FUSCHINO, FABIOFABIOFUSCHINOCAMPANA, RICCARDORICCARDOCAMPANALABANTI, CLAUDIOCLAUDIOLABANTIMarisaldi, M.M.MarisaldiAMATI, LORENZOLORENZOAMATIFIORINI, MAUROMAUROFIORINIUSLENGHI, MICHELAMICHELAUSLENGHIBaldazzi, G.G.BaldazziEVANGELISTA, YURIYURIEVANGELISTAElmi, I.I.ElmiFEROCI, MARCOMARCOFEROCIFrontera, F.F.FronteraRachevski, A.A.RachevskiRignanese, L. P.L. P.RignaneseVacchi, A.A.VacchiZampa, G.G.ZampaZampa, N.N.ZampaRashevskaya, I.I.RashevskayaBellutti, P.P.BelluttiPiemonte, C.C.Piemonte2020-04-292020-04-2920161742-6588http://hdl.handle.net/20.500.12386/24303Consolidated techniques used for space-borne X-ray and gamma-ray instruments are based on the use of scintillators coupled to Silicon photo-detectors. This technology associated with modern very low noise read-out electronics allows the design of innovative architectures able to reduce drastically the system complexity and power consumption, also with a moderate-to-high number of channels. These detector architectures can be exploited in the design of space instrumentation for gamma-spectroscopy with the benefit of possible smart background rejection strategies. We describe a detector prototype with 3D imaging capabilities to be employed in future gamma-ray and particle space missions in the 0.002-100 MeV energy range. The instrument is based on a stack of scintillating bars read out by Silicon Drift Detectors (SDDs) at both ends. The spatial segmentation and the crystal double-side readout allow a 3D position reconstruction with ∼3 mm accuracy within the full active volume, using a 2D readout along the two external faces of the detector. Furthermore, one of the side of SDDs can be used simultaneously to detect X-rays in the 2-30 keV energy range. The characteristics of this instrument make it suitable in next generation gamma-ray and particle space missions for Earth or outer space observations, and it will be briefly illustrated.STAMPAenThe XGS instrument on-board THESEUSConference paper10.1088/1742-6596/763/1/0120092-s2.0-84995376532000440356900009https://iopscience.iop.org/article/10.1088/1742-6596/763/1/0120092016JPhCS.763a2009FFIS/05 - ASTRONOMIA E ASTROFISICA