PlotPhotonTransferCurveTask¶
- class lsst.cp.pipe.PlotPhotonTransferCurveTask(datasetFilename, linearizerFileName=None, outDir='.', detNum=999, signalElectronsRelativeA=75000, plotNormalizedCovariancesNumberOfBins=10)¶
Bases:
objectA class to plot the dataset from MeasurePhotonTransferCurveTask.
- Parameters:
- datasetFileName
str datasetPtc (lsst.ip.isr.PhotonTransferCurveDataset) file name (fits).
- linearizerFileName
str, optional linearizer (isr.linearize.Linearizer) file name (fits).
- outDir
str, optional Path to the output directory where the final PDF will be placed.
- detNum
int, optional Detector number.
- 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
plotNormalizedCovariancesNumberfunction (Fig. 8, 10., of Astier+19).
- datasetFileName
Methods Summary
ab_vs_dist(aDict, bDict, pdfPages[, bRange])Fig.
binData(x, y, binIndex[, wy])Bin data (usually for display purposes).
covAstierMakeAllPlots(dataset, pdfPages[, log])Make plots for MeasurePhotonTransferCurve task when doCovariancesAstier=True.
findGroups(x, maxDiff)Group data into bins, with at most maxDiff distance between bins.
indexForBins(x, nBins)Builds an index with regular binning.
plotAcoeffsSum(aDict, bDict, pdfPages)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, pdfPages[, bRange])Fig.
run(filenameFull, datasetPtc[, linearizer, log])Make the plots for the PTC task
Methods Documentation
- static ab_vs_dist(aDict, bDict, pdfPages, 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
ptcFitTypeisFULLCOVARIANCE).- bDict
dict[numpy.array] Dictionary keyed by amp names containing the fitted ‘b’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitTypeisFULLCOVARIANCE).- pdfPages
matplotlib.backends.backend_pdf.PdfPages PDF file where the plots will be saved.
- 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
- covAstierMakeAllPlots(dataset, pdfPages, log=None)¶
Make plots for MeasurePhotonTransferCurve task when doCovariancesAstier=True.
This function call other functions that mostly reproduce the plots in Astier+19. Most of the code is ported from Pierre Astier’s repository https://github.com/PierreAstier/bfptc
- Parameters:
- dataset
lsst.ip.isr.ptcDataset.PhotonTransferCurveDataset The dataset containing the necessary information to produce the plots.
- pdfPages
matplotlib.backends.backend_pdf.PdfPages PDF file where the plots will be saved.
- log
logging.Logger, optional Logger to handle messages
- dataset
- static findGroups(x, maxDiff)¶
Group data into bins, with at most maxDiff distance between bins.
- 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):
- static plotAcoeffsSum(aDict, bDict, pdfPages)¶
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
ptcFitTypeisFULLCOVARIANCE).- bDict
dict[numpy.array] Dictionary keyed by amp names containing the fitted ‘b’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitTypeisFULLCOVARIANCE).- pdfPages
matplotlib.backends.backend_pdf.PdfPages PDF file where the plots will be saved.
- aDict
- static plotCovariances(mu, covs, covsModel, covsWeights, covsNoB, covsModelNoB, covsWeightsNoB, gainDict, noiseDict, aDict, bDict, pdfPages)¶
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).
- pdfPages
matplotlib.backends.backend_pdf.PdfPages PDF file where the plots will be saved.
- mu
- plotNormalizedCovariances(i, j, inputMu, covs, covsModel, covsWeights, covsNoB, covsModelNoB, covsWeightsNoB, pdfPages, offset=0.004, numberOfBins=10, plotData=True, topPlot=False, log=None)¶
Plot C_ij/mu vs mu.
Figs. 8, 10, and 11 of Astier+19
- Parameters:
- i
int Covariane 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.
- pdfPages
matplotlib.backends.backend_pdf.PdfPages PDF file where the plots will be saved.
- 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?
- log
logging.Logger, optional Logger to handle messages.
- i
- static plotRelativeBiasACoeffs(aDict, aDictNoB, fullCovsModel, fullCovsModelNoB, signalElectrons, gainDict, pdfPages, 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.
- pdfPages
matplotlib.backends.backend_pdf.PdfPages PDF file where the plots will be saved.
- 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, pdfPages, 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
ptcFitTypeisFULLCOVARIANCE).- bDict
dict[numpy.array] Dictionary keyed by amp names containing the fitted ‘b’ coefficients from the model in Eq. 20 of Astier+19 (if
ptcFitTypeisFULLCOVARIANCE).- pdfPages
matplotlib.backends.backend_pdf.PdfPages PDF file where the plots will be saved.
- bRange
int Maximum lag for b arrays.
- aDict
- run(filenameFull, datasetPtc, linearizer=None, log=None)¶
Make the plots for the PTC task