Configuration parameters for ProcessBrightStarsTask.
Definition at line 82 of file processBrightStars.py.
◆ annularFluxRadii
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.annularFluxRadii |
|
static |
Initial value:= pexConfig.ListField(
dtype=int,
doc="Inner and outer radii of the annulus used to compute the AnnularFlux for normalization, "
"in pixels.",
default=(40, 50)
)
Definition at line 125 of file processBrightStars.py.
◆ annularFluxStatistic
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.annularFluxStatistic |
|
static |
Initial value:= pexConfig.ChoiceField(
dtype=str,
doc="Type of statistic to use to compute annular flux.",
default="MEANCLIP",
allowed={
"MEAN": "mean",
"MEDIAN": "median",
"MEANCLIP": "clipped mean",
}
)
Definition at line 131 of file processBrightStars.py.
◆ badMaskPlanes
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.badMaskPlanes |
|
static |
Initial value:= pexConfig.ListField(
dtype=str,
doc="Mask planes that, if set, lead to associated pixels not being included in the computation of the"
" annular flux.",
default=('BAD', 'CR', 'CROSSTALK', 'EDGE', 'NO_DATA', 'SAT', 'SUSPECT', 'UNMASKEDNAN')
)
Definition at line 151 of file processBrightStars.py.
◆ discardNanFluxStars
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.discardNanFluxStars |
|
static |
Initial value:= pexConfig.Field(
dtype=bool,
doc="Should stars with NaN annular flux be discarded?",
default=False
)
Definition at line 168 of file processBrightStars.py.
◆ doApplySkyCorr
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.doApplySkyCorr |
|
static |
Initial value:= pexConfig.Field(
dtype=bool,
doc="Apply full focal plane sky correction before extracting stars?",
default=True
)
Definition at line 163 of file processBrightStars.py.
◆ doApplyTransform
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.doApplyTransform |
|
static |
Initial value:= pexConfig.Field(
dtype=bool,
doc="Apply transform to bright star stamps to correct for optical distortions?",
default=True
)
Definition at line 109 of file processBrightStars.py.
◆ doRemoveDetected
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.doRemoveDetected |
|
static |
Initial value:= pexConfig.Field(
dtype=bool,
doc="Whether DETECTION footprints, other than that for the central object, should be changed to "
"BAD",
default=True
)
Definition at line 103 of file processBrightStars.py.
◆ magLimit
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.magLimit |
|
static |
Initial value:= pexConfig.Field(
dtype=float,
doc="Magnitude limit, in Gaia G; all stars brighter than this value will be processed",
default=18
)
Definition at line 87 of file processBrightStars.py.
◆ minPixelsWithinFrame
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.minPixelsWithinFrame |
|
static |
Initial value:= pexConfig.Field(
dtype=int,
doc="Minimum number of pixels that must fall within the stamp boundary for the bright star to be"
" saved when its center is beyond the exposure boundary.",
default=50
)
Definition at line 157 of file processBrightStars.py.
◆ modelStampBuffer
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.modelStampBuffer |
|
static |
Initial value:= pexConfig.Field(
dtype=float,
doc="'Buffer' factor to be applied to determine the size of the stamp the processed stars will "
"be saved in. This will also be the size of the extended PSF model.",
default=1.1
)
Definition at line 97 of file processBrightStars.py.
◆ numIter
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.numIter |
|
static |
Initial value:= pexConfig.Field(
dtype=int,
doc="Number of iterations of outlier rejection; ignored if annularFluxStatistic != 'MEANCLIP'.",
default=3
)
Definition at line 146 of file processBrightStars.py.
◆ numSigmaClip
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.numSigmaClip |
|
static |
Initial value:= pexConfig.Field(
dtype=float,
doc="Sigma for outlier rejection; ignored if annularFluxStatistic != 'MEANCLIP'.",
default=4
)
Definition at line 141 of file processBrightStars.py.
◆ refObjLoader
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.refObjLoader |
|
static |
Initial value:= pexConfig.ConfigField(
dtype=LoadReferenceObjectsConfig,
doc="Reference object loader for astrometric calibration.",
)
Definition at line 173 of file processBrightStars.py.
◆ stampSize
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.stampSize |
|
static |
Initial value:= pexConfig.ListField(
dtype=int,
doc="Size of the stamps to be extracted, in pixels",
default=(250, 250)
)
Definition at line 92 of file processBrightStars.py.
◆ warpingKernelName
pexConfig lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.warpingKernelName |
|
static |
Initial value:= pexConfig.ChoiceField(
dtype=str,
doc="Warping kernel",
default="lanczos5",
allowed={
"bilinear": "bilinear interpolation",
"lanczos3": "Lanczos kernel of order 3",
"lanczos4": "Lanczos kernel of order 4",
"lanczos5": "Lanczos kernel of order 5",
}
)
Definition at line 114 of file processBrightStars.py.
The documentation for this class was generated from the following file: