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Input and output
The input file should be an ASTERIX binned XRT dataset, e.g. time series,
spectrum or image etc... This will most likely have a data array in counts
per bin. The output file will contain the corrected data array, now in
counts per second and in some cases an entry in the instrument box
within the header giving an array of energy dependent corrections which
need to be applied to the detector matrix rather than the data array.
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