Inheritance diagram for lsst.pipe.tasks.computeExposureSummaryStats.ComputeExposureSummaryStatsConfig:
Public Member Functions | |
| setDefaults (self) | |
Detailed Description
Config for ComputeExposureSummaryTask
Definition at line 41 of file computeExposureSummaryStats.py.
Member Function Documentation
◆ setDefaults()
| lsst.pipe.tasks.computeExposureSummaryStats.ComputeExposureSummaryStatsConfig.setDefaults | ( | self | ) |
Definition at line 135 of file computeExposureSummaryStats.py.
135 def setDefaults(self):
136 super().setDefaults()
137
138 self.starSelector.setDefaults()
139 self.starSelector.doFlags = True
140 self.starSelector.doSignalToNoise = True
141 self.starSelector.doUnresolved = False
142 self.starSelector.doIsolated = False
143 self.starSelector.doRequireFiniteRaDec = False
144 self.starSelector.doRequirePrimary = False
145
146 self.starSelector.signalToNoise.minimum = 50.0
147 self.starSelector.signalToNoise.maximum = 1000.0
148
149 self.starSelector.flags.bad = ["slot_Shape_flag", "slot_PsfFlux_flag"]
150 # Select stars used for PSF modeling.
151 self.starSelector.flags.good = ["calib_psf_used"]
152
153 self.starSelector.signalToNoise.fluxField = "slot_PsfFlux_instFlux"
154 self.starSelector.signalToNoise.errField = "slot_PsfFlux_instFluxErr"
155
156
Member Data Documentation
◆ badMaskPlanes
|
static |
Initial value:
= pexConfig.ListField(
dtype=str,
doc="Mask planes that, if set, the associated pixel should not be included sky noise calculation.",
default=("NO_DATA", "SUSPECT"),
)
Definition at line 53 of file computeExposureSummaryStats.py.
◆ clipIter
|
static |
Initial value:
= pexConfig.Field(
dtype=int,
doc="Number of iterations of outlier rejection for sky noise.",
default=2,
)
Definition at line 48 of file computeExposureSummaryStats.py.
◆ fiducialPsfSigma
|
static |
Initial value:
= pexConfig.DictField(
keytype=str,
itemtype=float,
doc="Fiducial PSF sigma (pixels) assumed when calculating effective exposure time. "
"Keyed by band.",
default={'u': 1.0, 'g': 1.0, 'r': 1.0, 'i': 1.0, 'z': 1.0, 'y': 1.0},
)
Definition at line 115 of file computeExposureSummaryStats.py.
◆ fiducialSkyBackground
|
static |
Initial value:
= pexConfig.DictField(
keytype=str,
itemtype=float,
doc="Fiducial sky background level (ADU/s) assumed when calculating effective exposure time. "
"Keyed by band.",
default={'u': 1.0, 'g': 1.0, 'r': 1.0, 'i': 1.0, 'z': 1.0, 'y': 1.0},
)
Definition at line 108 of file computeExposureSummaryStats.py.
◆ fiducialZeroPoint
|
static |
Initial value:
= pexConfig.DictField(
keytype=str,
itemtype=float,
doc="Fiducial zero point assumed when calculating effective exposure time. "
"Keyed by band.",
default={'u': 25.0, 'g': 25.0, 'r': 25.0, 'i': 25.0, 'z': 25.0, 'y': 25.0},
)
Definition at line 122 of file computeExposureSummaryStats.py.
◆ maxEffectiveTransparency
|
static |
Initial value:
= pexConfig.Field(
dtype=float,
doc="Maximum value allowed for effective transparency scale factor (often inf or 1.0).",
default=float('inf')
)
Definition at line 129 of file computeExposureSummaryStats.py.
◆ minPsfApRadiusPix
|
static |
Initial value:
= pexConfig.Field(
dtype=float,
doc="Minimum radius in pixels of the aperture within which to measure the flux of "
"the PSF model for the psfApFluxDelta metric calculation (the radius is computed as "
"max(``minPsfApRadius``, 3*psfSigma)).",
default=2.0,
)
Definition at line 89 of file computeExposureSummaryStats.py.
◆ psfApCorrFieldName
|
static |
Initial value:
= pexConfig.Field(
doc="Name of the flux column associated with the aperture correction of the PSF model "
"to use for the psfApCorrSigmaScaledDelta metric calculation.",
dtype=str,
default="base_PsfFlux_instFlux"
)
Definition at line 96 of file computeExposureSummaryStats.py.
◆ psfBadMaskPlanes
|
static |
Initial value:
= pexConfig.ListField(
dtype=str,
doc="Mask planes that, if set, the associated pixel should not be included in the PSF model "
"robutsness metric calculations (namely, maxDistToNearestPsf and psfTraceRadiusDelta).",
default=("BAD", "CR", "EDGE", "INTRP", "NO_DATA", "SAT", "SUSPECT"),
)
Definition at line 102 of file computeExposureSummaryStats.py.
◆ psfGridSampling
|
static |
Initial value:
= pexConfig.Field(
dtype=int,
doc="Sampling rate in pixels in each dimension for PSF model robustness metric "
"caclulations grid (the tradeoff is between adequate sampling versus speed).",
default=96,
)
Definition at line 83 of file computeExposureSummaryStats.py.
◆ psfSampling
|
static |
Initial value:
= pexConfig.Field(
dtype=int,
doc="Sampling rate in pixels in each dimension for the maxDistToNearestPsf metric "
"caclulation grid (the tradeoff is between adequate sampling versus speed).",
default=8,
)
Definition at line 77 of file computeExposureSummaryStats.py.
◆ psfShape
|
static |
Initial value:
= pexConfig.Field(
doc="Base name of columns to use for the PSF shape in the PSF statistics computation.",
dtype=str,
default="slot_PsfShape"
)
Definition at line 72 of file computeExposureSummaryStats.py.
◆ sigmaClip
|
static |
Initial value:
= pexConfig.Field(
dtype=float,
doc="Sigma for outlier rejection for sky noise.",
default=3.0,
)
Definition at line 43 of file computeExposureSummaryStats.py.
◆ starSelection
|
static |
Initial value:
= pexConfig.Field(
doc="Field to select full list of sources used for PSF modeling.",
dtype=str,
default="calib_psf_used",
)
Definition at line 58 of file computeExposureSummaryStats.py.
◆ starSelector
|
static |
Initial value:
= pexConfig.ConfigurableField(
target=ScienceSourceSelectorTask,
doc="Selection of sources to compute PSF star statistics.",
)
Definition at line 63 of file computeExposureSummaryStats.py.
◆ starShape
|
static |
Initial value:
= pexConfig.Field(
doc="Base name of columns to use for the source shape in the PSF statistics computation.",
dtype=str,
default="slot_Shape"
)
Definition at line 67 of file computeExposureSummaryStats.py.
The documentation for this class was generated from the following file:
- /j/snowflake/release/lsstsw/stack/lsst-scipipe-8.0.0/Linux64/pipe_tasks/ge6cb8fbbf7+0992c83eee/python/lsst/pipe/tasks/computeExposureSummaryStats.py
