lsst.ip.isr  16.0-15-g1417920
Public Member Functions | Static Public Attributes | List of all members
lsst.ip.isr.isrTask.IsrTaskConfig Class Reference
Inheritance diagram for lsst.ip.isr.isrTask.IsrTaskConfig:

Public Member Functions

def validate (self)
 

Static Public Attributes

 datasetType
 
 fallbackFilterName
 
 expectWcs
 
 fwhm
 
 qa
 
 doConvertIntToFloat
 
 doSaturation
 
 saturatedMaskName
 
 saturation
 
 growSaturationFootprintSize
 
 doSuspect
 
 suspectMaskName
 
 numEdgeSuspect
 
 doSetBadRegions
 
 badStatistic
 
 doOverscan
 
 overscanFitType
 
 overscanOrder
 
 overscanNumSigmaClip
 
 overscanIsInt
 
 overscanNumLeadingColumnsToSkip
 
 overscanNumTrailingColumnsToSkip
 
 overscanMaxDev
 
 overscanBiasJump
 
 overscanBiasJumpKeyword
 
 overscanBiasJumpDevices
 
 overscanBiasJumpLocation
 
 doAssembleCcd
 
 assembleCcd
 
 doAssembleIsrExposures
 
 doTrimToMatchCalib
 
 doBias
 
 biasDataProductName
 
 doVariance
 
 gain
 
 readNoise
 
 doEmpiricalReadNoise
 
 doLinearize
 
 doCrosstalk
 
 doCrosstalkBeforeAssemble
 
 crosstalk
 
 doWidenSaturationTrails
 
 doBrighterFatter
 
 brighterFatterLevel
 
 brighterFatterKernelFile
 
 brighterFatterMaxIter
 
 brighterFatterThreshold
 
 brighterFatterApplyGain
 
 doDefect
 
 doSaturationInterpolation
 
 doDark
 
 darkDataProductName
 
 doStrayLight
 
 strayLight
 
 doFlat
 
 flatDataProductName
 
 flatScalingType
 
 flatUserScale
 
 doTweakFlat
 
 doApplyGains
 
 normalizeGains
 
 doFringe
 
 fringe
 
 fringeAfterFlat
 
 doNanInterpAfterFlat
 
 doAddDistortionModel
 
 doMeasureBackground
 
 doCameraSpecificMasking
 
 masking
 
 fluxMag0T1
 
 defaultFluxMag0T1
 
 doVignette
 
 vignette
 
 doAttachTransmissionCurve
 
 doUseOpticsTransmission
 
 doUseFilterTransmission
 
 doUseSensorTransmission
 
 doUseAtmosphereTransmission
 
 doWrite
 

Detailed Description

Configuration parameters for IsrTask.

Items are grouped in the order in which they are executed by the task.

Definition at line 56 of file isrTask.py.

Member Function Documentation

◆ validate()

def lsst.ip.isr.isrTask.IsrTaskConfig.validate (   self)

Definition at line 540 of file isrTask.py.

Member Data Documentation

◆ assembleCcd

lsst.ip.isr.isrTask.IsrTaskConfig.assembleCcd
static
Initial value:
= pexConfig.ConfigurableField(
target=AssembleCcdTask,
doc="CCD assembly task",
)

Definition at line 229 of file isrTask.py.

◆ badStatistic

lsst.ip.isr.isrTask.IsrTaskConfig.badStatistic
static
Initial value:
= pexConfig.ChoiceField(
dtype=str,
doc="How to estimate the average value for BAD regions.",
default='MEANCLIP',
allowed={
"MEANCLIP": "Correct using the (clipped) mean of good data",
"MEDIAN": "Correct using the median of the good data",
},
)

Definition at line 139 of file isrTask.py.

◆ biasDataProductName

lsst.ip.isr.isrTask.IsrTaskConfig.biasDataProductName
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Name of the bias data product",
default="bias",
)

Definition at line 252 of file isrTask.py.

◆ brighterFatterApplyGain

lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterApplyGain
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=True,
doc="Should the gain be applied when applying the brighter fatter correction?"
)

Definition at line 342 of file isrTask.py.

