isrFunctions.py File Reference

Go to the source code of this file.

Namespaces
namespace	lsst
namespace	lsst::ip
namespace	lsst::ip::isr
namespace	lsst.ip.isr.isrFunctions

Functions
	lsst.ip.isr.isrFunctions.createPsf (fwhm)
	lsst.ip.isr.isrFunctions.transposeMaskedImage (maskedImage)
	lsst.ip.isr.isrFunctions.interpolateDefectList (maskedImage, defectList, fwhm, fallbackValue=None, maskNameList=None, useLegacyInterp=True)
	lsst.ip.isr.isrFunctions.makeThresholdMask (maskedImage, threshold, growFootprints=1, maskName='SAT')
	lsst.ip.isr.isrFunctions.growMasks (mask, radius=0, maskNameList=['BAD'], maskValue="BAD")
	lsst.ip.isr.isrFunctions.maskITLEdgeBleed (ccdExposure, badAmpDict, fpCore, itlEdgeBleedSatMinArea=10000, itlEdgeBleedSatMaxArea=100000, itlEdgeBleedThreshold=5000., itlEdgeBleedModelConstant=0.02, saturatedMaskName="SAT", log=None)
	lsst.ip.isr.isrFunctions._applyMaskITLEdgeBleed (ccdExposure, xCore, satLevel, widthSat, itlEdgeBleedThreshold=5000., itlEdgeBleedModelConstant=0.03, saturatedMaskName="SAT", log=None)
	lsst.ip.isr.isrFunctions.maskITLSatSag (ccdExposure, fpCore, saturatedMaskName="SAT")
	lsst.ip.isr.isrFunctions.maskITLDip (exposure, detectorConfig, maskPlaneNames=["SUSPECT", "ITL_DIP"], log=None)
	lsst.ip.isr.isrFunctions.interpolateFromMask (maskedImage, fwhm, growSaturatedFootprints=1, maskNameList=['SAT'], fallbackValue=None, useLegacyInterp=True)
	lsst.ip.isr.isrFunctions.saturationCorrection (maskedImage, saturation, fwhm, growFootprints=1, interpolate=True, maskName='SAT', fallbackValue=None, useLegacyInterp=True)
	lsst.ip.isr.isrFunctions.trimToMatchCalibBBox (rawMaskedImage, calibMaskedImage)
	lsst.ip.isr.isrFunctions.biasCorrection (maskedImage, biasMaskedImage, trimToFit=False)
	lsst.ip.isr.isrFunctions.darkCorrection (maskedImage, darkMaskedImage, expScale, darkScale, invert=False, trimToFit=False)
	lsst.ip.isr.isrFunctions.updateVariance (maskedImage, gain, readNoise, replace=True)
	lsst.ip.isr.isrFunctions.flatCorrection (maskedImage, flatMaskedImage, scalingType, userScale=1.0, invert=False, trimToFit=False)
	lsst.ip.isr.isrFunctions.illuminationCorrection (maskedImage, illumMaskedImage, illumScale, trimToFit=True)
	lsst.ip.isr.isrFunctions.brighterFatterCorrection (exposure, kernel, maxIter, threshold, applyGain, gains=None)
	lsst.ip.isr.isrFunctions.transferFlux (cFunc, fStep, correctionMode=True)
	lsst.ip.isr.isrFunctions.fluxConservingBrighterFatterCorrection (exposure, kernel, maxIter, threshold, applyGain, gains=None, correctionMode=True)
	lsst.ip.isr.isrFunctions.gainContext (exp, image, apply, gains=None, invert=False, isTrimmed=True)
	lsst.ip.isr.isrFunctions.attachTransmissionCurve (exposure, opticsTransmission=None, filterTransmission=None, sensorTransmission=None, atmosphereTransmission=None)
	lsst.ip.isr.isrFunctions.applyGains (exposure, normalizeGains=False, ptcGains=None, isTrimmed=True)
	lsst.ip.isr.isrFunctions.widenSaturationTrails (mask)
	lsst.ip.isr.isrFunctions.setBadRegions (exposure, badStatistic="MEDIAN")
	lsst.ip.isr.isrFunctions.checkFilter (exposure, filterList, log)
	lsst.ip.isr.isrFunctions.getPhysicalFilter (filterLabel, log)
	lsst.ip.isr.isrFunctions.countMaskedPixels (maskedIm, maskPlane)
	lsst.ip.isr.isrFunctions.getExposureGains (exposure)
	lsst.ip.isr.isrFunctions.getExposureReadNoises (exposure)
	lsst.ip.isr.isrFunctions.isTrimmedExposure (exposure)
	lsst.ip.isr.isrFunctions.isTrimmedImage (image, detector)