AlardLuptonSubtractTask¶
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class
lsst.ip.diffim.AlardLuptonSubtractTask(**kwargs)¶ Bases:
lsst.pipe.base.PipelineTaskCompute the image difference of a science and template image using the Alard & Lupton (1998) algorithm.
Attributes Summary
canMultiprocessMethods Summary
emptyMetadata()Empty (clear) the metadata for this Task and all sub-Tasks. finalize(template, science, difference, kernel)Decorrelate the difference image to undo the noise correlations caused by convolution. getAllSchemaCatalogs()Get schema catalogs for all tasks in the hierarchy, combining the results into a single dict. getFullMetadata()Get metadata for all tasks. getFullName()Get the task name as a hierarchical name including parent task names. getName()Get the name of the task. getResourceConfig()Return resource configuration for this task. getSchemaCatalogs()Get the schemas generated by this task. getTaskDict()Get a dictionary of all tasks as a shallow copy. makeField(doc)Make a lsst.pex.config.ConfigurableFieldfor this task.makeSubtask(name, **keyArgs)Create a subtask as a new instance as the nameattribute of this task.run(template, science, sources[, …])PSF match, subtract, and decorrelate two images. runConvolveScience(template, science, sources)Convolve the science image with a PSF-matching kernel and subtract the template image. runConvolveTemplate(template, science, sources)Convolve the template image with a PSF-matching kernel and subtract from the science image. runQuantum(butlerQC, inputRefs, outputRefs)Method to do butler IO and or transforms to provide in memory objects for tasks run method timer(name, logLevel)Context manager to log performance data for an arbitrary block of code. Attributes Documentation
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canMultiprocess= True¶
Methods Documentation
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emptyMetadata() → None¶ Empty (clear) the metadata for this Task and all sub-Tasks.
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finalize(template, science, difference, kernel, templateMatched=True, preConvMode=False, preConvKernel=None, spatiallyVarying=False)¶ Decorrelate the difference image to undo the noise correlations caused by convolution.
Parameters: - template :
lsst.afw.image.ExposureF Template exposure, warped to match the science exposure.
- science :
lsst.afw.image.ExposureF Science exposure to subtract from the template.
- difference :
lsst.afw.image.ExposureF Result of subtracting template and science.
- kernel :
lsst.afw.math.Kernel An (optionally spatially-varying) PSF matching kernel
- templateMatched :
bool, optional Was the template PSF-matched to the science image?
- preConvMode :
bool, optional Was the science image preconvolved with its own PSF before PSF matching the template?
- preConvKernel :
lsst.afw.detection.Psf, optional If not
None, then the science image was pre-convolved with (the reflection of) this kernel. Must be normalized to sum to 1.- spatiallyVarying :
bool, optional Compute the decorrelation kernel spatially varying across the image?
Returns: - correctedExposure :
lsst.afw.image.ExposureF The decorrelated image difference.
- template :
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getAllSchemaCatalogs() → Dict[str, Any]¶ Get schema catalogs for all tasks in the hierarchy, combining the results into a single dict.
Returns: - schemacatalogs :
dict Keys are butler dataset type, values are a empty catalog (an instance of the appropriate
lsst.afw.tableCatalog type) for all tasks in the hierarchy, from the top-level task down through all subtasks.
Notes
This method may be called on any task in the hierarchy; it will return the same answer, regardless.
The default implementation should always suffice. If your subtask uses schemas the override
Task.getSchemaCatalogs, not this method.- schemacatalogs :
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getFullMetadata() → lsst.pipe.base._task_metadata.TaskMetadata¶ Get metadata for all tasks.
Returns: - metadata :
TaskMetadata The keys are the full task name. Values are metadata for the top-level task and all subtasks, sub-subtasks, etc.
Notes
The returned metadata includes timing information (if
@timer.timeMethodis used) and any metadata set by the task. The name of each item consists of the full task name with.replaced by:, followed by.and the name of the item, e.g.:topLevelTaskName:subtaskName:subsubtaskName.itemName
using
:in the full task name disambiguates the rare situation that a task has a subtask and a metadata item with the same name.- metadata :
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getFullName() → str¶ Get the task name as a hierarchical name including parent task names.
Returns: - fullName :
str The full name consists of the name of the parent task and each subtask separated by periods. For example:
- The full name of top-level task “top” is simply “top”.
- The full name of subtask “sub” of top-level task “top” is “top.sub”.
- The full name of subtask “sub2” of subtask “sub” of top-level task “top” is “top.sub.sub2”.
- fullName :
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getResourceConfig() → Optional[ResourceConfig]¶ Return resource configuration for this task.
Returns: - Object of type
ResourceConfigorNoneif resource - configuration is not defined for this task.
- Object of type
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getSchemaCatalogs() → Dict[str, Any]¶ Get the schemas generated by this task.
Returns: - schemaCatalogs :
dict Keys are butler dataset type, values are an empty catalog (an instance of the appropriate
lsst.afw.tableCatalog type) for this task.
See also
Task.getAllSchemaCatalogs
Notes
Warning
Subclasses that use schemas must override this method. The default implementation returns an empty dict.
This method may be called at any time after the Task is constructed, which means that all task schemas should be computed at construction time, not when data is actually processed. This reflects the philosophy that the schema should not depend on the data.
Returning catalogs rather than just schemas allows us to save e.g. slots for SourceCatalog as well.
- schemaCatalogs :
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getTaskDict() → Dict[str, weakref]¶ Get a dictionary of all tasks as a shallow copy.
Returns: - taskDict :
dict Dictionary containing full task name: task object for the top-level task and all subtasks, sub-subtasks, etc.
