lsst.pipe.tasks.computeExposureSummaryStats.ComputeExposureSummaryStatsConfig Class Reference
Inheritance diagram for lsst.pipe.tasks.computeExposureSummaryStats.ComputeExposureSummaryStatsConfig:
Public Member Functions | |
| setDefaults (self) | |
Detailed Description
Config for ComputeExposureSummaryTask
Definition at line 42 of file computeExposureSummaryStats.py.
Member Function Documentation
◆ setDefaults()
| lsst.pipe.tasks.computeExposureSummaryStats.ComputeExposureSummaryStatsConfig.setDefaults | ( | self | ) |
Definition at line 141 of file computeExposureSummaryStats.py.
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 54 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 49 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 116 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 109 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 123 of file computeExposureSummaryStats.py.
◆ magLimSnr
|
static |
Initial value:
= pexConfig.Field(
dtype=float,
doc="Signal-to-noise ratio for computing the magnitude limit depth.",
default=5.0
)
Definition at line 135 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 130 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 90 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 97 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 103 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 84 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 78 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 73 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 44 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 59 of file computeExposureSummaryStats.py.
◆ starSelector
|
static |
Initial value:
= pexConfig.ConfigurableField(
target=ScienceSourceSelectorTask,
doc="Selection of sources to compute PSF star statistics.",
)
Definition at line 64 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 68 of file computeExposureSummaryStats.py.
The documentation for this class was generated from the following file:
- python/lsst/pipe/tasks/computeExposureSummaryStats.py
Generated on for lsst.pipe.tasks by
1.17.0