| Applications of Novel Scintillators for Research and Industry 2016 | |
| The XGS instrument on-board THESEUS | |
| 物理学;工业技术 | |
| Fuschino, F.^1,2,3 ; Campana, R.^2,3 ; Labanti, C.^2,3 ; Marisaldi, M.^2,3 ; Amati, L.^2 ; Fiorini, M.^4 ; Uslenghi, M.^4 ; Baldazzi, G.^1,3 ; Evangelista, Y.^5 ; Elmi, I.^6 ; Feroci, M.^5 ; Frontera, F.^2,7 ; Rachevski, A.^8 ; Rignanese, L.P.^1,3 ; Vacchi, A.^8,9 ; Zampa, G.^8 ; Zampa, N.^8 ; Rashevskaya, I.^10 ; Bellutti, P.^11 ; Piemonte, C.^11 | |
| Department of Physics, University of Bologna, Viale Berti Pichat 6/2, Bologna | |
| I-40127, Italy^1 | |
| INAF/IASF-Bologna, Via Gobetti 101, Bologna | |
| I-40129, Italy^2 | |
| INFN - Sezione di Bologna, Viale Berti Pichat 6/2, Bologna | |
| I-40127, Italy^3 | |
| INAF/IASF-Milano, Via Bassini 23, Milano | |
| I-20133, Italy^4 | |
| INAF/IAPS, Via Fosso del Cavaliere 100, Roma | |
| I-00133, Italy^5 | |
| CNR/IMM, Via Gobetti 101, Bologna | |
| I-40129, Italy^6 | |
| Department of Physics, University of Ferrara, Via Giuseppe Saragat 1, Ferrara | |
| I-44122, Italy^7 | |
| INFN - Sezione di Trieste, Padriciano 99, Trieste | |
| I-34127, Italy^8 | |
| Mathematics and Informatics Dept., Udine University, Via delle Scienze 206, Udine | |
| I- 33100, Italy | |
| (10) TIFPA Dept., Via Sommarive 14, Povo TN | |
| 38123, Italy | |
| (11) CMM Dept., Burno Kessler Foundation (FBK), Via Sommarive 18, Povo | |
| I-38123, Italy^9 | |
| 关键词: Background rejection; Gamma spectroscopy; Readout Electronics; Silicon Drift Detector; Silicon photo-detector; Space instrumentations; Spatial segmentation; System complexity; | |
| Others : https://iopscience.iop.org/article/10.1088/1742-6596/763/1/012009/pdf DOI : 10.1088/1742-6596/763/1/012009 |
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| 学科分类:工业工程学 | |
| 来源: IOP | |
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【 摘 要 】
Consolidated 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.
【 预 览 】
| Files | Size | Format | View |
|---|---|---|---|
| The XGS instrument on-board THESEUS | 1178KB |
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