The Gamma Ray Detection Capabilities of the Alpha Magnetic Spectrometer

(2) Department of Physics; Dipartimento di Fisica; E. Fiandrini (1); J. Petrakis (2); M. Biasini (1); M. H. Salamon (2) ((1) Sezione INFN; R. Battiston (1); Universita di Perugia; University of Utah)

arxiv: astro-ph/9909432 · v2 · pith:3BXCL7SKnew · submitted 1999-09-25 · 🌌 astro-ph

The Gamma Ray Detection Capabilities of the Alpha Magnetic Spectrometer

R. Battiston (1) , M. Biasini (1) , E. Fiandrini (1) , J. Petrakis (2) , M. H. Salamon (2) ((1) Sezione INFN , Dipartimento di Fisica , Universita di Perugia , (2) Department of Physics

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University of Utah)

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keywords alphagammamagneticspectrometerastrophysicscapabilitiesdescribeddetection

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The modeled performance of the Alpha Magnetic Spectrometer (AMS) as a high energy (0.3 to 100 GeV) gamma-ray detector is described, and its gamma ray astrophysics objectives are discussed.

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The Gamma Ray Detection Capabilities of the Alpha Magnetic Spectrometer

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