CompareWarpAssembleCoaddTask¶

class lsst.pipe.tasks.assembleCoadd.CompareWarpAssembleCoaddTask(*args, **kwargs)¶

Bases: lsst.pipe.tasks.assembleCoadd.AssembleCoaddTask

Assemble a compareWarp coadded image from a set of warps by masking artifacts detected by comparing PSF-matched warps.

In AssembleCoaddTask, we compute the coadd as an clipped mean (i.e., we clip outliers). The problem with doing this is that when computing the coadd PSF at a given location, individual visit PSFs from visits with outlier pixels contribute to the coadd PSF and cannot be treated correctly. In this task, we correct for this behavior by creating a new badMaskPlane ‘CLIPPED’ which marks pixels in the individual warps suspected to contain an artifact. We populate this plane on the input warps by comparing PSF-matched warps with a PSF-matched median coadd which serves as a model of the static sky. Any group of pixels that deviates from the PSF-matched template coadd by more than config.detect.threshold sigma, is an artifact candidate. The candidates are then filtered to remove variable sources and sources that are difficult to subtract such as bright stars. This filter is configured using the config parameters temporalThreshold and spatialThreshold. The temporalThreshold is the maximum fraction of epochs that the deviation can appear in and still be considered an artifact. The spatialThreshold is the maximum fraction of pixels in the footprint of the deviation that appear in other epochs (where other epochs is defined by the temporalThreshold). If the deviant region meets this criteria of having a significant percentage of pixels that deviate in only a few epochs, these pixels have the ‘CLIPPED’ bit set in the mask. These regions will not contribute to the final coadd. Furthermore, any routine to determine the coadd PSF can now be cognizant of clipped regions. Note that the algorithm implemented by this task is preliminary and works correctly for HSC data. Parameter modifications and or considerable redesigning of the algorithm is likley required for other surveys.

CompareWarpAssembleCoaddTask sub-classes AssembleCoaddTask and instantiates AssembleCoaddTask as a subtask to generate the TemplateCoadd (the model of the static sky).

Notes

The lsst.pipe.base.CmdLineTask interface supports a flag -d to import debug.py from your PYTHONPATH; see baseDebug for more about debug.py files.

This task supports the following debug variables:

saveCountIm

If True then save the Epoch Count Image as a fits file in the figPath
figPath

Path to save the debug fits images and figures

For example, put something like:

import lsstDebug
def DebugInfo(name):
    di = lsstDebug.getInfo(name)
    if name == "lsst.pipe.tasks.assembleCoadd":
        di.saveCountIm = True
        di.figPath = "/desired/path/to/debugging/output/images"
    return di
lsstDebug.Info = DebugInfo

into your debug.py file and run assemebleCoadd.py with the --debug flag. Some subtasks may have their own debug variables; see individual Task documentation.

Examples

CompareWarpAssembleCoaddTask assembles a set of warped images into a coadded image. The CompareWarpAssembleCoaddTask is invoked by running assembleCoadd.py with the flag --compareWarpCoadd. Usage of assembleCoadd.py expects a data reference to the tract patch and filter to be coadded (specified using ‘–id = [KEY=VALUE1[^VALUE2[^VALUE3…] [KEY=VALUE1[^VALUE2[^VALUE3…] …]]’) along with a list of coaddTempExps to attempt to coadd (specified using ‘–selectId [KEY=VALUE1[^VALUE2[^VALUE3…] [KEY=VALUE1[^VALUE2[^VALUE3…] …]]’). Only the warps that cover the specified tract and patch will be coadded. A list of the available optional arguments can be obtained by calling assembleCoadd.py with the --help command line argument:

assembleCoadd.py --help

To demonstrate usage of the CompareWarpAssembleCoaddTask in the larger context of multi-band processing, we will generate the HSC-I & -R band oadds from HSC engineering test data provided in the ci_hsc package. To begin, assuming that the lsst stack has been already set up, we must set up the obs_subaru and ci_hsc packages. This defines the environment variable $CI_HSC_DIR and points at the location of the package. The raw HSC data live in the $CI_HSC_DIR/raw directory. To begin assembling the coadds, we must first

processCcd process the individual ccds in $CI_HSC_RAW to produce calibrated exposures

makeSkyMap create a skymap that covers the area of the sky present in the raw exposures

makeCoaddTempExp warp the individual calibrated exposures to the tangent plane of the coadd

