ImageDifferenceTask¶
- class lsst.pipe.tasks.imageDifference.ImageDifferenceTask(butler=None, **kwargs)¶
Bases:
CmdLineTask
,PipelineTask
Subtract an image from a template and measure the result
Attributes Summary
Methods Summary
applyOverrides
(config)A hook to allow a task to change the values of its config after the camera-specific overrides are loaded but before any command-line overrides are applied.
checkTemplateIsSufficient
(templateExposure)Raise NoWorkFound if template coverage < requiredTemplateFraction
Empty (clear) the metadata for this Task and all sub-Tasks.
fitAstrometry
(templateSources, ...)Fit the relative astrometry between templateSources and selectSources
Get schema catalogs for all tasks in the hierarchy, combining the results into a single dict.
Get metadata for all tasks.
Get the task name as a hierarchical name including parent task names.
getName
()Get the name of the task.
Return resource configuration for this task.
Return a dict of empty catalogs for each catalog dataset produced by this task.
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.parseAndRun
([args, config, log, doReturnResults])Parse an argument list and run the command.
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.
runDataRef
(sensorRef[, templateIdList])Subtract an image from a template coadd and measure the result.
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.
writeConfig
(butler[, clobber, doBackup])Write the configuration used for processing the data, or check that an existing one is equal to the new one if present.
writeMetadata
(dataRef)Write the metadata produced from processing the data.
writePackageVersions
(butler[, clobber, ...])Compare and write package versions.
writeSchemas
(butler[, clobber, doBackup])Write the schemas returned by
lsst.pipe.base.Task.getAllSchemaCatalogs
.Attributes Documentation
Methods Documentation
- classmethod applyOverrides(config)¶
A hook to allow a task to change the values of its config after the camera-specific overrides are loaded but before any command-line overrides are applied.
- Parameters:
- configinstance of task’s
ConfigClass
Task configuration.
- configinstance of task’s
Notes
This is necessary in some cases because the camera-specific overrides may retarget subtasks, wiping out changes made in ConfigClass.setDefaults. See LSST Trac ticket #2282 for more discussion.
Warning
This is called by CmdLineTask.parseAndRun; other ways of constructing a config will not apply these overrides.
- checkTemplateIsSufficient(templateExposure)¶
Raise NoWorkFound if template coverage < requiredTemplateFraction
- Parameters:
- templateExposure
lsst.afw.image.ExposureF
The template exposure to check
- templateExposure
- Raises:
- NoWorkFound
Raised if fraction of good pixels, defined as not having NO_DATA set, is less then the configured requiredTemplateFraction
- 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.
- schemacatalogs
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() 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
- getResourceConfig() ResourceConfig | None ¶
Return resource configuration for this task.
- Returns:
- Object of type
ResourceConfig
orNone
if resource - configuration is not defined for this task.
- Object of type
- getSchemaCatalogs()¶
Return a dict of empty catalogs for each catalog dataset produced by this task.
- getTaskDict() Dict[str, ReferenceType[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")
- 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
.
- expId
- Returns:
- idFactory:
lsst.afw.table.IdFactory
- idFactory:
- 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
.
- classmethod parseAndRun(args=None, config=None, log=None, doReturnResults=False)¶
Parse an argument list and run the command.
- Parameters:
- args
list
, optional - config
lsst.pex.config.Config
-type, optional Config for task. If
None
useTask.ConfigClass
.- log
logging.Logger
-type, optional Log. If
None
use the default log.- doReturnResults
bool
, optional If
True
, return the results of this task. Default isFalse
. This is only intended for unit tests and similar use. It can easily exhaust memory (if the task returns enough data and you call it enough times) and it will fail when using multiprocessing if the returned data cannot be pickled.
- args
- Returns:
- struct
lsst.pipe.base.Struct
Fields are:
argumentParser
the argument parser (
lsst.pipe.base.ArgumentParser
).parsedCmd
the parsed command returned by the argument parser’s
parse_args
method (argparse.Namespace
).taskRunner
the task runner used to run the task (an instance of
Task.RunnerClass
).resultList
results returned by the task runner’s
run
method, one entry per invocation (list
). This will typically be a list ofStruct
, each containing at least anexitStatus
integer (0 or 1); seeTask.RunnerClass
(TaskRunner
by default) for more details.
