Digital electronics for the eXTP large area detector

IF 2.2 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Xianqi Wang, Paolo Bastia, Jörg Bayer, Federica Bonfitto, Franck Cadoux, Artur Emanuel Cardoso Coimbra, Francesco Ceraudo, Nicolas De Angelis, Giovanni Della Casa, Ettore Del Monte, Yannick Favre, Alejandro Guzman, Paul Hedderman, Malgorzata Michalska, Aline Meuris, Gabriele Minervini, Witold Nowosielski, Samuel Pliego Caballero, Andreas Putz, Andrea Santangelo, Christoph Tenzer, Alessio Trois, Francesco Villa, Hao Xiong
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引用次数: 0

Abstract

The Enhanced X-ray Timing and Polarimetry Mission (eXTP) is a flagship collaborative Sino-European X-ray mission currently in its Phase B study, led by the Institute of High Energy Physics (IHEP) of the Chinese Academy of Sciences (CAS). One of the primary instruments contributed by the European consortium to eXTP is the Large area detector (LAD), which consists of 40 modules of Silicon Drift Detector (SDD) operating in the 2–30 keV energy range. The Back-End Electronics (BEE) for the LAD are organized at two hierarchical levels: Module Back-End Electronics (MBEE) and Panel Back-End Electronics (PBEE), to manage the large number of detectors in the instrument. The Module Back-End Electronics (MBEE) acquires data from 8 Front-End Electronics (FEE) boards, which constitute half of a module and additionally preprocesses the acquired digital data. The PBEE, positioned one level higher in the hierarchy, is responsible for aggregating the data streams (science telemetry and Housekeeping (HK) data) from 20 MBEE to the Instrument Control Unit (ICU) using a single SpaceWire connection. Additionally, it distributes power, telecommands, and synchronized timing information from the ICU to the MBEE. The BEEs are designed using radiation-tolerant embedded and programmable logic systems to support data acquisition, processing, telecommand handling, and HK collection. This paper discusses the architecture of the LAD and its electronics system, with a focus on the BEE, and presents the test results and performance derived from a single-line LAD data acquisition chain setup.

用于eXTP大面积探测器的数字电子器件
增强型x射线计时和偏振测量任务(eXTP)是中欧合作的旗舰x射线任务,目前处于B阶段研究,由中国科学院高能物理研究所(IHEP)领导。欧洲财团为eXTP提供的主要仪器之一是大面积探测器(LAD),它由40个硅漂移探测器(SDD)模块组成,工作在2-30 keV的能量范围内。LAD的后端电子设备(BEE)分为两个层次:模块后端电子设备(MBEE)和面板后端电子设备(PBEE),以管理仪器中的大量探测器。模块后端电子(MBEE)从构成模块一半的8个前端电子(FEE)板采集数据,并对采集到的数字数据进行预处理。PBEE位于层次结构的更高一级,负责使用单个SpaceWire连接将20个MBEE的数据流(科学遥测和管家(HK)数据)聚合到仪器控制单元(ICU)。此外,它还将电力、远程控制和同步定时信息从ICU分发到MBEE。蜜蜂系统采用耐辐射嵌入式和可编程逻辑系统来支持数据采集、处理、远程指挥处理和HK采集。本文讨论了LAD及其电子系统的体系结构,重点介绍了BEE,并给出了单线LAD数据采集链设置的测试结果和性能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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