# Frames
Here the user can specify the number of distinct frames
(exposures) comprising their observation.
This is analogous to the "CR-SPLIT" parameter that was
popular in the early days of HST, but today has been supplanted by
distinct exposures taken in tandem with dithering, allowing not only
the rejection of cosmic rays but also the masking of detector
artifacts and a resampling of the point spread function.
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