Bases: drizzlepac.imageObject.imageObject
Convert the data to electrons
This converts all science data extensions and saves the results back to disk. We need to make sure the data inside the chips already in memory is altered as well.
Return the dark current for the NICMOS detectors.
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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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Method for retrieving a detector’s flat field.
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flat : array
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isCountRate: Method or IRInputObject used to indicate if the science data is in units of counts or count rate. This method assumes that the keyword ‘BUNIT’ is in the header of the input FITS file.
Bases: drizzlepac.nicmosData.NICMOSInputImage
This method overrides the superclass to set default values into the parameter dictionary, in case empty entries are provided.
Bases: drizzlepac.nicmosData.NICMOSInputImage
Add in a mask for the coronographic hole to the general static pixel mask.
This method overrides the superclass to set default values into the parameter dictionary, in case empty entries are provided.
Bases: drizzlepac.nicmosData.NICMOSInputImage
This method overrides the superclass to set default values into the parameter dictionary, in case empty entries are provided.