Hao Xiong, Jörg Bayer, Andrea Santangelo, Marco Feroci, Ettore Del Monte, Alejandro Guzman, Paul Hedderman, Gabriele Minervini, Samuel Pliego, Andreas Putz, Chris Tenzer, Alessio Trois, Xianqi Wang
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引用次数: 0
摘要
大面积探测器(LAD)是增强型x射线定时和偏振测量(eXTP)任务的科学有效载荷之一。LAD是一种具有广泛能量响应的光谱定时仪器,覆盖范围从2到30 keV,定时分辨率优于10µs,预期能量分辨率为260 eV在6 keV。LAD由640个大面积多阳极硅漂移检测器(sdd)组成。考虑到大量的探测器,LAD采用模块化设计。每个模块包括16个探测器,每个探测器配备专用前端电子设备(FEE),与两个独立的模块后端电子设备(MBEEs)接口。每个MBEE设计用于处理来自8个FEE(每个FEE 224个阳极通道)的1,792个阳极通道的数据,执行x射线事件的能量重建和时间标记。MBEE使用NanoXplore™的欧洲现场可编程门阵列(FPGA),基于管道概念,减少了死区时间,使LAD适用于更高通量的x射线检测,并且它可以处理>;500 mcab的持续通量和>;15 Crab的连续通量长达300分钟(Feroci et al. 2018)。此外,MBEE还充当配置模块电子设备(包括FEEs、电源供应单元(PSU)和MBEE本身)的中心集线器,它还负责收集管理数据以监控系统状态。MBEE原型机的设计、制造和编程采用FPGA固件,使用VHDL进行。本文进行了基本功能测试,结果表明MBEE可以在不同的模式下运行,以实现上述功能。分析和测试表明,它可以以2mbps的波特率传输包含时间标签、事件类型、位置ID和能量信息的事件数据包,事件丢失率为1.5%。
Preliminary design and development of the module back-end electronics for the large area detector onboard the eXTP mission
The Large Area Detector (LAD) is one of the science payloads of the enhanced X-ray Timing and Polarimetry (eXTP) mission. The LAD is a spectral-timing instrument with a broad energy response, covering a range from 2 to 30 keV, a good timing resolution of better than 10 µs, and an expected energy resolution of 260 eV at 6 keV. The LAD consists of 640 large-area multi-anode Silicon Drift Detectors (SDDs). Given the large number of detectors, the LAD uses a modular design. Each module comprises sixteen detectors, and each detector is equipped with dedicated Front-End Electronics (FEE), interfacing with two separate Module Back-End Electronics (MBEEs). Each MBEE is designed to process the data from 1,792 anode channels in 8 FEEs (224 anode channels per FEE), performing the energy reconstruction and time tagging for X-ray events. The MBEE uses the European Field Programmable Gate Array (FPGA) from NanoXplore™, based on a pipeline concept, which reduces dead time, making the LAD suitable for higher flux X-ray detection, and it can handle a sustained flux of >500 mCrab and a continuous flux of >15 Crab for up to 300 minutes (Feroci et al. 2018). Additionally, the MBEE serves as the central hub for configuring the module’s electronics, including the FEEs, the Power Supply Unit (PSU), and the MBEE itself, and it is also responsible for collecting housekeeping data to monitor the system’s status. The prototype MBEE was designed, manufactured, and programmed with FPGA firmware using VHDL. The basic functional test was conducted in this paper, and the results indicated that the MBEE could be operated in different modes to perform the functions mentioned above. Analysis and testing show that it can transmit event packets-containing timing tag, event type, position ID, and energy information-at a baud rate of 2 Mbps with an event loss fraction of 1.5%.
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.