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IntroductionThe Advanced Compton Telescope (ACT) is planned as the next generation space-based instrument devoted to observations of "low/medium"-energy gamma rays (~0.2--30 MeV). It follows upon the successful Compton Observatory COMPTEL, OSSE, and BATSE instruments, which discovered numerous interesting sources such as supernovae, black holes, pulsars, active galactic nuclei, and gamma-ray bursts. Further progress requires an instrument with significantly enhanced sensitivity, angular resolution, and energy resolution. The Advanced Compton Telescope will acheive the required performance through the use of new detector technologies and enhanced telescope design. Several institutions are currently developing fundamental detector technologies and investigating different telescope design approaches. Due to the complexities of Compton telescope design and the complex background in this energy regime, detailed computer simulations are a key element in the development process. Simulations of one possible design are shown at right, where 511 keV gamma rays are transported through an assembly of solid state detector modules. This site was established as part of an effort to achieve consistency in the simulations performed by the different research groups. It serves as a source of collaborative ACT simulation information. In the future, simulation software tools, references, and results will be distributed through the site. |
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Los Alamos National Laboratory
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CERN GEANT3
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