◆ brighterFatterKernelFile

lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterKernelFile
static
Initial value:
= pexConfig.Field(
dtype=str,
default='',
doc="Kernel file used for the brighter fatter correction"
)

Definition at line 325 of file isrTask.py.

◆ brighterFatterLevel

lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterLevel
static
Initial value:
= pexConfig.ChoiceField(
dtype=str,
default="DETECTOR",
doc="The level at which to correct for brighter-fatter.",
allowed={
"AMP": "Every amplifier treated separately.",
"DETECTOR": "One kernel per detector",
}
)

Definition at line 316 of file isrTask.py.

◆ brighterFatterMaxIter

lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterMaxIter
static
Initial value:
= pexConfig.Field(
dtype=int,
default=10,
doc="Maximum number of iterations for the brighter fatter correction"
)

Definition at line 330 of file isrTask.py.

◆ brighterFatterThreshold

lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterThreshold
static
Initial value:
= pexConfig.Field(
dtype=float,
default=1000,
doc="Threshold used to stop iterating the brighter fatter correction. It is the "
" absolute value of the difference between the current corrected image and the one"
" from the previous iteration summed over all the pixels."
)

Definition at line 335 of file isrTask.py.

◆ crosstalk

lsst.ip.isr.isrTask.IsrTaskConfig.crosstalk
static
Initial value:
= pexConfig.ConfigurableField(
target=CrosstalkTask,
doc="Intra-CCD crosstalk correction",
)

Definition at line 298 of file isrTask.py.

◆ darkDataProductName

lsst.ip.isr.isrTask.IsrTaskConfig.darkDataProductName
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Name of the dark data product",
default="dark",
)

Definition at line 371 of file isrTask.py.

◆ datasetType

lsst.ip.isr.isrTask.IsrTaskConfig.datasetType
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Dataset type for input data; users will typically leave this alone, "
"but camera-specific ISR tasks will override it",
default="raw",
)

Definition at line 62 of file isrTask.py.

◆ defaultFluxMag0T1

lsst.ip.isr.isrTask.IsrTaskConfig.defaultFluxMag0T1
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="Default value for fluxMag0T1 (for an unrecognized filter).",
default=pow(10.0, 0.4*28.0)
)

Definition at line 489 of file isrTask.py.

◆ doAddDistortionModel

lsst.ip.isr.isrTask.IsrTaskConfig.doAddDistortionModel
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply a distortion model based on camera geometry to the WCS?",
default=True,
)

Definition at line 457 of file isrTask.py.

◆ doApplyGains

lsst.ip.isr.isrTask.IsrTaskConfig.doApplyGains
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Correct the amplifiers for their gains instead of applying flat correction",
default=False,
)

Definition at line 421 of file isrTask.py.

◆ doAssembleCcd

lsst.ip.isr.isrTask.IsrTaskConfig.doAssembleCcd
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=True,
doc="Assemble amp-level exposures into a ccd-level exposure?"
)

Definition at line 224 of file isrTask.py.

◆ doAssembleIsrExposures

lsst.ip.isr.isrTask.IsrTaskConfig.doAssembleIsrExposures
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=False,
doc="Assemble amp-level calibration exposures into ccd-level exposure?"
)

Definition at line 235 of file isrTask.py.

◆ doAttachTransmissionCurve

lsst.ip.isr.isrTask.IsrTaskConfig.doAttachTransmissionCurve
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=False,
doc="Construct and attach a wavelength-dependent throughput curve for this CCD image?"
)

Definition at line 507 of file isrTask.py.

◆ doBias

lsst.ip.isr.isrTask.IsrTaskConfig.doBias
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply bias frame correction?",
default=True,
)

Definition at line 247 of file isrTask.py.

◆ doBrighterFatter

lsst.ip.isr.isrTask.IsrTaskConfig.doBrighterFatter
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=False,
doc="Apply the brighter fatter correction"
)

Definition at line 311 of file isrTask.py.

