Evaluation of the performance of a CdZnTe-based soft -ray detector for CubeSat payloads
arXiv:2401.09735 · doi:10.1007/s10686-024-09936-w
Abstract
The low-energy -ray (0.1-30 MeV) sky has been relatively unexplored since the decommissioning of the COMPTEL instrument on the Compton Gamma-Ray Observatory (CGRO) satellite in 2000. However, the study of this part of the energy spectrum (the ``MeV gap") is crucial for addressing numerous unresolved questions in high-energy and multi-messenger astrophysics. Although several large MeV -ray missions like AMEGO and e-ASTROGAM are being proposed, they are predominantly in the developmental phase, with launches not anticipated until the next decade at the earliest. In recent times, there has been a surge in proposed CubeSat missions as cost-effective and rapidly implementable ``pathfinder" alternatives. A MeV CubeSat dedicated to -ray astronomy has the potential to serve as a demonstrator for future, larger-scale MeV payloads. This paper presents a -ray payload design featuring a CdZnTe crystal calorimeter module developed by IDEAS. We report the detailed results of simulations to assess the performance of this proposed payload and compare it with those of previous -ray instruments.
Submitted in Experimental Astronomy(Springer), 25 pages, 7 figures
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