We can perform all of these steps by running

$CI_HSC_DIR scons warp-903986 warp-904014 warp-903990 warp-904010 warp-903988

This will produce warped coaddTempExps for each visit. To coadd the warped data, we call assembleCoadd.py as follows:

assembleCoadd.py --compareWarpCoadd $CI_HSC_DIR/DATA --id patch=5,4 tract=0 filter=HSC-I        --selectId visit=903986 ccd=16 --selectId visit=903986 ccd=22 --selectId visit=903986 ccd=23        --selectId visit=903986 ccd=100 --selectId visit=904014 ccd=1 --selectId visit=904014 ccd=6        --selectId visit=904014 ccd=12 --selectId visit=903990 ccd=18 --selectId visit=903990 ccd=25        --selectId visit=904010 ccd=4 --selectId visit=904010 ccd=10 --selectId visit=904010 ccd=100        --selectId visit=903988 ccd=16 --selectId visit=903988 ccd=17 --selectId visit=903988 ccd=23        --selectId visit=903988 ccd=24

This will process the HSC-I band data. The results are written in $CI_HSC_DIR/DATA/deepCoadd-results/HSC-I.

Attributes Summary

canMultiprocess

Methods Summary

`adaptArgsAndRun`(inputData, inputDataIds, …)	Assemble a coadd from a set of Warps.
`applyAltEdgeMask`(mask, altMaskList)	Propagate alt EDGE mask to SENSOR_EDGE AND INEXACT_PSF planes.
`applyAltMaskPlanes`(mask, altMaskSpans)	Apply in place alt mask formatted as SpanSets to a mask.
`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.
`assembleMetadata`(coaddExposure, …)	Set the metadata for the coadd.
`assembleSubregion`(coaddExposure, bbox, …)	Assemble the coadd for a sub-region.
`emptyMetadata`()	Empty (clear) the metadata for this Task and all sub-Tasks.
`filterArtifacts`(spanSetList, …[, …])	Filter artifact candidates.
`findArtifacts`(templateCoadd, tempExpRefList, …)	Find artifacts.
`getAllSchemaCatalogs`()	Get schema catalogs for all tasks in the hierarchy, combining the results into a single dict.
`getBadPixelMask`()	!
`getCoaddDatasetName`([warpType])	Return coadd name for given warpType and task config
`getDatasetTypes`(config, configClass)	Return dataset type descriptors defined in task configuration.
`getFullMetadata`()	Get metadata for all tasks.
`getFullName`()	Get the task name as a hierarchical name including parent task names.
`getInitInputDatasetTypes`(config)	Return dataset type descriptors that can be used to retrieve the `initInputs` constructor argument.
`getInitOutputDatasetTypes`(config)	Return dataset type descriptors that can be used to write the objects returned by `getOutputDatasets`.
`getInitOutputDatasets`()	Return persistable outputs that are available immediately after the task has been constructed.
`getInputDatasetTypes`(config)	Return input dataset type descriptors
`getName`()	Get the name of the task.
`getOutputDatasetTypes`(config)	Return output dataset type descriptors
`getResourceConfig`()	Return resource configuration for this task.
`getSchemaCatalogs`()	Get the schemas generated by this task.
`getSkyInfo`(patchRef)	!
`getTaskDict`()	Get a dictionary of all tasks as a shallow copy.
`getTempExpDatasetName`([warpType])	Return warp name for given warpType and task config
`getTempExpRefList`(patchRef, calExpRefList)	Generate list data references corresponding to warped exposures that lie within the patch to be coadded.
`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.
`makeSupplementaryData`(dataRef[, …])	Make inputs specific to Subclass.
`makeSupplementaryDataGen3`(inputData, …)	Make inputs specific to Subclass with Gen 3 API
`parseAndRun`([args, config, log, doReturnResults])	Parse an argument list and run the command.
`prefilterArtifacts`(spanSetList, exp)	Remove artifact candidates covered by bad mask plane.
`prepareInputs`(refList)	Prepare the input warps for coaddition by measuring the weight for each warp and the scaling for the photometric zero point.
`prepareStats`([mask])	Prepare the statistics for coadding images.
`processResults`(coaddExposure, dataRef)	Interpolate over missing data and mask bright stars.
`readBrightObjectMasks`(dataRef)	Retrieve the bright object masks.
`removeMaskPlanes`(maskedImage)	Unset the mask of an image for mask planes specified in the config.
`run`(skyInfo, tempExpRefList, …)	Assemble the coadd.
`runDataRef`(dataRef[, selectDataList, …])	Assemble a coadd from a set of Warps.
`runQuantum`(quantum, butler)	Execute PipelineTask algorithm on single quantum of data.
`saveStruct`(struct, outputDataRefs, butler)	Save data in butler.
`selectExposures`(patchRef[, skyInfo, …])	!
`setBrightObjectMasks`(exposure, dataId, …)	Set the bright object masks.
`setInexactPsf`(mask)	Set INEXACT_PSF mask plane.
`setRejectedMaskMapping`(statsCtrl)	Map certain mask planes of the warps to new planes for the coadd.
`shrinkValidPolygons`(coaddInputs)	Shrink coaddInputs’ ccds’ ValidPolygons in place.
`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

