The ground calibration of the HERMES-Pathfinder payload flight models

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Experimental Astronomy Pub Date : 2024-10-26 DOI:10.1007/s10686-024-09958-4
G. Dilillo, E. J. Marchesini, G. Baroni, G. Della Casa, R. Campana, Y. Evangelista, A. Guzmán, P. Hedderman, P. Bellutti, G. Bertuccio, F. Ceraudo, M. Citossi, D. Cirrincione, I. Dedolli, E. Demenev, M. Feroci, F. Ficorella, M. Fiorini, M. Gandola, M. Grassi, G. La Rosa, G. Lombardi, P. Malcovati, F. Mele, P. Nogara, A. Nuti, M. Perri, S. Pliego-Caballero, S. Pirrotta, S. Puccetti, I. Rashevskaya, F. Russo, G. Sottile, C. Tenzer, M. Trenti, S. Trevisan, A. Vacchi, G. Zampa, N. Zampa, F. Fiore
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Abstract

HERMES-Pathfinder is a space-borne mission based on a constellation of six nano-satellites flying in a low-Earth orbit. The 3U CubeSats, to be launched in early 2025, host miniaturized instruments with a hybrid Silicon Drift Detector/scintillator photodetector system, sensitive to both X-rays and gamma-rays. A seventh payload unit is installed onboard SpIRIT, an Australian-Italian nano-satellite developed by a consortium led by the University of Melbourne and launched in December 2023. The project aims at demonstrating the feasibility of Gamma-Ray Burst detection and localization using miniaturized instruments onboard nano-satellites. The HERMES flight model payloads were exposed to multiple well-known radioactive sources for spectroscopic calibration under controlled laboratory conditions. The analysis of the calibration data allows both to determine the detector parameters, necessary to map instrumental units to accurate energy measurements, and to assess the performance of the instruments. We report on these efforts and quantify features such as spectroscopic resolution and energy thresholds, at different temperatures and for all payloads of the constellation. Finally we review the performance of the HERMES payload as a photon counter, and discuss the strengths and the limitations of the architecture.

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HERMES 探路者有效载荷飞行模型的地面校准
HERMES-Pathfinder 是一项空间飞行任务,由六颗在低地球轨道上飞行的超小型卫星组成。这些将于 2025 年初发射的 3U 立方体卫星载有小型化仪器,配备了混合硅漂移探测器/闪烁体光电探测器系统,对 X 射线和伽马射线都很敏感。第七个有效载荷单元安装在 SpIRIT 上,这是一颗澳大利亚和意大利联合研制的超小型卫星,由墨尔本大学牵头,将于 2023 年 12 月发射。该项目旨在证明利用纳卫星上的微型仪器进行伽马射线暴探测和定位的可行性。在受控实验室条件下,HERMES 飞行模型有效载荷暴露于多个知名放射源,以进行光谱校准。通过对校准数据的分析,既可以确定探测器参数(这是将仪器单位映射到精确能量测量所必需的),也可以评估仪器的性能。我们报告了这些工作,并量化了不同温度下和星座所有有效载荷的光谱分辨率和能量阈值等特征。最后,我们回顾了作为光子计数器的 HERMES 有效载荷的性能,并讨论了该结构的优势和局限性。
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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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