LSST Applications 27.0.0,g0265f82a02+469cd937ee,g02d81e74bb+21ad69e7e1,g1470d8bcf6+cbe83ee85a,g2079a07aa2+e67c6346a6,g212a7c68fe+04a9158687,g2305ad1205+94392ce272,g295015adf3+81dd352a9d,g2bbee38e9b+469cd937ee,g337abbeb29+469cd937ee,g3939d97d7f+72a9f7b576,g487adcacf7+71499e7cba,g50ff169b8f+5929b3527e,g52b1c1532d+a6fc98d2e7,g591dd9f2cf+df404f777f,g5a732f18d5+be83d3ecdb,g64a986408d+21ad69e7e1,g858d7b2824+21ad69e7e1,g8a8a8dda67+a6fc98d2e7,g99cad8db69+f62e5b0af5,g9ddcbc5298+d4bad12328,ga1e77700b3+9c366c4306,ga8c6da7877+71e4819109,gb0e22166c9+25ba2f69a1,gb6a65358fc+469cd937ee,gbb8dafda3b+69d3c0e320,gc07e1c2157+a98bf949bb,gc120e1dc64+615ec43309,gc28159a63d+469cd937ee,gcf0d15dbbd+72a9f7b576,gdaeeff99f8+a38ce5ea23,ge6526c86ff+3a7c1ac5f1,ge79ae78c31+469cd937ee,gee10cc3b42+a6fc98d2e7,gf1cff7945b+21ad69e7e1,gfbcc870c63+9a11dc8c8f
LSST Data Management Base Package
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Public Member Functions | |
__init__ (self, schema=None, **kwds) | |
run (self, table, exposure, doSmooth=True, sigma=None, clearMask=True, expId=None, background=None) | |
display (self, exposure, results, convolvedImage=None) | |
applyTempLocalBackground (self, exposure, middle, results) | |
clearMask (self, mask) | |
calculateKernelSize (self, sigma) | |
getPsf (self, exposure, sigma=None) | |
convolveImage (self, maskedImage, psf, doSmooth=True) | |
applyThreshold (self, middle, bbox, factor=1.0, factorNeg=None) | |
finalizeFootprints (self, mask, results, sigma, factor=1.0, factorNeg=None) | |
reEstimateBackground (self, maskedImage, backgrounds) | |
clearUnwantedResults (self, mask, results) | |
detectFootprints (self, exposure, doSmooth=True, sigma=None, clearMask=True, expId=None, background=None) | |
removeBadPixels (self, middle) | |
setPeakSignificance (self, exposure, footprints, threshold, negative=False) | |
makeThreshold (self, image, thresholdParity, factor=1.0) | |
updatePeaks (self, fpSet, image, threshold) | |
tempWideBackgroundContext (self, exposure) | |
Static Public Member Functions | |
setEdgeBits (maskedImage, goodBBox, edgeBitmask) | |
Public Attributes | |
negativeFlagKey | |
Static Public Attributes | |
ConfigClass = SourceDetectionConfig | |
Static Protected Attributes | |
str | _DefaultName = "sourceDetection" |
Detect peaks and footprints of sources in an image. This task expects the image to have been background subtracted first. Running detection on images with a non-zero-centered background may result in a single source detected on the entire image containing thousands of peaks, or other pathological outputs. Parameters ---------- schema : `lsst.afw.table.Schema` Schema object used to create the output `lsst.afw.table.SourceCatalog` **kwds Keyword arguments passed to `lsst.pipe.base.Task.__init__` If schema is not None and configured for 'both' detections, a 'flags.negative' field will be added to label detections made with a negative threshold. Notes ----- This task convolves the image with a Gaussian approximation to the PSF, matched to the sigma of the input exposure, because this is separable and fast. The PSF would have to be very non-Gaussian or non-circular for this approximation to have a significant impact on the signal-to-noise of the detected sources.
Definition at line 170 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.__init__ | ( | self, | |
schema = None, | |||
** | kwds ) |
Reimplemented in lsst.meas.algorithms.dynamicDetection.DynamicDetectionTask.
Definition at line 200 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.applyTempLocalBackground | ( | self, | |
exposure, | |||
middle, | |||
results ) |
Apply a temporary local background subtraction This temporary local background serves to suppress noise fluctuations in the wings of bright objects. Peaks in the footprints will be updated. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure for which to fit local background. middle : `lsst.afw.image.MaskedImage` Convolved image on which detection will be performed (typically smaller than ``exposure`` because the half-kernel has been removed around the edges). results : `lsst.pipe.base.Struct` Results of the 'detectFootprints' method, containing positive and negative footprints (which contain the peak positions that we will plot). This is a `Struct` with ``positive`` and ``negative`` elements that are of type `lsst.afw.detection.FootprintSet`.
