27 from lsstDebug
import getDebugFrame
33 doInterpolate = pexConfig.Field(
35 doc=
"Interpolate over defects? (ignored unless you provide a list of defects)",
38 doCosmicRay = pexConfig.Field(
40 doc=
"Find and mask out cosmic rays?",
43 cosmicray = pexConfig.ConfigField(
44 dtype=measAlg.FindCosmicRaysConfig,
45 doc=
"Options for finding and masking cosmic rays",
47 interp = pexConfig.ConfigurableField(
48 target=InterpImageTask,
49 doc=
"Interpolate over bad image pixels",
53 self.
interp.useFallbackValueAtEdge =
True 54 self.
interp.fallbackValueType =
"MEANCLIP" 55 self.
interp.negativeFallbackAllowed =
True 69 @brief Interpolate over defects in an exposure and handle cosmic rays 71 @section pipe_tasks_repair_Contents Contents 73 - @ref pipe_tasks_repair_Purpose 74 - @ref pipe_tasks_repair_Initialize 75 - @ref pipe_tasks_repair_IO 76 - @ref pipe_tasks_repair_Config 77 - @ref pipe_tasks_repair_Debug 78 - @ref pipe_tasks_repair_Example 80 @section pipe_tasks_repair_Purpose Description 84 This task operates on an lsst.afw.image.Exposure in place to interpolate over a set of 85 lsst.meas.algorithms.Defect objects. 86 It will also, optionally, find and interpolate any cosmic rays in the lsst.afw.image.Exposure. 88 @section pipe_tasks_repair_Initialize Task initialization 90 See: lsst.pipe.base.task.Task.__init__ 92 @section pipe_tasks_repair_IO Inputs/Outputs to the run method 96 @section pipe_tasks_repair_Config Configuration parameters 100 @section pipe_tasks_repair_Debug Debug variables 102 The @link lsst.pipe.base.cmdLineTask.CmdLineTask command line task@endlink interface supports a 103 flag @c -d to import @b debug.py from your @c PYTHONPATH; see <a 104 href="http://lsst-web.ncsa.illinois.edu/~buildbot/doxygen/x_masterDoxyDoc/base_debug.html"> 105 Using lsstDebug to control debugging output</a> for more about @b debug.py files. 107 The available variables in RepairTask are: 110 <DD> A dictionary containing debug point names as keys with frame number as value. Valid keys are: 113 <DD> display image before any repair is done 115 <DD> display image after cosmic ray and defect correction 118 <DD> If True, display the exposure on ds9's frame 1 and overlay bounding boxes around detects CRs. 120 @section pipe_tasks_repair_Example A complete example of using RepairTask 122 This code is in runRepair.py in the examples directory, and can be run as @em e.g. 124 examples/runRepair.py 126 @dontinclude runRepair.py 127 Import the task. There are other imports. Read the source file for more info. 130 For this example, we manufacture a test image to run on. 132 First, create a pure Poisson noise image and a Psf to go with it. The mask plane 133 and variance can be constructed at the same time. 137 Inject some cosmic rays and generate the Exposure. Exposures are MaskedImages (image + mask + variance) 138 with other metadata (e.g. Psf and Wcs objects). 142 Defects are represented as bad columns of random lengths. A defect list must be constructed to pass 143 on to the RepairTask. 144 @bug This is addressed in <a href="https://jira.lsstcorp.org/browse/DM-963"> DM-963</a> 149 Finally, the exposure can be repaired. Create an instance of the task and run it. The exposure 150 is modified in place. 155 To investigate the @ref pipe_tasks_repair_Debug, put something like 159 di = lsstDebug.getInfo(name) # N.b. lsstDebug.Info(name) would call us recursively 160 if name == "lsst.pipe.tasks.repair": 161 di.display = {'repair.before':2, 'repair.after':3} 165 lsstDebug.Info = DebugInfo 167 into your debug.py file and run runRepair.py with the @c --debug flag. 171 Display code should be updated once we settle on a standard way of controlling what is displayed. 173 ConfigClass = RepairConfig
174 _DefaultName =
"repair" 177 pipeBase.Task.__init__(self, **kwargs)
178 if self.config.doInterpolate:
179 self.makeSubtask(
"interp")
182 def run(self, exposure, defects=None, keepCRs=None):
183 """!Repair an Exposure's defects and cosmic rays 185 @param[in, out] exposure lsst.afw.image.Exposure to process. Exposure must have a valid Psf. 187 @param[in] defects an lsst.meas.algorithms.DefectListT object. If None, do no 189 @param[in] keepCRs don't interpolate over the CR pixels (defer to RepairConfig if None) 191 @throws AssertionError with the following strings: 194 <DT> No exposure provided 195 <DD> The object provided as exposure evaluates to False 197 <DD> The Exposure has no associated Psf 200 assert exposure,
"No exposure provided" 201 psf = exposure.getPsf()
202 assert psf,
"No PSF provided" 208 if defects
is not None and self.config.doInterpolate:
209 self.interp.
run(exposure, defects=defects)
211 if self.config.doCosmicRay:
212 self.
cosmicRay(exposure, keepCRs=keepCRs)
221 @param[in,out] exposure Exposure to process 222 @param[in] keepCRs Don't interpolate over the CR pixels (defer to pex_config if None) 228 assert exposure,
"No exposure provided" 229 psf = exposure.getPsf()
230 assert psf,
"No psf provided" 234 mask = exposure.getMaskedImage().getMask()
235 crBit = mask.getMaskPlane(
"CR")
236 mask.clearMaskPlane(crBit)
241 binSize = self.config.cosmicray.background.binSize
242 nx, ny = exposure.getWidth()/binSize, exposure.getHeight()/binSize
252 exposure = exposure.Factory(exposure,
True)
253 subtractBackgroundTask = measAlg.SubtractBackgroundTask(config=self.config.cosmicray.background)
254 modelBg = subtractBackgroundTask.run(exposure).background
258 keepCRs = self.config.cosmicray.keepCRs
260 crs = measAlg.findCosmicRays(exposure.getMaskedImage(), psf, medianBg,
261 pexConfig.makePolicy(self.config.cosmicray), keepCRs)
264 img = exposure.getMaskedImage()
265 img += modelBg.getImageF()
268 exposure0.setMaskedImage(exposure.getMaskedImage())
273 ds9.mtv(exposure0, title=
"Failed CR")
278 mask = exposure0.getMaskedImage().getMask()
279 crBit = mask.getPlaneBitMask(
"CR")
280 afwDet.setMaskFromFootprintList(mask, crs, crBit)
283 if display
and displayCR:
287 ds9.incrDefaultFrame()
288 ds9.mtv(exposure0, title=
"Post-CR")
290 with ds9.Buffering():
292 displayUtils.drawBBox(cr.getBBox(), borderWidth=0.55)
294 self.log.
info(
"Identified %s cosmic rays." % (num,))
Fit spatial kernel using approximate fluxes for candidates, and solving a linear system of equations...
Statistics makeStatistics(lsst::afw::math::MaskedVector< EntryT > const &mv, std::vector< WeightPixel > const &vweights, int const flags, StatisticsControl const &sctrl=StatisticsControl())
The makeStatistics() overload to handle lsst::afw::math::MaskedVector<>
def run(self, exposure, defects=None, keepCRs=None)
Repair an Exposure's defects and cosmic rays.
def __init__(self, kwargs)
def cosmicRay(self, exposure, keepCRs=None)
def mtv(data, frame=None, title="", wcs=None, args, kwargs)
def getDebugFrame(debugDisplay, name)
Interpolate over defects in an exposure and handle cosmic rays.