CfhtIsrTaskConfig

class lsst.obs.cfht.cfhtIsrTask.CfhtIsrTaskConfig

Bases: lsst.ip.isr.isrTask.IsrTaskConfig

Attributes Summary

assembleCcd	CCD assembly task (ConfigurableInstance, default <class 'lsst.ip.isr.assembleCcdTask.AssembleCcdConfig'>)
biasDataProductName	Name of the bias data product (str, default 'bias')
brighterFatterApplyGain	Should the gain be applied when applying the brighter fatter correction? (bool, default True)
brighterFatterKernelFile	Kernel file used for the brighter fatter correction (str, default '')
brighterFatterLevel	The level at which to correct for brighter-fatter (str, default 'DETECTOR')
brighterFatterMaxIter	Maximum number of iterations for the brighter fatter correction (int, default 10)
brighterFatterThreshold	Threshold used to stop iterating the brighter fatter correction.
crosstalk	Intra-CCD crosstalk correction (ConfigurableInstance, default <class 'lsst.ip.isr.crosstalk.CrosstalkConfig'>)
darkDataProductName	Name of the dark data product (str, default 'dark')
datasetType	Dataset type for input data; users will typically leave this alone, but camera-specific ISR tasks will override it (str, default 'raw')
doAddDistortionModel	Apply a distortion model based on camera geometry to the WCS? (bool, default True)
doAssembleCcd	Assemble amp-level exposures into a ccd-level exposure? (bool, default True)
doAssembleIsrExposures	Assemble amp-level calibration exposures into ccd-level exposure? (bool, default False)
doAttachTransmissionCurve	Construct and attach a wavelength-dependent throughput curve for this CCD image? (bool, default False)
doBias	Apply bias frame correction? (bool, default True)
doBrighterFatter	Apply the brighter fatter correction (bool, default False)
doCrosstalk	Apply intra-CCD crosstalk correction? (bool, default False)
doDark	Apply dark frame correction? (bool, default True)
doDefect	Apply correction for CCD defects, e.g.
doEmpiricalReadNoise	Calculate empirical read noise instead of value from AmpInfo data? (bool, default False)
doFlat	Apply flat field correction? (bool, default True)
doFringe	Apply fringe correction? (bool, default True)
doLinearize	Correct for nonlinearity of the detector’s response? (bool, default True)
doNanInterpAfterFlat	If True, ensure we interpolate NaNs after flat-fielding, even if we also have to interpolate them before flat-fielding.
doSaturationInterpolation	Perform interpolation over pixels masked as saturated? (bool, default True)
doUseAtmosphereTransmission	Load and use transmission_atmosphere (if doAttachTransmissionCurve is True)? (bool, default True)
doUseFilterTransmission	Load and use transmission_filter (if doAttachTransmissionCurve is True)? (bool, default True)
doUseOpticsTransmission	Load and use transmission_optics (if doAttachTransmissionCurve is True)? (bool, default True)
doUseSensorTransmission	Load and use transmission_sensor (if doAttachTransmissionCurve is True)? (bool, default True)
doWrite	Persist postISRCCD? (bool, default True)
expectWcs	Expect input science images to have a WCS (set False for e.g.
fallbackFilterName	Fallback default filter name for calibrations (str, default None)
flatDataProductName	Name of the flat data product (str, default 'flat')
flatScalingType	The method for scaling the flat on the fly.
flatUserScale	If flatScalingType is ‘USER’ then scale flat by this amount; ignored otherwise (float, default 1.0)
fluxMag0T1	The approximate flux of a zero-magnitude object in a one-second exposure (float, default 10000000000.0)
fringe	Fringe subtraction task (ConfigurableInstance, default <class 'lsst.ip.isr.fringe.FringeConfig'>)
fringeAfterFlat	Do fringe subtraction after flat-fielding? (bool, default True)
fwhm	FWHM of PSF (arcsec) (float, default 1.0)
gain	The gain to use if no Detector is present in the Exposure (ignored if NaN) (float, default nan)
growSaturationFootprintSize	Number of pixels by which to grow the saturation footprints (int, default 1)
history
keysToRemoveFromAssembledCcd	fields to remove from the metadata of the assembled ccd.
overscanFitType	The method for fitting the overscan bias level.
overscanNumLeadingColumnsToSkip	Number of columns to skip in overscan, i.e.
overscanNumSigmaClip	Rejection threshold (sigma) for collapsing overscan before fit (float, default 3.0)
overscanNumTrailingColumnsToSkip	Number of columns to skip in overscan, i.e.
overscanOrder	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.
readNoise	The read noise to use if no Detector is present in the Exposure (float, default 0.0)
safe	Safety margin for CFHT sensors gain determination (float, default 0.95)
saturatedMaskName	Name of mask plane to use in saturation detection and interpolation (str, default 'SAT')
saturation	The saturation level to use if no Detector is present in the Exposure (ignored if NaN) (float, default nan)
suspectMaskName	Name of mask plane to use for suspect pixels (str, default 'SUSPECT')

