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LSSTApplications
16.0-10-g0ee56ad,16.0-11-ga33d1f2+2,16.0-12-g3ef5c14+1,16.0-12-g71e5ef5+14,16.0-12-gbdf3636+2,16.0-13-g118c103+2,16.0-13-g8f68b0a,16.0-15-gbf5c1cb,16.0-16-gfd17674+2,16.0-17-g7c01f5c+2,16.0-18-g0a50484,16.0-20-ga20f992+3,16.0-21-g0e05fd4+2,16.0-21-g15e2d33,16.0-22-g62d8060,16.0-22-g847a80f,16.0-24-gfa57b64+1,16.0-28-g3990c221,16.0-3-gf928089+2,16.0-32-g88a4f23,16.0-34-gd7987ad,16.0-36-g6d07a18,16.0-4-g10fc685,16.0-4-g18f3627+24,16.0-4-g5f3a788+25,16.0-5-gaf5c3d7+1,16.0-5-gcc1f4bb,16.0-6-g3b92700,16.0-6-g4412fcd+2,16.0-6-g7235603+1,16.0-68-gb45e8e9d,16.0-7-g0913a87,16.0-7-g56728dd,16.0-8-g14ebd58,16.0-8-g2df868b,16.0-8-g4cec79c+1,16.0-81-g9604f5049,16.0-9-g5400cdc,16.0-9-ge6233d7+1,master-g2880f2d8cf+1,w.2019.05
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") |
1.8.13