A Skipper CCD's readout time is minimized at a specific integration-time/sample-count combination that can be predicted from the measured noise spectrum and is set by the charge-transfer time per sample.
Design and development of the 3.2 gigapixel camera for the Large Synoptic Survey Telescope,
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Skipper CCD readout time optimization for astronomical applications
A Skipper CCD's readout time is minimized at a specific integration-time/sample-count combination that can be predicted from the measured noise spectrum and is set by the charge-transfer time per sample.