IsrMockConfig#

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

Bases: Config

Configuration parameters for isrMock.

These parameters produce generic fixed position signals from various sources, and combine them in a way that matches how those signals are combined to create real data. The camera used is the test camera defined by the afwUtils code.

Attributes Summary

`biasLevel`	Background contribution to be generated from the bias offset in adu.
`brighterFatterCalibType`	Type of calibration to generate if doGenerateData=True, otherwise ignored.
`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.
`doAddBias`	Add bias signal to data.
`doAddCrosstalk`	Apply simulated crosstalk to output image.
`doAddDark`	Add dark signal to data.
`doAddFlat`	Add flat signal to data.
`doAddFringe`	Add fringe signal to data.
`doAddOverscan`	If untrimmed, add overscan ramp to overscan and data regions.
`doAddSky`	Apply 'sky' signal to output image.
`doAddSource`	Add simulated source to output image.
`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.
`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.
`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.
`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'.

Attributes Documentation

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

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

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)

doAddBias#: Add bias signal to data. (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)

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

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

doAddOverscan#: If untrimmed, add overscan ramp to 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)

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)

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)

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

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

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])