◆ doCameraSpecificMasking

lsst.ip.isr.isrTask.IsrTaskConfig.doCameraSpecificMasking
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Mask camera-specific bad regions?",
default=False,
)

Definition at line 471 of file isrTask.py.

◆ doConvertIntToFloat

lsst.ip.isr.isrTask.IsrTaskConfig.doConvertIntToFloat
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Convert integer raw images to floating point values?",
default=True,
)

Definition at line 88 of file isrTask.py.

◆ doCrosstalk

lsst.ip.isr.isrTask.IsrTaskConfig.doCrosstalk
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply intra-CCD crosstalk correction?",
default=False,
)

Definition at line 288 of file isrTask.py.

◆ doCrosstalkBeforeAssemble

lsst.ip.isr.isrTask.IsrTaskConfig.doCrosstalkBeforeAssemble
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply crosstalk correction before CCD assembly, and before trimming?",
default=True,
)

Definition at line 293 of file isrTask.py.

◆ doDark

lsst.ip.isr.isrTask.IsrTaskConfig.doDark
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply dark frame correction?",
default=True,
)

Definition at line 366 of file isrTask.py.

◆ doDefect

lsst.ip.isr.isrTask.IsrTaskConfig.doDefect
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply correction for CCD defects, e.g. hot pixels?",
default=True,
)

Definition at line 349 of file isrTask.py.

◆ doEmpiricalReadNoise

lsst.ip.isr.isrTask.IsrTaskConfig.doEmpiricalReadNoise
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=False,
doc="Calculate empirical read noise instead of value from AmpInfo data?"
)

Definition at line 274 of file isrTask.py.

◆ doFlat

lsst.ip.isr.isrTask.IsrTaskConfig.doFlat
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply flat field correction?",
default=True,
)

Definition at line 389 of file isrTask.py.

◆ doFringe

lsst.ip.isr.isrTask.IsrTaskConfig.doFringe
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply fringe correction?",
default=True,
)

Definition at line 433 of file isrTask.py.

◆ doLinearize

lsst.ip.isr.isrTask.IsrTaskConfig.doLinearize
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Correct for nonlinearity of the detector's response?",
default=True,
)

Definition at line 281 of file isrTask.py.

◆ doMeasureBackground

lsst.ip.isr.isrTask.IsrTaskConfig.doMeasureBackground
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Measure the background level on the reduced image?",
default=False,
)

Definition at line 464 of file isrTask.py.

◆ doNanInterpAfterFlat

lsst.ip.isr.isrTask.IsrTaskConfig.doNanInterpAfterFlat
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc=("If True, ensure we interpolate NaNs after flat-fielding, even if we "
"also have to interpolate them before flat-fielding."),
default=False,
)

Definition at line 449 of file isrTask.py.

◆ doOverscan

lsst.ip.isr.isrTask.IsrTaskConfig.doOverscan
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Do overscan subtraction?",
default=True,
)

Definition at line 150 of file isrTask.py.

◆ doSaturation

lsst.ip.isr.isrTask.IsrTaskConfig.doSaturation
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Mask saturated pixels?",
default=True,
)

Definition at line 95 of file isrTask.py.

◆ doSaturationInterpolation

lsst.ip.isr.isrTask.IsrTaskConfig.doSaturationInterpolation
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Perform interpolation over pixels masked as saturated?",
default=True,
)

Definition at line 354 of file isrTask.py.

◆ doSetBadRegions

lsst.ip.isr.isrTask.IsrTaskConfig.doSetBadRegions
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Should we set the level of all BAD patches of the chip to the chip's average value?",
default=True,
)

Definition at line 134 of file isrTask.py.

◆ doStrayLight

lsst.ip.isr.isrTask.IsrTaskConfig.doStrayLight
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Subtract stray light in the y-band (due to encoder LEDs)?",
default=False,
)

Definition at line 378 of file isrTask.py.

◆ doSuspect

lsst.ip.isr.isrTask.IsrTaskConfig.doSuspect
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Mask suspect pixels?",
default=True,
)

Definition at line 117 of file isrTask.py.