Methods Summary

compare(other[, shortcut, rtol, atol, output])	!Compare two Configs for equality; return True if equal
formatHistory(name, **kwargs)	!Format the specified config field’s history to a more human-readable format
freeze()	!Make this Config and all sub-configs read-only
items()	!Return the list of (field name, field value) pairs
iteritems()	!Iterate over (field name, field value) pairs
iterkeys()	!Iterate over field names
itervalues()	!Iterate over field values
keys()	!Return the list of field names
load(filename[, root])	!Modify this config in place by executing the Python code in the named file.
loadFromStream(stream[, root, filename])	!Modify this config in place by executing the python code in the provided stream.
names()	!Return all the keys in a config recursively
save(filename[, root])	!Save a python script to the named file, which, when loaded, reproduces this Config
saveToStream(outfile[, root])	!Save a python script to a stream, which, when loaded, reproduces this Config
setDefaults()	Derived config classes that must compute defaults rather than using the Field defaults should do so here.
toDict()	!Return a dict of field name: value
update(**kw)	!Update values specified by the keyword arguments
validate()	!Validate the Config; raise an exception if invalid
values()	!Return the list of field values

Attributes Documentation

assembleCcd

CCD assembly task (ConfigurableInstance, default <class 'lsst.ip.isr.assembleCcdTask.AssembleCcdConfig'>)

biasDataProductName

Name of the bias data product (str, default 'bias')

brighterFatterApplyGain

Should the gain be applied when applying the brighter fatter correction? (bool, default True)

brighterFatterKernelFile

Kernel file used for the brighter fatter correction (str, default '')

brighterFatterLevel

The level at which to correct for brighter-fatter (str, default 'DETECTOR')

Allowed values:

'AMP'

Every amplifier treated separately

'DETECTOR'

One kernel per detector

'None'

Field is optional

brighterFatterMaxIter

Maximum number of iterations for the brighter fatter correction (int, default 10)

brighterFatterThreshold

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. (float, default 1000)

crosstalk

Intra-CCD crosstalk correction (ConfigurableInstance, default <class 'lsst.ip.isr.crosstalk.CrosstalkConfig'>)

darkDataProductName

Name of the dark data product (str, default 'dark')

datasetType

Dataset type for input data; users will typically leave this alone, but camera-specific ISR tasks will override it (str, default 'raw')

doAddDistortionModel

Apply a distortion model based on camera geometry to the WCS? (bool, default True)

doAssembleCcd

Assemble amp-level exposures into a ccd-level exposure? (bool, default True)

doAssembleIsrExposures

Assemble amp-level calibration exposures into ccd-level exposure? (bool, default False)

doAttachTransmissionCurve

Construct and attach a wavelength-dependent throughput curve for this CCD image? (bool, default False)

doBias

Apply bias frame correction? (bool, default True)

doBrighterFatter

Apply the brighter fatter correction (bool, default False)

doCrosstalk

Apply intra-CCD crosstalk correction? (bool, default False)

doDark

Apply dark frame correction? (bool, default True)

doDefect

Apply correction for CCD defects, e.g. hot pixels? (bool, default True)

doEmpiricalReadNoise

Calculate empirical read noise instead of value from AmpInfo data? (bool, default False)

doFlat

Apply flat field correction? (bool, default True)

doFringe

Apply fringe correction? (bool, default True)

doLinearize

Correct for nonlinearity of the detector’s response? (bool, default True)

doNanInterpAfterFlat

If True, ensure we interpolate NaNs after flat-fielding, even if we also have to interpolate them before flat-fielding. (bool, default False)

doSaturationInterpolation

Perform interpolation over pixels masked as saturated? (bool, default True)

doUseAtmosphereTransmission

Load and use transmission_atmosphere (if doAttachTransmissionCurve is True)? (bool, default True)

doUseFilterTransmission

Load and use transmission_filter (if doAttachTransmissionCurve is True)? (bool, default True)

doUseOpticsTransmission

Load and use transmission_optics (if doAttachTransmissionCurve is True)? (bool, default True)

doUseSensorTransmission

Load and use transmission_sensor (if doAttachTransmissionCurve is True)? (bool, default True)

doWrite

Persist postISRCCD? (bool, default True)

expectWcs

Expect input science images to have a WCS (set False for e.g. spectrographs) (bool, default True)

fallbackFilterName

Fallback default filter name for calibrations (str, default None)

flatDataProductName

Name of the flat data product (str, default 'flat')

flatScalingType

The method for scaling the flat on the fly. (str, default 'USER')

Allowed values:

'USER'

Scale by flatUserScale

'MEAN'

Scale by the inverse of the mean

'MEDIAN'

Scale by the inverse of the median

'None'

