Simulated Performance of a Germanium Compton Telescope

Steven E. Boggs; Pierre Jean

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arXiv · astro-ph/0010331

Simulated Performance of a Germanium Compton Telescope

Steven E. Boggs·Pierre Jean

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Abstract

To build upon the goals of the upcoming INTEGRAL mission, the next generation soft gamma-ray (0.2-20 MeV) observatory will require improved sensitivity to nuclear line emission while maintaining high spectral resolution. We present the simulated performance of a germanium Compton telescope (GCT) design, which will allow a factor of ten improvement in sensitivity over INTEGRAL/SPI. We also discuss a number of issues concerning reconstruction techniques and event cuts, and demonstrate how these affect the overall performance of the telescope.

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Steven E. Boggs, Pierre Jean. 2000-10-17. Simulated Performance of a Germanium Compton Telescope. https://arxiv.org/abs/astro-ph/0010331

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