AlardLuptonPreconvolveSubtractTask¶
- class lsst.ip.diffim.AlardLuptonPreconvolveSubtractTask(**kwargs)¶
- Bases: - AlardLuptonSubtractTask- Subtract a template from a science image, convolving the science image before computing the kernel, and also convolving the template before subtraction. - Attributes Summary - Methods Summary - 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. - Get metadata for all tasks. - Get the task name as a hierarchical name including parent task names. - getName()- Get the name of the task. - 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[, ...])- Preconvolve the science image with its own PSF, convolve the template image with a PSF-matching kernel and subtract from the preconvolved science image. - runConvolveScience(template, science, ...)- Convolve the science image with a PSF-matching kernel and subtract the template image. - runConvolveTemplate(template, science, ...)- Convolve the template image with a PSF-matching kernel and subtract from the science image. - runPreconvolve(template, science, ...)- Convolve the science image with its own PSF, then convolve the template with a matching kernel and subtract to form the Score exposure. - runQuantum(butlerQC, inputRefs, outputRefs)- Do butler IO and transform to provide in memory objects for tasks - runmethod.- timer(name[, logLevel])- Context manager to log performance data for an arbitrary block of code. - updateMasks(template, science)- Update the science and template mask planes before differencing. - Attributes Documentation - Methods Documentation - 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:
- templatelsst.afw.image.ExposureF
- Template exposure, warped to match the science exposure. 
- sciencelsst.afw.image.ExposureF
- Science exposure to subtract from the template. 
- differencelsst.afw.image.ExposureF
- Result of subtracting template and science. 
- kernellsst.afw.math.Kernel
- An (optionally spatially-varying) PSF matching kernel 
- templateMatchedbool, optional
- Was the template PSF-matched to the science image? 
- preConvModebool, optional
- Was the science image preconvolved with its own PSF before PSF matching the template? 
- preConvKernellsst.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.
- spatiallyVaryingbool, optional
- Compute the decorrelation kernel spatially varying across the image? 
 
- template
- Returns:
- correctedExposurelsst.afw.image.ExposureF
- The decorrelated image difference. 
 
- correctedExposure
 
 - getFullMetadata() TaskMetadata¶
- Get metadata for all tasks. - Returns:
- metadataTaskMetadata
- The keys are the full task name. Values are metadata for the top-level task and all subtasks, sub-subtasks, etc. 
 
- metadata
 - 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.
 - getFullName() str¶
- Get the task name as a hierarchical name including parent task names. - Returns:
- fullNamestr
- 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
 
 - getName() str¶
- Get the name of the task. - Returns:
- taskNamestr
- Name of the task. 
 
- taskName
 - See also - getFullName
- Get the full name of the task. 
 
 - getTaskDict() dict[str, weakref.ReferenceType[lsst.pipe.base.task.Task]]¶
- Get a dictionary of all tasks as a shallow copy. - Returns:
- taskDictdict
- Dictionary containing full task name: task object for the top-level task and all subtasks, sub-subtasks, etc. 
 
- taskDict
 
 - classmethod makeField(doc: str) ConfigurableField¶
- Make a - lsst.pex.config.ConfigurableFieldfor this task.- Parameters:
- docstr
- Help text for the field. 
 
- doc
- Returns:
- configurableFieldlsst.pex.config.ConfigurableField
- A - ConfigurableFieldfor this task.
 
- configurableField
 - 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") 
 - makeSubtask(name: str, **keyArgs: Any) None¶
- Create a subtask as a new instance as the - nameattribute of this task.- Parameters:
- namestr
- 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.
 
 
- name
 - Notes - The subtask must be defined by - Task.config.name, an instance of- ConfigurableFieldor- RegistryField.
 - run(template, science, sources, finalizedPsfApCorrCatalog=None, visitSummary=None)¶
- Preconvolve the science image with its own PSF, convolve the template image with a PSF-matching kernel and subtract from the preconvolved science image. - Parameters:
- templatelsst.afw.image.ExposureF
- The template image, which has previously been warped to the science image. The template bbox will be padded by a few pixels compared to the science bbox. 
- sciencelsst.afw.image.ExposureF
- The science exposure. 
- sourceslsst.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. 
- finalizedPsfApCorrCataloglsst.afw.table.ExposureCatalog, optional
- Exposure catalog with finalized psf models and aperture correction maps to be applied. Catalog uses the detector id for the catalog id, sorted on id for fast lookup. Deprecated in favor of - visitSummary, and will be removed after v26.
- visitSummarylsst.afw.table.ExposureCatalog, optional
- Exposure catalog with complete external calibrations. Catalog uses the detector id for the catalog id, sorted on id for fast lookup. Ignored (for temporary backwards compatibility) if - finalizedPsfApCorrCatalogis provided.
 
- template
- Returns:
- resultslsst.pipe.base.Struct
- scoreExposure- lsst.afw.image.ExposureF
- Result of subtracting the convolved template and science images. Attached PSF is that of the original science image. 
- matchedTemplate- lsst.afw.image.ExposureF
- Warped and PSF-matched template exposure. Attached PSF is that of the original science image. 
- matchedScience- lsst.afw.image.ExposureF
- The science exposure after convolving with its own PSF. Attached PSF is that of the original science image. 
- backgroundModel- lsst.afw.math.Function2D
- Background model that was fit while solving for the PSF-matching kernel 
- psfMatchingKernel- lsst.afw.math.Kernel
- Final kernel used to PSF-match the template to the science image. 
 
