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.ConfigurableField
for this task.makeSubtask
(name, **keyArgs)Create a subtask as a new instance as the
name
attribute 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
run
method.timer
(name[, logLevel])Context manager to log performance data for an arbitrary block of code.
updateMasks
(template, science, difference)Update the mask planes on images for finalizing.
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:
- 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?
- template
- Returns:
- correctedExposure
lsst.afw.image.ExposureF
The decorrelated image difference.
- correctedExposure
- getFullMetadata() 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.
- metadata
Notes
The returned metadata includes timing information (if
@timer.timeMethod
is 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:
- 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
- getTaskDict() dict[str, weakref.ReferenceType[lsst.pipe.base.task.Task]] ¶
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
- classmethod makeField(doc: str) ConfigurableField ¶
Make a
lsst.pex.config.ConfigurableField
for this task.- Parameters:
- doc
str
Help text for the field.
- doc
- Returns:
- configurableField
lsst.pex.config.ConfigurableField
A
ConfigurableField
for 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
name
attribute 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
.
- name
Notes
The subtask must be defined by
Task.config.name
, an instance ofConfigurableField
orRegistryField
.
- 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:
- template
lsst.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.
- science
lsst.afw.image.ExposureF
The science exposure.
- 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. 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.- visitSummary
lsst.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
finalizedPsfApCorrCatalog
is provided.
- template
- Returns:
- results
lsst.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:
- 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.
- selectSources
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.
- template
- Returns:
- results
lsst.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:
- 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.
- selectSources
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.
- template
- Returns:
- results
lsst.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:
- 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.
- matchedScience
lsst.afw.image.ExposureF
The science exposure, convolved with the reflection of its own PSF.
- selectSources
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.
- preConvKernel
lsst.afw.math.Kernel
The reflection of the kernel that was used to preconvolve the
science
exposure. Must be normalized to sum to 1.
- template
- Returns:
- results
lsst.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
run
method.- Parameters:
- butlerQC
QuantumContext
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
PipelineTaskConnections
class. The values of these attributes are thelsst.daf.butler.DatasetRef
objects associated with the defined input/prerequisite connections.- outputRefs
OutputQuantizedConnection
Datastructure whose attribute names are the names that identify connections defined in corresponding
PipelineTaskConnections
class. The values of these attributes are thelsst.daf.butler.DatasetRef
objects 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
Examples
Creating a timer context:
with self.timer("someCodeToTime"): pass # code to time
- updateMasks(template, science, difference)¶
Update the mask planes on images for finalizing.