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LSST Data Management Base Package
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Public Member Functions | Static Public Attributes | List of all members
lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig Class Reference
Inheritance diagram for lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig:
lsst.meas.algorithms.detection.SourceDetectionConfig

Public Member Functions

 setDefaults (self)
 

Static Public Attributes

 prelimThresholdFactor
 
 prelimNegMultiplier
 
 skyObjects = ConfigurableField(target=SkyObjectsTask, doc="Generate sky objects.")
 
 doBackgroundTweak
 
 minFractionSources
 
 doBrightPrelimDetection
 
 brightMultiplier
 
 brightNegFactor
 
 brightGrowFactor
 
 brightMaskFractionMax
 
 bisectFactor
 

Detailed Description

Configuration for DynamicDetectionTask

Definition at line 22 of file dynamicDetection.py.

Member Function Documentation

◆ setDefaults()

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.setDefaults ( self)

Reimplemented from lsst.meas.algorithms.detection.SourceDetectionConfig.

Definition at line 64 of file dynamicDetection.py.

64 def setDefaults(self):
65 SourceDetectionConfig.setDefaults(self)
66 self.skyObjects.nSources = 1000 # For good statistics
67 for maskStr in ["SAT"]:
68 if maskStr not in self.skyObjects.avoidMask:
69 self.skyObjects.avoidMask.append(maskStr)
70
71

Member Data Documentation

◆ bisectFactor

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.bisectFactor
static
Initial value:
= Field(dtype=float, default=1.2,
doc="Factor by which to increase thresholds in brightMaskFractionMax loop.")

Definition at line 61 of file dynamicDetection.py.

◆ brightGrowFactor

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.brightGrowFactor
static
Initial value:
= Field(dtype=int, default=40,
doc="Factor by which to grow the footprints of sources detected in the "
"\"bright\" detections stage (want this to be large to mask wings of "
"bright sources).")

Definition at line 51 of file dynamicDetection.py.

◆ brightMaskFractionMax

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.brightMaskFractionMax
static
Initial value:
= Field(dtype=float, default=0.95,
doc="Maximum allowed fraction of masked pixes from the \"bright\" "
"detection stage (to mask regions unsuitable for sky sourcess). "
"If this fraction is exeeded, the detection threshold for this stage "
"will be increased by bisectFactor until the fraction of masked "
"pixels drops below this threshold.")

Definition at line 55 of file dynamicDetection.py.

◆ brightMultiplier

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.brightMultiplier
static
Initial value:
= Field(dtype=float, default=2000.0,
doc="Multiplier to apply to the prelimThresholdFactor for the "
"\"bright\" detections stage (want this to be large to only "
"detect the brightest sources).")

Definition at line 42 of file dynamicDetection.py.

◆ brightNegFactor

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.brightNegFactor
static
Initial value:
= Field(dtype=float, default=2.2,
doc="Factor by which to multiply the threshold for the negative polatiry "
"detections for the \"bright\" detections stage (this needs to be fairly "
"low given the nature of the negative polarity detections in the very "
"large positive polarity threshold).")

Definition at line 46 of file dynamicDetection.py.

◆ doBackgroundTweak

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.doBackgroundTweak
static
Initial value:
= Field(dtype=bool, default=True,
doc="Tweak background level so median PSF flux of sky objects is zero?")

Definition at line 32 of file dynamicDetection.py.

◆ doBrightPrelimDetection

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.doBrightPrelimDetection
static
Initial value:
= Field(dtype=bool, default=True,
doc="Do initial bright detection pass where footprints are grown "
"by brightGrowFactor?")

Definition at line 39 of file dynamicDetection.py.

◆ minFractionSources

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.minFractionSources
static
Initial value:
= Field(dtype=float, default=0.02,
doc="Minimum fraction of the requested number of sky sources for dynamic "
"detection to be considered a success. If the number of good sky sources "
"identified falls below this threshold, a NoWorkFound error is raised so "
"that this dataId is no longer considered in downstream processing.")

Definition at line 34 of file dynamicDetection.py.

◆ prelimNegMultiplier

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.prelimNegMultiplier
static
Initial value:
= Field(dtype=float, default=2.5,
doc="Multiplier for the negative (relative to positive) polarity "
"detections threshold to use for first pass (to find sky objects).")

Definition at line 28 of file dynamicDetection.py.

◆ prelimThresholdFactor

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.prelimThresholdFactor
static
Initial value:
= Field(dtype=float, default=0.5,
doc="Factor by which to multiply the main detection threshold "
"(thresholdValue) to use for first pass (to find sky objects).")

Definition at line 25 of file dynamicDetection.py.

◆ skyObjects

lsst.meas.algorithms.dynamicDetection.DynamicDetectionConfig.skyObjects = ConfigurableField(target=SkyObjectsTask, doc="Generate sky objects.")
static

Definition at line 31 of file dynamicDetection.py.


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