Preprint
Oct 2026
Optimal Photon Counting with Fast, Low Noise Astronomical Imagers
Measuring rapid astrophysical phenomena requires many short exposures, which suffer from repeated read noise. A variety of recent technologies are achieving sub-electron read noise, which enable rapid time-domain studies of faint sources. These data can be analyzed with traditional methods, but the ability to resolve i...
Jack T. Dinsmore, Christopher Layden, R. Romani et al.
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