- struct
Notes
Calling this method with no arguments specified is the standard way to run a command-line task from the command-line. For an example see
pipe_tasks
bin/makeSkyMap.py
or almost any other file in that directory.If one or more of the dataIds fails then this routine will exit (with a status giving the number of failed dataIds) rather than returning this struct; this behaviour can be overridden by specifying the
--noExit
command-line option.
- 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.
- exposure
- Returns:
- exposure
lsst.afw.image.exposure.Exposure
Exposure with adjusted calibrations.
- exposure
- 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
andmatchingSources
specified.- templateExposure
lsst.afw.image.ExposureF
, optional The template to be subtracted from
exposure
in the image subtraction.templateExposure
is modified in place ifconfig.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 ifconfig.doSubtract==False
andsubtractedExposure
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
andconfig.doDetection==True
, performs the post subtraction source detection only on this exposure. Otherwise should be None.
- exposure
- Returns:
- results
lsst.pipe.base.Struct
subtractedExposure
lsst.afw.image.ExposureF
Difference image.
scoreExposure
lsst.afw.image.ExposureF
orNone
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.
- results
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
.
- runDataRef(sensorRef, templateIdList=None)¶
Subtract an image from a template coadd and measure the result.
Data I/O wrapper around
run
using the butler in Gen2.- Parameters:
- sensorRef
lsst.daf.persistence.ButlerDataRef
Sensor-level butler data reference, used for the following data products:
Input only: - calexp - psf - ccdExposureId - ccdExposureId_bits - self.config.coaddName + “Coadd_skyMap” - self.config.coaddName + “Coadd” Input or output, depending on config: - self.config.coaddName + “Diff_subtractedExp” Output, depending on config: - self.config.coaddName + “Diff_matchedExp” - self.config.coaddName + “Diff_src”
- sensorRef
- Returns:
- results
lsst.pipe.base.Struct
Returns the Struct by
run
.
- results
- runDebug(exposure, subtractRes, selectSources, kernelSources, diaSources)¶
Make debug plots and displays.
- runQuantum(butlerQC: ButlerQuantumContext, inputRefs: InputQuantizedConnection, outputRefs: 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 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
timer.logInfo
Examples
Creating a timer context:
with self.timer("someCodeToTime"): pass # code to time
- writeConfig(butler, clobber=False, doBackup=True)¶
Write the configuration used for processing the data, or check that an existing one is equal to the new one if present.
- Parameters:
- butler
lsst.daf.persistence.Butler
Data butler used to write the config. The config is written to dataset type
CmdLineTask._getConfigName
.- clobber
bool
, optional A boolean flag that controls what happens if a config already has been saved:
- doBackup
bool
, optional Set to
True
to backup the config files if clobbering.
- butler
- writeMetadata(dataRef)¶
Write the metadata produced from processing the data.
- Parameters:
- dataRef
Butler data reference used to write the metadata. The metadata is written to dataset type
CmdLineTask._getMetadataName
.
- writePackageVersions(butler, clobber=False, doBackup=True, dataset='packages')¶
Compare and write package versions.
- Parameters:
- butler
lsst.daf.persistence.Butler
Data butler used to read/write the package versions.
- clobber
bool
, optional A boolean flag that controls what happens if versions already have been saved:
- doBackup
bool
, optional If
True
and clobbering, old package version files are backed up.- dataset
str
, optional Name of dataset to read/write.
- butler
- Raises:
- TaskError
Raised if there is a version mismatch with current and persisted lists of package versions.
Notes
Note that this operation is subject to a race condition.
- writeSchemas(butler, clobber=False, doBackup=True)¶
Write the schemas returned by
lsst.pipe.base.Task.getAllSchemaCatalogs
.- Parameters:
- butler
lsst.daf.persistence.Butler
Data butler used to write the schema. Each schema is written to the dataset type specified as the key in the dict returned by
getAllSchemaCatalogs
.- clobber
bool
, optional A boolean flag that controls what happens if a schema already has been saved:
- doBackup
bool
, optional Set to
True
to backup the schema files if clobbering.
- butler
Notes
If
clobber
isFalse
and an existing schema does not match a current schema, then some schemas may have been saved successfully and others may not, and there is no easy way to tell which is which.