DetectAndMeasureScoreTask¶
- class lsst.ip.diffim.DetectAndMeasureScoreTask(**kwargs)¶
Bases:
DetectAndMeasureTask
Detect 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.ConfigurableField
for this task.makeSubtask
(name, **keyArgs)Create a subtask as a new instance as the
name
attribute 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
run
method.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.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
- getName() str ¶
Get the name of the task.
- Returns:
- taskName
str
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:
- 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
.
- 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, positiveFootprints=None, negativeFootprints=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.
- positiveFootprints
lsst.afw.detection.FootprintSet
, optional Positive polarity footprints.
- negativeFootprints
lsst.afw.detection.FootprintSet
, optional Negative polarity footprints.
- science
- Returns:
- measurementResults
lsst.pipe.base.Struct
subtractedMeasuredExposure
lsst.afw.image.ExposureF
Subtracted exposure with detection mask applied.
diaSources
lsst.afw.table.SourceCatalog
The 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
subtractedMeasuredExposure
lsst.afw.image.ExposureF
Subtracted exposure with detection mask applied.
diaSources
lsst.afw.table.SourceCatalog
The catalog of detected sources.
- measurementResults
- runQuantum(butlerQC: QuantumContext, inputRefs: InputQuantizedConnection, outputRefs: OutputQuantizedConnection)¶
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