw exposure dict suitable for ISR.
952 """
953 def __init__(self, **kwargs):
954 super().__init__(**kwargs)
955 self.config.doGenerateAmpDict = True
956
957
959 """Parent class for those that make master calibrations.
960 """
961 def __init__(self, **kwargs):
962 super().__init__(**kwargs)
963 self.config.isTrimmed = True
964 self.config.doGenerateImage = True
965 self.config.doAddOverscan = False
966 self.config.doAddSky = False
967 self.config.doAddSource = False
968 self.config.doAddCrosstalk = False
969
970 self.config.doAddBias = False
971 self.config.doAddDark = False
972 self.config.doAddFlat = False
973 self.config.doAddFringe = False
974
975
977 """Simulated master bias calibration.
978 """
979 def __init__(self, **kwargs):
980 super().__init__(**kwargs)
981 self.config.doAddBias = True
982 self.config.readNoise = 10.0
983
984
986 """Simulated master dark calibration.
987 """
988 def __init__(self, **kwargs):
989 super().__init__(**kwargs)
990 self.config.doAddDark = True
991 self.config.darkTime = 1.0
992
993
995 """Simulated master flat calibration.
996 """
997 def __init__(self, **kwargs):
998 super().__init__(**kwargs)
999 self.config.doAddFlat = True
1000
1001
1003 """Simulated master fringe calibration.
1004 """
1005 def __init__(self, **kwargs):
1006 super().__init__(**kwargs)
1007 self.config.doAddFringe = True
1008
1009
1011 """Simulated untrimmed master fringe calibration.
1012 """
1013 def __init__(self, **kwargs):
1014 super().__init__(**kwargs)
1015 self.config.isTrimmed = False
1016
1017
1019 """Simulated brighter-fatter kernel.
1020 """
1021 def __init__(self, **kwargs):
1022 super().__init__(**kwargs)
1023 self.config.doGenerateImage = False
1024 self.config.doGenerateData = True
1025 self.config.doBrighterFatter = True
1026 self.config.doDefects = False
1027 self.config.doCrosstalkCoeffs = False
1028 self.config.doTransmissionCurve = False
1029
1030
1032 """Simulated deferred charge calibration.
1033 """
1034 def __init__(self, **kwargs):
1035 super().__init__(**kwargs)
1036 self.config.doGenerateImage = False
1037 self.config.doGenerateData = True
1038 self.config.doDeferredCharge = True
1039 self.config.doDefects = False
1040 self.config.doCrosstalkCoeffs = False
1041 self.config.doTransmissionCurve = False
1042
1043
1045 """Simulated defect list.
1046 """
1047 def __init__(self, **kwargs):
1048 super().__init__(**kwargs)
1049 self.config.doGenerateImage = False
1050 self.config.doGenerateData = True
1051 self.config.doBrighterFatter = False
1052 self.config.doDefects = True
1053 self.config.doCrosstalkCoeffs = False
1054 self.config.doTransmissionCurve = False
1055
1056
1058 """Simulated crosstalk coefficient matrix.
1059 """
1060 def __init__(self, **kwargs):
1061 super().__init__(**kwargs)
1062 self.config.doGenerateImage = False
1063 self.config.doGenerateData = True
1064 self.config.doBrighterFatter = False
1065 self.config.doDefects = False
1066 self.config.doCrosstalkCoeffs = True
1067 self.config.doTransmissionCurve = False
1068
1069
1071 """Simulated transmission curve.
1072 """
1073 def __init__(self, **kwargs):
1074 super().__init__(**kwargs)
1075 self.config.doGenerateImage = False
1076 self.config.doGenerateData = True
1077 self.config.doBrighterFatter = False
1078 self.config.doDefects = False
1079 self.config.doCrosstalkCoeffs = False
1080 self.config.doTransmissionCurve = True
1081
1082
1083class MockDataContainer(object):
1084 """Container for holding ISR mock objects.
1085 """
1086 dataId = "isrMock Fake Data"
1087 darkval = 2. # electron/sec
1088 oscan = 250. # adu
1089 gradient = .10
1090 exptime = 15.0 # seconds
1091 darkexptime = 15.0 # seconds
1092
1093 def __init__(self, **kwargs):
1094 if 'config' in kwargs.keys():
1095 self.config = kwargs['config']
1096 else:
1097 self.config = None
1098
1099 def expectImage(self):
1100 if self.config is None:
1101 self.config = IsrMockConfig()
1102 self.config.doGenerateImage = True
1103 self.config.doGenerateData = False
1104
1105 def expectData(self):
1106 if self.config is None:
1107 self.config = IsrMockConfig()
1108 self.config.doGenerateImage = False
1109 self.config.doGenerateData = True
1110
1111 def get(self, dataType, **kwargs):
1112 """Return an appropriate data product.