◆ doTrimToMatchCalib

lsst.ip.isr.isrTask.IsrTaskConfig.doTrimToMatchCalib
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=False,
doc="Trim raw data to match calibration bounding boxes?"
)

Definition at line 240 of file isrTask.py.

◆ doTweakFlat

lsst.ip.isr.isrTask.IsrTaskConfig.doTweakFlat
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Tweak flats to match observed amplifier ratios?",
default=False
)

Definition at line 414 of file isrTask.py.

◆ doUseAtmosphereTransmission

lsst.ip.isr.isrTask.IsrTaskConfig.doUseAtmosphereTransmission
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=True,
doc="Load and use transmission_atmosphere (if doAttachTransmissionCurve is True)?"
)

Definition at line 527 of file isrTask.py.

◆ doUseFilterTransmission

lsst.ip.isr.isrTask.IsrTaskConfig.doUseFilterTransmission
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=True,
doc="Load and use transmission_filter (if doAttachTransmissionCurve is True)?"
)

Definition at line 517 of file isrTask.py.

◆ doUseOpticsTransmission

lsst.ip.isr.isrTask.IsrTaskConfig.doUseOpticsTransmission
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=True,
doc="Load and use transmission_optics (if doAttachTransmissionCurve is True)?"
)

Definition at line 512 of file isrTask.py.

◆ doUseSensorTransmission

lsst.ip.isr.isrTask.IsrTaskConfig.doUseSensorTransmission
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=True,
doc="Load and use transmission_sensor (if doAttachTransmissionCurve is True)?"
)

Definition at line 522 of file isrTask.py.

◆ doVariance

lsst.ip.isr.isrTask.IsrTaskConfig.doVariance
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Calculate variance?",
default=True
)

Definition at line 259 of file isrTask.py.

◆ doVignette

lsst.ip.isr.isrTask.IsrTaskConfig.doVignette
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply vignetting parameters?",
default=False,
)

Definition at line 496 of file isrTask.py.

◆ doWidenSaturationTrails

lsst.ip.isr.isrTask.IsrTaskConfig.doWidenSaturationTrails
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Widen bleed trails based on their width?",
default=True
)

Definition at line 304 of file isrTask.py.

◆ doWrite

lsst.ip.isr.isrTask.IsrTaskConfig.doWrite
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Persist postISRCCD?",
default=True,
)

Definition at line 534 of file isrTask.py.

◆ expectWcs

lsst.ip.isr.isrTask.IsrTaskConfig.expectWcs
static
Initial value:
= pexConfig.Field(
dtype=bool,
default=True,
doc="Expect input science images to have a WCS (set False for e.g. spectrographs)."
)

Definition at line 72 of file isrTask.py.

◆ fallbackFilterName

lsst.ip.isr.isrTask.IsrTaskConfig.fallbackFilterName
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Fallback default filter name for calibrations.",
optional=True)

Definition at line 68 of file isrTask.py.

◆ flatDataProductName

lsst.ip.isr.isrTask.IsrTaskConfig.flatDataProductName
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Name of the flat data product",
default="flat",
)

Definition at line 394 of file isrTask.py.

◆ flatScalingType

lsst.ip.isr.isrTask.IsrTaskConfig.flatScalingType
static
Initial value:
= pexConfig.ChoiceField(
dtype=str,
doc="The method for scaling the flat on the fly.",
default='USER',
allowed={
"USER": "Scale by flatUserScale",
"MEAN": "Scale by the inverse of the mean",
"MEDIAN": "Scale by the inverse of the median",
},
)

Definition at line 399 of file isrTask.py.

◆ flatUserScale

lsst.ip.isr.isrTask.IsrTaskConfig.flatUserScale
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="If flatScalingType is 'USER' then scale flat by this amount; ignored otherwise",
default=1.0,
)

Definition at line 409 of file isrTask.py.

◆ fluxMag0T1

lsst.ip.isr.isrTask.IsrTaskConfig.fluxMag0T1
static
Initial value:
= pexConfig.DictField(
keytype=str,
itemtype=float,
doc="The approximate flux of a zero-magnitude object in a one-second exposure, per filter.",
default=dict((f, pow(10.0, 0.4*m)) for f, m in (("Unknown", 28.0),
))
)

Definition at line 482 of file isrTask.py.

