CloughTocher2DInterpolateTask¶
- class lsst.pipe.tasks.interpImage.CloughTocher2DInterpolateTask(config: Config | None = None, *, name: str | None = None, parentTask: Task | None = None, log: logging.Logger | lsst.utils.logging.LsstLogAdapter | None = None)¶
Bases:
Task
Interpolated over bad pixels using CloughTocher2DInterpolator.
Pixels with mask bits set to any of those listed
badMaskPlanes
config are considered bad and are interpolated over. All good (non-bad) pixels withininterpLength
pixels of a bad pixel in either direction are used to construct the interpolant. An extended streak of bad pixels at an edge, longer thaninterpLength
, is set tofillValue`
specified in config.Methods Summary
Empty (clear) the metadata for this Task and all sub-Tasks.
Get metadata for all tasks.
Get the task name as a hierarchical name including parent task names.
getName
()Get the name of the task.
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
(maskedImage[, badpix, goodpix])Interpolate over bad pixels in a masked image.
timer
(name[, logLevel])Context manager to log performance data for an arbitrary block of code.
Methods Documentation
- getFullMetadata() 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.
- metadata
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() 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
- getName() str ¶
Get the name of the task.
- Returns:
- taskName
str
Name of the task.
- taskName
See also
getFullName
Get the full name of the task.
- 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) ConfigurableField ¶
Make a
lsst.pex.config.ConfigurableField
for this task.- Parameters:
- doc
str
Help text for the field.
- doc
- Returns:
- configurableField
lsst.pex.config.ConfigurableField
A
ConfigurableField
for this task.
- configurableField
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")
- makeSubtask(name: str, **keyArgs: Any) 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
.
- name
Notes
The subtask must be defined by
Task.config.name
, an instance ofConfigurableField
orRegistryField
.
- run(maskedImage, badpix: set[tuple[int, int]] | None = None, goodpix: dict | None = None)¶
Interpolate over bad pixels in a masked image.
This modifies the
image
attribute of themaskedImage
in place. This method returns, and accepts, the coordinates of the bad pixels that were interpolated over, and the coordinates and values of the good pixels that were used to construct the interpolant. This avoids having to search for the bad and the good pixels repeatedly when the mask plane is shared among many images, as would be the case with noise realizations.- Parameters:
- maskedImage
MaskedImage
Image on which to perform interpolation (and modify in-place).
- badpix: `set` [`tuple` [`int`, `int`]], optional
The coordinates of the bad pixels to interpolate over. If None, then the coordinates of the bad pixels are determined by an exhaustive search over the image.
- goodpix: `dict` [`tuple` [`int`, `int`], `float`], optional
A mapping whose keys are the coordinates of the good pixels around
badpix
that must be included when constructing the interpolant. Ifbadpix
is provided, then the pixels ingoodpix
are used as to construct the interpolatant. If not, any additional good pixels around internally determinedbadpix
are added togoodpix
and used to construct the interpolant. In all cases, the values are populated from the image plane of themaskedImage
(provided values will be ignored.
- maskedImage
- Returns:
- Raises:
- RuntimeError
If a pixel passed in as
goodpix
is found to be bad as specified bymaskPlanes
.- ValueError
If an input
badpix
is not found to be bad as specified bymaskPlanes
.