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arXiv · astro-ph/0110129

The MEGA Advanced Compton Telescope Project

P. F. Bloser·R. Andritschke·G. Kanbach·V. Schoenfelder·F. Schopper·A. Zoglauer
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Abstract

The goal of the Medium Energy Gamma-ray Astronomy (MEGA) telescope is to improve sensitivity at medium gamma-ray energies (0.4-50 MeV) by at least an order of magnitude over that of COMPTEL. This will be achieved with a new compact design that allows for a very wide field of view, permitting a sensitive all-sky survey and the monitoring of transient and variable sources. The key science objectives for MEGA include the investigation of cosmic high-energy particle accelerators, studies of nucleosynthesis sites using gamma-ray lines, and determination of the large-scale structure of galactic and cosmic diffuse background emission. MEGA records and images gamma-ray events by completely tracking both Compton and pair creation interactions in a tracker of double-sided silicon strip detectors and a calorimeter of CsI crystals able to resolve in three dimensions. We present initial laboratory calibration results from a small prototype MEGA telescope.

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P. F. Bloser, R. Andritschke, G. Kanbach, V. Schoenfelder, F. Schopper, A. Zoglauer. 2001-10-05. The MEGA Advanced Compton Telescope Project. https://doi.org/10.1016/s1387-6473(02)00209-9

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