canMultiprocess = True¶

Methods Documentation

adaptArgsAndRun(inputData, inputDataIds, outputDataIds, butler)¶

Assemble a coadd from a set of Warps.

PipelineTask (Gen3) entry point to Coadd a set of Warps. Analogous to runDataRef, it prepares all the data products to be passed to run, and processes the results before returning to struct of results to be written out. AssembleCoadd cannot fit all Warps in memory. Therefore, its inputs are accessed subregion by subregion by the lsst.daf.butler.ShimButler that quacks like a Gen2 lsst.daf.persistence.Butler. Updates to this method should correspond to an update in runDataRef while both entry points are used.

Parameters:

inputData : dict: Keys are the names of the configs describing input dataset types. Values are input Python-domain data objects (or lists of objects) retrieved from data butler.
inputDataIds : dict: Keys are the names of the configs describing input dataset types. Values are DataIds (or lists of DataIds) that task consumes for corresponding dataset type.
outputDataIds : dict: Keys are the names of the configs describing input dataset types. Values are DataIds (or lists of DataIds) that task is to produce for corresponding dataset type.
butler : lsst.daf.butler.Butler: Gen3 Butler object for fetching additional data products before running the Task

Returns:

result : lsst.pipe.base.Struct

Result struct with components:

coaddExposure : coadded exposure (lsst.afw.image.Exposure)
nImage: N Image (lsst.afw.image.Image)

applyAltEdgeMask(mask, altMaskList)¶

Propagate alt EDGE mask to SENSOR_EDGE AND INEXACT_PSF planes.

Parameters:	mask : `lsst.afw.image.Mask` Original mask. altMaskList : `list` List of Dicts containing `spanSet` lists. Each element contains the new mask plane name (e.g. “CLIPPED and/or “NO_DATA”) as the key, and list of `SpanSets` to apply to the mask.

applyAltMaskPlanes(mask, altMaskSpans)¶

Apply in place alt mask formatted as SpanSets to a mask.

Parameters:	mask : `lsst.afw.image.Mask` Original mask. altMaskSpans : `dict` SpanSet lists to apply. Each element contains the new mask plane name (e.g. “CLIPPED and/or “NO_DATA”) as the key, and list of SpanSets to apply to the mask.
Returns:	mask : `lsst.afw.image.Mask` Updated mask.

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:	config : instance of task’s `ConfigClass` Task configuration.

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.

assembleMetadata(coaddExposure, tempExpRefList, weightList)¶

Set the metadata for the coadd.

This basic implementation sets the filter from the first input.

Parameters:	coaddExposure : `lsst.afw.image.Exposure` The target exposure for the coadd. tempExpRefList : `list` List of data references to tempExp. weightList : `list` List of weights.

assembleSubregion(coaddExposure, bbox, tempExpRefList, imageScalerList, weightList, altMaskList, statsFlags, statsCtrl, nImage=None)¶

Assemble the coadd for a sub-region.

For each coaddTempExp, check for (and swap in) an alternative mask if one is passed. Remove mask planes listed in config.removeMaskPlanes. Finally, stack the actual exposures using lsst.afw.math.statisticsStack with the statistic specified by statsFlags. Typically, the statsFlag will be one of lsst.afw.math.MEAN for a mean-stack or lsst.afw.math.MEANCLIP for outlier rejection using an N-sigma clipped mean where N and iterations are specified by statsCtrl. Assign the stacked subregion back to the coadd.