 
- results
 
 - runConvolveScience(template, science, selectSources)¶
- Convolve the science image with a PSF-matching kernel and subtract the template image. - Parameters:
- templatelsst.afw.image.ExposureF
- Template exposure, warped to match the science exposure. 
- sciencelsst.afw.image.ExposureF
- Science exposure to subtract from the template. 
- selectSourceslsst.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. 
 
- template
- Returns:
- resultslsst.pipe.base.Struct
- difference- lsst.afw.image.ExposureF
- Result of subtracting template and science. 
- matchedTemplate- lsst.afw.image.ExposureF
- Warped template exposure. Note that in this case, the template is not PSF-matched to the science image. 
- backgroundModel- lsst.afw.math.Function2D
- Background model that was fit while solving for the PSF-matching kernel 
- psfMatchingKernel- lsst.afw.math.Kernel
- Kernel used to PSF-match the science image to the template. 
 
 
- results
 
 - runConvolveTemplate(template, science, selectSources)¶
- Convolve the template image with a PSF-matching kernel and subtract from the science image. - Parameters:
- templatelsst.afw.image.ExposureF
- Template exposure, warped to match the science exposure. 
- sciencelsst.afw.image.ExposureF
- Science exposure to subtract from the template. 
- selectSourceslsst.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. 
 
- template
- Returns:
- resultslsst.pipe.base.Struct
- difference- lsst.afw.image.ExposureF
- Result of subtracting template and science. 
- matchedTemplate- lsst.afw.image.ExposureF
- Warped and PSF-matched template exposure. 
- backgroundModel- lsst.afw.math.Function2D
- Background model that was fit while solving for the PSF-matching kernel 
- psfMatchingKernel- lsst.afw.math.Kernel
- Kernel used to PSF-match the template to the science image. 
 
 
- results
 
 - runPreconvolve(template, science, matchedScience, selectSources, preConvKernel)¶
- Convolve the science image with its own PSF, then convolve the template with a matching kernel and subtract to form the Score exposure. - Parameters:
- templatelsst.afw.image.ExposureF
- Template exposure, warped to match the science exposure. 
- sciencelsst.afw.image.ExposureF
- Science exposure to subtract from the template. 
- matchedSciencelsst.afw.image.ExposureF
- The science exposure, convolved with the reflection of its own PSF. 
- selectSourceslsst.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. 
- preConvKernellsst.afw.math.Kernel
- The reflection of the kernel that was used to preconvolve the - scienceexposure. Must be normalized to sum to 1.
 
- template
- Returns:
- resultslsst.pipe.base.Struct
- scoreExposure- lsst.afw.image.ExposureF
- Result of subtracting the convolved template and science images. Attached PSF is that of the original science image. 
- matchedTemplate- lsst.afw.image.ExposureF
- Warped and PSF-matched template exposure. Attached PSF is that of the original science image. 
- matchedScience- lsst.afw.image.ExposureF
- The science exposure after convolving with its own PSF. Attached PSF is that of the original science image. 
- backgroundModel- lsst.afw.math.Function2D
- Background model that was fit while solving for the PSF-matching kernel 
- psfMatchingKernel- lsst.afw.math.Kernel
- Final kernel used to PSF-match the template to the science image. 
 
 
- results
 
 - runQuantum(butlerQC: QuantumContext, inputRefs: InputQuantizedConnection, outputRefs: OutputQuantizedConnection) None¶
- Do butler IO and transform to provide in memory objects for tasks - runmethod.- Parameters:
- butlerQCQuantumContext
- A butler which is specialized to operate in the context of a - lsst.daf.butler.Quantum.
- inputRefsInputQuantizedConnection
- Datastructure whose attribute names are the names that identify connections defined in corresponding - PipelineTaskConnectionsclass. The values of these attributes are the- lsst.daf.butler.DatasetRefobjects associated with the defined input/prerequisite connections.
- outputRefsOutputQuantizedConnection
- Datastructure whose attribute names are the names that identify connections defined in corresponding - PipelineTaskConnectionsclass. The values of these attributes are the- lsst.daf.butler.DatasetRefobjects associated with the defined output connections.
 
- butlerQC
 
 - timer(name: str, logLevel: int = 10) Iterator[None]¶
- Context manager to log performance data for an arbitrary block of code. - Parameters:
 - See also - lsst.utils.timer.logInfo
- Implementation function. 
 - Examples - Creating a timer context: - with self.timer("someCodeToTime"): pass # code to time 
 - updateMasks(template, science)¶
- Update the science and template mask planes before differencing. - Parameters:
- templatelsst.afw.image.Exposure
- Template exposure, warped to match the science exposure. The template mask planes will be erased, except for a few specified in the task config. 
- sciencelsst.afw.image.Exposure
- Science exposure to subtract from the template. The DETECTED and DETECTED_NEGATIVE mask planes of the science image will be erased. 
 
- template