Definition at line 360 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.applyThreshold | ( | self, | |
middle, | |||
bbox, | |||
factor = 1.0, | |||
factorNeg = None ) |
Apply thresholds to the convolved image Identifies `~lsst.afw.detection.Footprint`\s, both positive and negative. The threshold can be modified by the provided multiplication ``factor``. Parameters ---------- middle : `lsst.afw.image.MaskedImage` Convolved image to threshold. bbox : `lsst.geom.Box2I` Bounding box of unconvolved image. factor : `float` Multiplier for the configured threshold. factorNeg : `float` or `None` Multiplier for the configured threshold for negative detection polarity. If `None`, will be set equal to ``factor`` (i.e. equal to the factor used for positive detection polarity). Returns ------- results : `lsst.pipe.base.Struct` The `~lsst.pipe.base.Struct` contains: ``positive`` Positive detection footprints, if configured. (`lsst.afw.detection.FootprintSet` or `None`) ``negative`` Negative detection footprints, if configured. (`lsst.afw.detection.FootprintSet` or `None`) ``factor`` Multiplier for the configured threshold. (`float`) ``factorNeg`` Multiplier for the configured threshold for negative detection polarity. (`float`)
Definition at line 525 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.calculateKernelSize | ( | self, | |
sigma ) |
Calculate the size of the smoothing kernel. Uses the ``nSigmaForKernel`` configuration parameter. Note that that is the full width of the kernel bounding box (so a value of 7 means 3.5 sigma on either side of center). The value will be rounded up to the nearest odd integer. Parameters ---------- sigma : `float` Gaussian sigma of smoothing kernel. Returns ------- size : `int` Size of the smoothing kernel.
Definition at line 409 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.clearMask | ( | self, | |
mask ) |
Clear the DETECTED and DETECTED_NEGATIVE mask planes. Removes any previous detection mask in preparation for a new detection pass. Parameters ---------- mask : `lsst.afw.image.Mask` Mask to be cleared.
Definition at line 396 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.clearUnwantedResults | ( | self, | |
mask, | |||
results ) |
Clear unwanted results from the Struct of results If we specifically want only positive or only negative detections, drop the ones we don't want, and its associated mask plane. Parameters ---------- mask : `lsst.afw.image.Mask` Mask image. results : `lsst.pipe.base.Struct` Detection results, with ``positive`` and ``negative`` elements; modified.
Definition at line 690 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.convolveImage | ( | self, | |
maskedImage, | |||
psf, | |||
doSmooth = True ) |
Convolve the image with the PSF. We convolve the image with a Gaussian approximation to the PSF, because this is separable and therefore fast. It's technically a correlation rather than a convolution, but since we use a symmetric Gaussian there's no difference. The convolution can be disabled with ``doSmooth=False``. If we do convolve, we mask the edges as ``EDGE`` and return the convolved image with the edges removed. This is because we can't convolve the edges because the kernel would extend off the image. Parameters ---------- maskedImage : `lsst.afw.image.MaskedImage` Image to convolve. psf : `lsst.afw.detection.Psf` PSF to convolve with (actually with a Gaussian approximation to it). doSmooth : `bool` Actually do the convolution? Set to False when running on e.g. a pre-convolved image, or a mask plane. Returns ------- results : `lsst.pipe.base.Struct` The `~lsst.pipe.base.Struct` contains: ``middle`` Convolved image, without the edges. (`lsst.afw.image.MaskedImage`) ``sigma`` Gaussian sigma used for the convolution. (`float`)
Definition at line 463 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.detectFootprints | ( | self, | |
exposure, | |||
doSmooth = True, | |||
sigma = None, | |||
clearMask = True, | |||
expId = None, | |||
background = None ) |
Detect footprints on an exposure. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure to process; DETECTED{,_NEGATIVE} mask plane will be set in-place. doSmooth : `bool`, optional If True, smooth the image before detection using a Gaussian of width ``sigma``, or the measured PSF width of ``exposure``. Set to False when running on e.g. a pre-convolved image, or a mask plane. sigma : `float`, optional Gaussian Sigma of PSF (pixels); used for smoothing and to grow detections; if `None` then measure the sigma of the PSF of the ``exposure``. clearMask : `bool`, optional Clear both DETECTED and DETECTED_NEGATIVE planes before running detection. expId : `dict`, optional Exposure identifier; unused by this implementation, but used for RNG seed by subclasses. background : `lsst.afw.math.BackgroundList`, optional Background that was already subtracted from the exposure; will be modified in-place if ``reEstimateBackground=True``. Returns ------- results : `lsst.pipe.base.Struct` A `~lsst.pipe.base.Struct` containing: ``positive`` Positive polarity footprints. (`lsst.afw.detection.FootprintSet` or `None`) ``negative`` Negative polarity footprints. (`lsst.afw.detection.FootprintSet` or `None`) ``numPos`` Number of footprints in positive or 0 if detection polarity was negative. (`int`) ``numNeg`` Number of footprints in negative or 0 if detection polarity was positive. (`int`) ``background`` Re-estimated background. `None` or the input ``background`` if ``reEstimateBackground==False``. (`lsst.afw.math.BackgroundList`) ``factor`` Multiplication factor applied to the configured detection threshold. (`float`)
Reimplemented in lsst.meas.algorithms.dynamicDetection.DynamicDetectionTask.
