Definition at line 117 of file anetBasicAstrometry.py.
◆ allFluxes
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.allFluxes |
|
static |
Initial value:= Field(
doc="Retrieve all available fluxes (and errors) from catalog?",
dtype=bool,
default=True,
)
Definition at line 200 of file anetBasicAstrometry.py.
◆ badFlags
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.badFlags |
|
static |
Initial value:= ListField(
doc="List of flags which cause a source to be rejected as bad",
dtype=str,
default=[
"slot_Centroid_flag",
"base_PixelFlags_flag_edge",
"base_PixelFlags_flag_saturated",
"base_PixelFlags_flag_crCenter",
],
)
Definition at line 190 of file anetBasicAstrometry.py.
◆ calculateSip
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.calculateSip |
|
static |
Initial value:= Field(
doc="Compute polynomial SIP distortion terms?",
dtype=bool,
default=True,
)
Definition at line 179 of file anetBasicAstrometry.py.
◆ catalogMatchDist
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.catalogMatchDist |
|
static |
Initial value:= RangeField(
doc="Matching radius (arcsec) for matching sources to reference objects",
dtype=float,
default=1.0,
min=0.0,
)
Definition at line 167 of file anetBasicAstrometry.py.
◆ cleaningParameter
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.cleaningParameter |
|
static |
Initial value:= RangeField(
doc="Sigma-clipping parameter in cleanBadPoints.py",
dtype=float,
default=3.0,
min=0.0,
)
Definition at line 173 of file anetBasicAstrometry.py.
◆ matchDistanceSigma
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.matchDistanceSigma |
|
static |
Initial value:= RangeField(
doc="The match and fit loop stops when maxMatchDist minimized: "
" maxMatchDist = meanMatchDist + matchDistanceSigma*stdDevMatchDistance " +
" (where the mean and std dev are computed using outlier rejection);" +
" ignored if not fitting a WCS",
dtype=float,
default=2,
min=0,
)
Definition at line 212 of file anetBasicAstrometry.py.
◆ matchThreshold
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.matchThreshold |
|
static |
Initial value:= RangeField(
doc="Matching threshold for Astrometry.net solver (log-odds)",
dtype=float,
default=math.log(1e12),
min=math.log(1e6),
)
Definition at line 125 of file anetBasicAstrometry.py.
◆ maxCpuTime
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.maxCpuTime |
|
static |
Initial value:= RangeField(
doc="Maximum CPU time to spend solving, in seconds",
dtype=float,
default=0.,
min=0.,
)
Definition at line 119 of file anetBasicAstrometry.py.
◆ maxIter
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.maxIter |
|
static |
Initial value:= RangeField(
doc="maximum number of iterations of match sources and fit WCS" +
"ignored if not fitting a WCS",
dtype=int,
default=5,
min=1,
)
Definition at line 205 of file anetBasicAstrometry.py.
◆ maxStars
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.maxStars |
|
static |
Initial value:= RangeField(
doc="Maximum number of stars to use in Astrometry.net solving",
dtype=int,
default=50,
min=10,
)
Definition at line 131 of file anetBasicAstrometry.py.
◆ pixelScaleUncertainty
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.pixelScaleUncertainty |
|
static |
Initial value:= RangeField(
doc="Range of pixel scales, around the value in the WCS header, to search. " +
"If the value of this field is X and the nominal scale is S, " +
"the range searched will be S/X to S*X",
dtype=float,
default=1.1,
min=1.001,
)
Definition at line 159 of file anetBasicAstrometry.py.
◆ raDecSearchRadius
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.raDecSearchRadius |
|
static |
Initial value:= RangeField(
doc="When useWcsRaDecCenter=True, this is the radius, in degrees, around the RA,Dec center " +
"specified in the input exposure\'s WCS to search for a solution.",
dtype=float,
default=1.0,
min=0.0,
)
Definition at line 152 of file anetBasicAstrometry.py.
◆ sipOrder
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.sipOrder |
|
static |
Initial value:= RangeField(
doc="Polynomial order of SIP distortion terms",
dtype=int,
default=4,
min=2,
)
Definition at line 184 of file anetBasicAstrometry.py.
◆ useWcsParity
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.useWcsParity |
|
static |
Initial value:= Field(
doc="Use the parity (flip / handedness) of the image from the input exposure\'s WCS headers?",
dtype=bool,
default=True,
)
Definition at line 147 of file anetBasicAstrometry.py.
◆ useWcsPixelScale
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.useWcsPixelScale |
|
static |
Initial value:= Field(
doc="Use the pixel scale from the input exposure\'s WCS headers?",
dtype=bool,
default=True,
)
Definition at line 137 of file anetBasicAstrometry.py.
◆ useWcsRaDecCenter
lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig.useWcsRaDecCenter |
|
static |
Initial value:= Field(
doc="Use the RA,Dec center information from the input exposure\'s WCS headers?",
dtype=bool,
default=True,
)
Definition at line 142 of file anetBasicAstrometry.py.
The documentation for this class was generated from the following file: