首页> 外文期刊>Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment >HERMES: An ultra-wide band X and gamma-ray transient monitor on board a nano-satellite constellation
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HERMES: An ultra-wide band X and gamma-ray transient monitor on board a nano-satellite constellation

机译:HERMES:纳卫星星座上的超宽带X和伽马射线瞬变监测仪

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摘要

The High Energy Modular Ensemble of Satellites (HERMES) project is aimed to realize a modular X/gamma-ray monitor for transient events, to be placed on-board of a nano-satellite bus (e.g. CubeSat). This expandable platform will achieve a significant impact on Gamma Ray Burst (GRB) science and on the detection of Gravitational Wave (GW) electromagnetic counterparts: the recent LIGO/VIRGO discoveries demonstrated that the high-energy transient sky is still a field of extreme interest. The very complex temporal variability of GRBs (experimentally verified up to the millisecond scale) combined with the spatial and temporal coincidence between GWs and their electromagnetic counterparts suggest that upcoming instruments require sub-microsecond time resolution combined with a transient localization accuracy lower than a degree. The current phase of the ongoing HERMES project is focused on the realization of a technological pathfinder with a small network (3 units) of nano-satellites to be launched in mid 2020. We will show the potential and prospects for short and medium-term development of the project, demonstrating the disrupting possibilities for scientific investigations provided by the innovative concept of a new "modular astronomy" with nano-satellites (e.g. low developing costs, very short realization time). Finally, we will illustrate the characteristics of the HERMES Technological Pathfinder project, demonstrating how the scientific goals discussed are actually already reachable with the first nano-satellites of this constellation. The detector architecture will be described in detail, showing that the new generation of scintillators (e.g. GAGG:Ce) coupled with very performing Silicon Drift Detectors (SDD) and low noise FrontEnd-Electronics (FEE) are able to extend down to few keV the sensitivity band of the detector. The technical solutions for FEE, Back-End-Electronics (BEE) and Data Handling will be also described.
机译:高能卫星组合卫星(HERMES)项目旨在实现用于瞬变事件的模块化X /γ射线监测器,并将其放置在纳米卫星总线(例如CubeSat)的板上。这个可扩展的平台将对伽玛射线爆裂(GRB)科学和引力波(GW)电磁对应物的探测产生重大影响:LIGO / VIRGO的最新发现表明,高能瞬变天空仍然是人们极为关注的领域。 GRB的非常复杂的时间变异性(通过实验验证到毫秒级)与GWs及其电磁对应物之间的时空一致性相结合,表明即将推出的仪器需要亚微秒级的时间分辨率以及瞬态定位精度低于1度。正在进行的HERMES项目的当前阶段着重于实现将于2020年中期推出的带有小型(3个单位)纳米卫星网络的技术探路者。我们将展示短期和中期发展的潜力和前景该项目的成果,证明了具有纳米卫星的新型“模块化天文学”的创新概念所提供的科学研究的突破性可能性(例如,较低的开发成本,非常短的实现时间)。最后,我们将说明HERMES技术探路者项目的特征,说明该星座的第一批纳米卫星实际上已经可以实现所讨论的科学目标。将详细描述检测器架构,表明新一代闪烁体(例如GAGG:Ce)与性能非常出色的硅漂移检测器(SDD)和低噪声前端电子设备(FEE)可以扩展到几keV。探测器的灵敏度带。还介绍了FEE,后端电子(BEE)和数据处理的技术解决方案。

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  • 作者单位

    INAF, OAS Bologna, Via Gobetti 101, I-40129 Bologna, Italy|Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy;

    INAF, OAS Bologna, Via Gobetti 101, I-40129 Bologna, Italy|Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy;

    INAF, OAS Bologna, Via Gobetti 101, I-40129 Bologna, Italy|Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy;

    Ist Nazl Fis Nucl, IAPS, Via Fosso Cavaliere 100, I-00133 Rome, Italy|Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci 1, I-00133 Rome, Italy;

    Ist Nazl Fis Nucl, IAPS, Via Fosso Cavaliere 100, I-00133 Rome, Italy|Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci 1, I-00133 Rome, Italy;

    Univ Cagliari, Dept Phys, SP Monserrato Sestu Km 0,700, I-09042 Monserrato, CA, Italy;

    Ist Nazl Fis Nucl, OATs, Via GB Tiepolo 11, I-34143 Trieste, Italy;

    Ist Nazl Fis Nucl, IAPS, Via Fosso Cavaliere 100, I-00133 Rome, Italy;

