DecorrelateALKernelMapper¶
-
class
lsst.ip.diffim.
DecorrelateALKernelMapper
(*args, **kwargs)¶ Bases:
lsst.ip.diffim.DecorrelateALKernelTask
,lsst.ip.diffim.ImageMapper
Task to be used as an ImageMapper for performing A&L decorrelation on subimages on a grid across a A&L difference image.
This task subclasses DecorrelateALKernelTask in order to implement all of that task’s configuration parameters, as well as its
run
method.Methods Summary
computeCorrectedDiffimPsf
(kappa, psf[, …])Compute the (decorrelated) difference image’s new PSF. computeVarianceMean
(exposure)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. getSchemaCatalogs
()Get the schemas generated by 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
(subExposure, expandedSubExposure, …[, …])Perform decorrelation operation on subExposure
, usingexpandedSubExposure
to allow for invalid edge pixels arising from convolutions.timer
(name[, logLevel])Context manager to log performance data for an arbitrary block of code. Methods Documentation
-
static
computeCorrectedDiffimPsf
(kappa, psf, svar=0.04, tvar=0.04)¶ Compute the (decorrelated) difference image’s new PSF. new_psf = psf(k) * sqrt((svar + tvar) / (svar + tvar * kappa_ft(k)**2))
Parameters: - kappa :
numpy.ndarray
A matching kernel array derived from Alard & Lupton PSF matching
- psf :
numpy.ndarray
The uncorrected psf array of the science image (and also of the diffim)
- svar :
float
, optional Average variance of science image used for PSF matching
- tvar :
float
, optional Average variance of template image used for PSF matching
Returns: - pcf :
numpy.ndarray
a 2-d numpy.array containing the new PSF
- kappa :
-
computeVarianceMean
(exposure)¶
-
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.
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 :
-
getFullMetadata
()¶ Get metadata for all tasks.
Returns: - metadata :
lsst.daf.base.PropertySet
The
PropertySet
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
()¶ 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 :
-
getSchemaCatalogs
()¶ 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 implemenation 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 :
-
getTaskDict
()¶ 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)¶ 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("a brief description of what this task does")
- doc :
-
makeSubtask
(name, **keyArgs)¶ 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 of pex_config ConfigurableField or RegistryField.- name :
-
run
(subExposure, expandedSubExposure, fullBBox, template, science, alTaskResult=None, psfMatchingKernel=None, preConvKernel=None, **kwargs)¶ Perform decorrelation operation on
subExposure
, usingexpandedSubExposure
to allow for invalid edge pixels arising from convolutions.This method performs A&L decorrelation on
subExposure
using local measures for image variances and PSF.subExposure
is a sub-exposure of the non-decorrelated A&L diffim. It also requires the corresponding sub-exposures of the template (template
) and science (science
) exposures.Parameters: - subExposure :
lsst.afw.image.Exposure
the sub-exposure of the diffim
- expandedSubExposure :
lsst.afw.image.Exposure
the expanded sub-exposure upon which to operate
- fullBBox :
lsst.geom.Box2I
the bounding box of the original exposure
- template :
lsst.afw.image.Exposure
the corresponding sub-exposure of the template exposure
- science :
lsst.afw.image.Exposure
the corresponding sub-exposure of the science exposure
- alTaskResult :
lsst.pipe.base.Struct
the result of A&L image differencing on
science
andtemplate
, importantly containing the resultingpsfMatchingKernel
. Can beNone
, only ifpsfMatchingKernel
is notNone
.- psfMatchingKernel : Alternative parameter for passing the
A&L
psfMatchingKernel
directly.- preConvKernel : If not None, then pre-filtering was applied
to science exposure, and this is the pre-convolution kernel.
- kwargs :
additional keyword arguments propagated from
ImageMapReduceTask.run
.
Returns: - A `pipeBase.Struct` containing:
subExposure
: the result of thesubExposure
processing.decorrelationKernel
: the decorrelation kernel, currently- not used.
Notes
This
run
method accepts parameters identical to those ofImageMapper.run
, since it is called from theImageMapperTask
. See that class for more information.- subExposure :
-
timer
(name, logLevel=10000)¶ Context manager to log performance data for an arbitrary block of code.
Parameters: - name :
str
Name of code being timed; data will be logged using item name:
Start
andEnd
.- logLevel
A
lsst.log
level constant.
See also
timer.logInfo
Examples
Creating a timer context:
with self.timer("someCodeToTime"): pass # code to time
- name :
-
static