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
{"title":"Digital electronics for the eXTP large area detector","authors":"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","doi":"10.1007/s10686-025-10017-9","DOIUrl":null,"url":null,"abstract":"<div><p>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.</p></div>","PeriodicalId":551,"journal":{"name":"Experimental Astronomy","volume":"60 1","pages":""},"PeriodicalIF":2.2000,"publicationDate":"2025-07-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s10686-025-10017-9.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Experimental Astronomy","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10686-025-10017-9","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
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.
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.