1113
1114 Parameters
1115 ----------
1116 dataType : `str`
1117 Type of data product to return.
1118
1119 Returns
1120 -------
1121 mock : IsrMock.run() result
1122 The output product.
1123 """
1124 if "_filename" in dataType:
1125 self.expectData()
1126 return tempfile.mktemp(), "mock"
1127 elif 'transmission_' in dataType:
1128 self.expectData()
1129 return TransmissionMock(config=self.config).run()
1130 elif dataType == 'ccdExposureId':
1131 self.expectData()
1132 return 20090913
1133 elif dataType == 'camera':
1134 self.expectData()
1135 return IsrMock(config=self.config).getCamera()
1136 elif dataType == 'raw':
1137 self.expectImage()
1138 return RawMock(config=self.config).run()
1139 elif dataType == 'bias':
1140 self.expectImage()
1141 return BiasMock(config=self.config).run()
1142 elif dataType == 'dark':
1143 self.expectImage()
1144 return DarkMock(config=self.config).run()
1145 elif dataType == 'flat':
1146 self.expectImage()
1147 return FlatMock(config=self.config).run()
1148 elif dataType == 'fringe':
1149 self.expectImage()
1150 return FringeMock(config=self.config).run()
1151 elif dataType == 'defects':
1152 self.expectData()
1153 return DefectMock(config=self.config).run()
1154 elif dataType == 'bfKernel':
1155 self.expectData()
1156 return BfKernelMock(config=self.config).run()
1157 elif dataType == 'linearizer':
1158 return None
1159 elif dataType == 'crosstalkSources':
1160 return None
1161 else:
1162 raise RuntimeError("ISR DataRefMock cannot return %s.", dataType)
1163
1164
1166 """Container for mock fringe data.
1167 """
1168 dataId = "isrMock Fake Data"
1169 darkval = 2. # electron/sec
1170 oscan = 250. # adu
1171 gradient = .10
1172 exptime = 15 # seconds
1173 darkexptime = 40. # seconds
1174
1175 def __init__(self, **kwargs):
1176 if 'config' in kwargs.keys():
1177 self.config = kwargs['config']
1178 else:
1179 self.config = IsrMockConfig()
1180 self.config.isTrimmed = True
1181 self.config.doAddFringe = True
1182 self.config.readNoise = 10.0
1183
1184 def get(self, dataType, **kwargs):
1185 """Return an appropriate data product.
1186
1187 Parameters
1188 ----------
1189 dataType : `str`
1190 Type of data product to return.
1191
1192 Returns
1193 -------
1194 mock : IsrMock.run() result
1195 The output product.
1196 """
1197 if "_filename" in dataType:
1198 return tempfile.mktemp(), "mock"
1199 elif 'transmission_' in dataType:
1200 return TransmissionMock(config=self.config).run()
1201 elif dataType == 'ccdExposureId':
1202 return 20090913
1203 elif dataType == 'camera':
1204 return IsrMock(config=self.config).getCamera()
1205 elif dataType == 'raw':
1206 return CalibratedRawMock(config=self.config).run()
1207 elif dataType == 'bias':
1208 return BiasMock(config=self.config).run()
1209 elif dataType == 'dark':
1210 return DarkMock(config=self.config).run()
1211 elif dataType == 'flat':
1212 return FlatMock(config=self.config).run()
1213 elif dataType == 'fringe':
1214 fringes = []
1215 configCopy = copy.deepcopy(self.config)
1216 for scale, x, y in zip(self.config.fringeScale, self.config.fringeX0, self.config.fringeY0):
1217 configCopy.fringeScale = [1.0]
1218 configCopy.fringeX0 = [x]
1219 configCopy.fringeY0 = [y]
1220 fringes.append(FringeMock(config=configCopy).run())
1221 return fringes
1222 elif dataType == 'defects':
1223 return DefectMock(config=self.config).run()
1224 elif dataType == 'bfKernel':
1225 return BfKernelMock(config=self.config).run()
1226 elif dataType == 'linearizer':
1227 return None
1228 elif dataType == 'crosstalkSources':
1229 return None
1230 else:
1231 return None
Represent a 2-dimensional array of bitmask pixels.
Definition Mask.h:82
Information about a single exposure of an imaging camera.
Definition VisitInfo.h:68
An integer coordinate rectangle.
Definition Box.h:55
Point in an unspecified spherical coordinate system.
Definition SpherePoint.h:57
localCoordToExpCoord(self, ampData, x, y)
Definition isrMock.py:739
amplifierAddNoise(self, ampData, mean, sigma, rng=None)
Definition isrMock.py:770
amplifierAddSource(self, ampData, scale, x0, y0)
Definition isrMock.py:814
amplifierMultiplyFlat(self, amp, ampData, fracDrop, u0=100.0, v0=100.0)
Definition isrMock.py:868
amplifierAddYGradient(self, ampData, start, end)
Definition isrMock.py:795
getCamera(self, isForAssembly=False)
Definition isrMock.py:558
getExposure(self, isTrimmed=None)
Definition isrMock.py:585
amplifierAddFringe(self, amp, ampData, scale, x0=100, y0=0)
Definition isrMock.py:836
__init__(self, **kwargs)
Definition isrMock.py:284
get(self, dataType, **kwargs)
Definition isrMock.py:1111
get(self, dataType, **kwargs)
Definition isrMock.py:1184
__init__(self, **kwargs)
Definition isrMock.py:907
std::shared_ptr< SkyWcs > makeSkyWcs(daf::base::PropertySet &metadata, bool strip=false)
Construct a SkyWcs from FITS keywords.
Definition SkyWcs.cc:521
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:133
MaskedImage< ImagePixelT, MaskPixelT, VariancePixelT > * makeMaskedImage(typename std::shared_ptr< Image< ImagePixelT > > image, typename std::shared_ptr< Mask< MaskPixelT > > mask=Mask< MaskPixelT >(), typename std::shared_ptr< Image< VariancePixelT > > variance=Image< VariancePixelT >())
A function to return a MaskedImage of the correct type (cf.
std::shared_ptr< Exposure< ImagePixelT, MaskPixelT, VariancePixelT > > makeExposure(MaskedImage< ImagePixelT, MaskPixelT, VariancePixelT > &mimage, std::shared_ptr< geom::SkyWcs const > wcs=std::shared_ptr< geom::SkyWcs const >())
A function to return an Exposure of the correct type (cf.
Definition Exposure.h:484