Paper
11 March 2003 Concept study for the next generation medium-energy gamma-ray astronomy mission: MEGA
Gottfried Kanbach, Robert Andritschke, Peter Forbes Bloser, Florian Schopper, Volker Schoenfelder, Andreas Zoglauer
Author Affiliations +
Abstract
A new telescope for Medium Energy Gamma-Ray Astronomy, MEGA, is being developed for the energy band 0.4 - 50 MeV as a successor to COMPTEL on CGRO. MEGA aims to improve the sensitivity for astronomical sources by at least an order of magnitude with respect to past instruments and will fill a severe sensitivity gap between already scheduled hard-X-ray and high-energy gamma-ray missions. MEGA records and images gamma rays by completely tracking Compton and pair creation events in a stack of double sided Si-strip track detectors surrounded by a pixelated CsI calorimeter. MEGA will have an effective area of ~100 square cm, a large field of view of ~130 degrees, angular resolution of ~2 degrees, and energy resolution of ~8% (all FWHM at ~2 MeV). Key science objectives for MEGA are the investigation of cosmic high-energy accelerators, nucleosynthesis sites with gamma-ray lines, and the mapping of large-scale structures in the Galaxy and beyond. If operated on a zenith pointing satellite MEGA will be an ideal continuous all-sky monitor for transient sources. This paper describes the development of a small scale prototype and the concept of a space mission for MEGA.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gottfried Kanbach, Robert Andritschke, Peter Forbes Bloser, Florian Schopper, Volker Schoenfelder, and Andreas Zoglauer "Concept study for the next generation medium-energy gamma-ray astronomy mission: MEGA", Proc. SPIE 4851, X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy, (11 March 2003); https://doi.org/10.1117/12.461348
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Cited by 24 scholarly publications.
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KEYWORDS
Sensors

Telescopes

Space telescopes

Prototyping

Satellites

Silicon

Electronics

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