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LSSTApplications
17.0+11,17.0+34,17.0+56,17.0+57,17.0+59,17.0+7,17.0-1-g377950a+33,17.0.1-1-g114240f+2,17.0.1-1-g4d4fbc4+28,17.0.1-1-g55520dc+49,17.0.1-1-g5f4ed7e+52,17.0.1-1-g6dd7d69+17,17.0.1-1-g8de6c91+11,17.0.1-1-gb9095d2+7,17.0.1-1-ge9fec5e+5,17.0.1-1-gf4e0155+55,17.0.1-1-gfc65f5f+50,17.0.1-1-gfc6fb1f+20,17.0.1-10-g87f9f3f+1,17.0.1-11-ge9de802+16,17.0.1-16-ga14f7d5c+4,17.0.1-17-gc79d625+1,17.0.1-17-gdae4c4a+8,17.0.1-2-g26618f5+29,17.0.1-2-g54f2ebc+9,17.0.1-2-gf403422+1,17.0.1-20-g2ca2f74+6,17.0.1-23-gf3eadeb7+1,17.0.1-3-g7e86b59+39,17.0.1-3-gb5ca14a,17.0.1-3-gd08d533+40,17.0.1-30-g596af8797,17.0.1-4-g59d126d+4,17.0.1-4-gc69c472+5,17.0.1-6-g5afd9b9+4,17.0.1-7-g35889ee+1,17.0.1-7-gc7c8782+18,17.0.1-9-gc4bbfb2+3,w.2019.22
LSSTDataManagementBasePackage
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Go to the source code of this file.
Namespaces | |
| lsst.ip.isr.isrFunctions | |
Functions | |
| def | lsst.ip.isr.isrFunctions.createPsf (fwhm) |
| def | lsst.ip.isr.isrFunctions.transposeMaskedImage (maskedImage) |
| def | lsst.ip.isr.isrFunctions.interpolateDefectList (maskedImage, defectList, fwhm, fallbackValue=None) |
| def | lsst.ip.isr.isrFunctions.defectListFromFootprintList (fpList) |
| def | lsst.ip.isr.isrFunctions.transposeDefectList (defectList) |
| def | lsst.ip.isr.isrFunctions.maskPixelsFromDefectList (maskedImage, defectList, maskName='BAD') |
| def | lsst.ip.isr.isrFunctions.getDefectListFromMask (maskedImage, maskName) |
| def | lsst.ip.isr.isrFunctions.makeThresholdMask (maskedImage, threshold, growFootprints=1, maskName='SAT') |
| def | lsst.ip.isr.isrFunctions.interpolateFromMask (maskedImage, fwhm, growSaturatedFootprints=1, maskNameList=['SAT'], fallbackValue=None) |
| def | lsst.ip.isr.isrFunctions.saturationCorrection (maskedImage, saturation, fwhm, growFootprints=1, interpolate=True, maskName='SAT', fallbackValue=None) |
| def | lsst.ip.isr.isrFunctions.trimToMatchCalibBBox (rawMaskedImage, calibMaskedImage) |
| def | lsst.ip.isr.isrFunctions.biasCorrection (maskedImage, biasMaskedImage, trimToFit=False) |
| def | lsst.ip.isr.isrFunctions.darkCorrection (maskedImage, darkMaskedImage, expScale, darkScale, invert=False, trimToFit=False) |
| def | lsst.ip.isr.isrFunctions.updateVariance (maskedImage, gain, readNoise) |
| def | lsst.ip.isr.isrFunctions.flatCorrection (maskedImage, flatMaskedImage, scalingType, userScale=1.0, invert=False, trimToFit=False) |
| def | lsst.ip.isr.isrFunctions.illuminationCorrection (maskedImage, illumMaskedImage, illumScale) |
| def | lsst.ip.isr.isrFunctions.overscanCorrection (ampMaskedImage, overscanImage, fitType='MEDIAN', order=1, collapseRej=3.0, statControl=None, overscanIsInt=True) |
| def | lsst.ip.isr.isrFunctions.brighterFatterCorrection (exposure, kernel, maxIter, threshold, applyGain) |
| def | lsst.ip.isr.isrFunctions.gainContext (exp, image, apply) |
| def | lsst.ip.isr.isrFunctions.attachTransmissionCurve (exposure, opticsTransmission=None, filterTransmission=None, sensorTransmission=None, atmosphereTransmission=None) |
| def | lsst.ip.isr.isrFunctions.addDistortionModel (exposure, camera) |
| Update the WCS in exposure with a distortion model based on camera geometry. More... | |
| def | lsst.ip.isr.isrFunctions.applyGains (exposure, normalizeGains=False) |
| def | lsst.ip.isr.isrFunctions.widenSaturationTrails (mask) |
| def | lsst.ip.isr.isrFunctions.setBadRegions (exposure, badStatistic="MEDIAN") |
1.8.13