Parameters:

coaddExposure : lsst.afw.image.Exposure: The target exposure for the coadd.
bbox : lsst.afw.geom.Box: Sub-region to coadd.
tempExpRefList : list: List of data reference to tempExp.
imageScalerList : list: List of image scalers.
weightList : list: List of weights.
altMaskList : list: List of alternate masks to use rather than those stored with tempExp, or None. Each element is dict with keys = mask plane name to which to add the spans.
statsFlags : lsst.afw.math.Property: Property object for statistic for coadd.
statsCtrl : lsst.afw.math.StatisticsControl: Statistics control object for coadd.
nImage : lsst.afw.image.ImageU, optional: Keeps track of exposure count for each pixel.

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

filterArtifacts(spanSetList, epochCountImage, nImage, footprintsToExclude=None)¶

Filter artifact candidates.

Parameters:	spanSetList : `list` List of SpanSets representing artifact candidates. epochCountImage : `lsst.afw.image.Image` Image of accumulated number of warpDiff detections. nImage : `lsst.afw.image.Image` Image of the accumulated number of total epochs contributing.
Returns:	maskSpanSetList : `list` List of SpanSets with artifacts.

findArtifacts(templateCoadd, tempExpRefList, imageScalerList)¶

Find artifacts.

Loop through warps twice. The first loop builds a map with the count of how many epochs each pixel deviates from the templateCoadd by more than config.chiThreshold sigma. The second loop takes each difference image and filters the artifacts detected in each using count map to filter out variable sources and sources that are difficult to subtract cleanly.

Parameters:	templateCoadd : `lsst.afw.image.Exposure` Exposure to serve as model of static sky. tempExpRefList : `list` List of data references to warps. imageScalerList : `list` List of image scalers.
Returns:	altMasks : `list` List of dicts containing information about CLIPPED (i.e., artifacts), NO_DATA, and EDGE pixels.

getAllSchemaCatalogs()¶

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.

getBadPixelMask()¶: ! @brief Convenience method to provide the bitmask from the mask plane names

getCoaddDatasetName(warpType='direct')¶

Return coadd name for given warpType and task config

Parameters:	warpType : string Either ‘direct’ or ‘psfMatched’
Returns:	CoaddDatasetName : `string`

classmethod getDatasetTypes(config, configClass)¶

Return dataset type descriptors defined in task configuration.

This method can be used by other methods that need to extract dataset types from task configuration (e.g. getInputDatasetTypes or sub-class methods).

Parameters:	config : `Config` Configuration for this task. Typically datasets are defined in a task configuration. configClass : `type` Class of the configuration object which defines dataset type.
Returns:	Dictionary where key is the name (arbitrary) of the output dataset and value is the `DatasetTypeDescriptor` instance. Default implementation uses configuration field name as dictionary key. Returns empty dict if configuration has no fields with the specified ``configClass``.

getFullMetadata()¶

Get metadata for all tasks.

Returns:	metadata : `lsst.daf.base.PropertySet` The `PropertySet` 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()¶

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”.

classmethod getInitInputDatasetTypes(config)¶

Return dataset type descriptors that can be used to retrieve the initInputs constructor argument.

Datasets used in initialization may not be associated with any Dimension (i.e. their data IDs must be empty dictionaries).

Default implementation finds all fields of type InitInputInputDatasetConfig in configuration (non-recursively) and uses them for constructing DatasetTypeDescriptor instances. The names of these fields are used as keys in returned dictionary. Subclasses can override this behavior.

Parameters:	config : `Config` Configuration for this task. Typically datasets are defined in a task configuration.
Returns:	Dictionary where key is the name (arbitrary) of the input dataset and value is the `DatasetTypeDescriptor` instance. Default implementation uses configuration field name as dictionary key. When the task requires no initialization inputs, should return an empty dict.

classmethod getInitOutputDatasetTypes(config)¶

Return dataset type descriptors that can be used to write the objects returned by getOutputDatasets.

Datasets used in initialization may not be associated with any Dimension (i.e. their data IDs must be empty dictionaries).

Default implementation finds all fields of type InitOutputDatasetConfig in configuration (non-recursively) and uses them for constructing DatasetTypeDescriptor instances. The names of these fields are used as keys in returned dictionary. Subclasses can override this behavior.

Parameters:	config : `Config` Configuration for this task. Typically datasets are defined in a task configuration.
Returns:	Dictionary where key is the name (arbitrary) of the output dataset and value is the `DatasetTypeDescriptor` instance. Default implementation uses configuration field name as dictionary key. When the task produces no initialization outputs, should return an empty dict.

getInitOutputDatasets()¶

Return persistable outputs that are available immediately after the task has been constructed.

