作者: R.M. Kippen , W.S. Paciesas , G.N. Pendleton , D.A. Swartz
DOI: 10.1109/NSSMIC.1998.775238
关键词: Instrumentation (computer programming) 、 Gamma-ray astronomy 、 Compton telescope 、 Sky 、 Angular resolution 、 Physics 、 Astrophysics 、 Astronomy 、 COSMIC cancer database 、 High-energy astronomy 、 Compton scattering
摘要: The highly transient nature of cosmic low-energy gamma-ray sources offers unique insight into the astrophysics extreme processes. Sensitive, long-term, all-sky monitoring is required to make sense variable emission. Instrumentation for such observations must have combination large effective collection area, wide field-of-view and good angular resolution. Recent advances in position-sensitive detectors associated electronics it possible consider a multi-scatter Compton telescope, combined with coded mask, as an monitor energy range /spl sim/10 keV few MeV. We present simulations various configurations instrument show that can provide substantial improvement over other sky strategies this regime.