Abstract
Modern CCDs are fairly predictable in their operation and characteristics, but there are still many subtleties to successful operation, especially for devices customized for astronomy. Issues include maximizing the ratio of signal to noise, obtaining stability and repeatability in performance, and finding suitable methods of control. These topics are treated by recounting some of the developments which uncovered problems and led to today’s solutions. There is no intention here to provide a “constructor’s manual”, only to alert the potential user to a host of practical issues. Many of the same practical issues apply for other detectors and other wavelength regimes.
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References and Suggested Further Reading
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(2008). Practical operation of CCDs. In: Electronic Imaging in Astronomy. Springer Praxis Books. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-76583-7_8
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DOI: https://doi.org/10.1007/978-3-540-76583-7_8
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