Subclasses that operate on catalogs should override this method to return the schema(s) of the catalog(s) they produce.

It is not necessary to return the PipelineTask’s configuration or other provenance information in order for it to be persisted; that is the responsibility of the execution system.

Returns:	datasets : `dict` Dictionary with keys that match those of the dict returned by `getInitOutputDatasetTypes` values that can be written by calling `Butler.put` with those DatasetTypes and no data IDs. An empty `dict` should be returned by tasks that produce no initialization outputs.

classmethod getInputDatasetTypes(config)¶

Return input dataset type descriptors

Remove input dataset types not used by the Task

getName()¶

Get the name of the task.

Returns:	taskName : `str` Name of the task.

See also

Task.getAllSchemaCatalogs

Notes

Warning

Subclasses that use schemas must override this method. The default implemenation 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.

getSkyInfo(patchRef)¶

! @brief Use @ref getSkyinfo to return the skyMap, tract and patch information, wcs and the outer bbox of the patch.

@param[in] patchRef data reference for sky map. Must include keys “tract” and “patch”

@return pipe_base Struct containing: - skyMap: sky map - tractInfo: information for chosen tract of sky map - patchInfo: information about chosen patch of tract - wcs: WCS of tract - bbox: outer bbox of patch, as an afwGeom Box2I

getTaskDict()¶

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..

getTempExpDatasetName(warpType='direct')¶

Return warp name for given warpType and task config

Parameters:	warpType : string Either ‘direct’ or ‘psfMatched’
Returns:	WarpDatasetName : `string`

getTempExpRefList(patchRef, calExpRefList)¶

Generate list data references corresponding to warped exposures that lie within the patch to be coadded.

Parameters:	patchRef : `dataRef` Data reference for patch. calExpRefList : `list` List of data references for input calexps.
Returns:	tempExpRefList : `list` List of Warp/CoaddTempExp data references.

classmethod makeField(doc)¶

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("a brief description of what this task does")

makeSubtask(name, **keyArgs)¶

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 pex_config ConfigurableField or RegistryField.

makeSupplementaryData(dataRef, selectDataList=None, warpRefList=None)¶

Make inputs specific to Subclass.

Generate a templateCoadd to use as a native model of static sky to subtract from warps.

Parameters:	dataRef : `lsst.daf.persistence.butlerSubset.ButlerDataRef` Butler dataRef for supplementary data. selectDataList : `list` (optional) Optional List of data references to Calexps. warpRefList : `list` (optional) Optional List of data references to Warps.
Returns:	result : `lsst.pipe.base.Struct` Result struct with components: `templateCoadd`: coadded exposure (`lsst.afw.image.Exposure`) `nImage`: N Image (`lsst.afw.image.Image`)

makeSupplementaryDataGen3(inputData, inputDataIds, outputDataIds, butler)¶

Make inputs specific to Subclass with Gen 3 API

Calls Gen3 adaptArgsAndRun instead of the Gen2 specific runDataRef

Duplicates interface of`adaptArgsAndRun` method. Available to be implemented by subclasses only if they need the coadd dataRef for performing preliminary processing before assembling the coadd.

Parameters:

inputData : dict: Keys are the names of the configs describing input dataset types. Values are input Python-domain data objects (or lists of objects) retrieved from data butler.
inputDataIds : dict: Keys are the names of the configs describing input dataset types. Values are DataIds (or lists of DataIds) that task consumes for corresponding dataset type. DataIds are guaranteed to match data objects in inputData.
outputDataIds : dict: Keys are the names of the configs describing input dataset types. Values are DataIds (or lists of DataIds) that task is to produce for corresponding dataset type.
butler : lsst.daf.butler.Butler: Gen3 Butler object for fetching additional data products before running the Task

Returns:

result : lsst.pipe.base.Struct

Result struct with components:

templateCoadd : coadded exposure (lsst.afw.image.Exposure)
nImage: N Image (lsst.afw.image.Image)

classmethod parseAndRun(args=None, config=None, log=None, doReturnResults=False)¶

Parse an argument list and run the command.

Parameters:

args : list, optional: List of command-line arguments; if None use sys.argv.
config : lsst.pex.config.Config-type, optional: Config for task. If None use Task.ConfigClass.
log : lsst.log.Log-type, optional: Log. If None use the default log.
doReturnResults : bool, optional: If True, return the results of this task. Default is False. 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.

