Real-Time RFI Mitigation for the Apertif Radio Transient System

A. Sclocco, D. Vohl, R. V. Nieuwpoort
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引用次数: 6

Abstract

Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new and mysterious radio sources of astrophysical origin. While this increased sensitivity improves the likelihood of discoveries, it also makes these instruments more susceptible to the deleterious effects of Radio Frequency Interference (RFI). The challenge posed by RFI is exacerbated by the high data-rates achieved by modern radio telescopes, which require real-time processing to keep up with the data. Furthermore, the high data-rates do not allow for permanent storage of observations at high resolution. Offline RFI mitigation is therefore not possible anymore. The real-time requirement makes RFI mitigation even more challenging because, on one side, the techniques used for mitigation need to be fast and simple, and on the other side they also need to be robust enough to cope with just a partial view of the data.The Apertif Radio Transient System (ARTS) is the real-time, time-domain, transient detection instrument of the Westerbork Synthesis Radio Telescope (WSRT), and it is a perfect example of this challenging scenario. This system processes 73 Gb of data per second, in real-time, searching for faint pulsars and Fast Radio Bursts. Despite the radio quiet zone around WSRT, the generation of RFI is becoming increasingly part of anthropic activities, especially in a densely populated environment like the Netherlands where the telescope is located. Furthermore, our sky is populated by a growing number of satellites for world-wide telecommunication. Hence, the ARTS pipeline requires state-of-the-art real-time RFI mitigation, even if it contains a deep learning classifier to reduce the number of false-positive detections.Our solution to this challenge is RFIm, a high-performance, open-source, tuned, and extensible RFI mitigation library. The goal of this library is to provide users with RFI mitigation routines that are designed to run in real-time on many-core accelerators, such as Graphics Processing Units, and that can be highly-tuned to achieve code and performance portability to different hardware platforms and scientific use-cases. Results on ARTS show that we can achieve real-time RFI mitigation, with a minimal impact on the total execution time of the search pipeline, and considerably reduce the number of false-positives.
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Apertif无线电瞬变系统的实时RFI缓解
目前和即将到来的射电望远镜正在被设计得越来越灵敏,以探测天体物理起源的新的和神秘的射电源。虽然这种灵敏度的提高提高了发现的可能性,但也使这些仪器更容易受到无线电频率干扰(RFI)的有害影响。现代射电望远镜实现了高数据速率,需要实时处理以跟上数据,这加剧了RFI带来的挑战。此外,高数据速率不允许以高分辨率永久存储观测数据。因此,离线RFI缓解不再可能。实时需求使RFI缓解更具挑战性,因为一方面,用于缓解的技术需要快速和简单,另一方面,它们还需要足够健壮,以处理数据的部分视图。Apertif射电瞬变系统(ARTS)是韦斯特伯克综合射电望远镜(WSRT)的实时、时域、瞬变探测仪器,它是这种具有挑战性的场景的完美例子。这个系统每秒实时处理73 Gb的数据,搜索微弱的脉冲星和快速射电暴。尽管WSRT周围有无线电安静区,但RFI的产生正日益成为人类活动的一部分,特别是在像望远镜所在的荷兰这样人口稠密的环境中。此外,我们的天空布满了越来越多的卫星,用于世界范围的通信。因此,ARTS管道需要最先进的实时RFI缓解,即使它包含深度学习分类器以减少假阳性检测的数量。我们针对这一挑战的解决方案是RFIm,它是一个高性能、开源、可调优和可扩展的RFI缓解库。此库的目标是为用户提供RFI缓解例程,这些例程旨在在多核加速器(如图形处理单元)上实时运行,并且可以高度调整以实现不同硬件平台和科学用例的代码和性能可移植性。在ARTS上的结果表明,我们可以实现实时RFI缓解,对搜索管道的总执行时间的影响最小,并大大减少误报的数量。
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