lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig Class Reference

Inheritance diagram for lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig:

Public Member Functions
def	setDefaults

Static Public Attributes
tuple	nCrPixelMax
tuple	minSigma
tuple	min_DN
tuple	cond3_fac
tuple	cond3_fac2
tuple	niteration
tuple	keepCRs
tuple	background

Detailed Description

Config for the findCosmicRays function

Definition at line 26 of file findCosmicRaysConfig.py.

Member Function Documentation

def lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.setDefaults

(

self

)

Definition at line 69 of file findCosmicRaysConfig.py.

    def setDefaults(self):
        self.background.useApprox = False
        self.background.binSize = 100000
        self.background.statisticsProperty = "MEDIAN"
        self.background.undersampleStyle = "REDUCE_INTERP_ORDER"
        self.background.algorithm = "AKIMA_SPLINE"

Member Data Documentation

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.background

static

Initial value:

= pexConfig.ConfigField(
        dtype = detection.estimateBackground.ConfigClass,
        doc = "Background estimation configuration"
        )

Definition at line 64 of file findCosmicRaysConfig.py.

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.cond3_fac

static

Initial value:

= pexConfig.Field(
        dtype = float,
        doc = "used in condition 3 for CR; see CR.cc code",
        default = 2.5,
    )

Definition at line 44 of file findCosmicRaysConfig.py.

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.cond3_fac2

static

Initial value:

= pexConfig.Field(
        dtype = float,
        doc = "used in condition 3 for CR; see CR.cc code",
        default = 0.6,
    )

Definition at line 49 of file findCosmicRaysConfig.py.

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.keepCRs

static

Initial value:

= pexConfig.Field(
        dtype = bool,
        doc = "Don't interpolate over CR pixels",
        default = False,
    )

Definition at line 59 of file findCosmicRaysConfig.py.

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.min_DN

static

Initial value:

= pexConfig.Field(
        dtype = float,
        doc = "CRs must have > this many DN (== electrons/gain) in initial detection",
        default = 150.0,
    )

Definition at line 39 of file findCosmicRaysConfig.py.

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.minSigma

static

Initial value:

= pexConfig.Field(
        dtype = float,
        doc = "CRs must be > this many sky-sig above sky",
        default = 6.0,
    )

Definition at line 34 of file findCosmicRaysConfig.py.

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.nCrPixelMax

static

Initial value:

= pexConfig.Field(
        dtype = int,
        doc = "maximum number of contaminated pixels",
        default = 10000,
    )

Definition at line 29 of file findCosmicRaysConfig.py.

tuple lsst.meas.algorithms.findCosmicRaysConfig.FindCosmicRaysConfig.niteration

static

Initial value:

= pexConfig.Field(
        dtype = int,
        doc = "number of times to look for contaminated pixels near known CR pixels",
        default = 3,
    )

Definition at line 54 of file findCosmicRaysConfig.py.

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

• /home/lsstsw/stack/Linux64/meas_algorithms/11.0-2-gb8b8ce7/python/lsst/meas/algorithms/findCosmicRaysConfig.py