LSSTApplications  10.0-2-g4f67435,11.0.rc2+1,11.0.rc2+12,11.0.rc2+3,11.0.rc2+4,11.0.rc2+5,11.0.rc2+6,11.0.rc2+7,11.0.rc2+8
LSSTDataManagementBasePackage
Static Public Attributes | List of all members
lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig Class Reference
Inheritance diagram for lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig:

Static Public Attributes

tuple maxCpuTime
 
tuple matchThreshold
 
tuple maxStars
 
tuple useWcsPixelScale
 
tuple useWcsRaDecCenter
 
tuple useWcsParity
 
tuple raDecSearchRadius
 
tuple pixelScaleUncertainty
 
tuple catalogMatchDist
 
tuple cleaningParameter
 
tuple calculateSip
 
tuple sipOrder
 
tuple badFlags
 
tuple allFluxes
 

Detailed Description

Definition at line 84 of file anetBasicAstrometry.py.

Member Data Documentation

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.allFluxes
static
Initial value:
1 = Field(
2  doc = "Retrieve all available fluxes (and errors) from catalog?",
3  dtype = bool,
4  default = True,
5  )

Definition at line 166 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.badFlags
static
Initial value:
1 = ListField(
2  doc = "List of flags which cause a source to be rejected as bad",
3  dtype = str,
4  default = [
5  "slot_Centroid_flag", # bad centroids
6  "base_PixelFlags_flag_edge",
7  "base_PixelFlags_flag_saturated",
8  "base_PixelFlags_flag_crCenter", # cosmic rays
9  ],
10  )

Definition at line 156 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.calculateSip
static
Initial value:
1 = Field(
2  doc = "Compute polynomial SIP distortion terms?",
3  dtype = bool,
4  default=True,
5  )

Definition at line 145 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.catalogMatchDist
static
Initial value:
1 = RangeField(
2  doc = "Matching radius (arcsec) for matching sources to reference objects",
3  dtype = float,
4  default=1.0,
5  min=0.0,
6  )

Definition at line 133 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.cleaningParameter
static
Initial value:
1 = RangeField(
2  doc = "Sigma-clipping parameter in sip/cleanBadPoints.py",
3  dtype = float,
4  default=3.0,
5  min=0.0,
6  )

Definition at line 139 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.matchThreshold
static
Initial value:
1 = RangeField(
2  doc = "Matching threshold for Astrometry.net solver (log-odds)",
3  dtype = float,
4  default=math.log(1e12),
5  min=math.log(1e6),
6  )

Definition at line 92 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.maxCpuTime
static
Initial value:
1 = RangeField(
2  doc = "Maximum CPU time to spend solving, in seconds",
3  dtype = float,
4  default = 0.,
5  min = 0.,
6  )

Definition at line 86 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.maxStars
static
Initial value:
1 = RangeField(
2  doc = "Maximum number of stars to use in Astrometry.net solving",
3  dtype = int,
4  default=50,
5  min=10,
6  )

Definition at line 98 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.pixelScaleUncertainty
static
Initial value:
1 = RangeField(
2  doc = "Range of pixel scales, around the value in the WCS header, to search. If the value of this field " +
3  "is X and the nominal scale is S, the range searched will be S/X to S*X",
4  dtype = float,
5  default = 1.1,
6  min=1.001,
7  )

Definition at line 126 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.raDecSearchRadius
static
Initial value:
1 = RangeField(
2  doc = "When useWcsRaDecCenter=True, this is the radius, in degrees, around the RA,Dec center " +
3  "specified in the input exposure\'s WCS to search for a solution.",
4  dtype = float,
5  default=1.0,
6  min=0.0,
7  )

Definition at line 119 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.sipOrder
static
Initial value:
1 = RangeField(
2  doc = "Polynomial order of SIP distortion terms",
3  dtype = int,
4  default=4,
5  min=2,
6  )

Definition at line 150 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.useWcsParity
static
Initial value:
1 = Field(
2  doc="Use the parity (flip / handedness) of the image from the input exposure\'s WCS headers?",
3  dtype=bool,
4  default=True,
5  )

Definition at line 114 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.useWcsPixelScale
static
Initial value:
1 = Field(
2  doc = "Use the pixel scale from the input exposure\'s WCS headers?",
3  dtype = bool,
4  default = True,
5  )

Definition at line 104 of file anetBasicAstrometry.py.

tuple lsst.meas.astrom.anetBasicAstrometry.ANetBasicAstrometryConfig.useWcsRaDecCenter
static
Initial value:
1 = Field(
2  doc="Use the RA,Dec center information from the input exposure\'s WCS headers?",
3  dtype=bool,
4  default=True,
5  )

Definition at line 109 of file anetBasicAstrometry.py.


The documentation for this class was generated from the following file: