DeferredChargeTask¶
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class
lsst.ip.isr.
DeferredChargeTask
(config: Optional[Config] = None, name: Optional[str] = None, parentTask: Optional[Task] = None, log: Optional[Union[logging.Logger, lsst.utils.logging.LsstLogAdapter]] = None)¶ Bases:
lsst.pipe.base.Task
Task to correct an exposure for charge transfer inefficiency.
This uses the methods described by Snyder et al. 2021, Journal of Astronimcal Telescopes, Instruments, and Systems, 7, 048002. doi:10.1117/1.JATIS.7.4.048002 (Snyder+21).
Methods Summary
emptyMetadata
()Empty (clear) the metadata for this Task and all sub-Tasks. flipData
(ampData, amp)Flip data array such that readout corner is at lower-left. 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. getSchemaCatalogs
()Get the schemas generated by this task. getTaskDict
()Get a dictionary of all tasks as a shallow copy. local_offset_inverse
(inputArr, drift_scale, …)Remove CTI effects from local offsets. local_trap_inverse
(inputArr, trap[, …])Apply localized trapping inverse operator to pixel signals. 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, ctiCalib[, gains])Correct deferred charge/CTI issues. timer
(name, logLevel)Context manager to log performance data for an arbitrary block of code. Methods Documentation
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emptyMetadata
() → None¶ Empty (clear) the metadata for this Task and all sub-Tasks.
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static
flipData
(ampData, amp)¶ Flip data array such that readout corner is at lower-left.
Parameters: - ampData :
numpy.ndarray
, (nx, ny) Image data to flip.
- amp :
lsst.afw.cameraGeom.Amplifier
Amplifier to get readout corner information.
Returns: - ampData :
numpy.ndarray
, (nx, ny) Flipped image data.
- ampData :
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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.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.- 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.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 :
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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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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.
- schemaCatalogs :
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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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static
local_offset_inverse
(inputArr, drift_scale, decay_time, num_previous_pixels=15)¶ Remove CTI effects from local offsets.
This implements equation 10 of Snyder+21. For an image with CTI, s’(m, n), the correction factor is equal to the maximum value of the set of:
Parameters: - inputArr :
numpy.ndarray
, (nx, ny) Input image data to correct.
- drift_scale :
float
Drift scale (Snyder+21 A_L value) to use in correction.
- decay_time :
float
Decay time (Snyder+21 tau_L) of the correction.
- num_previous_pixels :
int
, optional Number of previous pixels to use for correction. As the CTI has an exponential decay, this essentially truncates the correction where that decay scales the input charge to near zero.
Returns: - outputArr :
numpy.ndarray
, (nx, ny) Corrected image data.
- inputArr :
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static
local_trap_inverse
(inputArr, trap, global_cti=0.0, num_previous_pixels=6)¶ Apply localized trapping inverse operator to pixel signals.
This implements equation 13 of Snyder+21. For an image with CTI, s’(m, n), the correction factor is equal to the maximum value of the set of:
Parameters: - inputArr :
numpy.ndarray
, (nx, ny) Input image data to correct.
- trap :
lsst.ip.isr.SerialTrap
Serial trap describing the capture and release of charge.
- global_cti: `float`
Mean charge transfer inefficiency, b from Snyder+21.
- num_previous_pixels :
int
, optional Number of previous pixels to use for correction.
Returns: - outputArr :
numpy.ndarray
, (nx, ny) Corrected image data.
- inputArr :
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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 :
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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 :
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run
(exposure, ctiCalib, gains=None)¶ Correct deferred charge/CTI issues.
Parameters: - exposure :
lsst.afw.image.Exposure
Exposure to correct the deferred charge on.
- ctiCalib :
lsst.ip.isr.DeferredChargeCalib
Calibration object containing the charge transfer inefficiency model.
- gains :
dict
[str
,float
] A dictionary, keyed by amplifier name, of the gains to use. If gains is None, the nominal gains in the amplifier object are used.
Returns: - exposure :
lsst.afw.image.Exposure
The corrected exposure.
- exposure :
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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
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