Field is optional

flatUserScale

If flatScalingType is ‘USER’ then scale flat by this amount; ignored otherwise (float, default 1.0)

fluxMag0T1

The approximate flux of a zero-magnitude object in a one-second exposure (float, default 10000000000.0)

fringe

Fringe subtraction task (ConfigurableInstance, default <class 'lsst.ip.isr.fringe.FringeConfig'>)

fringeAfterFlat

Do fringe subtraction after flat-fielding? (bool, default True)

fwhm

FWHM of PSF (arcsec) (float, default 1.0)

gain

The gain to use if no Detector is present in the Exposure (ignored if NaN) (float, default nan)

growSaturationFootprintSize

Number of pixels by which to grow the saturation footprints (int, default 1)

history

keysToRemoveFromAssembledCcd

fields to remove from the metadata of the assembled ccd. (List, default [])

overscanFitType

The method for fitting the overscan bias level. (str, default 'MEDIAN')

Allowed values:

'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

'None'

Field is optional

overscanNumLeadingColumnsToSkip

Number of columns to skip in overscan, i.e. those closest to amplifier (int, default 0)

overscanNumSigmaClip

Rejection threshold (sigma) for collapsing overscan before fit (float, default 3.0)

overscanNumTrailingColumnsToSkip

Number of columns to skip in overscan, i.e. those farthest from amplifier (int, default 0)

overscanOrder

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. (int, default 1)

readNoise

The read noise to use if no Detector is present in the Exposure (float, default 0.0)

safe

Safety margin for CFHT sensors gain determination (float, default 0.95)

saturatedMaskName

Name of mask plane to use in saturation detection and interpolation (str, default 'SAT')

saturation

The saturation level to use if no Detector is present in the Exposure (ignored if NaN) (float, default nan)

suspectMaskName

Name of mask plane to use for suspect pixels (str, default 'SUSPECT')

Methods Documentation

compare(other, shortcut=True, rtol=1e-08, atol=1e-08, output=None)

!Compare two Configs for equality; return True if equal

If the Configs contain RegistryFields or ConfigChoiceFields, unselected Configs will not be compared.

@param[in] other Config object to compare with self. @param[in] shortcut If True, return as soon as an inequality is found. @param[in] rtol Relative tolerance for floating point comparisons. @param[in] atol Absolute tolerance for floating point comparisons. @param[in] output If not None, a callable that takes a string, used (possibly repeatedly)

to report inequalities.

Floating point comparisons are performed by numpy.allclose; refer to that for details.

formatHistory(name, **kwargs)

!Format the specified config field’s history to a more human-readable format

@param[in] name name of field whose history is wanted @param[in] kwargs keyword arguments for lsst.pex.config.history.format @return a string containing the formatted history

freeze()

!Make this Config and all sub-configs read-only

items()

!Return the list of (field name, field value) pairs

iteritems()

!Iterate over (field name, field value) pairs

iterkeys()

!Iterate over field names

itervalues()

!Iterate over field values

keys()

!Return the list of field names

load(filename, root='config')

!Modify this config in place by executing the Python code in the named file.

@param[in] filename name of file containing config override code @param[in] root name of variable in file that refers to the config being overridden

For example: if the value of root is “config” and the file contains this text: “config.myField = 5” then this config’s field “myField” is set to 5.

@deprecated For purposes of backwards compatibility, older config files that use root=”root” instead of root=”config” will be loaded with a warning printed to sys.stderr. This feature will be removed at some point.

loadFromStream(stream, root='config', filename=None)

!Modify this config in place by executing the python code in the provided stream.

@param[in] stream open file object, string or compiled string containing config override code @param[in] root name of variable in stream that refers to the config being overridden @param[in] filename name of config override file, or None if unknown or contained

in the stream; used for error reporting

For example: if the value of root is “config” and the stream contains this text: “config.myField = 5” then this config’s field “myField” is set to 5.

@deprecated For purposes of backwards compatibility, older config files that use root=”root” instead of root=”config” will be loaded with a warning printed to sys.stderr. This feature will be removed at some point.

names()

!Return all the keys in a config recursively

save(filename, root='config')

!Save a python script to the named file, which, when loaded, reproduces this Config

@param[in] filename name of file to which to write the config @param[in] root name to use for the root config variable; the same value must be used when loading

saveToStream(outfile, root='config')

!Save a python script to a stream, which, when loaded, reproduces this Config

@param outfile [inout] open file object to which to write the config. Accepts strings not bytes. @param root [in] name to use for the root config variable; the same value must be used when loading

setDefaults()

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

toDict()

!Return a dict of field name: value

Correct behavior is dependent on proper implementation of Field.toDict. If implementing a new Field type, you may need to implement your own toDict method.

update(**kw)

!Update values specified by the keyword arguments

@warning The ‘__at’ and ‘__label’ keyword arguments are special internal keywords. They are used to strip out any internal steps from the history tracebacks of the config. Modifying these keywords allows users to lie about a Config’s history. Please do not do so!

validate()

!Validate the Config; raise an exception if invalid

The base class implementation performs type checks on all fields by calling Field.validate().

Complex single-field validation can be defined by deriving new Field types. As syntactic sugar, some derived Field types are defined in this module which handle recursing into sub-configs (ConfigField, ConfigChoiceField)

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

values()

!Return the list of field values