ImageDifferenceTask

class lsst.pipe.tasks.imageDifference.ImageDifferenceTask(butler=None, **kwargs)

Bases: lsst.pipe.base.PipelineTask

Subtract an image from a template and measure the result

Deprecated since version v24.0: This Task has been replaced with lsst.ip.diffim.subtractImages and lsst.ip.diffim.detectAndMeasure. Will be removed after v25.

Attributes Summary

canMultiprocess

Methods Summary

checkTemplateIsSufficient(templateExposure) Raise NoWorkFound if template coverage < requiredTemplateFraction
emptyMetadata() Empty (clear) the metadata for this Task and all sub-Tasks.
fitAstrometry(templateSources, …) Fit the relative astrometry between templateSources and selectSources
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.ConfigurableField for this task.
makeIdFactory(expId, expBits) Create IdFactory instance for unique 64 bit diaSource id-s.
makeSubtask(name, **keyArgs) Create a subtask as a new instance as the name attribute of this task.
prepareCalibratedExposure(exposure[, …]) Prepare a calibrated exposure and apply finalized psf if so configured.
run([exposure, selectSources, …]) PSF matches, subtract two images and perform detection on the difference image.
runDebug(exposure, subtractRes, …) Make debug plots and displays.
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

canMultiprocess = True

Methods Documentation

checkTemplateIsSufficient(templateExposure)

Raise NoWorkFound if template coverage < requiredTemplateFraction

Parameters:
templateExposure : lsst.afw.image.ExposureF

The template exposure to check

Raises:
NoWorkFound

Raised if fraction of good pixels, defined as not having NO_DATA set, is less then the configured requiredTemplateFraction

emptyMetadata() → None

Empty (clear) the metadata for this Task and all sub-Tasks.

fitAstrometry(templateSources, templateExposure, selectSources)

Fit the relative astrometry between templateSources and selectSources

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.table Catalog 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.

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.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”.
getName() → str

Get the name of the task.

Returns:
taskName : str

Name of the task.

See also

getFullName
getResourceConfig() → Optional[ResourceConfig]

Return resource configuration for this task.

Returns:
Object of type ResourceConfig or None if resource
configuration is not defined for this task.
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.table Catalog 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.

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.

classmethod makeField(doc: str) → lsst.pex.config.configurableField.ConfigurableField

Make a lsst.pex.config.ConfigurableField for this task.

Parameters:
doc : str

Help text for the field.

Returns:
configurableField : lsst.pex.config.ConfigurableField

A ConfigurableField for 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")
static makeIdFactory(expId, expBits)

Create IdFactory instance for unique 64 bit diaSource id-s.

Parameters:
expId : int

Exposure id.

expBits: `int`

Number of used bits in expId.

Returns:
idFactory: lsst.afw.table.IdFactory
makeSubtask(name: str, **keyArgs) → 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”.

Notes

The subtask must be defined by Task.config.name, an instance of ConfigurableField or RegistryField.

prepareCalibratedExposure(exposure, finalizedPsfApCorrCatalog=None)

Prepare a calibrated exposure and apply finalized psf if so configured.

Parameters:
exposure : lsst.afw.image.exposure.Exposure

Input exposure to adjust calibrations.

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:
exposure : lsst.afw.image.exposure.Exposure

Exposure with adjusted calibrations.

run(exposure=None, selectSources=None, templateExposure=None, templateSources=None, idFactory=None, calexpBackgroundExposure=None, subtractedExposure=None)

PSF matches, subtract two images and perform detection on the difference image.

Parameters:
exposure : lsst.afw.image.ExposureF, optional

The science exposure, the minuend in the image subtraction. Can be None only if config.doSubtract==False.

selectSources : lsst.afw.table.SourceCatalog, optional

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. The selection steps depend on config options and whether templateSources and matchingSources specified.

templateExposure : lsst.afw.image.ExposureF, optional

The template to be subtracted from exposure in the image subtraction. templateExposure is modified in place if config.doScaleTemplateVariance==True. The template exposure should cover the same sky area as the science exposure. It is either a stich of patches of a coadd skymap image or a calexp of the same pointing as the science exposure. Can be None only if config.doSubtract==False and subtractedExposure is not None.

templateSources : lsst.afw.table.SourceCatalog, optional

Identified sources on the template exposure.

idFactory : lsst.afw.table.IdFactory

Generator object to assign ids to detected sources in the difference image.

calexpBackgroundExposure : lsst.afw.image.ExposureF, optional

Background exposure to be added back to the science exposure if config.doAddCalexpBackground==True

subtractedExposure : lsst.afw.image.ExposureF, optional

If config.doSubtract==False and config.doDetection==True, performs the post subtraction source detection only on this exposure. Otherwise should be None.

Returns:
results : lsst.pipe.base.Struct
subtractedExposure : lsst.afw.image.ExposureF

Difference image.

scoreExposure : lsst.afw.image.ExposureF or None

The zogy score exposure, if calculated.

matchedExposure : lsst.afw.image.ExposureF

The matched PSF exposure.

subtractRes : lsst.pipe.base.Struct

The returned result structure of the ImagePsfMatchTask subtask.

diaSources : lsst.afw.table.SourceCatalog

The catalog of detected sources.

selectSources : lsst.afw.table.SourceCatalog

The input source catalog with optionally added Qa information.

Notes

The following major steps are included:

  • warp template coadd to match WCS of image
  • PSF match image to warped template
  • subtract image from PSF-matched, warped template
  • detect sources
  • measure sources

For details about the image subtraction configuration modes see lsst.ip.diffim.

runDebug(exposure, subtractRes, selectSources, kernelSources, diaSources)

Make debug plots and displays.

runQuantum(butlerQC: lsst.pipe.base.butlerQuantumContext.ButlerQuantumContext, inputRefs: lsst.pipe.base.connections.InputQuantizedConnection, outputRefs: lsst.pipe.base.connections.OutputQuantizedConnection)

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 PipelineTaskConnections class. The values of these attributes are the lsst.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 the lsst.daf.butler.DatasetRef objects associated with the defined output connections.

timer(name: str, logLevel: int = 10) → Iterator[None]

Context manager to log performance data for an arbitrary block of code.

Parameters:
name : str

Name of code being timed; data will be logged using item name: Start and End.

logLevel

A logging level constant.

See also

timer.logInfo

Examples

Creating a timer context:

with self.timer("someCodeToTime"):
    pass  # code to time