CharacterizeImageTask¶
-
class
lsst.pipe.tasks.characterizeImage.
CharacterizeImageTask
(butler=None, refObjLoader=None, schema=None, **kwargs)¶ Bases:
lsst.pipe.base.PipelineTask
Measure 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
displayAstrometry
for 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
canMultiprocess
Methods 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. 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. getTaskDict
()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.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
-
canMultiprocess
= True¶
Methods Documentation
-
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:
exposure
Characterized exposure (
lsst.afw.image.ExposureF
).sourceCat
Detected sources (
lsst.afw.table.SourceCatalog
).background
Model of subtracted background (
lsst.afw.math.BackgroundList
).psfCellSet
Spatial cells of PSF candidates (
lsst.afw.math.SpatialCellSet
).
Raises: - LengthError
Raised if there are too many CR pixels.
-
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 :
-
emptyMetadata
() → None¶ Empty (clear) the metadata for this Task and all sub-Tasks.
-
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.- metadata :
-
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
() → Optional[ResourceConfig]¶ Return resource configuration for this task.
Returns: - Object of type
ResourceConfig
orNone
if resource - configuration is not defined for this task.
- Object of type
-
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) → 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")
- doc :
-
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 ofConfigurableField
orRegistryField
.- name :
-
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:
exposure
Characterized exposure (
lsst.afw.image.ExposureF
).sourceCat
Detected sources (
lsst.afw.table.SourceCatalog
).background
Model of subtracted background (
lsst.afw.math.BackgroundList
).psfCellSet
Spatial cells of PSF candidates (
lsst.afw.math.SpatialCellSet
).characterized
Another reference to
exposure
for compatibility.backgroundModel
Another reference to
background
for compatibility.
Raises: - RuntimeError
Raised if PSF sigma is NaN.
-
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
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
- butler :