Config for BrightStarMaskTask.
Definition at line 42 of file diffractionSpikeMask.py.
◆ angleMargin
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.angleMargin |
|
static |
Initial value:= Field(
dtype=float,
default=60.,
doc="Margin outside the exposure bounding box to include bright "
"sources. In arcseconds.",
)
Definition at line 77 of file diffractionSpikeMask.py.
◆ applyColorTerms
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.applyColorTerms |
|
static |
Initial value:= Field(
dtype=bool,
default=False,
doc=("Apply photometric color terms to reference stars?\n"
"`True`: attempt to apply color terms; fail if color term data is "
"not available for the specified reference catalog and filter.\n"
"`False`: do not apply color terms."),
optional=True,
)
Definition at line 47 of file diffractionSpikeMask.py.
◆ colorterms
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.colorterms |
|
static |
Initial value:= ConfigField(
dtype=ColortermLibrary,
doc="Library of photometric reference catalog name: color term dict"
" (see also applyColorTerms).",
)
Definition at line 56 of file diffractionSpikeMask.py.
◆ decKey
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.decKey |
|
static |
Initial value:= Field(
dtype=str,
default="coord_dec",
doc="Declination column name in the reference catalog.",
)
Definition at line 72 of file diffractionSpikeMask.py.
◆ diffractAngle
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.diffractAngle |
|
static |
Initial value:= Field(
dtype=float,
default=45,
doc="Angle in degrees of the location of diffraction spikes with "
"respect to camera at 0 rotation angle.",
)
Definition at line 89 of file diffractionSpikeMask.py.
◆ fallbackFluxField
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.fallbackFluxField |
|
static |
Initial value:= Field(
dtype=str,
default="phot_g_mean",
doc="Fallback flux field in the reference catalog to use for sources"
" that don't have measurements in the science image's band.",
)
Definition at line 119 of file diffractionSpikeMask.py.
◆ fallbackMagnitude
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.fallbackMagnitude |
|
static |
Initial value:= Field(
dtype=float,
default=12.,
doc="Default magnitude to use for sources in the reference catalog"
" with missing magnitudes that land in regions of saturated pixels.",
)
Definition at line 113 of file diffractionSpikeMask.py.
◆ magnitudeThreshold
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.magnitudeThreshold |
|
static |
Initial value:= Field(
dtype=float,
default=15,
doc="Threshold magnitude for treating a star from the reference catalog"
" as bright.",
)
Definition at line 83 of file diffractionSpikeMask.py.
◆ magOffset
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.magOffset |
|
static |
Initial value:= Field(
dtype=float,
default=3.8,
doc="Intercept of the fit for the log(spike length) as a function of"
" magnitude.",
)
Definition at line 107 of file diffractionSpikeMask.py.
◆ magSlope
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.magSlope |
|
static |
Initial value:= Field(
dtype=float,
default=-0.12,
doc="Slope of the fit for the log(spike length) as a function of"
" magnitude.",
)
Definition at line 101 of file diffractionSpikeMask.py.
◆ photoCatName
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.photoCatName |
|
static |
Initial value:= Field(
dtype=str,
optional=True,
doc=("Name of photometric reference catalog; used to select a color"
" term dict in colorterms. See also applyColorTerms."),
)
Definition at line 61 of file diffractionSpikeMask.py.
◆ raKey
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.raKey |
|
static |
Initial value:= Field(
dtype=str,
default="coord_ra",
doc="RA column name in the reference catalog.",
)
Definition at line 67 of file diffractionSpikeMask.py.
◆ refObjLoader
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.refObjLoader |
|
static |
Initial value:= ConfigField(dtype=LoadReferenceObjectsConfig,
doc="Configuration of reference object loader")
Definition at line 45 of file diffractionSpikeMask.py.
◆ saturatedMaskPlane
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.saturatedMaskPlane |
|
static |
Initial value:= Field(
dtype=str,
default="SAT",
doc="Name of the mask plane indicating a saturated pixel.",
)
Definition at line 131 of file diffractionSpikeMask.py.
◆ spikeAspectRatio
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.spikeAspectRatio |
|
static |
Initial value:= Field(
dtype=float,
default=10,
doc="Ratio of the length of a diffraction spike to it's width in the"
" core of the star.",
)
Definition at line 95 of file diffractionSpikeMask.py.
◆ spikeMask
| lsst.pipe.tasks.diffractionSpikeMask.DiffractionSpikeMaskConfig.spikeMask |
|
static |
Initial value:= Field(
dtype=str,
default="SPIKE",
doc="Name of the mask plane indicating likely contamination from"
" a diffraction spike.",
)
Definition at line 125 of file diffractionSpikeMask.py.
The documentation for this class was generated from the following file: