A GPU based single-pulse search pipeline (GSP) with database and its application to the Commensal Radio Astronomy FAST Survey (CRAFTS)

被引:7
作者
You, Shan-Ping [1 ,2 ]
Wang, Pei [3 ]
Yu, Xu-Hong [2 ]
Xie, Xiao-Yao [1 ,2 ]
Li, Di [3 ,4 ]
Liu, Zhi-Jie [2 ]
Pan, Zhi-Chen [3 ]
Yue, You-Ling [3 ]
Qian, Lei [3 ]
Zhang, Bin [2 ]
Chen, Zong-Hao [2 ]
机构
[1] Guizhou Univ, Sch Comp Sci & Technol, Guiyang 550025, Peoples R China
[2] Guizhou Normal Univ, Key Lab Informat & Comp Sci Guizhou Prov, Guiyang 550001, Peoples R China
[3] Chinese Acad Sci, CAS Key Lab FAST, NAOC, Beijing 100101, Peoples R China
[4] Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, ZA-4000 Durban, South Africa
基金
中国国家自然科学基金;
关键词
methods; data analysis; pulsars; general; surveys; astronomical databases; BURST;
D O I
10.1088/1674-4527/21/12/314
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We developed a GPU based single-pulse search pipeline (GSP) with a candidate-archiving database. Largely based upon the infrastructure of the open source PulsaR Exploration and Search Toolkit (PRESTO), GSP implements GPU acceleration of the de-dispersion and integrates a candidate-archiving database. We applied GSP to the data streams from the Commensal Radio Astronomy FAST Survey (CRAFTS), which resulted in quasi-real-time processing. The integrated candidate database facilitates synergistic usage of multiple machine-learning tools and thus improves efficient identification of radio pulsars such as rotating radio transients (RRATs) and fast radio bursts (FRBs). We first tested GSP on pilot CRAFTS observations with the FAST Ultra-Wide Band (UWB) receiver. GSP detected all pulsars known from the the Parkes multibeam pulsar survey in the corresponding sky area covered by the FAST-UWB. GSP also discovered 13 new pulsars. We measured the computational efficiency of GSP to be similar to 120 times faster than the original PRESTO and similar to 60 times faster than an MPI-parallelized version of PRESTO.
引用
收藏
页数:11
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