CharacterizeImageTask¶
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class
lsst.pipe.tasks.characterizeImage.CharacterizeImageTask(butler=None, refObjLoader=None, schema=None, **kwargs)¶ Bases:
lsst.pipe.base.PipelineTaskMeasure bright sources and use this to estimate background and PSF of an exposure.
Given an exposure with defects repaired (masked and interpolated over, e.g. as output by
IsrTask): - detect and measure bright sources - repair cosmic rays - measure and subtract background - measure PSFParameters: - butler :
None Compatibility parameter. Should always be
None.- refObjLoader :
lsst.meas.algorithms.ReferenceObjectLoader, optional Reference object loader if using a catalog-based star-selector.
- schema :
lsst.afw.table.Schema, optional Initial schema for icSrc catalog.
- **kwargs
Additional keyword arguments.
Notes
Debugging: CharacterizeImageTask has a debug dictionary with the following keys:
- frame
- int: if specified, the frame of first debug image displayed (defaults to 1)
- repair_iter
- bool; if True display image after each repair in the measure PSF loop
- background_iter
- bool; if True display image after each background subtraction in the measure PSF loop
- measure_iter
- bool; if True display image and sources at the end of each iteration of the measure PSF loop
See
displayAstrometryfor the meaning of the various symbols. - psf
- bool; if True display image and sources after PSF is measured; this will be identical to the final image displayed by measure_iter if measure_iter is true
- repair
- bool; if True display image and sources after final repair
- measure
- bool; if True display image and sources after final measurement
Attributes Summary
canMultiprocessMethods Summary
detectMeasureAndEstimatePsf(exposure, …)Perform one iteration of detect, measure, and estimate PSF. display(itemName, exposure[, sourceCat])Display exposure and sources on next frame (for debugging). emptyMetadata()Empty (clear) the metadata for this Task and all sub-Tasks. 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()Return a dict of empty catalogs for each catalog dataset produced by this task. getTaskDict()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.run(exposure[, exposureIdInfo, background])Characterize a science image. 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
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canMultiprocess= True¶
Methods Documentation
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detectMeasureAndEstimatePsf(exposure, exposureIdInfo, background)¶ Perform one iteration of detect, measure, and estimate PSF.
Performs the following operations:
if config.doMeasurePsf or not exposure.hasPsf():
- install a simple PSF model (replacing the existing one, if need be)
interpolate over cosmic rays with keepCRs=True
estimate background and subtract it from the exposure
detect, deblend and measure sources, and subtract a refined background model;
- if config.doMeasurePsf:
- measure PSF
Parameters: - exposure :
lsst.afw.image.ExposureF Exposure to characterize.
- exposureIdInfo :
lsst.obs.baseExposureIdInfo Exposure ID info.
- background :
lsst.afw.math.BackgroundList, optional Initial model of background already subtracted from exposure.
Returns: - result :
lsst.pipe.base.Struct Results as a struct with attributes:
exposureCharacterized exposure (
lsst.afw.image.ExposureF).sourceCatDetected sources (
lsst.afw.table.SourceCatalog).backgroundModel of subtracted background (
lsst.afw.math.BackgroundList).psfCellSetSpatial cells of PSF candidates (
lsst.afw.math.SpatialCellSet).
Raises: - LengthError
Raised if there are too many CR pixels.
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display(itemName, exposure, sourceCat=None)¶ Display exposure and sources on next frame (for debugging).
Parameters: - itemName :
str Name of item in
debugInfo.- exposure :
lsst.afw.image.ExposureF Exposure to display.
- sourceCat :
lsst.afw.table.SourceCatalog, optional Catalog of sources detected on the exposure.
- itemName :
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emptyMetadata() → None¶ Empty (clear) the metadata for this Task and all sub-Tasks.
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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.tableCatalog 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.- schemacatalogs :
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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.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.- metadata :
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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 :
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getResourceConfig() → Optional[ResourceConfig]¶ Return resource configuration for this task.
Returns: - Object of type
ResourceConfigorNoneif resource - configuration is not defined for this task.
- Object of type
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getSchemaCatalogs()¶ Return a dict of empty catalogs for each catalog dataset produced by this task.
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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.
- taskDict :
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classmethod
makeField(doc: str) → lsst.pex.config.configurableField.ConfigurableField¶ Make a
lsst.pex.config.ConfigurableFieldfor this task.Parameters: - doc :
str Help text for the field.
Returns: - configurableField :
lsst.pex.config.ConfigurableField A
ConfigurableFieldfor 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")
- doc :
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makeSubtask(name: str, **keyArgs) → 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”.
Notes
The subtask must be defined by
Task.config.name, an instance ofConfigurableFieldorRegistryField.- name :
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run(exposure, exposureIdInfo=None, background=None)¶ Characterize a science image.
Peforms the following operations: - Iterate the following config.psfIterations times, or once if config.doMeasurePsf false:
- detect and measure sources and estimate PSF (see detectMeasureAndEstimatePsf for details)
- interpolate over cosmic rays
- perform final measurement
Parameters: - exposure :
lsst.afw.image.ExposureF Exposure to characterize.
- exposureIdInfo :
lsst.obs.baseExposureIdInfo, optional Exposure ID info. If not provided, returned SourceCatalog IDs will not be globally unique.
- background :
lsst.afw.math.BackgroundList, optional Initial model of background already subtracted from exposure.
Returns: - result :
lsst.pipe.base.Struct Results as a struct with attributes:
exposureCharacterized exposure (
lsst.afw.image.ExposureF).sourceCatDetected sources (
lsst.afw.table.SourceCatalog).backgroundModel of subtracted background (
lsst.afw.math.BackgroundList).psfCellSetSpatial cells of PSF candidates (
lsst.afw.math.SpatialCellSet).characterizedAnother reference to
exposurefor compatibility.backgroundModelAnother reference to
backgroundfor compatibility.
Raises: - RuntimeError
Raised if PSF sigma is NaN.
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runQuantum(butlerQC, inputRefs, outputRefs)¶ 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
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 :
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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
- butler :