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Hard X-ray and gamma-ray detectors

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Observing Photons in Space

Part of the book series: ISSI Scientific Report Series ((ISSI,volume 9))

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Abstract

The detection of photons above 10 keV up to gigaelectronvolt energies is challenging due to the penetrating nature of the radiation, which can require large detector volumes, resulting in correspondingly high background. In this energy range, most detectors in space are either scintillators or solid-state detectors. The choice of detector technology depends on the energy range of interest, expected levels of signal and background, required energy and spatial resolution, particle environment on orbit, and other factors. This section covers the materials and configurations commonly used from 10 keV to > 1 GeV.

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Acknowledgement

I would like to thank Mark McConnell for very helpful suggestions on the manuscript of this chapter.

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Smith, D.M. (2013). Hard X-ray and gamma-ray detectors. In: Huber, M.C.E., Pauluhn, A., Culhane, J.L., Timothy, J.G., Wilhelm, K., Zehnder, A. (eds) Observing Photons in Space. ISSI Scientific Report Series, vol 9. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-7804-1_21

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