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一种用于立方星平台上伽马射线暴探测的紧凑型仪器I:设计驱动因素和预期性能

A compact instrument for gamma-ray burst detection on a CubeSat platform I: Design drivers and expected performance.

作者信息

Murphy David, Ulyanov Alexey, McBreen Sheila, Doyle Maeve, Dunwoody Rachel, Mangan Joseph, Thompson Joseph, Shortt Brian, Martin-Carrillo Antonio, Hanlon Lorraine

机构信息

School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.

School of Mechanical and Materials Engineering and Centre for Space Research, University College Dublin, Dublin 4, Ireland.

出版信息

Exp Astron (Dordr). 2021;52(1-2):59-84. doi: 10.1007/s10686-021-09779-9. Epub 2021 Aug 13.

DOI:10.1007/s10686-021-09779-9
PMID:34744308
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8556213/
Abstract

The Educational Irish Research Satellite 1 (EIRSAT-1) is a 2U CubeSat being developed under ESA's Fly Your Satellite! programme. The project has many aspects, which are primarily educational, but also include space qualification of new detector technologies for gamma-ray astronomy and the detection of gamma-ray bursts (GRBs). The Gamma-ray Module (GMOD), the main mission payload, is a small gamma-ray spectrometer comprising a 25 mm × 25 mm × 40 mm cerium bromide scintillator coupled to an array of 16 silicon photomultipliers. The readout is provided by IDE3380 (SIPHRA), a low-power and radiation tolerant readout ASIC. GMOD will detect gamma-rays and measure their energies in a range from tens of keV to a few MeV. Monte Carlo simulations were performed using the Medium Energy Gamma-ray Astronomy Library to evaluate GMOD's capability for the detection of GRBs in low Earth orbit. The simulations used a detailed mass model of the full spacecraft derived from a very high-fidelity 3D CAD model. The sky-average effective area of GMOD on board EIRSAT-1 was found to be 10 cm at 120 keV. The instrument is expected to detect between 11 and 14 GRBs, at a significance greater than 10 (and up to 32 at 5), during a nominal one-year mission. The shape of the scintillator in GMOD results in omni-directional sensitivity which allows for a nearly all-sky field of view.

摘要

爱尔兰教育研究卫星1号(EIRSAT - 1)是一颗2U立方星,正在欧洲航天局的“放飞你的卫星!”计划下研制。该项目有许多方面,主要是教育方面,但也包括用于伽马射线天文学的新探测器技术的空间鉴定以及伽马射线暴(GRB)的探测。伽马射线模块(GMOD)是主要的任务有效载荷,是一种小型伽马射线光谱仪,由一个25毫米×25毫米×40毫米的溴化铈闪烁体与16个硅光电倍增管阵列耦合而成。读出由低功耗且耐辐射的读出专用集成电路IDE3380(SIPHRA)提供。GMOD将探测伽马射线并测量其能量,范围从几十千电子伏特到几兆电子伏特。使用中能伽马射线天文学库进行了蒙特卡罗模拟,以评估GMOD在低地球轨道探测伽马射线暴的能力。模拟使用了从非常高保真的3D CAD模型导出的整个航天器的详细质量模型。发现EIRSAT - 1上GMOD的天空平均有效面积在120千电子伏特时为10平方厘米。在名义上为期一年的任务期间,该仪器预计将探测到11至14次伽马射线暴,显著性大于10(在5时可达32次)。GMOD中闪烁体的形状导致全向灵敏度,从而实现几乎全天空的视野。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/fcbde0539a31/10686_2021_9779_Fig13_HTML.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/648fd7436396/10686_2021_9779_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/ded171bf2b6b/10686_2021_9779_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/5800fefdc3d4/10686_2021_9779_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/208f9b3955c8/10686_2021_9779_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/ea87514d8c80/10686_2021_9779_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/92ea74d2929d/10686_2021_9779_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/27d7fdd5a9d8/10686_2021_9779_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/80d7/8556213/fcbde0539a31/10686_2021_9779_Fig13_HTML.jpg

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