lsst.pipe.tasks g147c7b1cba+d8ec0ec89a
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Public Member Functions | |
def | __init__ (self, *args, **kwargs) |
def | run (self, skyInfo, tempExpRefList, imageScalerList, weightList, supplementaryData) |
def | applyAltEdgeMask (self, mask, altMaskList) |
def | findArtifacts (self, templateCoadd, tempExpRefList, imageScalerList) |
def | prefilterArtifacts (self, spanSetList, exp) |
def | filterArtifacts (self, spanSetList, epochCountImage, nImage, footprintsToExclude=None) |
Static Public Attributes | |
ConfigClass = CompareWarpAssembleCoaddConfig | |
Assemble a compareWarp coadded image from a set of warps by masking artifacts detected by comparing PSF-matched warps. In ``AssembleCoaddTask``, we compute the coadd as an clipped mean (i.e., we clip outliers). The problem with doing this is that when computing the coadd PSF at a given location, individual visit PSFs from visits with outlier pixels contribute to the coadd PSF and cannot be treated correctly. In this task, we correct for this behavior by creating a new badMaskPlane 'CLIPPED' which marks pixels in the individual warps suspected to contain an artifact. We populate this plane on the input warps by comparing PSF-matched warps with a PSF-matched median coadd which serves as a model of the static sky. Any group of pixels that deviates from the PSF-matched template coadd by more than config.detect.threshold sigma, is an artifact candidate. The candidates are then filtered to remove variable sources and sources that are difficult to subtract such as bright stars. This filter is configured using the config parameters ``temporalThreshold`` and ``spatialThreshold``. The temporalThreshold is the maximum fraction of epochs that the deviation can appear in and still be considered an artifact. The spatialThreshold is the maximum fraction of pixels in the footprint of the deviation that appear in other epochs (where other epochs is defined by the temporalThreshold). If the deviant region meets this criteria of having a significant percentage of pixels that deviate in only a few epochs, these pixels have the 'CLIPPED' bit set in the mask. These regions will not contribute to the final coadd. Furthermore, any routine to determine the coadd PSF can now be cognizant of clipped regions. Note that the algorithm implemented by this task is preliminary and works correctly for HSC data. Parameter modifications and or considerable redesigning of the algorithm is likley required for other surveys. ``CompareWarpAssembleCoaddTask`` sub-classes ``AssembleCoaddTask`` and instantiates ``AssembleCoaddTask`` as a subtask to generate the TemplateCoadd (the model of the static sky). Notes ----- Debugging: This task supports the following debug variables: - ``saveCountIm`` If True then save the Epoch Count Image as a fits file in the `figPath` - ``figPath`` Path to save the debug fits images and figures
Definition at line 1375 of file assembleCoadd.py.
def lsst.pipe.tasks.assembleCoadd.CompareWarpAssembleCoaddTask.__init__ | ( | self, | |
* | args, | ||
** | kwargs | ||
) |
Reimplemented from lsst.pipe.tasks.assembleCoadd.AssembleCoaddTask.
Definition at line 1423 of file assembleCoadd.py.
def lsst.pipe.tasks.assembleCoadd.CompareWarpAssembleCoaddTask.applyAltEdgeMask | ( | self, | |
mask, | |||
altMaskList | |||
) |
Propagate alt EDGE mask to SENSOR_EDGE AND INEXACT_PSF planes. Parameters ---------- mask : `lsst.afw.image.Mask` Original mask. altMaskList : `list` of `dict` List of Dicts containing ``spanSet`` lists. Each element contains the new mask plane name (e.g. "CLIPPED and/or "NO_DATA") as the key, and list of ``SpanSets`` to apply to the mask.
Definition at line 1540 of file assembleCoadd.py.
def lsst.pipe.tasks.assembleCoadd.CompareWarpAssembleCoaddTask.filterArtifacts | ( | self, | |
spanSetList, | |||
epochCountImage, | |||
nImage, | |||
footprintsToExclude = None |
|||
) |
Filter artifact candidates. Parameters ---------- spanSetList : `list` of `lsst.afw.geom.SpanSet` List of SpanSets representing artifact candidates. epochCountImage : `lsst.afw.image.Image` Image of accumulated number of warpDiff detections. nImage : `lsst.afw.image.ImageU` Image of the accumulated number of total epochs contributing. Returns ------- maskSpanSetList : `list` List of SpanSets with artifacts.
Definition at line 1717 of file assembleCoadd.py.
def lsst.pipe.tasks.assembleCoadd.CompareWarpAssembleCoaddTask.findArtifacts | ( | self, | |
templateCoadd, | |||
tempExpRefList, | |||
imageScalerList | |||
) |
Find artifacts. Loop through warps twice. The first loop builds a map with the count of how many epochs each pixel deviates from the templateCoadd by more than ``config.chiThreshold`` sigma. The second loop takes each difference image and filters the artifacts detected in each using count map to filter out variable sources and sources that are difficult to subtract cleanly. Parameters ---------- templateCoadd : `lsst.afw.image.Exposure` Exposure to serve as model of static sky. tempExpRefList : `list` List of data references to warps. imageScalerList : `list` List of image scalers. Returns ------- altMasks : `list` of `dict` List of dicts containing information about CLIPPED (i.e., artifacts), NO_DATA, and EDGE pixels.
Definition at line 1559 of file assembleCoadd.py.
def lsst.pipe.tasks.assembleCoadd.CompareWarpAssembleCoaddTask.prefilterArtifacts | ( | self, | |
spanSetList, | |||
exp | |||
) |
Remove artifact candidates covered by bad mask plane. Any future editing of the candidate list that does not depend on temporal information should go in this method. Parameters ---------- spanSetList : `list` of `lsst.afw.geom.SpanSet` List of SpanSets representing artifact candidates. exp : `lsst.afw.image.Exposure` Exposure containing mask planes used to prefilter. Returns ------- returnSpanSetList : `list` of `lsst.afw.geom.SpanSet` List of SpanSets with artifacts.
Definition at line 1685 of file assembleCoadd.py.
def lsst.pipe.tasks.assembleCoadd.CompareWarpAssembleCoaddTask.run | ( | self, | |
skyInfo, | |||
tempExpRefList, | |||
imageScalerList, | |||
weightList, | |||
supplementaryData | |||
) |
Assemble the coadd. Find artifacts and apply them to the warps' masks creating a list of alternative masks with a new "CLIPPED" plane and updated "NO_DATA" plane. Then pass these alternative masks to the base class's ``run`` method.
Reimplemented from lsst.pipe.tasks.assembleCoadd.AssembleCoaddTask.
Definition at line 1501 of file assembleCoadd.py.
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static |
Definition at line 1420 of file assembleCoadd.py.