Definition at line 714 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.display | ( | self, | |
exposure, | |||
results, | |||
convolvedImage = None ) |
Display detections if so configured Displays the ``exposure`` in frame 0, overlays the detection peaks. Requires that ``lsstDebug`` has been set up correctly, so that ``lsstDebug.Info("lsst.meas.algorithms.detection")`` evaluates `True`. If the ``convolvedImage`` is non-`None` and ``lsstDebug.Info("lsst.meas.algorithms.detection") > 1``, the ``convolvedImage`` will be displayed in frame 1. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure to display, on which will be plotted the detections. results : `lsst.pipe.base.Struct` Results of the 'detectFootprints' method, containing positive and negative footprints (which contain the peak positions that we will plot). This is a `Struct` with ``positive`` and ``negative`` elements that are of type `lsst.afw.detection.FootprintSet`. convolvedImage : `lsst.afw.image.Image`, optional Convolved image used for thresholding.
Definition at line 303 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.finalizeFootprints | ( | self, | |
mask, | |||
results, | |||
sigma, | |||
factor = 1.0, | |||
factorNeg = None ) |
Finalize the detected footprints. Grow the footprints, set the ``DETECTED`` and ``DETECTED_NEGATIVE`` mask planes, and log the results. ``numPos`` (number of positive footprints), ``numPosPeaks`` (number of positive peaks), ``numNeg`` (number of negative footprints), ``numNegPeaks`` (number of negative peaks) entries are added to the ``results`` struct. Parameters ---------- mask : `lsst.afw.image.Mask` Mask image on which to flag detected pixels. results : `lsst.pipe.base.Struct` Struct of detection results, including ``positive`` and ``negative`` entries; modified. sigma : `float` Gaussian sigma of PSF. factor : `float` Multiplier for the configured threshold. Note that this is only used here for logging purposes. factorNeg : `float` or `None` Multiplier used for the negative detection polarity threshold. If `None`, a factor equal to ``factor`` (i.e. equal to the one used for positive detection polarity) is assumed. Note that this is only used here for logging purposes.
Definition at line 591 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.getPsf | ( | self, | |
exposure, | |||
sigma = None ) |
Create a single Gaussian PSF for an exposure. If ``sigma`` is provided, we make a `~lsst.afw.detection.GaussianPsf` with that, otherwise use the sigma from the psf of the ``exposure`` to make the `~lsst.afw.detection.GaussianPsf`. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure from which to retrieve the PSF. sigma : `float`, optional Gaussian sigma to use if provided. Returns ------- psf : `lsst.afw.detection.GaussianPsf` PSF to use for detection. Raises ------ RuntimeError Raised if ``sigma`` is not provided and ``exposure`` does not contain a ``Psf`` object.
Definition at line 429 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.makeThreshold | ( | self, | |
image, | |||
thresholdParity, | |||
factor = 1.0 ) |
Make an afw.detection.Threshold object corresponding to the task's configuration and the statistics of the given image. Parameters ---------- image : `afw.image.MaskedImage` Image to measure noise statistics from if needed. thresholdParity: `str` One of "positive" or "negative", to set the kind of fluctuations the Threshold will detect. factor : `float` Factor by which to multiply the configured detection threshold. This is useful for tweaking the detection threshold slightly. Returns ------- threshold : `lsst.afw.detection.Threshold` Detection threshold.
Definition at line 870 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.reEstimateBackground | ( | self, | |
maskedImage, | |||
backgrounds ) |
Estimate the background after detection Parameters ---------- maskedImage : `lsst.afw.image.MaskedImage` Image on which to estimate the background. backgrounds : `lsst.afw.math.BackgroundList` List of backgrounds; modified. Returns ------- bg : `lsst.afw.math.backgroundMI` Empirical background model.
Definition at line 661 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.removeBadPixels | ( | self, | |
middle ) |
Set the significance of flagged pixels to zero. Parameters ---------- middle : `lsst.afw.image.ExposureF` Score or maximum likelihood difference image. The image plane will be modified in place.
