IsrStatisticsTask¶
-
class
lsst.ip.isr.
IsrStatisticsTask
(statControl=None, **kwargs)¶ Bases:
lsst.pipe.base.Task
Task to measure arbitrary statistics on ISR processed exposures.
The goal is to wrap a number of optional measurements that are useful for calibration production and detector stability.
Methods Summary
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. getTaskDict
()Get a dictionary of all tasks as a shallow copy. makeField
(doc)Make a lsst.pex.config.ConfigurableField
for this task.makeKernel
(kernelSize)Make a boxcar smoothing kernel. makeSubtask
(name, **keyArgs)Create a subtask as a new instance as the name
attribute of this task.measureBanding
(inputExp, overscans)Task to measure banding statistics. measureCti
(inputExp, overscans, gains)Task to measure CTI statistics. measureProjectionStatistics
(inputExp, overscans)Task to measure metrics from image slicing. run
(inputExp[, ptc, overscanResults])Task to run arbitrary statistics. 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.
-
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 :
-
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 :
-
static
makeKernel
(kernelSize)¶ Make a boxcar smoothing kernel.
Parameters: - kernelSize :
int
Size of the kernel in pixels.
Returns: - kernel :
np.array
Kernel for boxcar smoothing.
- kernelSize :
-
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 :
-
measureBanding
(inputExp, overscans)¶ Task to measure banding statistics.
Parameters: - inputExp :
lsst.afw.image.Exposure
Exposure to measure.
- overscans :
list
[lsst.pipe.base.Struct
] List of overscan results. Expected fields are:
imageFit
Value or fit subtracted from the amplifier image data (scalar or
lsst.afw.image.Image
).overscanFit
Value or fit subtracted from the overscan image data (scalar or
lsst.afw.image.Image
).overscanImage
Image of the overscan region with the overscan correction applied (
lsst.afw.image.Image
). This quantity is used to estimate the amplifier read noise empirically.
Returns: - inputExp :
-
measureCti
(inputExp, overscans, gains)¶ Task to measure CTI statistics.
Parameters: - inputExp :
lsst.afw.image.Exposure
Exposure to measure.
- overscans :
list
[lsst.pipe.base.Struct
] List of overscan results. Expected fields are:
imageFit
Value or fit subtracted from the amplifier image data (scalar or
lsst.afw.image.Image
).overscanFit
Value or fit subtracted from the overscan image data (scalar or
lsst.afw.image.Image
).overscanImage
Image of the overscan region with the overscan correction applied (
lsst.afw.image.Image
). This quantity is used to estimate the amplifier read noise empirically.
- gains :
dict
[str
float
] Dictionary of per-amplifier gains, indexed by amplifier name.
Returns: - inputExp :
-
measureProjectionStatistics
(inputExp, overscans)¶ Task to measure metrics from image slicing.
Parameters: - inputExp :
lsst.afw.image.Exposure
Exposure to measure.
- overscans :
list
[lsst.pipe.base.Struct
] List of overscan results. Expected fields are:
imageFit
Value or fit subtracted from the amplifier image data (scalar or
lsst.afw.image.Image
).overscanFit
Value or fit subtracted from the overscan image data (scalar or
lsst.afw.image.Image
).overscanImage
Image of the overscan region with the overscan correction applied (
lsst.afw.image.Image
). This quantity is used to estimate the amplifier read noise empirically.
Returns: - inputExp :
-
run
(inputExp, ptc=None, overscanResults=None, **kwargs)¶ Task to run arbitrary statistics.
The statistics should be measured by individual methods, and add to the dictionary in the return struct.
Parameters: - inputExp :
lsst.afw.image.Exposure
The exposure to measure.
- ptc :
lsst.ip.isr.PtcDataset
, optional A PTC object containing gains to use.
- overscanResults :
list
[lsst.pipe.base.Struct
], optional List of overscan results. Expected fields are:
imageFit
Value or fit subtracted from the amplifier image data (scalar or
lsst.afw.image.Image
).overscanFit
Value or fit subtracted from the overscan image data (scalar or
lsst.afw.image.Image
).overscanImage
Image of the overscan region with the overscan correction applied (
lsst.afw.image.Image
). This quantity is used to estimate the amplifier read noise empirically.
Returns: - resultStruct :
lsst.pipe.base.Struct
Contains the measured statistics as a dict stored in a field named
results
.
Raises: - RuntimeError
Raised if the amplifier gains could not be found.
- inputExp :
-
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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