Configuration parameters for ProcessBrightStarsTask.
Definition at line 85 of file processBrightStars.py.
◆ annularFluxRadii
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.annularFluxRadii |
|
static |
Initial value:= ListField(
dtype=int,
doc="Inner and outer radii of the annulus used to compute AnnularFlux for normalization, in pixels.",
default=(40, 50),
)
Definition at line 127 of file processBrightStars.py.
◆ annularFluxStatistic
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.annularFluxStatistic |
|
static |
Initial value:= 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 132 of file processBrightStars.py.
◆ badMaskPlanes
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.badMaskPlanes |
|
static |
Initial value:= ListField(
dtype=str,
doc="Mask planes that identify pixels to not include in the computation of the annular flux.",
default=("BAD", "CR", "CROSSTALK", "EDGE", "NO_DATA", "SAT", "SUSPECT", "UNMASKEDNAN"),
)
Definition at line 152 of file processBrightStars.py.
◆ discardNanFluxStars
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.discardNanFluxStars |
|
static |
Initial value:= Field(
dtype=bool,
doc="Should stars with NaN annular flux be discarded?",
default=False,
)
Definition at line 170 of file processBrightStars.py.
◆ doApplySkyCorr
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.doApplySkyCorr |
|
static |
Initial value:= Field(
dtype=bool,
doc="Apply full focal plane sky correction before extracting stars?",
default=True,
)
Definition at line 165 of file processBrightStars.py.
◆ doApplyTransform
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.doApplyTransform |
|
static |
Initial value:= Field(
dtype=bool,
doc="Apply transform to bright star stamps to correct for optical distortions?",
default=True,
)
Definition at line 111 of file processBrightStars.py.
◆ doRemoveDetected
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.doRemoveDetected |
|
static |
Initial value:= Field(
dtype=bool,
doc="Whether DETECTION footprints, other than that for the central object, should be changed to BAD.",
default=True,
)
Definition at line 106 of file processBrightStars.py.
◆ magLimit
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.magLimit |
|
static |
Initial value:= Field(
dtype=float,
doc="Magnitude limit, in Gaia G; all stars brighter than this value will be processed.",
default=18,
)
Definition at line 88 of file processBrightStars.py.
◆ minPixelsWithinFrame
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.minPixelsWithinFrame |
|
static |
Initial value:= 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
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.modelStampBuffer |
|
static |
Initial value:= 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 98 of file processBrightStars.py.
◆ numIter
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.numIter |
|
static |
Initial value:= Field(
dtype=int,
doc="Number of iterations of outlier rejection; ignored if annularFluxStatistic != 'MEANCLIP'.",
default=3,
)
Definition at line 147 of file processBrightStars.py.
◆ numSigmaClip
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.numSigmaClip |
|
static |
Initial value:= Field(
dtype=float,
doc="Sigma for outlier rejection; ignored if annularFluxStatistic != 'MEANCLIP'.",
default=4,
)
Definition at line 142 of file processBrightStars.py.
◆ refObjLoader
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.refObjLoader |
|
static |
Initial value:= ConfigField(
dtype=LoadReferenceObjectsConfig,
doc="Reference object loader for astrometric calibration.",
)
Definition at line 175 of file processBrightStars.py.
◆ stampSize
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.stampSize |
|
static |
Initial value:= ListField(
dtype=int,
doc="Size of the stamps to be extracted, in pixels.",
default=(250, 250),
)
Definition at line 93 of file processBrightStars.py.
◆ warpingKernelName
lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.warpingKernelName |
|
static |
Initial value:= 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 116 of file processBrightStars.py.
The documentation for this class was generated from the following file: