DetectAndMeasureScoreTask¶
- class lsst.ip.diffim.DetectAndMeasureScoreTask(**kwargs)¶
Bases:
DetectAndMeasureTaskDetect DIA sources using a score image, and measure the detections on the difference image.
Source detection is run on the supplied score, or maximum likelihood, image. Note that no additional convolution will be done in this case. Close positive and negative detections will optionally be merged into dipole diaSources. Sky sources, or forced detections in background regions, will optionally be added, and the configured measurement algorithm will be run on all detections.
Attributes Summary
Methods Summary
addSkySources(diaSources, mask, seed[, subtask])Add sources in empty regions of the difference image for measuring the background.
calculateMetrics(difference)Add difference image QA metrics to the Task metadata.
Empty (clear) the metadata for this Task and all sub-Tasks.
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.measureDiaSources(diaSources, science, ...)Use (matched) template and science image to constrain dipole fitting.
measureForcedSources(diaSources, science, wcs)Perform forced measurement of the diaSources on the science image.
processResults(science, matchedTemplate, ...)Measure and process the results of source detection.
run(science, matchedTemplate, difference, ...)Detect and measure sources on a score image.
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.
Attributes Documentation
Methods Documentation
- addSkySources(diaSources, mask, seed, subtask=None)¶
Add sources in empty regions of the difference image for measuring the background.
- Parameters:
- diaSources
lsst.afw.table.SourceCatalog The catalog of detected sources.
- mask
lsst.afw.image.Mask Mask plane for determining regions where Sky sources can be added.
- seed
int Seed value to initialize the random number generator.
- diaSources
- calculateMetrics(difference)¶
Add difference image QA metrics to the Task metadata.
This may be used to produce corresponding metrics (see lsst.analysis.tools.tasks.diffimTaskDetectorVisitMetricAnalysis).
- Parameters:
- difference
lsst.afw.image.Exposure The target difference image to calculate metrics for.
- difference
- 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.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:
- 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
- getName() str¶
Get the name of the task.
- Returns:
- taskName
str Name of the task.
- taskName
See also
getFullNameGet 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:
- 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.ConfigurableFieldfor this task.- Parameters:
- doc
str Help text for the field.
- doc
- Returns:
- configurableField
lsst.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:
- 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 ofConfigurableFieldorRegistryField.
- measureDiaSources(diaSources, science, difference, matchedTemplate)¶
Use (matched) template and science image to constrain dipole fitting.
- Parameters:
- diaSources
lsst.afw.table.SourceCatalog The catalog of detected sources.
- science
lsst.afw.image.ExposureF Science exposure that the template was subtracted from.
- difference
lsst.afw.image.ExposureF Result of subtracting template from the science image.
- matchedTemplate
lsst.afw.image.ExposureF Warped and PSF-matched template that was used produce the difference image.
- diaSources
- measureForcedSources(diaSources, science, wcs)¶
Perform forced measurement of the diaSources on the science image.
- Parameters:
- diaSources
lsst.afw.table.SourceCatalog The catalog of detected sources.
- science
lsst.afw.image.ExposureF Science exposure that the template was subtracted from.
- wcs
lsst.afw.geom.SkyWcs Coordinate system definition (wcs) for the exposure.
- diaSources
- processResults(science, matchedTemplate, difference, sources, idFactory, positives=None, negatives=None)¶
Measure and process the results of source detection.
- Parameters:
- science
lsst.afw.image.ExposureF Science exposure that the template was subtracted from.
- matchedTemplate
lsst.afw.image.ExposureF Warped and PSF-matched template that was used produce the difference image.
- difference
lsst.afw.image.ExposureF Result of subtracting template from the science image.
- sources
lsst.afw.table.SourceCatalog Detected sources on the difference exposure.
- idFactory
lsst.afw.table.IdFactory Generator object used to assign ids to detected sources in the difference image.
- positives
lsst.afw.table.SourceCatalog, optional Positive polarity footprints.
- negatives
lsst.afw.table.SourceCatalog, optional Negative polarity footprints.
- science
- Returns:
- measurementResults
lsst.pipe.base.Struct subtractedMeasuredExposurelsst.afw.image.ExposureFSubtracted exposure with detection mask applied.
diaSourceslsst.afw.table.SourceCatalogThe catalog of detected sources.
- measurementResults
- run(science, matchedTemplate, difference, scoreExposure, idFactory=None)¶
Detect and measure sources on a score image.
- Parameters:
- science
lsst.afw.image.ExposureF Science exposure that the template was subtracted from.
- matchedTemplate
lsst.afw.image.ExposureF Warped and PSF-matched template that was used produce the difference image.
- difference
lsst.afw.image.ExposureF Result of subtracting template from the science image.
- scoreExposure
lsst.afw.image.ExposureF Score or maximum likelihood difference image
- idFactory
lsst.afw.table.IdFactory, optional Generator object used to assign ids to detected sources in the difference image. Ids from this generator are not set until after deblending and merging positive/negative peaks.
- science
- Returns:
- measurementResults
lsst.pipe.base.Struct subtractedMeasuredExposurelsst.afw.image.ExposureFSubtracted exposure with detection mask applied.
diaSourceslsst.afw.table.SourceCatalogThe catalog of detected sources.
- measurementResults
- runQuantum(butlerQC: QuantumContext, inputRefs: InputQuantizedConnection, outputRefs: OutputQuantizedConnection)¶
Do butler IO and transform to provide in memory objects for tasks
runmethod.- 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
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