◆ fringe

lsst.ip.isr.isrTask.IsrTaskConfig.fringe
static
Initial value:
= pexConfig.ConfigurableField(
target=FringeTask,
doc="Fringe subtraction task",
)

Definition at line 438 of file isrTask.py.

◆ fringeAfterFlat

lsst.ip.isr.isrTask.IsrTaskConfig.fringeAfterFlat
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Do fringe subtraction after flat-fielding?",
default=True,
)

Definition at line 442 of file isrTask.py.

◆ fwhm

lsst.ip.isr.isrTask.IsrTaskConfig.fwhm
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="FWHM of PSF in arcseconds.",
default=1.0,
)

Definition at line 77 of file isrTask.py.

◆ gain

lsst.ip.isr.isrTask.IsrTaskConfig.gain
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="The gain to use if no Detector is present in the Exposure (ignored if NaN)",
default=float("NaN"),
)

Definition at line 264 of file isrTask.py.

◆ growSaturationFootprintSize

lsst.ip.isr.isrTask.IsrTaskConfig.growSaturationFootprintSize
static
Initial value:
= pexConfig.Field(
dtype=int,
doc="Number of pixels by which to grow the saturation footprints",
default=1,
)

Definition at line 110 of file isrTask.py.

◆ masking

lsst.ip.isr.isrTask.IsrTaskConfig.masking
static
Initial value:
= pexConfig.ConfigurableField(
target=MaskingTask,
doc="Masking task."
)

Definition at line 476 of file isrTask.py.

◆ normalizeGains

lsst.ip.isr.isrTask.IsrTaskConfig.normalizeGains
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Normalize all the amplifiers in each CCD to have the same median value.",
default=False,
)

Definition at line 426 of file isrTask.py.

◆ numEdgeSuspect

lsst.ip.isr.isrTask.IsrTaskConfig.numEdgeSuspect
static
Initial value:
= pexConfig.Field(
dtype=int,
doc="Number of edge pixels to be flagged as untrustworthy.",
default=0,
)

Definition at line 127 of file isrTask.py.

◆ overscanBiasJump

lsst.ip.isr.isrTask.IsrTaskConfig.overscanBiasJump
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Fit the overscan in a piecewise-fashion to correct for bias jumps?",
default=False,
)

Definition at line 202 of file isrTask.py.

◆ overscanBiasJumpDevices

lsst.ip.isr.isrTask.IsrTaskConfig.overscanBiasJumpDevices
static
Initial value:
= pexConfig.ListField(
dtype=str,
doc="List of devices that need piecewise overscan correction.",
default=(),
)

Definition at line 212 of file isrTask.py.

◆ overscanBiasJumpKeyword

lsst.ip.isr.isrTask.IsrTaskConfig.overscanBiasJumpKeyword
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Header keyword containing information about devices.",
default="NO_SUCH_KEY",
)

Definition at line 207 of file isrTask.py.

◆ overscanBiasJumpLocation

lsst.ip.isr.isrTask.IsrTaskConfig.overscanBiasJumpLocation
static
Initial value:
= pexConfig.Field(
dtype=int,
doc="Location of bias jump along y-axis.",
default=0,
)

Definition at line 217 of file isrTask.py.

◆ overscanFitType

lsst.ip.isr.isrTask.IsrTaskConfig.overscanFitType
static
Initial value:
= pexConfig.ChoiceField(
dtype=str,
doc="The method for fitting the overscan bias level.",
default='MEDIAN',
allowed={
"POLY": "Fit ordinary polynomial to the longest axis of the overscan region",
"CHEB": "Fit Chebyshev polynomial to the longest axis of the overscan region",
"LEG": "Fit Legendre polynomial to the longest axis of the overscan region",
"NATURAL_SPLINE": "Fit natural spline to the longest axis of the overscan region",
"CUBIC_SPLINE": "Fit cubic spline to the longest axis of the overscan region",
"AKIMA_SPLINE": "Fit Akima spline to the longest axis of the overscan region",
"MEAN": "Correct using the mean of the overscan region",
"MEANCLIP": "Correct using a clipped mean of the overscan region",
"MEDIAN": "Correct using the median of the overscan region",
},
)

Definition at line 155 of file isrTask.py.

