GPU Accelerated Anomaly Detection of Large Scale Light Curves

Austin Chase Minor, Zhihui Du, Yankui Sun, David A. Bader, Chao Wu, Jianyan Wei
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Abstract

Identifying anomalies in millions of stars in real time is a great challenge. In this paper, we develop a matched filtering based algorithm to detect a typical anomaly, microlensing. The algorithm can detect short timescale microlensing events with high accuracy at their early stage with a very low false-positive rate. Furthermore, a GPU accelerated scalable computational framework, which can enable real time follow-up observation, is designed. This framework efficiently divides the algorithm between CPU and GPU, accelerating large scale light curve processing to meet low latency requirements. Experimental results show that the proposed method can process 200,000 stars (the maximum number of stars processed by a single GWAC telescope) in approximately 3.34 seconds with current commodity hardware while achieving an accuracy of 92% and an average detection occurring approximately 14% before the peak of the anomaly with zero false alarm. Working together with the proposed sharding mechanism, the framework is positioned to be extendable to multiple GPUs to improve the performance further for the higher data throughput requirements of next-generation telescopes.
大规模光曲线的GPU加速异常检测
实时识别数百万颗恒星的异常是一项巨大的挑战。在本文中,我们开发了一种基于匹配滤波的算法来检测典型的微透镜异常。该算法能够在短时间尺度微透镜事件早期检测出高精度的微透镜事件,假阳性率极低。在此基础上,设计了GPU加速可扩展计算框架,实现实时跟踪观测。该框架有效地将算法划分为CPU和GPU,加速大规模光曲线处理以满足低延迟要求。实验结果表明,在现有商用硬件条件下,该方法可以在约3.34秒内处理20万颗恒星(单个GWAC望远镜处理的最大恒星数量),准确率达到92%,平均检测率约为异常峰值前14%,且无误报。与提议的分片机制一起工作,该框架定位为可扩展到多个gpu,以进一步提高性能,以满足下一代望远镜更高的数据吞吐量要求。
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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