Definition at line 802 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.run | ( | self, | |
table, | |||
exposure, | |||
doSmooth = True, | |||
sigma = None, | |||
clearMask = True, | |||
expId = None, | |||
background = None ) |
Detect sources and return catalog(s) of detections. Parameters ---------- table : `lsst.afw.table.SourceTable` Table object that will be used to create the SourceCatalog. exposure : `lsst.afw.image.Exposure` Exposure to process; DETECTED mask plane will be set in-place. doSmooth : `bool`, optional If True, smooth the image before detection using a Gaussian of width ``sigma``, or the measured PSF width. Set to False when running on e.g. a pre-convolved image, or a mask plane. sigma : `float`, optional Sigma of PSF (pixels); used for smoothing and to grow detections; if None then measure the sigma of the PSF of the exposure clearMask : `bool`, optional Clear DETECTED{,_NEGATIVE} planes before running detection. expId : `int`, optional Exposure identifier; unused by this implementation, but used for RNG seed by subclasses. background : `lsst.afw.math.BackgroundList`, optional Background that was already subtracted from the exposure; will be modified in-place if ``reEstimateBackground=True``. Returns ------- result : `lsst.pipe.base.Struct` The `~lsst.pipe.base.Struct` contains: ``sources`` Detected sources on the exposure. (`lsst.afw.table.SourceCatalog`) ``positive`` Positive polarity footprints. (`lsst.afw.detection.FootprintSet` or `None`) ``negative`` Negative polarity footprints. (`lsst.afw.detection.FootprintSet` or `None`) ``numPos`` Number of footprints in positive or 0 if detection polarity was negative. (`int`) ``numNeg`` Number of footprints in negative or 0 if detection polarity was positive. (`int`) ``background`` Re-estimated background. `None` if ``reEstimateBackground==False``. (`lsst.afw.math.BackgroundList`) ``factor`` Multiplication factor applied to the configured detection threshold. (`float`) Raises ------ ValueError Raised if flags.negative is needed, but isn't in table's schema. lsst.pipe.base.TaskError Raised if sigma=None, doSmooth=True and the exposure has no PSF. Notes ----- If you want to avoid dealing with Sources and Tables, you can use `detectFootprints()` to just get the `~lsst.afw.detection.FootprintSet`\s.
Definition at line 220 of file detection.py.
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static |
Set the edgeBitmask bits for all of maskedImage outside goodBBox Parameters ---------- maskedImage : `lsst.afw.image.MaskedImage` Image on which to set edge bits in the mask. goodBBox : `lsst.geom.Box2I` Bounding box of good pixels, in ``LOCAL`` coordinates. edgeBitmask : `lsst.afw.image.MaskPixel` Bit mask to OR with the existing mask bits in the region outside ``goodBBox``.
Definition at line 949 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.setPeakSignificance | ( | self, | |
exposure, | |||
footprints, | |||
threshold, | |||
negative = False ) |
Set the significance of each detected peak to the pixel value divided by the appropriate standard-deviation for ``config.thresholdType``. Only sets significance for "stdev" and "pixel_stdev" thresholdTypes; we leave it undefined for "value" and "variance" as it does not have a well-defined meaning in those cases. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure that footprints were detected on, likely the convolved, local background-subtracted image. footprints : `lsst.afw.detection.FootprintSet` Footprints detected on the image. threshold : `lsst.afw.detection.Threshold` Threshold used to find footprints. negative : `bool`, optional Are we calculating for negative sources?
Definition at line 815 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.tempWideBackgroundContext | ( | self, | |
exposure ) |
Context manager for removing wide (large-scale) background Removing a wide (large-scale) background helps to suppress the detection of large footprints that may overwhelm the deblender. It does, however, set a limit on the maximum scale of objects. The background that we remove will be restored upon exit from the context manager. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure on which to remove large-scale background. Returns ------- context : context manager Context manager that will ensure the temporary wide background is restored.
Definition at line 979 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.updatePeaks | ( | self, | |
fpSet, | |||
image, | |||
threshold ) |
Update the Peaks in a FootprintSet by detecting new Footprints and Peaks in an image and using the new Peaks instead of the old ones. Parameters ---------- fpSet : `afw.detection.FootprintSet` Set of Footprints whose Peaks should be updated. image : `afw.image.MaskedImage` Image to detect new Footprints and Peak in. threshold : `afw.detection.Threshold` Threshold object for detection. Input Footprints with fewer Peaks than self.config.nPeaksMaxSimple are not modified, and if no new Peaks are detected in an input Footprint, the brightest original Peak in that Footprint is kept.
Definition at line 906 of file detection.py.
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staticprotected |
Definition at line 198 of file detection.py.
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static |
Definition at line 197 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.negativeFlagKey |
Definition at line 203 of file detection.py.