◆ overscanIsInt

lsst.ip.isr.isrTask.IsrTaskConfig.overscanIsInt
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Treat overscan as an integer image for purposes of overscan.FitType=MEDIAN",
default=True,
)

Definition at line 182 of file isrTask.py.

◆ overscanMaxDev

lsst.ip.isr.isrTask.IsrTaskConfig.overscanMaxDev
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="Maximum deviation from the median for overscan",
default=1000.0, check=lambda x: x > 0
)

Definition at line 197 of file isrTask.py.

◆ overscanNumLeadingColumnsToSkip

lsst.ip.isr.isrTask.IsrTaskConfig.overscanNumLeadingColumnsToSkip
static
Initial value:
= pexConfig.Field(
dtype=int,
doc="Number of columns to skip in overscan, i.e. those closest to amplifier",
default=0,
)

Definition at line 187 of file isrTask.py.

◆ overscanNumSigmaClip

lsst.ip.isr.isrTask.IsrTaskConfig.overscanNumSigmaClip
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="Rejection threshold (sigma) for collapsing overscan before fit",
default=3.0,
)

Definition at line 177 of file isrTask.py.

◆ overscanNumTrailingColumnsToSkip

lsst.ip.isr.isrTask.IsrTaskConfig.overscanNumTrailingColumnsToSkip
static
Initial value:
= pexConfig.Field(
dtype=int,
doc="Number of columns to skip in overscan, i.e. those farthest from amplifier",
default=0,
)

Definition at line 192 of file isrTask.py.

◆ overscanOrder

lsst.ip.isr.isrTask.IsrTaskConfig.overscanOrder
static
Initial value:
= pexConfig.Field(
dtype=int,
doc=("Order of polynomial or to fit if overscan fit type is a polynomial, " +
"or number of spline knots if overscan fit type is a spline."),
default=1,
)

Definition at line 171 of file isrTask.py.

◆ qa

lsst.ip.isr.isrTask.IsrTaskConfig.qa
static
Initial value:
= pexConfig.ConfigField(
dtype=isrQa.IsrQaConfig,
doc="QA related configuration options.",
)

Definition at line 82 of file isrTask.py.

◆ readNoise

lsst.ip.isr.isrTask.IsrTaskConfig.readNoise
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="The read noise to use if no Detector is present in the Exposure",
default=0.0,
)

Definition at line 269 of file isrTask.py.

◆ saturatedMaskName

lsst.ip.isr.isrTask.IsrTaskConfig.saturatedMaskName
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Name of mask plane to use in saturation detection and interpolation",
default="SAT",
)

Definition at line 100 of file isrTask.py.

◆ saturation

lsst.ip.isr.isrTask.IsrTaskConfig.saturation
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="The saturation level to use if no Detector is present in the Exposure (ignored if NaN)",
default=float("NaN"),
)

Definition at line 105 of file isrTask.py.

◆ strayLight

lsst.ip.isr.isrTask.IsrTaskConfig.strayLight
static
Initial value:
= pexConfig.ConfigurableField(
target=StrayLightTask,
doc="y-band stray light correction"
)

Definition at line 383 of file isrTask.py.

◆ suspectMaskName

lsst.ip.isr.isrTask.IsrTaskConfig.suspectMaskName
static
Initial value:
= pexConfig.Field(
dtype=str,
doc="Name of mask plane to use for suspect pixels",
default="SUSPECT",
)

Definition at line 122 of file isrTask.py.

◆ vignette

lsst.ip.isr.isrTask.IsrTaskConfig.vignette
static
Initial value:
= pexConfig.ConfigurableField(
target=VignetteTask,
doc="Vignetting task.",
)

Definition at line 501 of file isrTask.py.


The documentation for this class was generated from the following file: