IsrMockLSSTConfig#

class lsst.ip.isr.IsrMockLSSTConfig(*args, **kw)#

Bases: IsrMockConfig

Configuration parameters for isrMockLSST.

Attributes Summary

assembleCcd

CCD assembly task; used for defect box conversions.

badParallelOverscanColumnLevel

Bright parallel overscan column level (electron).

badParallelOverscanColumnNeighborsLevel

Bright parallel overscan column neighbors level (electron).

bfStrength

The brighter fatter effect scaling parameter (cannot be zero).Nominally = 1, but = 2 is more realistic.

biasLevel

Background contribution to be generated from the bias offset in adu.

brightDefectLevel

Bright defect level (electron).

brighterFatterCalibType

Type of calibration to generate if doGenerateData=True, otherwise ignored.

calibMode

Set to true to produce mock calibration products, e.g. combined bias, dark, flat, etc.

clockInjectedOffsetLevel

Clock-injected offset (on-chip bias level), in electron.

darkRate

Background level contribution (in electron/s) to be generated from dark current.

darkTime

Exposure time for the dark current contribution.

detectorIndex

Index for the detector to use.

doAdd2DBias

Add 2D bias residual frame to data.

doAddBadParallelOverscanColumn

Add a bad column to the parallel overscan.

doAddBadParallelOverscanColumnNeighbors

Add low-level bad columns next to parallel overscan bad column.

doAddBias

Add bias signal to data.

doAddBrightDefects

Add bright defects (bad column) to data.

doAddBrighterFatter

Add brighter fatter and/or diffusion effects to image.

doAddClockInjectedOffset

Add clock-injected offset to data (on-chip bias level).

doAddCrosstalk

Apply simulated crosstalk to output image.

doAddDark

Add dark signal to data.

doAddDarkNoiseOnly

Add only dark current noise, for testing consistency.

doAddDeferredCharge

Add serial CTI at the amp level? (bool, default False)

doAddFlat

Add flat signal to data.

doAddFringe

Add fringe signal to data.

doAddHighSignalNonlinearity

Add high signal non-linearity to overscan and data regions? (bool, default True)

doAddLowSignalNonlinearity

Add low signal non-linearity to overscan and data regions? (Not supported yet.) (bool, default False)

doAddOverscan

If untrimmed, add overscan ramp to overscan and data regions.

doAddParallelOverscanRamp

Add overscan ramp to parallel overscan and data regions.

doAddSerialOverscanRamp

Add overscan ramp to serial overscan and data regions.

doAddSky

Apply 'sky' signal to output image.

doAddSource

Add simulated source to output image.

doApplyGain

Add gain to data.

doBrighterFatter

Return a simulated brighter-fatter kernel.

doCrosstalkCoeffs

Return the matrix of crosstalk coefficients.

doDataRef

Return a simulated gen2 butler dataRef.

doDefects

Return a simulated defect list.

doDeferredCharge

Return a simulated deferred charge calibration.

doGenerateAmpDict

Return a dict of exposure amplifiers instead of an afwImage.Exposure.

doGenerateData

Return a non-image data structure if True.

doGenerateImage

Return the generated output image if True.

doLinearizer

Return linearizer dataset.

doRoundAdu

Round adu values to nearest integer.

doTransmissionCurve

Return a simulated transmission curve.

expTime

Exposure time for simulated data.

flatDrop

Fractional flux drop due to flat from center to edge of detector along x-axis.

fringeScale

Peak fluxes for the components of the fringe ripple in adu (IsrTask) or electron (IsrTaskLSST).

fringeX0

Center position for the fringe ripples.

fringeY0

Center position for the fringe ripples.

gain

Gain for simulated data in electron/adu.

gainDict

Dictionary of amp name to gain; any amps not listed will use config.gain as the value.

highSignalNonlinearityThreshold

Threshold (in adu) for the non-linearity to be considered high signal.

isLsstLike

If True, products have one raw image per amplifier, otherwise, one raw image per detector.

isTrimmed

If True, amplifiers have been trimmed and mosaicked to remove regions outside the data BBox.

nRecalc

Number of electrons to accumulate before recalculating pixel shapes.

noise2DBias

Noise (in electron) to generate a 2D bias residual frame.

overscanScale

Amplitude of the ramp function to add to overscan data in adu (IsrTask) or electron (IsrTaskLSST) (float, default 100.0)

plateScale

Plate scale used in constructing mock camera.

radialDistortion

Radial distortion term used in constructing mock camera.

readNoise

Read noise of the detector in electron.

rngSeed

Seed for random number generator used to add noise.

skyLevel

Background contribution to be generated from 'the sky' in adu (IsrTask) or electron (IsrTaskLSST).

sourceAmp

Amplifier to place simulated 'astronomical sources'.

sourceFlux

Peak flux level of simulated 'astronomical sources' in adu (IsrTask) or electron (IsrTaskLSST).

sourceX

Peak position (in amplifier coordinates) of simulated 'astronomical sources'.

sourceY

Peak position (in amplifier coordinates) of simulated 'astronomical sources'.

Methods Summary

setDefaults()

Subclass hook for computing defaults.

validate()

Validate the Config, raising an exception if invalid.

Attributes Documentation

assembleCcd#

CCD assembly task; used for defect box conversions. (ConfigurableInstance, default <class 'lsst.ip.isr.assembleCcdTask.AssembleCcdConfig'>)

badParallelOverscanColumnLevel#

Bright parallel overscan column level (electron). Should be above saturation. (float, default 300000.0)

badParallelOverscanColumnNeighborsLevel#

Bright parallel overscan column neighbors level (electron). (float, default 50.0)

bfStrength#

The brighter fatter effect scaling parameter (cannot be zero).Nominally = 1, but = 2 is more realistic. (float, default 2.0)

biasLevel#

Background contribution to be generated from the bias offset in adu. (float, default 8000.0)

brightDefectLevel#

Bright defect level (electron). (float, default 30000.0)

brighterFatterCalibType#

Type of calibration to generate if doGenerateData=True, otherwise ignored. (str, default 'KERNEL')

Allowed values:

'KERNEL'

No default suspect values; only config overrides will be used.

'ELECTROSTATIC'

Use the default from the camera model (old defaults).

'None'

Field is optional

calibMode#

Set to true to produce mock calibration products, e.g. combined bias, dark, flat, etc. (bool, default False)

clockInjectedOffsetLevel#

Clock-injected offset (on-chip bias level), in electron. (float, default 8500.0)

darkRate#

Background level contribution (in electron/s) to be generated from dark current. (float, default 5.0)

darkTime#

Exposure time for the dark current contribution. (float, default 5.0)

detectorIndex#

Index for the detector to use. The default value uses a standard 2x4 array of amps. (int, default 20)

doAdd2DBias#

Add 2D bias residual frame to data. (bool, default True)

doAddBadParallelOverscanColumn#

Add a bad column to the parallel overscan. (bool, default True)

doAddBadParallelOverscanColumnNeighbors#

Add low-level bad columns next to parallel overscan bad column. (bool, default True)

doAddBias#

Add bias signal to data. (bool, default True)

doAddBrightDefects#

Add bright defects (bad column) to data. (bool, default True)

doAddBrighterFatter#

Add brighter fatter and/or diffusion effects to image. (bool, default False)

doAddClockInjectedOffset#

Add clock-injected offset to data (on-chip bias level). (bool, default True)

doAddCrosstalk#

Apply simulated crosstalk to output image. This cannot be corrected by ISR, as detector.hasCrosstalk()==False. (bool, default False)

doAddDark#

Add dark signal to data. (bool, default True)

doAddDarkNoiseOnly#

Add only dark current noise, for testing consistency. (bool, default False)

doAddDeferredCharge#

Add serial CTI at the amp level? (bool, default False)

doAddFlat#

Add flat signal to data. (bool, default True)

doAddFringe#

Add fringe signal to data. (bool, default True)

doAddHighSignalNonlinearity#

Add high signal non-linearity to overscan and data regions? (bool, default True)

doAddLowSignalNonlinearity#

Add low signal non-linearity to overscan and data regions? (Not supported yet.) (bool, default False)

doAddOverscan#

If untrimmed, add overscan ramp to overscan and data regions. (bool, default True)

doAddParallelOverscanRamp#

Add overscan ramp to parallel overscan and data regions. (bool, default True)

doAddSerialOverscanRamp#

Add overscan ramp to serial overscan and data regions. (bool, default True)

doAddSky#

Apply ‘sky’ signal to output image. (bool, default True)

doAddSource#

Add simulated source to output image. (bool, default True)

doApplyGain#

Add gain to data. (bool, default True)

doBrighterFatter#

Return a simulated brighter-fatter kernel. (bool, default False)

doCrosstalkCoeffs#

Return the matrix of crosstalk coefficients. (bool, default False)

doDataRef#

Return a simulated gen2 butler dataRef. (bool, default False)

doDefects#

Return a simulated defect list. (bool, default False)

doDeferredCharge#

Return a simulated deferred charge calibration. (bool, default False)

doGenerateAmpDict#

Return a dict of exposure amplifiers instead of an afwImage.Exposure. (bool, default False)

doGenerateData#

Return a non-image data structure if True. (bool, default False)

doGenerateImage#

Return the generated output image if True. (bool, default False)

doLinearizer#

Return linearizer dataset. (bool, default False)

doRoundAdu#

Round adu values to nearest integer. (bool, default True)

doTransmissionCurve#

Return a simulated transmission curve. (bool, default False)

expTime#

Exposure time for simulated data. (float, default 5.0)

flatDrop#

Fractional flux drop due to flat from center to edge of detector along x-axis. (float, default 0.1)

fringeScale#

Peak fluxes for the components of the fringe ripple in adu (IsrTask) or electron (IsrTaskLSST). (List, default [200.0])

fringeX0#

Center position for the fringe ripples. (List, default [-100])

fringeY0#

Center position for the fringe ripples. (List, default [0])

gain#

Gain for simulated data in electron/adu. (float, default 1.0)

gainDict#

Dictionary of amp name to gain; any amps not listed will use config.gain as the value. Units are electron/adu. (Dict, default {'C:0,0': 1.65, 'C:0,1': 1.6, 'C:0,2': 1.55, 'C:0,3': 1.7, 'C:1,0': 1.75, 'C:1,1': 1.8, 'C:1,2': 1.85, 'C:1,3': 1.7})

highSignalNonlinearityThreshold#

Threshold (in adu) for the non-linearity to be considered high signal. (float, default 40000.0)

isLsstLike#

If True, products have one raw image per amplifier, otherwise, one raw image per detector. (bool, default True)

isTrimmed#

If True, amplifiers have been trimmed and mosaicked to remove regions outside the data BBox. (bool, default True)

nRecalc#

Number of electrons to accumulate before recalculating pixel shapes. (int, default 10000)

noise2DBias#

Noise (in electron) to generate a 2D bias residual frame. (float, default 2.0)

overscanScale#

Amplitude of the ramp function to add to overscan data in adu (IsrTask) or electron (IsrTaskLSST) (float, default 100.0)

plateScale#

Plate scale used in constructing mock camera. (float, default 20.0)

radialDistortion#

Radial distortion term used in constructing mock camera. (float, default 0.925)

readNoise#

Read noise of the detector in electron. (float, default 5.0)

rngSeed#

Seed for random number generator used to add noise. (int, default 20000913)

skyLevel#

Background contribution to be generated from ‘the sky’ in adu (IsrTask) or electron (IsrTaskLSST). (float, default 1000.0)

sourceAmp#

Amplifier to place simulated ‘astronomical sources’. (List, default [0])

sourceFlux#

Peak flux level of simulated ‘astronomical sources’ in adu (IsrTask) or electron (IsrTaskLSST). (List, default [45000.0])

sourceX#

Peak position (in amplifier coordinates) of simulated ‘astronomical sources’. (List, default [50.0])

sourceY#

Peak position (in amplifier coordinates) of simulated ‘astronomical sources’. (List, default [25.0])

Methods Documentation

setDefaults()#

Subclass hook for computing defaults.

Notes#

Derived Config classes that must compute defaults rather than using the Field instances’s defaults should do so here. To correctly use inherited defaults, implementations of setDefaults must call their base class’s setDefaults.

validate()#

Validate the Config, raising an exception if invalid.

Raises#

lsst.pex.config.FieldValidationError

Raised if verification fails.

Notes#

The base class implementation performs type checks on all fields by calling their validate methods.

Complex single-field validation can be defined by deriving new Field types. For convenience, some derived lsst.pex.config.Field-types (ConfigField and ConfigChoiceField) are defined in lsst.pex.config that handle recursing into subconfigs.

Inter-field relationships should only be checked in derived Config classes after calling this method, and base validation is complete.