Inheritance diagram for lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig:
Public Member Functions | |
| def | setDefaults (self) |
Detailed Description
Configuration parameters for ProcessBrightStarsTask
Definition at line 82 of file processBrightStars.py.
Member Function Documentation
◆ setDefaults()
| def lsst.pipe.tasks.processBrightStars.ProcessBrightStarsConfig.setDefaults | ( | self | ) |
Definition at line 177 of file processBrightStars.py.
Member Data Documentation
◆ 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 124 of file processBrightStars.py.
◆ 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 130 of file processBrightStars.py.
◆ 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 150 of file processBrightStars.py.
◆ brightStarStamps
|
staticinherited |
Initial value:
= cT.Output(
doc="Set of preprocessed postage stamps, each centered on a single bright star.",
name="brightStarStamps",
storageClass="BrightStarStamps",
dimensions=("visit", "detector")
)
Definition at line 69 of file processBrightStars.py.
◆ discardNanFluxStars
|
static |
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Should stars with NaN annular flux be discarded?",
default=False
)
Definition at line 167 of file processBrightStars.py.
◆ doApplySkyCorr
|
static |
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Apply full focal plane sky correction before extracting stars?",
default=True
)
Definition at line 162 of file processBrightStars.py.
◆ 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 108 of file processBrightStars.py.
◆ 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 102 of file processBrightStars.py.
◆ inputExposure
|
staticinherited |
Initial value:
= cT.Input(
doc="Input exposure from which to extract bright star stamps",
name="calexp",
storageClass="ExposureF",
dimensions=("visit", "detector")
)
Definition at line 49 of file processBrightStars.py.
◆ 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 86 of file processBrightStars.py.
◆ 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 156 of file processBrightStars.py.
◆ 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 96 of file processBrightStars.py.
◆ numIter
|
static |
Initial value:
= pexConfig.Field(
dtype=int,
doc="Number of iterations of outlier rejection; ignored if annularFluxStatistic != 'MEANCLIP'.",
default=3
)
Definition at line 145 of file processBrightStars.py.
◆ numSigmaClip
|
static |
Initial value:
= pexConfig.Field(
dtype=float,
doc="Sigma for outlier rejection; ignored if annularFluxStatistic != 'MEANCLIP'.",
default=4
)
Definition at line 140 of file processBrightStars.py.
◆ refCat
|
staticinherited |
Initial value:
= cT.PrerequisiteInput(
doc="Reference catalog that contains bright star positions",
name="gaia_dr2_20200414",
storageClass="SimpleCatalog",
dimensions=("skypix",),
multiple=True,
deferLoad=True
)
Definition at line 61 of file processBrightStars.py.
◆ refObjLoader
|
static |
Initial value:
= pexConfig.ConfigurableField(
target=LoadIndexedReferenceObjectsTask,
doc="Reference object loader for astrometric calibration.",
)
Definition at line 172 of file processBrightStars.py.
◆ skyCorr
|
staticinherited |
Initial value:
= cT.Input(
doc="Input Sky Correction to be subtracted from the calexp if doApplySkyCorr=True",
name="skyCorr",
storageClass="Background",
dimensions=("instrument", "visit", "detector")
)
Definition at line 55 of file processBrightStars.py.
◆ stampSize
|
static |
Initial value:
= pexConfig.ListField(
dtype=int,
doc="Size of the stamps to be extracted, in pixels",
default=(250, 250)
)
Definition at line 91 of file processBrightStars.py.
◆ 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 113 of file processBrightStars.py.
The documentation for this class was generated from the following file:
- /j/snowflake/release/lsstsw/stack/lsst-scipipe-0.7.0/Linux64/pipe_tasks/21.0.0-172-gfb10e10a+18fedfabac/python/lsst/pipe/tasks/processBrightStars.py
