PlotPhotonTransferCurveTask¶
- class lsst.cp.pipe.PlotPhotonTransferCurveTask(*, config: PipelineTaskConfig | None = None, log: logging.Logger | LsstLogAdapter | None = None, initInputs: dict[str, Any] | None = None, **kwargs: Any)¶
Bases:
PipelineTask
A class to plot the dataset from MeasurePhotonTransferCurveTask.
- Parameters:
- outDir
str
, optional Path to the output directory where the final PDF will be placed.
- signalElectronsRelativeA
float
, optional Signal value for relative systematic bias between different methods of estimating a_ij (Fig. 15 of Astier+19).
- plotNormalizedCovariancesNumberOfBins
float
, optional Number of bins in
plotNormalizedCovariancesNumber
function (Fig. 8, 10., of Astier+19).
- outDir
Notes
See DM-36388 for usage exammple.
Attributes Summary
Methods Summary
ab_vs_dist
(aDict, bDict[, bRange])Fig.
binData
(x, y, binIndex[, wy])Bin data (usually for display purposes).
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.
indexForBins
(x, nBins)Builds an index with regular binning.
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.plotAcoeffsSum
(aDict, bDict)Fig.
plotCovariances
(mu, covs, covsModel, ...)Plot covariances and models: Cov00, Cov10, Cov01.
plotNormalizedCovariances
(i, j, inputMu, ...)Plot C_ij/mu vs mu.
plotRelativeBiasACoeffs
(aDict, aDictNoB, ...)Fig.
plot_a_b
(aDict, bDict[, bRange])Fig.
run
(inputPtcDataset[, camera])Make the plots for the PTC task.
runQuantum
(butlerQC, inputRefs, outputRefs)Do butler IO and transform 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
Methods Documentation
- static ab_vs_dist(aDict, bDict, bRange=4)¶
Fig. 13 of Astier+19.
Values of a and b arrays fits, averaged over amplifiers, as a function of distance.
- Parameters:
- aDict
dict
[numpy.array
] Dictionary keyed by amp names containing the fitted ‘a’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitType
isFULLCOVARIANCE
).- bDict
dict
[numpy.array
] Dictionary keyed by amp names containing the fitted ‘b’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitType
isFULLCOVARIANCE
).- bRange
int
Maximum lag for b arrays.
- aDict
- static binData(x, y, binIndex, wy=None)¶
Bin data (usually for display purposes).
- Parameters:
- x
numpy.array
Data to bin.
- y
numpy.array
Data to bin.
- binIdex
list
Bin number of each datum.
- wy
numpy.array
Inverse rms of each datum to use when averaging (the actual weight is wy**2).
- x
- Returns:
- xbin
numpy.array
Binned data in x.
- ybin
numpy.array
Binned data in y.
- wybin
numpy.array
Binned weights in y, computed from wy’s in each bin.
- sybin
numpy.array
Uncertainty on the bin average, considering actual scatter, and ignoring weights.
- xbin
- 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
- 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
- static indexForBins(x, nBins)¶
Builds an index with regular binning. The result can be fed into binData.
- Parameters:
- x
numpy.array
Data to bin.
- nBins
int
Number of bin.
- x
- Returns:
- np.digitize(x, bins):
numpy.array
Bin indices.
- np.digitize(x, bins):
- 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
.
- static plotAcoeffsSum(aDict, bDict)¶
Fig. 14. of Astier+19
Cumulative sum of a_ij as a function of maximum separation. This plot displays the average over channels.
- Parameters:
- aDict
dict
[numpy.array
] Dictionary keyed by amp names containing the fitted ‘a’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitType
isFULLCOVARIANCE
).- bDict
dict
[numpy.array
] Dictionary keyed by amp names containing the fitted ‘b’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitType
isFULLCOVARIANCE
).
- aDict
- static plotCovariances(mu, covs, covsModel, covsWeights, covsNoB, covsModelNoB, covsWeightsNoB, gainDict, noiseDict, aDict, bDict)¶
Plot covariances and models: Cov00, Cov10, Cov01.
Figs. 6 and 7 of Astier+19
- Parameters:
- mu
dict
[str
,list
] Dictionary keyed by amp name with mean signal values.
- covs
dict
[str
,list
] Dictionary keyed by amp names containing a list of measued covariances per mean flux.
- covsModel
dict
[str
,list
] Dictionary keyed by amp names containinging covariances model (Eq. 20 of Astier+19) per mean flux.
- covsWeights
dict
[str
,list
] Dictionary keyed by amp names containinging sqrt. of covariances weights.
- covsNoB
dict
[str
,list
] Dictionary keyed by amp names containing a list of measued covariances per mean flux (‘b’=0 in Astier+19).
