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SPOTLIGHT脉冲星搜索管道:一种GPU加速的FFT方法

The SPOTLIGHT Pulsar Search Pipeline: A GPU-Accelerated FFT Approach

Jyotirmoy Das, Jayanta Roy, Nishant Pradeep Deo, Karel Adámek, Wes Armour, Kshitij Bane, Jayaram Chengalur, Kenil Ajudiya, Chahat Dudeja, Sridhar Gajendran, Zhaocheng Gong, Param Joshi, Sanjay Kudale, Arpan Pal, Ujjwal Panda, Adityan S, Raghav Wani, Junhao Zhang, Deepak Bhong, Shelton Gnanaraj, Santaji N. Katore, Mekhala Muley, Harshavardhan Reddy

arXiv 2607.08854首次发表:更新:

AI 中文总结

介绍SPOTLIGHT的脉冲星搜索组件,其为uGMRT上的GPU加速通用后端。开发基于FFT的可扩展搜索管道,结合多种技术。经估计可发现约450颗新脉冲星,管道已验证,展示了通用脉冲星调查潜力,是SKA时代相关搜索先驱。

AI 中文摘要

我们展示了SPOTLIGHT(通过升级后的巨米波射电望远镜(uGMRT)上的通用多波束GPU驱动的HPC进行零星射电暴调查)的脉冲星搜索组件,这是一个在uGMRT运行的GPU加速通用后端。它主要用于快速射电暴(FRB)的实时检测和定位,同时记录用于周期性搜索的波束形成数据子集,无需专门的望远镜时间。为处理调查产生的大量数据,我们开发了基于FFT的可扩展脉冲星搜索管道,结合了射频干扰缓解、GPU加速去色散和周期性搜索、多波束候选筛选、高效折叠及机器学习分类。通过总体合成和uGMRT存档观测估计,一个完全运行的具有160个PC和一个IA波束的SPOTLIGHT调查在三年半的通用观测中可发现约450颗新脉冲星,探测高天空覆盖率和微弱脉冲星。该管道已在GMRT第48和49周期观测中得到验证,成功重新检测到许多具有不同周期、色散量和通量密度的已知脉冲星,目前用于SPOTLIGHT通用数据处理。我们描述了SPOTLIGHT观测系统、脉冲星调查设计、搜索参数空间、候选选择策略、当前状态和未来发展。SPOTLIGHT展示了通用脉冲星调查的科学潜力,是SKA时代实时、大规模脉冲星和瞬态搜索的先驱。

英文摘要

We present the pulsar search component of SPOTLIGHT (Survey for sPoradic radiO bursTs via a commensaL multI-beam Gpu-powered Hpc at the gmrT), a GPU-accelerated commensal backend operating at the upgraded Giant Metrewave Radio Telescope (uGMRT). While SPOTLIGHT is primarily designed for real-time detection and localisation of fast radio bursts (FRBs), it simultaneously records a subset of beamformed data products for periodicity searches without requiring dedicated telescope time. To process the large data volumes generated by the survey, we have developed a scalable FFT-based pulsar search pipeline that combines radio-frequency interference mitigation, GPU-accelerated dedispersion and periodicity searches, multi-beam candidate sifting, efficient folding and machine-learning classification. Using population synthesis and archival uGMRT observations, we estimate that a fully operational SPOTLIGHT survey with 160 PC and one IA beam could discover $\sim$ 450 new pulsars, probing both high-sky coverage and faint pulsars over three and a half years of commensal observations. The pipeline has been validated on GMRT Cycle 48 and 49 observations (i.e. April 2025 to Mar 2026), successfully re-detecting numerous known pulsars with a wide range of Period, DM and flux densities, and is currently operational for SPOTLIGHT commensal data processing. We describe the SPOTLIGHT observing system, pulsar survey design, search parameter space, candidate-selection strategy, current status, and future developments. SPOTLIGHT demonstrates the scientific potential of commensal pulsar surveys and serves as a pathfinder for real-time, large-scale pulsar and transient searches in the SKA era.

Comments15 pages and 8 figures; Submitted to Astrophysical Journal (ApJ)

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