Definition at line 46 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.assembleCcd |
|
static |
Initial value: 1 = pexConfig.ConfigurableField(
2 target=AssembleCcdTask,
3 doc=
"CCD assembly task",
Definition at line 77 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterApplyGain |
|
static |
Initial value:
4 doc=
"Should the gain be applied when applying the brighter fatter correction?"
Definition at line 218 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterKernelFile |
|
static |
Initial value:
4 doc=
"Kernel file used for the brighter fatter correction"
Definition at line 201 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterMaxIter |
|
static |
Initial value:
4 doc=
"Maximum number of iterations for the brighter fatter correction"
Definition at line 206 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.brighterFatterThreshold |
|
static |
Initial value:
4 doc=
"Threshold used to stop iterating the brighter fatter correction. It is the "
5 " absolute value of the difference between the current corrected image and the one"
6 " from the previous iteration summed over all the pixels."
Definition at line 211 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.datasetType |
|
static |
Initial value:
3 doc=
"Dataset type for input data; users will typically leave this alone, "
4 "but camera-specific ISR tasks will override it",
Definition at line 223 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doAssembleCcd |
|
static |
Initial value:
4 doc=
"Assemble amp-level exposures into a ccd-level exposure?"
Definition at line 186 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doAssembleIsrExposures |
|
static |
Initial value:
4 doc=
"Assemble amp-level calibration exposures into ccd-level exposure?"
Definition at line 181 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doBias |
|
static |
Initial value:
3 doc=
"Apply bias frame correction?",
Definition at line 47 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doBrighterFatter |
|
static |
Initial value:
4 doc=
"Apply the brighter fatter correction"
Definition at line 196 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doDark |
|
static |
Initial value:
3 doc=
"Apply dark frame correction?",
Definition at line 52 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doDefect |
|
static |
Initial value:
3 doc=
"Apply correction for CCD defects, e.g. hot pixels?",
Definition at line 67 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doFlat |
|
static |
Initial value:
3 doc=
"Apply flat field correction?",
Definition at line 57 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doFringe |
|
static |
Initial value:
3 doc=
"Apply fringe correction?",
Definition at line 62 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doLinearize |
|
static |
Initial value:
3 doc=
"Correct for nonlinearity of the detector's response?",
Definition at line 191 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doSaturationInterpolation |
|
static |
Initial value:
3 doc=
"Perform interpolation over pixels masked as saturated?",
Definition at line 166 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.doWrite |
|
static |
Initial value:
3 doc=
"Persist postISRCCD?",
Definition at line 72 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.fallbackFilterName |
|
static |
Initial value: 1 = pexConfig.Field(dtype=str,
2 doc=
"Fallback default filter name for calibrations", optional=
True)
Definition at line 229 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.flatScalingType |
|
static |
Initial value: 1 = pexConfig.ChoiceField(
3 doc=
"The method for scaling the flat on the fly.",
6 "USER":
"Scale by flatUserScale",
7 "MEAN":
"Scale by the inverse of the mean",
8 "MEDIAN":
"Scale by the inverse of the median",
Definition at line 120 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.flatUserScale |
|
static |
Initial value:
3 doc=
"If flatScalingType is 'USER' then scale flat by this amount; ignored otherwise",
Definition at line 130 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.fluxMag0T1 |
|
static |
Initial value:
3 doc=
"The approximate flux of a zero-magnitude object in a one-second exposure",
Definition at line 171 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.fringe |
|
static |
Initial value: 1 = pexConfig.ConfigurableField(
3 doc=
"Fringe subtraction task",
Definition at line 101 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.fringeAfterFlat |
|
static |
Initial value:
3 doc=
"Do fringe subtraction after flat-fielding?",
Definition at line 96 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.fwhm |
|
static |
Initial value:
3 doc=
"FWHM of PSF (arcsec)",
Definition at line 105 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.gain |
|
static |
Initial value:
3 doc=
"The gain to use if no Detector is present in the Exposure (ignored if NaN)",
Definition at line 81 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.growSaturationFootprintSize |
|
static |
Initial value:
3 doc=
"Number of pixels by which to grow the saturation footprints",
Definition at line 161 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.keysToRemoveFromAssembledCcd |
|
static |
Initial value:
3 doc=
"fields to remove from the metadata of the assembled ccd.",
Definition at line 176 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.overscanFitType |
|
static |
Initial value: 1 = pexConfig.ChoiceField(
3 doc=
"The method for fitting the overscan bias level.",
6 "POLY":
"Fit ordinary polynomial to the longest axis of the overscan region",
7 "CHEB":
"Fit Chebyshev polynomial to the longest axis of the overscan region",
8 "LEG":
"Fit Legendre polynomial to the longest axis of the overscan region",
9 "NATURAL_SPLINE":
"Fit natural spline to the longest axis of the overscan region",
10 "CUBIC_SPLINE":
"Fit cubic spline to the longest axis of the overscan region",
11 "AKIMA_SPLINE":
"Fit Akima spline to the longest axis of the overscan region",
12 "MEAN":
"Correct using the mean of the overscan region",
13 "MEDIAN":
"Correct using the median of the overscan region",
Definition at line 135 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.overscanOrder |
|
static |
Initial value:
3 doc=(
"Order of polynomial or to fit if overscan fit type is a polynomial, " +
4 "or number of spline knots if overscan fit type is a spline."),
Definition at line 150 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.overscanRej |
|
static |
Initial value:
3 doc=
"Rejection threshold (sigma) for collapsing overscan before fit",
Definition at line 156 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.readNoise |
|
static |
Initial value:
3 doc=
"The read noise to use if no Detector is present in the Exposure",
Definition at line 86 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.saturatedMaskName |
|
static |
Initial value:
3 doc=
"Name of mask plane to use in saturation detection and interpolation",
Definition at line 110 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.saturation |
|
static |
Initial value:
3 doc=
"The saturation level to use if no Detector is present in the Exposure (ignored if NaN)",
Definition at line 91 of file isrTask.py.
tuple lsst.ip.isr.isrTask.IsrTaskConfig.suspectMaskName |
|
static |
Initial value:
3 doc=
"Name of mask plane to use for suspect pixels",
Definition at line 115 of file isrTask.py.
The documentation for this class was generated from the following file: