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Charge-coupled devices

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Abstract

At the heart of all astronomical instruments is some form of detector to convert electromagnetic energy into an electrical signal. Having indicated that the dominant detector in modern astronomy is the charge-coupled device (CCD), it is important to consider these remarkable detectors in more detail. We begin with a brief historical review of CCDs from invention to present day, an amazing story by itself, and then cover the basic principles of how CCDs work. Practical details will follow in the next chapter.

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References and Suggestions for Further Reading

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Web sites

  • Bonn shutters: http://www.astro.uni-bonn.de/~ccd/shutters/

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  • For low light level CCDs: http://www.e2v.com/products/ccd-and-cmos-imaging-and-semiconductors/imaging-scientific-sensors.cfm

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  • For orthogonal transfer CCDs: http://pan-starrs.ifa.hawaii.edu/public/ and http://www.noao.edu/wiyn/ODI/index.htm

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© 2008 Praxis Publishing Ltd, Chichester, UK

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(2008). Charge-coupled devices. In: Electronic Imaging in Astronomy. Springer Praxis Books. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-76583-7_7

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