LSST Applications  21.0.0+04719a4bac,21.0.0-1-ga51b5d4+f5e6047307,21.0.0-11-g2b59f77+a9c1acf22d,21.0.0-11-ga42c5b2+86977b0b17,21.0.0-12-gf4ce030+76814010d2,21.0.0-13-g1721dae+760e7a6536,21.0.0-13-g3a573fe+768d78a30a,21.0.0-15-g5a7caf0+f21cbc5713,21.0.0-16-g0fb55c1+b60e2d390c,21.0.0-19-g4cded4ca+71a93a33c0,21.0.0-2-g103fe59+bb20972958,21.0.0-2-g45278ab+04719a4bac,21.0.0-2-g5242d73+3ad5d60fb1,21.0.0-2-g7f82c8f+8babb168e8,21.0.0-2-g8f08a60+06509c8b61,21.0.0-2-g8faa9b5+616205b9df,21.0.0-2-ga326454+8babb168e8,21.0.0-2-gde069b7+5e4aea9c2f,21.0.0-2-gecfae73+1d3a86e577,21.0.0-2-gfc62afb+3ad5d60fb1,21.0.0-25-g1d57be3cd+e73869a214,21.0.0-3-g357aad2+ed88757d29,21.0.0-3-g4a4ce7f+3ad5d60fb1,21.0.0-3-g4be5c26+3ad5d60fb1,21.0.0-3-g65f322c+e0b24896a3,21.0.0-3-g7d9da8d+616205b9df,21.0.0-3-ge02ed75+a9c1acf22d,21.0.0-4-g591bb35+a9c1acf22d,21.0.0-4-g65b4814+b60e2d390c,21.0.0-4-gccdca77+0de219a2bc,21.0.0-4-ge8a399c+6c55c39e83,21.0.0-5-gd00fb1e+05fce91b99,21.0.0-6-gc675373+3ad5d60fb1,21.0.0-64-g1122c245+4fb2b8f86e,21.0.0-7-g04766d7+cd19d05db2,21.0.0-7-gdf92d54+04719a4bac,21.0.0-8-g5674e7b+d1bd76f71f,master-gac4afde19b+a9c1acf22d,w.2021.13
LSST Data Management Base Package
Static Public Attributes | List of all members
lsst.ip.isr.overscan.OverscanCorrectionTaskConfig Class Reference
Inheritance diagram for lsst.ip.isr.overscan.OverscanCorrectionTaskConfig:

Static Public Attributes

 fitType
 
 order
 
 numSigmaClip
 
 maskPlanes
 
 overscanIsInt
 

Detailed Description

Overscan correction options.

Definition at line 31 of file overscan.py.

Member Data Documentation

◆ fitType

lsst.ip.isr.overscan.OverscanCorrectionTaskConfig.fitType
static
Initial value:
= pexConfig.ChoiceField(
dtype=str,
doc="The method for fitting the overscan bias level.",
default='MEDIAN',
allowed={
"POLY": "Fit ordinary polynomial to the longest axis of the overscan region",
"CHEB": "Fit Chebyshev polynomial to the longest axis of the overscan region",
"LEG": "Fit Legendre polynomial to the longest axis of the overscan region",
"NATURAL_SPLINE": "Fit natural spline to the longest axis of the overscan region",
"CUBIC_SPLINE": "Fit cubic spline to the longest axis of the overscan region",
"AKIMA_SPLINE": "Fit Akima spline to the longest axis of the overscan region",
"MEAN": "Correct using the mean of the overscan region",
"MEANCLIP": "Correct using a clipped mean of the overscan region",
"MEDIAN": "Correct using the median of the overscan region",
"MEDIAN_PER_ROW": "Correct using the median per row of the overscan region",
},
)

Definition at line 34 of file overscan.py.

◆ maskPlanes

lsst.ip.isr.overscan.OverscanCorrectionTaskConfig.maskPlanes
static
Initial value:
= pexConfig.ListField(
dtype=str,
doc="Mask planes to reject when measuring overscan",
default=['SAT'],
)

Definition at line 62 of file overscan.py.

◆ numSigmaClip

lsst.ip.isr.overscan.OverscanCorrectionTaskConfig.numSigmaClip
static
Initial value:
= pexConfig.Field(
dtype=float,
doc="Rejection threshold (sigma) for collapsing overscan before fit",
default=3.0,
)

Definition at line 57 of file overscan.py.

◆ order

lsst.ip.isr.overscan.OverscanCorrectionTaskConfig.order
static
Initial value:
= pexConfig.Field(
dtype=int,
doc=("Order of polynomial to fit if overscan fit type is a polynomial, "
"or number of spline knots if overscan fit type is a spline."),
default=1,
)

Definition at line 51 of file overscan.py.

◆ overscanIsInt

lsst.ip.isr.overscan.OverscanCorrectionTaskConfig.overscanIsInt
static
Initial value:
= pexConfig.Field(
dtype=bool,
doc="Treat overscan as an integer image for purposes of fitType=MEDIAN"
" and fitType=MEDIAN_PER_ROW.",
default=True,
)

Definition at line 67 of file overscan.py.


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