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High Time Resolution Astrophysics pp 291–310Cite as

Geiger-mode Avalanche Photodiodes for High Time Resolution Astrophysics

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 351))

Abstract

Geiger-mode Avalanche Photodiodes (GM-APDs) are establishing themselves as potential candidates for the broad temporal range covered in high time resolution astrophysics (HTRA). These detectors have already been employed in astronomical instrumentation and significant results have been obtained to date. Their high time resolution and quantum efficiency make these single photon event counting detectors ideal for observations of stochastic phenomena, and ultimately for extreme HTRA observations. In this chapter, we review the technology and to illustrate their potential we briefly touch on specific science goals and astronomical applications. We then focus on the fabrication and characterisation of GM-APDs, and discuss the development and challenges posed in designing array devices.

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Author information

Authors and Affiliations

  1. Dept. of Experimental Physics, National University of Ireland, Galway, Ireland

    Don Phelan

  2. Dept. of Electrical and Electronic Engineering, University College Cork, Ireland

    Alan P. Morrison

Authors
  1. Don Phelan
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  2. Alan P. Morrison
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Editor information

Editors and Affiliations

  1. NUI, Galway, Ireland

    Don Phelan

  2. NUI, Galway, Ireland

    Oliver Ryan

  3. NUI, Galway, Ireland

    Andrew Shearer

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Phelan, D., Morrison, A.P. (2008). Geiger-mode Avalanche Photodiodes for High Time Resolution Astrophysics. In: Phelan, D., Ryan, O., Shearer, A. (eds) High Time Resolution Astrophysics. Astrophysics and Space Science Library, vol 351. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-6518-7_15

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