Inheritance diagram for lsst.meas.extensions.astrometryNet.anetBasicAstrometry.ANetBasicAstrometryConfig:
Detailed Description
Definition at line 110 of file anetBasicAstrometry.py.
Member Data Documentation
◆ allFluxes
|
static |
Initial value:
= Field(
doc="Retrieve all available fluxes (and errors) from catalog?",
dtype=bool,
default=True,
)
Definition at line 193 of file anetBasicAstrometry.py.
◆ badFlags
|
static |
Initial value:
= ListField(
doc="List of flags which cause a source to be rejected as bad",
dtype=str,
default=[
"slot_Centroid_flag", # bad centroids
"base_PixelFlags_flag_edge",
"base_PixelFlags_flag_saturated",
"base_PixelFlags_flag_crCenter", # cosmic rays
],
)
Definition at line 183 of file anetBasicAstrometry.py.
◆ calculateSip
|
static |
Initial value:
= Field(
doc="Compute polynomial SIP distortion terms?",
dtype=bool,
default=True,
)
Definition at line 172 of file anetBasicAstrometry.py.
◆ 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 160 of file anetBasicAstrometry.py.
◆ cleaningParameter
|
static |
Initial value:
= RangeField(
doc="Sigma-clipping parameter in cleanBadPoints.py",
dtype=float,
default=3.0,
min=0.0,
)
Definition at line 166 of file anetBasicAstrometry.py.
◆ 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 205 of file anetBasicAstrometry.py.
◆ 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 118 of file anetBasicAstrometry.py.
◆ maxCpuTime
|
static |
Initial value:
= RangeField(
doc="Maximum CPU time to spend solving, in seconds",
dtype=float,
default=0.,
min=0.,
)
Definition at line 112 of file anetBasicAstrometry.py.
◆ 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 198 of file anetBasicAstrometry.py.
◆ 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 124 of file anetBasicAstrometry.py.
◆ 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 152 of file anetBasicAstrometry.py.
◆ raDecSearchRadius
|
static |
Initial value:
= RangeField(
doc="When useWcsRaDecCenter=True, this is the radius, in degrees, around the RA,Dec center "
r"specified in the input exposure\'s WCS to search for a solution.",
dtype=float,
default=1.0,
min=0.0,
)
Definition at line 145 of file anetBasicAstrometry.py.
◆ sipOrder
|
static |
Initial value:
= RangeField(
doc="Polynomial order of SIP distortion terms",
dtype=int,
default=4,
min=2,
)
Definition at line 177 of file anetBasicAstrometry.py.
◆ 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 140 of file anetBasicAstrometry.py.
◆ useWcsPixelScale
|
static |
Initial value:
= Field(
doc="Use the pixel scale from the input exposure\'s WCS headers?",
dtype=bool,
default=True,
)
Definition at line 130 of file anetBasicAstrometry.py.
◆ 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 135 of file anetBasicAstrometry.py.
The documentation for this class was generated from the following file:
- /j/snowflake/release/lsstsw/stack/Linux64/meas_extensions_astrometryNet/18.1.0-3-g9bc06b8+7/python/lsst/meas/extensions/astrometryNet/anetBasicAstrometry.py
