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Deep sub electron noise readout in CCD systems using digital filtering techniques

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arxiv 1107.0925 v1 pith:FLV7RNYL submitted 2011-07-05 astro-ph.IM

classification astro-ph.IM
keywords noisereadouttechniquesccdsdigitalelectronhighsignal
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Scientific CCDs designed in thick high resistivity silicon (Si) are excellent detectors for astronomy, high energy and nuclear physics, and instrumentation. Many applications can benefit from CCDs ultra low noise readout systems. The present work shows how sub electron noise CCD images can be achieved using digital signal processing techniques. These techniques allow readout bandwidths of up to 10 K pixels per second and keep the full CCD spatial resolution and signal dynamic range.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Skipper CCD readout time optimization for astronomical applications

    astro-ph.IM 2026-07 conditional novelty 6.0 of 10

    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.

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