Paper
18 October 1996 Crystal diffraction telescopes for nuclear astrophysics
Peter von Ballmoos, Antje Kohnle, Juan E. Naya, Jean-Francois Olive, Gilbert Vedrenne, Robert K. Smither, Mohamed Faiz, Patricia B. Fernandez, Timothy Graber
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Abstract
Until recently, focusing of gamma-radiation was regarded as an impracticable task. Today, gamma-ray lenses have become feasible and present promising perspectives for future instrumentation. For the first time in high energy astronomy the signal/noise ratio will be dramatically improved as gamma-rays are collected on the large area of a lens from where they are focused onto a small detector. Besides an unprecedented sensitivity, such instruments feature very high angular and energy resolution.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Peter von Ballmoos, Antje Kohnle, Juan E. Naya, Jean-Francois Olive, Gilbert Vedrenne, Robert K. Smither, Mohamed Faiz, Patricia B. Fernandez, and Timothy Graber "Crystal diffraction telescopes for nuclear astrophysics", Proc. SPIE 2806, Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions, (18 October 1996); https://doi.org/10.1117/12.253999
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CITATIONS
Cited by 1 scholarly publication.
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KEYWORDS
Crystals

Sensors

Space telescopes

Telescopes

Diffraction

Gamma radiation

Germanium

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