Accelerating Dedispersion Using Many-core Architectures

IF 8.6 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astrophysical Journal Supplement Series Pub Date : 2023-11-01 DOI:10.3847/1538-4365/acfef6
Jan Novotný, Karel Adámek, M. A. Clark, Mike Giles, Wes Armour
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Abstract

Abstract Astrophysical radio signals are excellent probes of extreme physical processes that emit them. However, to reach Earth, electromagnetic radiation passes through the ionized interstellar medium, introducing a frequency-dependent time delay (dispersion) to the emitted signal. Removing dispersion enables searches for transient signals like fast radio bursts or repeating signals from isolated pulsars or those in orbit around other compact objects. The sheer volume and high resolution of data that next-generation radio telescopes will produce require high-performance computing solutions and algorithms to be used in time-domain data-processing pipelines to extract scientifically valuable results in real time. This paper presents a state-of-the-art implementation of brute force incoherent dedispersion on NVIDIA graphics-processing units and on Intel and AMD central-processing units. We show that our implementation is 4× faster (8-bit 8192 channels input) than other available solutions, and we demonstrate, using 11 existing telescopes, that our implementation is at least 20× faster than real time. This work is part of the AstroAccelerate package.
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使用多核架构加速去分散
天体物理无线电信号是探测发射它们的极端物理过程的绝佳工具。然而,为了到达地球,电磁辐射要经过电离的星际介质,对发射的信号引入频率相关的时间延迟(色散)。消除色散可以搜索瞬态信号,如快速射电暴或来自孤立脉冲星或其他紧凑物体轨道上的重复信号。下一代射电望远镜将产生庞大的数据量和高分辨率,需要高性能的计算解决方案和算法,用于时域数据处理管道,以实时提取有科学价值的结果。本文介绍了在NVIDIA图形处理单元和Intel和AMD中央处理单元上最先进的蛮力非相干去散的实现。我们证明了我们的实现比其他可用的解决方案快4倍(8位8192通道输入),并且我们使用11个现有的望远镜证明,我们的实现至少比实时快20倍。这项工作是AstroAccelerate软件包的一部分。
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来源期刊
Astrophysical Journal Supplement Series
Astrophysical Journal Supplement Series 地学天文-天文与天体物理
CiteScore
14.50
自引率
5.70%
发文量
264
审稿时长
2 months
期刊介绍: The Astrophysical Journal Supplement (ApJS) serves as an open-access journal that publishes significant articles featuring extensive data or calculations in the field of astrophysics. It also facilitates Special Issues, presenting thematically related papers simultaneously in a single volume.
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