Bases: drizzlepac.imageObject.imageObject
Bases: drizzlepac.wfc3Data.WFC3InputImage
Return the dark current for the WFC3 UVIS detector. This value will be contained within an instrument specific keyword.
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darkcurrent: float :
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This method overrides the superclass to set default values into the parameter dictionary, in case empty entries are provided.
Bases: drizzlepac.wfc3Data.WFC3InputImage
WF3 IR data come out in electrons, and I imagine the photometry keywords will be calculated as such, so no image manipulation needs be done between native and electrons
Return the dark current for the WFC3/IR detector. This value will be contained within an instrument specific keyword.
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darkcurrent: float :
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Return an array representing the dark image for the detector.
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dark: array :
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Return an array representing the exposure time per pixel for the detector.
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dark: array :
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This method overrides the superclass to set default values into the parameter dictionary, in case empty entries are provided.