Returns:

struct : lsst.pipe.base.Struct

Fields are:

argumentParser: the argument parser.
parsedCmd: the parsed command returned by the argument parser’s lsst.pipe.base.ArgumentParser.parse_args method.
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.

This will typically be a list of None unless doReturnResults is True; see Task.RunnerClass (TaskRunner by default) for more information.

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.

prefilterArtifacts(spanSetList, exp)¶

Remove artifact candidates covered by bad mask plane.

Any future editing of the candidate list that does not depend on temporal information should go in this method.

Parameters:	spanSetList : `list` List of SpanSets representing artifact candidates. exp : `lsst.afw.image.Exposure` Exposure containing mask planes used to prefilter.
Returns:	returnSpanSetList : `list` List of SpanSets with artifacts.

prepareInputs(refList)¶

Prepare the input warps for coaddition by measuring the weight for each warp and the scaling for the photometric zero point.

Each Warp has its own photometric zeropoint and background variance. Before coadding these Warps together, compute a scale factor to normalize the photometric zeropoint and compute the weight for each Warp.

Parameters:	refList : `list` List of data references to tempExp
Returns:	result : `lsst.pipe.base.Struct` Result struct with components: `tempExprefList`: `list` of data references to tempExp. `weightList`: `list` of weightings. `imageScalerList`: `list` of image scalers.

prepareStats(mask=None)¶

Prepare the statistics for coadding images.

Parameters:	mask : `int`, optional Bit mask value to exclude from coaddition.
Returns:	stats : `lsst.pipe.base.Struct` Statistics structure with the following fields: `statsCtrl`: Statistics control object for coadd (`lsst.afw.math.StatisticsControl`) `statsFlags`: Statistic for coadd (`lsst.afw.math.Property`)

processResults(coaddExposure, dataRef)¶

Interpolate over missing data and mask bright stars.

Parameters:	coaddExposure : `lsst.afw.image.Exposure` The coadded exposure to process. dataRef : `lsst.daf.persistence.ButlerDataRef` Butler data reference for supplementary data.

readBrightObjectMasks(dataRef)¶

Retrieve the bright object masks.

Returns None on failure.

Parameters:	dataRef : `lsst.daf.persistence.butlerSubset.ButlerDataRef` A Butler dataRef.
Returns:	result : `lsst.daf.persistence.butlerSubset.ButlerDataRef` Bright object mask from the Butler object, or None if it cannot be retrieved.

removeMaskPlanes(maskedImage)¶

Unset the mask of an image for mask planes specified in the config.

Parameters:	maskedImage : `lsst.afw.image.MaskedImage` The masked image to be modified.

run(skyInfo, tempExpRefList, imageScalerList, weightList, supplementaryData, *args, **kwargs)¶

Assemble the coadd.

Find artifacts and apply them to the warps’ masks creating a list of alternative masks with a new “CLIPPED” plane and updated “NO_DATA” plane. Then pass these alternative masks to the base class’s run method.

Parameters:	skyInfo : `lsst.pipe.base.Struct` Patch geometry information. tempExpRefList : `list` List of data references to warps. imageScalerList : `list` List of image scalers. weightList : `list` List of weights. supplementaryData : `lsst.pipe.base.Struct` This Struct must contain a `templateCoadd` that serves as the model of the static sky.
Returns:	result : `lsst.pipe.base.Struct` Result struct with components: `coaddExposure`: coadded exposure (`lsst.afw.image.Exposure`). `nImage`: exposure count image (`lsst.afw.image.Image`), if requested.

runDataRef(dataRef, selectDataList=None, warpRefList=None)¶

Assemble a coadd from a set of Warps.

Pipebase.CmdlineTask entry point to Coadd a set of Warps. Compute weights to be applied to each Warp and find scalings to match the photometric zeropoint to a reference Warp. Assemble the Warps using run. Interpolate over NaNs and optionally write the coadd to disk. Return the coadded exposure.

Parameters:

dataRef : lsst.daf.persistence.butlerSubset.ButlerDataRef: Data reference defining the patch for coaddition and the reference Warp (if config.autoReference=False). Used to access the following data products: - self.config.coaddName + "Coadd_skyMap" - self.config.coaddName + "Coadd_ + <warpType> + "Warp" (optionally) - self.config.coaddName + "Coadd"
selectDataList : list: List of data references to Calexps. Data to be coadded will be selected from this list based on overlap with the patch defined by dataRef, grouped by visit, and converted to a list of data references to warps.
warpRefList : list: List of data references to Warps to be coadded. Note: warpRefList is just the new name for tempExpRefList.

