LSSTApplications
16.0-10-g0ee56ad+5,16.0-11-ga33d1f2+5,16.0-12-g3ef5c14+3,16.0-12-g71e5ef5+18,16.0-12-gbdf3636+3,16.0-13-g118c103+3,16.0-13-g8f68b0a+3,16.0-15-gbf5c1cb+4,16.0-16-gfd17674+3,16.0-17-g7c01f5c+3,16.0-18-g0a50484+1,16.0-20-ga20f992+8,16.0-21-g0e05fd4+6,16.0-21-g15e2d33+4,16.0-22-g62d8060+4,16.0-22-g847a80f+4,16.0-25-gf00d9b8+1,16.0-28-g3990c221+4,16.0-3-gf928089+3,16.0-32-g88a4f23+5,16.0-34-gd7987ad+3,16.0-37-gc7333cb+2,16.0-4-g10fc685+2,16.0-4-g18f3627+26,16.0-4-g5f3a788+26,16.0-5-gaf5c3d7+4,16.0-5-gcc1f4bb+1,16.0-6-g3b92700+4,16.0-6-g4412fcd+3,16.0-6-g7235603+4,16.0-69-g2562ce1b+2,16.0-8-g14ebd58+4,16.0-8-g2df868b+1,16.0-8-g4cec79c+6,16.0-8-gadf6c7a+1,16.0-8-gfc7ad86,16.0-82-g59ec2a54a+1,16.0-9-g5400cdc+2,16.0-9-ge6233d7+5,master-g2880f2d8cf+3,v17.0.rc1
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, growFootprints=1, maskName='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") |