    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy|Univ Bologna, Dept Phys & Astron, DIFA, Viale Berti Pichat 6-2, I-40127 Bologna, Italy;

    FBK, Via Sommarive 18, I-38123 Trento, Italy;

    Italian Space Agcy ASI, Via Politecn Snc, I-00133 Rome, Italy;

    Politecn Milan, Dept Elect Informat & Bioengn, Via Anzani 42, I-22100 Como 22100, Italy|Ist Nazl Fis Nucl, Sez Milano, Via Celoria 16, I-20133 Milan, Italy;

    FBK, Via Sommarive 18, I-38123 Trento, Italy;

    Univ Udine, Via Sci 206, I-33100 Udine, Italy|Ist Nazl Fis Nucl, Sez Trieste, Padriciano 99, I-34127 Trieste, Italy;

    Univ Udine, Via Sci 206, I-33100 Udine, Italy|INFN Udine, Via Sci 206, I-33100 Udine, Italy;

    FBK, Via Sommarive 18, I-38123 Trento, Italy;

    Ist Nazl Fis Nucl, IASF Milano, Via Bassini 15, I-20100 Milan, Italy;

    Politecn Milan, Dept Elect Informat & Bioengn, Via Anzani 42, I-22100 Como 22100, Italy|Ist Nazl Fis Nucl, Sez Milano, Via Celoria 16, I-20133 Milan, Italy;

    Univ Pavia, Dept Elect Comp & Biomed Engn, Via Ferrara 3, I-27100 Pavia, Italy|Ist Nazl Fis Nucl, Sez Pavia, Via Ferrara 3, I-27100 Pavia, Italy;

    Univ Tubingen, IAAT, Sand 1, D-72076 Tubingen, Germany;

    IASF Palermo, INAF, Via Ugo La Malfa 153, I-90146 Palermo, Italy;

    Politecn Milan, Bovisa Campus,Via La Masa 34, I-20156 Milan, Italy;

    Politecn Milan, Bovisa Campus,Via La Masa 34, I-20156 Milan, Italy;

    Univ Pavia, Dept Elect Comp & Biomed Engn, Via Ferrara 3, I-27100 Pavia, Italy|Ist Nazl Fis Nucl, Sez Pavia, Via Ferrara 3, I-27100 Pavia, Italy;

    INAF, OAS Bologna, Via Gobetti 101, I-40129 Bologna, Italy;

    Italian Space Agcy ASI, Via Politecn Snc, I-00133 Rome, Italy;

    INFN Udine, Via Sci 206, I-33100 Udine, Italy;

    Ist Nazl Fis Nucl, IAPS, Via Fosso Cavaliere 100, I-00133 Rome, Italy;

    FBK, Via Sommarive 18, I-38123 Trento, Italy;

    Italian Space Agcy ASI, Via Politecn Snc, I-00133 Rome, Italy;

    Univ Tubingen, IAAT, Sand 1, D-72076 Tubingen, Germany;

    Italian Space Agcy ASI, Via Politecn Snc, I-00133 Rome, Italy;

    Ist Nazl Fis Nucl, Sez Trieste, Padriciano 99, I-34127 Trieste, Italy;

    Ist Nazl Fis Nucl, TIFPA, Via Sornmarive 14, I-38123 Trento, Italy;

    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy|Univ Bologna, Dept Phys & Astron, DIFA, Viale Berti Pichat 6-2, I-40127 Bologna, Italy;

    Univ Tubingen, IAAT, Sand 1, D-72076 Tubingen, Germany;

    Univ Tubingen, IAAT, Sand 1, D-72076 Tubingen, Germany;

    Politecn Milan, Bovisa Campus,Via La Masa 34, I-20156 Milan, Italy;

    IASF Palermo, INAF, Via Ugo La Malfa 153, I-90146 Palermo, Italy;

    Univ Tubingen, IAAT, Sand 1, D-72076 Tubingen, Germany;

    Univ Tubingen, IAAT, Sand 1, D-72076 Tubingen, Germany;

    Ist Nazl Fis Nucl, Sez Trieste, Padriciano 99, I-34127 Trieste, Italy;

    Ist Nazl Fis Nucl, Sez Trieste, Padriciano 99, I-34127 Trieste, Italy;

    FBK, Via Sommarive 18, I-38123 Trento, Italy;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Nanosatellites; Gamma-ray burst; Silicon Drift Detectors; Scintillator detectors;

    机译:纳米卫星;伽马射线暴;硅漂移探测器;闪烁探测器;
  • 入库时间 2022-08-18 04:20:01

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