Returns:

retStruct : lsst.pipe.base.Struct

Result struct with components:

coaddExposure: coadded exposure (Exposure).
nImage: exposure count image (Image).

runQuantum(quantum, butler)¶

Execute PipelineTask algorithm on single quantum of data.

Typical implementation of this method will use inputs from quantum to retrieve Python-domain objects from data butler and call adaptArgsAndRun method on that data. On return from adaptArgsAndRun this method will extract data from returned Struct instance and save that data to butler.

The Struct returned from adaptArgsAndRun is expected to contain data attributes with the names equal to the names of the configuration fields defining output dataset types. The values of the data attributes must be data objects corresponding to the DataIds of output dataset types. All data objects will be saved in butler using DataRefs from Quantum’s output dictionary.

This method does not return anything to the caller, on errors corresponding exception is raised.

Parameters:	quantum : `Quantum` Object describing input and output corresponding to this invocation of PipelineTask instance. butler : object Data butler instance.
Raises:	`ScalarError` if a dataset type is configured as scalar but receives multiple DataIds in `quantum`. Any exceptions that happen in data butler or in `adaptArgsAndRun` method.

saveStruct(struct, outputDataRefs, butler)¶

Save data in butler.

Convention is that struct returned from run() method has data field(s) with the same names as the config fields defining output DatasetTypes. Subclasses may override this method to implement different convention for Struct content or in case any post-processing of data may be needed.

Parameters:	struct : `Struct` Data produced by the task packed into `Struct` instance outputDataRefs : `dict` Dictionary whose keys are the names of the configuration fields describing output dataset types and values are lists of DataRefs. DataRefs must match corresponding data objects in `struct` in number and order. butler : object Data butler instance.

selectExposures(patchRef, skyInfo=None, selectDataList=[])¶

! @brief Select exposures to coadd

Get the corners of the bbox supplied in skyInfo using @ref afwGeom.Box2D and convert the pixel positions of the bbox corners to sky coordinates using @ref skyInfo.wcs.pixelToSky. Use the @ref WcsSelectImagesTask_ “WcsSelectImagesTask” to select exposures that lie inside the patch indicated by the dataRef.

@param[in] patchRef data reference for sky map patch. Must include keys “tract”, “patch”,: plus the camera-specific filter key (e.g. “filter” or “band”)

@param[in] skyInfo geometry for the patch; output from getSkyInfo @return a list of science exposures to coadd, as butler data references

setBrightObjectMasks(exposure, dataId, brightObjectMasks)¶

Set the bright object masks.

Parameters:	exposure : `lsst.afw.image.Exposure` Exposure under consideration. dataId : `lsst.daf.persistence.dataId` Data identifier dict for patch. brightObjectMasks : `lsst.afw.table` Table of bright objects to mask.

setInexactPsf(mask)¶

Set INEXACT_PSF mask plane.

If any of the input images isn’t represented in the coadd (due to clipped pixels or chip gaps), the CoaddPsf will be inexact. Flag these pixels.

Parameters:	mask : `lsst.afw.image.Mask` Coadded exposure’s mask, modified in-place.

static setRejectedMaskMapping(statsCtrl)¶

Map certain mask planes of the warps to new planes for the coadd.

If a pixel is rejected due to a mask value other than EDGE, NO_DATA, or CLIPPED, set it to REJECTED on the coadd. If a pixel is rejected due to EDGE, set the coadd pixel to SENSOR_EDGE. If a pixel is rejected due to CLIPPED, set the coadd pixel to CLIPPED.

Parameters:	statsCtrl : `lsst.afw.math.StatisticsControl` Statistics control object for coadd
Returns:	maskMap : `list` of `tuple` of `int` A list of mappings of mask planes of the warped exposures to mask planes of the coadd.

shrinkValidPolygons(coaddInputs)¶

Shrink coaddInputs’ ccds’ ValidPolygons in place.

Either modify each ccd’s validPolygon in place, or if CoaddInputs does not have a validPolygon, create one from its bbox.

Parameters:	coaddInputs : `lsst.afw.image.coaddInputs` Original mask.

timer(name, logLevel=10000)¶

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 `lsst.log` level constant.

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CompareWarpAssembleCoaddTask¶