- taskDict :
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classmethod
makeField(doc: str) → lsst.pex.config.configurableField.ConfigurableField¶ Make a
lsst.pex.config.ConfigurableFieldfor this task.Parameters: - doc :
str Help text for the field.
Returns: - configurableField :
lsst.pex.config.ConfigurableField A
ConfigurableFieldfor this task.
Examples
Provides a convenient way to specify this task is a subtask of another task.
Here is an example of use:
class OtherTaskConfig(lsst.pex.config.Config): aSubtask = ATaskClass.makeField("brief description of task")
- doc :
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makeSubtask(name: str, **keyArgs) → None¶ Create a subtask as a new instance as the
nameattribute of this task.Parameters: - name :
str Brief name of the subtask.
- keyArgs
Extra keyword arguments used to construct the task. The following arguments are automatically provided and cannot be overridden:
- “config”.
- “parentTask”.
Notes
The subtask must be defined by
Task.config.name, an instance ofConfigurableFieldorRegistryField.- name :
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run(template, science, sources, finalizedPsfApCorrCatalog=None)¶ PSF match, subtract, and decorrelate two images.
Parameters: - template :
lsst.afw.image.ExposureF Template exposure, warped to match the science exposure.
- science :
lsst.afw.image.ExposureF Science exposure to subtract from the template.
- sources :
lsst.afw.table.SourceCatalog Identified sources on the science exposure. This catalog is used to select sources in order to perform the AL PSF matching on stamp images around them.
- finalizedPsfApCorrCatalog :
lsst.afw.table.ExposureCatalog, optional Exposure catalog with finalized psf models and aperture correction maps to be applied if config.doApplyFinalizedPsf=True. Catalog uses the detector id for the catalog id, sorted on id for fast lookup.
Returns: - results :
lsst.pipe.base.Struct difference:lsst.afw.image.ExposureFResult of subtracting template and science.
matchedTemplate:lsst.afw.image.ExposureFWarped and PSF-matched template exposure.
backgroundModel:lsst.afw.math.Function2DBackground model that was fit while solving for the PSF-matching kernel
psfMatchingKernel:lsst.afw.math.KernelKernel used to PSF-match the convolved image.
Raises: - RuntimeError
If an unsupported convolution mode is supplied.
- lsst.pipe.base.NoWorkFound
Raised if fraction of good pixels, defined as not having NO_DATA set, is less then the configured requiredTemplateFraction
- template :
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runConvolveScience(template, science, sources)¶ Convolve the science image with a PSF-matching kernel and subtract the template image.
Parameters: - template :
lsst.afw.image.ExposureF Template exposure, warped to match the science exposure.
- science :
lsst.afw.image.ExposureF Science exposure to subtract from the template.
- sources :
lsst.afw.table.SourceCatalog Identified sources on the science exposure. This catalog is used to select sources in order to perform the AL PSF matching on stamp images around them.
Returns: - results :
lsst.pipe.base.Struct difference:lsst.afw.image.ExposureFResult of subtracting template and science.
matchedTemplate:lsst.afw.image.ExposureFWarped template exposure. Note that in this case, the template is not PSF-matched to the science image.
backgroundModel:lsst.afw.math.Function2DBackground model that was fit while solving for the PSF-matching kernel
psfMatchingKernel:lsst.afw.math.KernelKernel used to PSF-match the science image to the template.
- template :
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runConvolveTemplate(template, science, sources)¶ Convolve the template image with a PSF-matching kernel and subtract from the science image.
Parameters: - template :
lsst.afw.image.ExposureF Template exposure, warped to match the science exposure.
- science :
lsst.afw.image.ExposureF Science exposure to subtract from the template.
- sources :
lsst.afw.table.SourceCatalog Identified sources on the science exposure. This catalog is used to select sources in order to perform the AL PSF matching on stamp images around them.
Returns: - results :
lsst.pipe.base.Struct difference:lsst.afw.image.ExposureFResult of subtracting template and science.
matchedTemplate:lsst.afw.image.ExposureFWarped and PSF-matched template exposure.
backgroundModel:lsst.afw.math.Function2DBackground model that was fit while solving for the PSF-matching kernel
psfMatchingKernel:lsst.afw.math.KernelKernel used to PSF-match the template to the science image.
- template :
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runQuantum(butlerQC: lsst.pipe.base.butlerQuantumContext.ButlerQuantumContext, inputRefs: lsst.pipe.base.connections.InputQuantizedConnection, outputRefs: lsst.pipe.base.connections.OutputQuantizedConnection) → None¶ Method to do butler IO and or transforms to provide in memory objects for tasks run method
Parameters: - butlerQC :
ButlerQuantumContext A butler which is specialized to operate in the context of a
lsst.daf.butler.Quantum.- inputRefs :
InputQuantizedConnection Datastructure whose attribute names are the names that identify connections defined in corresponding
PipelineTaskConnectionsclass. The values of these attributes are thelsst.daf.butler.DatasetRefobjects associated with the defined input/prerequisite connections.- outputRefs :
OutputQuantizedConnection Datastructure whose attribute names are the names that identify connections defined in corresponding
PipelineTaskConnectionsclass. The values of these attributes are thelsst.daf.butler.DatasetRefobjects associated with the defined output connections.
- butlerQC :
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timer(name: str, logLevel: int = 10) → Iterator[None]¶ Context manager to log performance data for an arbitrary block of code.
Parameters: See also
timer.logInfo
Examples
Creating a timer context:
with self.timer("someCodeToTime"): pass # code to time
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