- covsModelNoB
dict
[str
,list
] Dictionary keyed by amp names containing covariances model (with ‘b’=0 in Eq. 20 of Astier+19) per mean flux.
- covsWeightsNoB
dict
[str
,list
] Dictionary keyed by amp names containing sqrt. of covariances weights (‘b’ = 0 in Eq. 20 of Astier+19).
- gainDict
dict
[str
,float
] Dictionary keyed by amp names containing the gains in e-/ADU.
- noiseDict
dict
[str
,float
] Dictionary keyed by amp names containing the rms redout noise in e-.
- aDict
dict
[str
,numpy.array
] Dictionary keyed by amp names containing ‘a’ coefficients (Eq. 20 of Astier+19).
- bDict
dict
[str
,numpy.array
] Dictionary keyed by amp names containing ‘b’ coefficients (Eq. 20 of Astier+19).
- mu
- plotNormalizedCovariances(i, j, inputMu, covs, covsModel, covsWeights, covsNoB, covsModelNoB, covsWeightsNoB, offset=0.004, numberOfBins=10, plotData=True, topPlot=False)¶
Plot C_ij/mu vs mu.
Figs. 8, 10, and 11 of Astier+19
- Parameters:
- i
int
Covariance lag.
- j
int
Covariance lag.
- inputMu
dict
[str
,list
] Dictionary keyed by amp name with mean signal values.
- covs
dict
[str
,list
] Dictionary keyed by amp names containing a list of measued covariances per mean flux.
- covsModel
dict
[str
,list
] Dictionary keyed by amp names containinging covariances model (Eq. 20 of Astier+19) per mean flux.
- covsWeights
dict
[str
,list
] Dictionary keyed by amp names containinging sqrt. of covariances weights.
- covsNoB
dict
[str
,list
] Dictionary keyed by amp names containing a list of measued covariances per mean flux (‘b’=0 in Astier+19).
- covsModelNoB
dict
[str
,list
] Dictionary keyed by amp names containing covariances model (with ‘b’=0 in Eq. 20 of Astier+19) per mean flux.
- covsWeightsNoB
dict
[str
,list
] Dictionary keyed by amp names containing sqrt. of covariances weights (‘b’ = 0 in Eq. 20 of Astier+19).
- expIdMask
dict
[str
,list
] Dictionary keyed by amp names containing the masked exposure pairs.
- offset
float
, optional Constant offset factor to plot covariances in same panel (so they don’t overlap).
- numberOfBins
int
, optional Number of bins for top and bottom plot.
- plotData
bool
, optional Plot the data points?
- topPlot
bool
, optional Plot the top plot with the covariances, and the bottom plot with the model residuals?
- i
- static plotRelativeBiasACoeffs(aDict, aDictNoB, fullCovsModel, fullCovsModelNoB, signalElectrons, gainDict, maxr=None)¶
Fig. 15 in Astier+19.
Illustrates systematic bias from estimating ‘a’ coefficients from the slope of correlations as opposed to the full model in Astier+19.
- Parameters:
- aDict
dict
Dictionary of ‘a’ matrices (Eq. 20, Astier+19), with amp names as keys.
- aDictNoB
dict
Dictionary of ‘a’ matrices (‘b’= 0 in Eq. 20, Astier+19), with amp names as keys.
- fullCovsModel
dict
[str
,list
] Dictionary keyed by amp names containing covariances model per mean flux.
- fullCovsModelNoB
dict
[str
,list
] Dictionary keyed by amp names containing covariances model (with ‘b’=0 in Eq. 20 of Astier+19) per mean flux.
- signalElectrons
float
Signal at which to evaluate the a_ij coefficients.
- gainDict
dict
[str
,float
] Dicgionary keyed by amp names with the gains in e-/ADU.
- maxr
int
, optional Maximum lag.
- aDict
- static plot_a_b(aDict, bDict, bRange=3)¶
Fig. 12 of Astier+19
Color display of a and b arrays fits, averaged over channels.
- Parameters:
- aDict
dict
[numpy.array
] Dictionary keyed by amp names containing the fitted ‘a’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitType
isFULLCOVARIANCE
).- bDict
dict
[numpy.array
] Dictionary keyed by amp names containing the fitted ‘b’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitType
isFULLCOVARIANCE
).- bRange
int
Maximum lag for b arrays.
- aDict
- run(inputPtcDataset, camera=None)¶
Make the plots for the PTC task.
- Parameters:
- inputPtcDataset
lsst.ip.isr.PhotonTransferCurveDataset
Output dataset from Photon Transfer Curve task.
- camera
lsst.afw.cameraGeom.Camera
Camera to use for camera geometry information.
- inputPtcDataset
- runQuantum(butlerQC, inputRefs, outputRefs)¶
Do butler IO and transform to provide in memory objects for tasks
run
method.- Parameters:
- butlerQC
QuantumContext
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